#advanced-pdes
1 messages · Page 5 of 1
I just don't know what the definition of unconditional stability is
In this article
Again 😮💨
We've developed the basic weak existence theory (Lax-Milgram, Fredholm Alternative, spectrum results) for linear elliptic PDES with Dirichlet boundary conditions, but I'm wondering how such results generalize to Neumann conditions
Have you heard of the dirichlet to neumann operator
How do the Dirichlet boundary conditions appear in the theorems, if at all? Are the Dirichlet boundary conditions only imposed in some examples?
?
That would be super helpful thanks
Not familiar with that no
Ok so the DtN operator lets you turn dirichlet boundary data into neumann boundary data
sucksuko
I'm having some trouble deriving this. ($L$ is the Lagrangian.)
I've got up to $\delta S = \sum_i \int_{t_1} ^{t_2} \pdv{L}{q_i} \delta q_i + \pdv{L}{\dot{q}_i} \delta \dot{q}_i + \pdv{L}{\ddot{q}_i} \delta \ddot{q}_i \dd{t}$.
I know that for the first order version, you take $\dv{t} (\pdv{L}{\dot{q}_i} \delta q_i)$ and re-arrange it. So I've tried doing a similar thing, i.e. $\dv{t} (\pdv{L}{\ddot{q}_i} \delta q_i) $ and then differentiate once more wrt $t$, but I'm really not sure if what I'm getting is right.
My working says that $\pdv{L}{\ddot{q}_i} \delta \ddot{q}_i = \dv[2]{t} (\pdv{L}{\ddot{q}_i} \delta q_i ) - \dv[2]{t} (\pdv{L}{\ddot{q}_i ) \delta q_i - 2 \dv{t} (\pdv{L}{\ddot{q}_i} \delta \dot{q}_i ).$
Douglas
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So the trouble I'm having is with the $\delta \dot{q}_i$ term right at the end
Douglas
You can do integration by parts, but this gives
actually, i've got it now
painful question tho
All you should be needing to do is apply integration by parts twice
that's why there's two derivatives of time
can I ask where did you find this? or what book? I might be able to help
euler lagrangian equation for second order?
@hazy mortar clerk told me to tell you to friend his alt "barconstruction" so that he can talk to you about ocaml
hope youre doing well✌️
Lol
LMAO
why did u ping me here lil bro
not that disruptive
Does anyone have a reference for Ladyzhenskaya's proof of 2d euler/NS well posedness
I believe you're looking for "Solution "in the Large" to the Boundary-Value Problem for the Navier-Stokes Equations in Two Space Variables"
Is there a source where I can read up further on the shallow-water equations?
I'm kinda cramming my brain on two particular sources, which are from Introduction to Climate Modeling by Prof. T. Stocker, and Harvey Segur's Lecture 8 on the shallow-water equations.
Shallow water waves ?
https://en.wikipedia.org/wiki/Shallow_water_equations
These things.
The shallow-water equations (SWE) are a set of hyperbolic partial differential equations (or parabolic if viscous shear is considered) that describe the flow below a pressure surface in a fluid (sometimes, but not necessarily, a free surface). The shallow-water equations in unidirectional form are also called Saint-Venant equations, after Adhém...
I'm mainly wanting to derive them, and the two sources I'm looking at do a good job, but there are some parts where I just want to know why certain things happen in the derivation.
Also, let me take a look!
Check in the references
There are 3 in the aforementioned document, but I'll take a look at the first two that are mentioned!
The lecture itself was really good to me when I was a student.
The one by Harvey Segur?
no the file I sent you
Oh, they're lecture notes. Interesting.
I'll take a look at this, though I do believe that it's probably a bit more complicated than what I'm expected to do.
Which certain things
Does anyone know references for eigenvalues of elliptic operators with neumann boundary conditions? Evans does dirichlet only
In particular I want to know conditions for when the operator is pos def
@steep oyster What do you want to know exactly ?
Doesn't this follows directly from the construction by sesquilinear forms
i'm not sure what that is. are you saying that the condition always holds?
You want to investigate operators -div(A Nabla .) on bounded Lipschitz domains, A being uniformly elliptic and with boundary condition A Nabla u . n = 0 on the boundary ?
yeah i think that's right. specifically, my operator is laplacian + a 0th order term
Okay the 0 order term is wat can actually would messed everything up
the only thing i know on the 0th order term f is int f = 0. in particular, no information on the sign of f
Like
Functionanatolysis
yeah that's right
So knowing this has non negative eigen value is the same as knowing that
$$\langle \nabla u, \nabla u\rangle + \langle f u, u\rangle \geqslant 0$$
Functionanatolysis
for all u in H^1.
agreed this is the weak form of the above
do you know of any non-pointwise conditions on f to gauarntee that?
only conditions that are not compatible with the mean 0 : f being non negative
(but this implies f =0 if you ask for 0 mean)
oh yeah i do want to eventually conclude that f equiv 0.
i wanted to use a spectral argument to go from int f = 0 -> f = 0. but this requires pos def of e.g. the above operator
The Neumann Laplacian has eignein value 0, and then non negative eigenvalues
you mean -Delta u = 0 + neumann conditions? that doesn't invovle f though
so adding a term that could have negative value as a multiplication operator should shift the spectrum on the left by the essential infimum of f
I didn't finish my explanation at time
sry for interrupting
My bad
I should have provided the whole explanation in a row
(This is purely moral)
so what i'm after is (morally?) equivalent to f^- = 0 in Linf ?
do you have a reference for this spectrum shifting idea
yeah
There are plenty of references
my favourite being
Cheverry & Raymond A guide through spectral theory.
thanks a bunch!
Exercise 3.15. p.69-70
hi does anyone have An introduction to partial differential equations by Michael Renardy and Robert C. Rogers
a paper im reading quotes theorem 12.44 but im confused about what its stating so i want the original theorem
I didn't get the ping for this, but I think I got it figured out! I went to office hours today with my professor. Thank you!
I would love some feedback on this attempted solution to the problem in attached screenshot:
For Helmholtz equation:
$$
u''(x) + \alpha^2 u(x) = f(x), x\in [-1,1]
$$
With bcs = $u(\pm 1) = 0$.
We define $L(u) = u''(x) + \alpha^2 u(x)$, and $R = L(u) - f$ and $R_N = L(u_N) - f$.
We seek to find an approximation solution $u_n \in V_n$ where $V_n$ is the span of $\psi_i$, for $\psi_i (\pm 1) = 0$. By Galerkin's method we find $u_N \in V_N$ such that $(R_N,v)=0 \forall v \in V_n$.
Expressing as linear algebra problem:
$$
(u_N'' + \alpha^2 u_N - f, \psi_i) = 0, i \in 0,1,\dots,N
$$
With some manipulation we get:
$$
\Rightarrow \sum_{j=0}^N \hat{u}_j ((\psi_j'',\psi_i) + \alpha^2(\psi_j, \psi_i)) = (f,\psi_i), i \in 0,1,\dots,N
$$
We define $\mathbf{x}$ such that $x_i = \hat{u}j$, $\mathbf{b}$ such that $b_i = (f, \psi_i)$, and $A$ such that $a{ij} = \alpha^2(\psi_j, \psi_i) - (\psi_j',\psi_i')$.
As such, $u_N$ may be found by solving $A\mathbf{x} = \mathbf{b}$ for $\mathbf{x}$.
madlor
i hope im in the right channel for this, numerical analysis could perhaps be the correct place too
Numerical analysis
ok. delete to not clog up channel or can i leave it here?
what is this? (Ordinary Differential Equations by Vladimir I. Arnold)
for this problem from evans, doesn't u automatically satisfy the entropy condition since it's decreasing in x? or am i tripping
(ofc i still have to check that it's an integral solution of the PDE)
ahh evan's, my favourite past time
it's a pretty nice textbook
its just this one thing that i'm confused over
do we even need to care about entropy? because it's a shock wave not a rarefaction wave right?
I have no idea. I only studied the parabolic and the strong/weak maximum principles sections for my MFE
@candid token You'll struggle to get help here though. Even though evan's book is very nice, PDEs in mathematics is definitely a minority topic in math departments. I would try out the physics discord channel. They might not know the book, but these PDEs are use a lot in stat mech
PDEs in mathematics is definitely a minority topic in math departments
What?
lol
They might not know the book, but these PDEs are use a lot in stat mech
i think physics phd students know what evans PDE is lmfao
also why single out stat mech
because I'm familiar with it in from my physics undergrad
Could be used in others, but I just know it's true for stat mech
could be
like uh
all of the others
general relativity comes to mind as an unbelievably powerful and central aspect of modern physics
Generalising statements are pointless. Sure, every field has pde's, but how many use them on a daily basis and require the understanding of fundamental theorems of pde's
There are whole departments of mathematics that are dedicated to studying PDEs, both as PDEs in itself and studying PDEs arriving from different phenomena. Quite a lot of Field medalists have been given their medal for notable contributions in PDEs.
im pretty sure PDE is by far the most common thing in math departments worldwide
@lilac barn Not my experience at my university
go to a better school then
Generalising statements are pointless.
it's ranked top 3 in Aus 
Huh
the world is a big place
exactly
as you will learn
unless you're comparing to the resources of a university like oxford/MIT, there's not a whole lot of difference between the universities from the class below.
You would only care about specialisation
see here
this is not a “generalizing statement”
you can look at basically any university
I mean like, some universities that are very "low ranked" can be decent
yours is in a very very small minority
in subfields
but bad in other fields. I.e. my local university is in a mining town and money is pumped into the engineering department
And you might also not be a good judge of the research interests of the professors at your university. It might be they're tackling some obscure problem but the motivation or the technique could be very PDE.
So globally, top ranked 20-50 universities, there's not a whole lot of difference between them.
I don't have enough fingers to count how many of my professors went to princeton for example
This is wrong as well but doesn't have much relevance to the current topic. Also, it seems like the discussion is getting tangential so let's move it to #math-discussion if necessary
Just not true
I actually agree with Ange. @grave oyster Activity about a field can be easily measured by the amount de preprint on Arxiv on a daily basis
Math.AP (Analysis of PDEs) just utterly destroys any other category.
I don't know about the quality of the research itself, but there is so much work uploaded there.
and Pde is connected with lots of other areas of math
this seems wrong, combinatorics definitely has way more publications than pde
probability theory also has way more than PDE
my question spawned a flamewar ig lmao
we've discussed how to use the galerkin method to prove existence of solutions to linear evolution equations but I'm having trouble seeing how to apply it to non linear equations. In particular there's two steps in the process bringing complications: first global existence of finite dimensional solutions (the non linear solutions usually make the resulting system of ODEs only admit local solutions) and convergence of the non-linear terms when passing from finite to infinite dimensions
are there general tricks for dealing with those?
No lol
hurb i will cry alone then
If nonlinear equations were easy to deal with then the field of pdes wouldn't exist
yeah fair point haha, i was just hoping for an easy way out of my struggle
Galerkin still can be useful for non-linear equations. Usually to get global solutions you look for additional estimates indep of time and to pass to the limit you'll need some other nice bounds on your solutions so you can pass to the limit in the non-linear terms via some div-curl type lemma
i dont think math.PR is at all close to math.AP in terms of activity
you are right about math.CO though
Yeah I ended up figuring it out for my specific case, thanks
v(x)=u(Mx) where M is rotational matrix and u is a harmonic function. we write this to prove that laplace operator is invariant. But my point is since u is harmonic in Rn and any rotation to vector will be inside Rn only so as lap(u) = 0 regardless of what we put in place of x in Rn what is the point in proving it is invariant?
is anything even worthwhile if it's not one day used in a PDE /j
Is it possible to have a distribution that is given by integration against a function $f$ but $f \notin L^1_{loc}$?
L
You can get distributions out of some functions that aren't locally integrable in a couple of ways at least. For simplicity let's assume that there is only one point the function fails to be locally integrable at and we are in dimension 1. The ideas generalise a bit, but not always in a canonical way.
-
By understanding the integral in a a limiting sense (principal value). e.g. p.v. (1/x) is one that shows up often. Integrate your input multiplied by 1/x outside the interval (-r,r) and take r->0.
-
Sometimes when you do the process in 1., the integral need not converge (this is the case with 1/x^2 instead of 1/x for example). Then instead as r->0 you get an asymptotic expansion in r, involving some negative order terms as well. Nevertheless, if you drop you "divergent part" (the negative order in r terms), you can then take the limit and get a well defined distribution. This process is called Hadamard regularisation, and the resulting distributions are finite part (p.f.) distributions.
They behave a bit like one might guess. E.g. p.v.(1/x) has distributional derivative p.f.(-1/x^2).
So hamilton jacobi equation induces the two hamilton equations by method of characteristics
Can you go the other way around?
Your question is a bit vague to me, but I think yes. The HJE can come about (amongst other ways) by starting with Hamilton's equations and solving for the symplectomorphism that changes variables to those in which the Hamiltonian is trivial.
The solution to the HJE is then a generating function (in the symplectic geo sense) for this symplectomorphism.
You can pass between all these different mechanics formulations pretty freely. HJE is particularly cool because in some sense it passes closest to quantum mechanics.
Basically the professor said that there are three different equivalent ways
Hamilton Jacobi equation is $u_t+H(x,Du)=0$
Whoever
Hamilton equations are $\dot{x^i}=\partial_{p_i}H$, $\dot{p_i}=-\partial_{x^i}H$
Whoever
Whoever
Tbh idk any of the words you said to me 🙃
But the answer was that the solution to the hamilton equations is the path x that minimizes this integral if H = L* which is the Legendre transformation
Lol. Well yes these are the three formalisms I was referring to. It sounds like you understand some directions of their equivalence. For a complete picture though you should really learn some symplectic geometry, this is the natural language to speak in.
This is passing from Lagrangian to Hamiltonian, not from Hamiltonian to HJE, as you originally asked.
Oh I see
I won't be able to do this in undergrad I'm afraid 🙃
there are other things I will have to learn like
Logic
And algebraic geometry
Actually next semester is geometry time so I might learn some of that
But I have to say this theory is so beautiful to me
Yeah I like it too, mostly when the symplectic geometry enters the picture though. Before that it felt kind of ad hoc even though it worked.
Actually I am doing a reading course next semester on some geometry stuff
I forgot the name
But sung jin oh is leading the reading course
Cool 🙂
It is very gomez brand to 🐶 whoever.
Hey, I'm trying to work out the action of an operator with Fourier symbol $a(\xi)$ on an oscillatory function but I'm a bit stuck on a part. All is gonna be in $\bR$, it doesn't change much.
Not 100% sure what assumptions are the right ones, but I'm taking $a$ such that for all $n\in\bN$, there is $C_n$ such that $|a^{(n)}(\xi)|\le C_n\sqrt{1+\xi^2}^{1-n}$.
I wanna look at the action of the operator $ia(-i\partial_x)$ on an oscillatory function of the form $u_\varepsilon(x)=b(x)e^{i\frac{S(x)}\varepsilon}$, where, say, $b\in\mathcal S, S\in C^\infty$ and $\varepsilon$ goes to $0$.
Then I got $$a(-i\partial_x) u_\varepsilon(x)=\frac1{2\pi}\int_{\bR} a(\xi)b(y)e^{i\frac{S(y)}\varepsilon} e^{i(x-y)\cdot\xi},\dd y,\dd\xi.$$
Then I can rescale it as $$\frac1{2\pi\varepsilon}\int_\bR a(\frac\xi\varepsilon)b(y)e^{\frac i\varepsilon(S(y)+(x-y)\xi)},\dd y,\dd\xi,$$ and I'm in the right setting to apply the stationary phase approximation, but I'd like to get one more term in the approximation, in order to (ideally, not sure that's the right formula it's just the one I expect to get) reach $$ia(-i\partial_x)u_\varepsilon(x)=ia(\frac{S'(x)}{\varepsilon})u_\varepsilon(x)-a'(\frac{S'(x)}\varepsilon)b'(x)e^{i\frac{S(x)}{\varepsilon}}+o(1).$$Any hint regarding how I can achieve that, or anywhere I can find lower order terms in the stationary phase method?
upheaval
Could you expand on this btw, I know symplectic geometry is the natural setting for control theory, but I've always been curious
At conference dinner, will reply at some point over the next few days.
Thanks! Enjoy dinner
Otherwise just read some of Arnold's classical mechanics book for quite a readable exposition of a lot of these ideas. Great book.
Abraham Marsden too, but that is maybe less good for gaining intuition.
So we have initially this perioidic eigenvalue Sturm-Lioiville problem
$$ - u^{''}n (x) + \left( V(x) - \lambda \right) u_n (x) =0,$$
with $u_n (0) = u_n (L)$ and $u' n (0) = u' _ (L).$
Now we plug in $u{\kappa} = q{\kappa} (x) e^{i \kappa x}$ in the eigenvalue problem so basically we replace $u_n$ by $u_{\kappa}$, where $\kappa = \frac{2\pi x}{a}$ and $a=\frac{L}{N}$, we get
$$-e^{i \kappa x} q^{''}{\kappa} - 2e^{i \kappa x} i \kappa q' {\kappa} (x) + e^{i \kappa x}q_{\kappa} (x) * \left( \kappa ^2 + V(x) - \lambda \right)=0,$$
where $q_{\kappa} (0) = q_{\kappa} (a)$ and $q' {\kappa} (0) = q' _ {\kappa} (a)$.
We can write $V(x)$ as a trigonometric polynomial
$$V(x) = \frac{1}{2}V{0} - V{0}\frac{e^{i\frac{2\pi}{a}x} + e^{-i\frac{2\pi}{a}x}}{4},$$
with the fact that $V(x+a) = V(x).$
Now we can solve this with the Frobenius method, but instead with a power series, we use a Fourier series
$$q{\kappa , n} (x) = \frac{1}{\sqrt{a}} \sum_{k \in Z} \hat{q_{\kappa , n , k}} e^{\frac{ i 2 \pi k x}{a}}.$$
Plugging it in the new eigenvalue problem, and applying frobenius method we get
$$\frac{1}{\sqrt{a}} \sum_{- \infty}^{\infty} \hat{q_{\kappa , n , k}} e^{\frac{i 2 \pi k x}{a}} \left( \frac{16 \pi ^2 k^2}{a^2} + \frac{V_0}{2} - \lambda \right) \frac{- V_0}{4} \hat{q_{\kappa , n , k-1}} e^{\frac{i 2 \pi k x}{a}} - \frac{V_0}{4} \hat{q_{\kappa , n , k+1}} e^{\frac{i 2 \pi k x}{a}} = 0.$$
From this we get the following recurrence relation
$$\hat{q_{\kappa , n , k+1}} = \hat{q_{\kappa , n , k}} \left( \frac{64 \pi ^2 k^2 }{a^2 V_0} + 2 - \frac{4 \lambda}{V_0} \right) - \hat{q_{\kappa , n , k-1}}.$$
Now my question is if we set $V(x) = 0 $ then we only have $\hat{q_{\kappa , n , k}}$ the other q's will vanish. How can we solve the eigenvalue problem with $V(x)=0$ then?
Fractalogist
I need to find the eigenvalues $\lambda _{\kappa, n}$ and their respective eigenfunctions.
Fractalogist
Hey for the Navier Stokes equation the left side builds a total differential of the acceleration which is the local acceleration and convective acceleration or the total differential of velocity differentiated with respect to time, however im a little confused on the following
this would just be the way its written down in general
however when you just look at the x-direction a lot of publications show it as the following: https://cdn.discordapp.com/attachments/423244559682764800/1185330239727997009/image.png?ex=658f37cf&is=657cc2cf&hm=410ba0fffe93577ff38cbbfd43567ebe796a3d6efc4599e520d38f9180ac1bc0&
but if the total derivative with respect to time is the following:
then, ignoring the density rho, how is the velocity in x direction u inside the derivative and squared?
So partial(u^2)/partial x=2*u*u_x right
This is what you want but there's an extra factor of 2
If you ignore rho and suppose the fluid is incompressible, then d_x u + d_y v + d_z w = 0 (the velocity field is divergence free).
I know that but thats not what i was originally asking, im still confused why the notation seems so different in different publications
like even Wikipedia seems weird about it
The two expressions are equal
if you take this into account
in particular, $$\partial_x(u^2) + \partial_y (uv) + \partial_z(uw) = u \partial_x u + v\partial_y u + w \partial_z u = [(\vec{v} \cdot \nabla) \vec{v} ]_1$$
ryc
this isn't quite the formula for the total derivative in the first coordinate
so that holds when the laplace operator of vec field v = 0 ?
you apply a directional derivative to u in the (u, v, w) direction
the divergence of v = 0 in this case
to see that, we can expand this
using the product rule on the left hand side (i'll even use it on the square), we have
\begin{align*}\partial_x(u^2) + \partial_y (uv) + \partial_z(uw) &= u \partial_x u + u \partial_x u + u \partial_y v + v \partial_y u + u \partial_z w + z \partial_z u \
&= u (\partial_x u + \partial_y v + \partial_z w) + u \partial_x u + v\partial_y u + w \partial_z u \
&= 0 + u \partial_x u + v\partial_y u + w \partial_z u
\end{align*}
ryc
omg ok that makes a lot of sense now
went through 3 books on this and no one ever went to the effort to show this and just wrote it down
(if you include a density, you no longer have that the velocity field is divergence free. instead you have the conservation of mass equation for the density, which lets you do the same cancellation)
i had the exact same experience for ages lol, it's so dumb
but yeah i guess the math still holds true, so in the end with incompressibility it doesnt matter which notation i use tho right?
of course it doesnt theyre equivelent
but it's very very useful to be able to decide whether you want to write $\vec{u} \cdot \nabla \vec{u}$ or $\nabla \cdot (\vec{u} \otimes \vec{u})$ in more advanced pdes, so it's a good thing to remember that divergence freeness kills half the product rule here
ryc
also happns when you dont just have u twice, but the FIRST vector field is divergence free (not necessarily the second!)
it's the outer product (matrix where the ijth entry is u_i * u_j)
oh
so here the stuff in the derivatives is the first row of the outer product: u^2, uv, uw
and the next row would be uv, v^2, wv, and then uw, vw, w^2
and each of those you take the divergence of
ah right
it's a little shorthand
you mentioned this btw can you expand?
you wrote down $\partial_t u + u \partial_x u + u \partial_y v + u \partial_z w$ but i think you meant to write down $\partial_t u + u \partial_x u + v \partial_y u + w \partial_z u$
ryc
the easy way to remember the order is to remember that it looks like $[(u, v, w) \cdot (\partial_x, \partial_y, \partial_z)] u$. it's a directional derivative from multivariable calc
ryc
it's just that the direction is also a function now
and ofc, what i just wrote is exactly $(\vec{u} \cdot \nabla) u$
ryc
ok i always get a little confused with the notation since ive also read from literature thats its referred to as pseudovectorial notation
ya
it's confusing
like when you apply a differential operator to a vector, you just apply it to each coordinate or whatever
lots of fluids comes down to keeping track of what indices match what haha
so its v dotproduct grad v right?=
yes
and the dot product happens first
then you apply the thing you get (which is a linear combination of derivatives) to each component of v
it says "the x component of v moves in the direction (u,v,w)"
and so do the y component and z component
this makes sense since as the fluid particles move, they conserve momentum (they bring their velocity components along with them in the direction they're moving) until a force or pressure forces it to change
but if the dot product happens first
wait now im really confused
isnt the dot product that happens first = du/dx + dv/dy + dw/dz
and so if i multiply the scalar with the vector of u again i get u du/dx + u dv/dy + u dw/dz
so
really important here
even for single variable functions, the operator $\frac{d}{dx} f$ and the operator $f \frac{d}{dx}$ are not the same
ryc
multiplication of functions and differential operators is not commutative
this sounds ridiculous if you havent seen it before, but this is actually the thing that causes heisenberg's uncertainty principle
I mean yeah ive been told before that operators are supposed to be treated differently
since they arent really numbers or variables or whatever
but in this case, it's important because if we multiply either of these by a function g, we get different answers
which is also where my confusions from the beginning stems from how the u ended up in the derivative
(g on the right)
so in this case, we have (v dot nabla) v
the stuff in the parenthesis first. since v is on the left, we can't swap the order of the derivative and v, so we just leave it next to the derivative. in this case, that gives u d_x + v d_y + w d_z (each component, and then summed)
oh i see
is that ok? after that we can apply to the v outside the parenthesis
now we have (u d_x + v d_y + w d_z) vec(v)
the left hand side is now a "scalar" (its not a vector anymore, after all the dot product outputs scalars)
so we just do scalar multiplication into each component of vec(v)
exactly
ok nice that cleared things up
so in the first slot, you get all the differentials applied to u. in the second slot, they all apply to v. etc
btw while we are on topic do you know perhaps where $\left(\vec{v}\cdot\nabla\right)\vec{v}=\nabla\left(\frac{1}{2}\vec{v}^2\right)-\vec{v}\times\nabla\times\vec{v}$ comes from?
lennygo
hmmm
or $grad\left(\frac{1}{2}\vec{v}^2\right)-\vec{v}\times rot\vec{v}$
lennygo
anything with these double cross products is a huge mess
I mean when i went to write it all out it is true
im just wondering how anyone came up with it
It comes from Schlichtings Boundary Layer Theorie if youve heard of it
hmm
i dont have a good reason for why this should be true off the top of my head. it's oftentimes useful to find gradients that you can extract from one term or another because they can be stuffed into the p (which doesnt care as long as what you stuff into it is a gradient)
so at least on an algebraic level, it gives you a new nonlinear term v x rot v that you can screw with. which might be nice if you want to say stuff about vorticity (rot v)
ok
i guess it's the "rotational correction" in some sense
if you're rotating in a circle
rot v points you perpendicular to the plane of the circle
v points you tangent to the circle
so -(v cross rot v) (youve got to check the sign) points you towards the center of the circle
that's just like centripetal force
huh
grad(v^2) just says "go mostly in the direction where the velocity is growing" and -v cross rot v says "but make sure to get nudged towards the direction the veclocity field is turning". which together I guess adds to following the velocity field exactly.
shrug
its a good exercise to try to interpret this stuff as physics so i appreciate being made to do it
its supposed to represent the convective acceleration btw
Ok uhm shortly after my previous problem i have another one... has anyone here encountered div and Div?
The book author uses div and Div and there is a difference between them but he never goes into detail what the difference is
it just sort of jumps from one equation to the other
Its probably because these books care more about the answers and applications of the theory than the mathematical background
ive got a physical copy but i can quickly write it down
Explicitly for the Navier-Stokes-Equations under a symbolic writing:
$\rho\frac{D\vec{v}}{Dt}=\vec{f}-grad\left(p\right)+Div\left(\tau\right) with \tau=\mu\left(2\dot{\epsilon}-\frac{2}{3}\deltadiv\left(\vec{v}\right)\right)$
lennygo
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Potentially because tau is a tensor
thats confusing then because matrix dont have divergences no?
or does that only apply to special tensors
The derivatives of scalars, vectors, and second-order tensors with respect to second-order tensors are of considerable use in continuum mechanics. These derivatives are used in the theories of nonlinear elasticity and plasticity, particularly in the design of algorithms for numerical simulations.The directional derivative provides a systematic w...
Yeah i was just about to say found the ressources for it, thanks
didnt even know you could do this
But also if you're working with newtonian fluids this doesn't matter that much
terrance tau? 
In fluids, divergence of a matrix always means "take the divergence of each row vector". The result is a column vector, each entry is the divergence of each row
You know what im just gonna drop the book for now and switch to the Anderson and see what he has to say, a lot of people recommended that one
I bet Schlichting's book is pretty good but its just not a book that introduces you to the topics you need to know when approaching this stuff damn
Boundary layer theory?
Say we have a uniformly bounded sequence ${u_k}_{k=1}^\infty$ in $W^{1,m}(\Omega)$. Here $m$ is greater than the dimension $N$ of the ambient Euclidean space $\mathbb{R}^N$.
By weak sequential compactness of $L^m(\Omega)$, we have $u_k \rightharpoonup u \in L^m(\Omega)$ as $k \to \infty$.
And for each $i$:th weak partial derivative we have $ \displaystyle \frac {\partial u_k}{\partial x_i} \rightharpoonup \frac {\partial u}{\partial x_i} \in L^m(\Omega) $ as $k \to \infty$.
Say moreover we have a bound $C$ on the gradients, where the bound $C$ does not depend on $k$:
[
\left( \int_\Omega |\nabla u_k|^m dx \right)^{\frac 1m} \leq C < \infty
]
How can I show that this inequality passes over to the limit $u \in W^{1,m}(\Omega)$? In essence, how can I justify letting $k \to \infty$ in the inequality above? Namely I would like to verify
[
\left( \int_\Omega |\nabla u|^m dx \right)^{\frac 1m} \leq C
]
I have only managed to prove for each weak partial derivative that
[
\left( \int_\Omega \left| \frac { \partial u }{ \partial x_i } \right|^m dx \right)^{\frac 1m} \leq C < \infty
]
But how can this be used to obtain the inequality for the whole gradient $|\nabla u|$ and not just its components?
hardisc
Prove that weak convergence, in general, implies Fatou's lemma for the corresponding norm.
As for the Gradient, once you have the m-norm bounded for each component, use lm into l2 inclusion, so you can use "Fubini" to bring the summation outside to get something like a bound NC
shiburin
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So many typos🤦♂️
Anyway I want to know why my proposed variational problem for $u(r, \theta)\in \dot{H}^1_{0, \text{div-free}}(\Omega)$ is wrong
shiburin
are spectral bases like the nearly orthigional hat functions from the fem?
ah is this related to the reinmann lebeque lemma?
Sort of but not really?
alright, im just trying to understand this. my teacher talked highly of this book so im reading it
A spectral basis is a truncation of a fourier series
got it, and the sums there look similar it as well
Yes
got it, thanks for that. this book is really cool gotta say 🙂
the signials going to zero, and the the inverse problem is amplflying them blew my mind too cool
i appreciate the help man!
thank you for the quick input, and apologies for a delayed response. I can see how by assuming $m$ is strictly larger than 2, we can use Hölder's inequality to show that $L^m$-integrability implies $L^2$-integrability. But I fail to see in detail how "Fubini" comes to our aid.
Of courseby definition we have $|\nabla u|^2 = \sum_{i=1}^N \left| \frac {\partial u}{\partial x_i} \right|^2
$, and this we can certainly integrate, and then interchange summation and integration, as the summation is finite.
How can we appropriately insert $ |\nabla u|^m$ into the picture here? I can certainly bound all the integrals $\int_\Omega \left| \frac {\partial u}{\partial x_i} \right|^2 dx$ upwards in terms of an appropriate constant, which in effect enables me to bound $\int_\Omega |\nabla u|^2 dx$ upwards.
hardisc
I wish I could say I knew exactly what you had in mind here, but unfortunately no. Fatou's lemma I certainly know, but in the context of norms and weak convergence, I am not quite sure what tool it is and how it potentially leads one right
Something like ( \lVert \lVert , \cdot , \rVert_{\ell^2} \rVert_{L^m} \leq C \lVert \lVert , \cdot , \rVert_{\ell^m} \rVert_{L^m} = C \lVert \lVert , \cdot , \rVert_{L^m} \rVert_{\ell^m} =C \left( \sum_{i\leq N} \lVert ,\cdot,\rVert_{L^m} \right)^{1/m})
cocat
So written in gradient language, this means we have (\lVert \nabla u\rVert_{L^m}\leq C \left( \sum_{i\leq N} \lVert \partial_i u\rVert_{L^m}\right)^{1/m})
cocat
hi again, I have been trying to understand and implement your suggestions over the holidays, but have struggled to do so. For the inclusion, I certainly have that, for any $m$ such that $m > 2$:
\begin{align*}
\int_\Omega \left| \frac { \partial u }{ \partial x_i } \right|^2 dx
& \leq
\left( \int_\Omega \left| \frac { \partial u }{ \partial x_i } \right|^{ 2 \cdot \frac m2 } dx \right)^{ \frac 2m } |\Omega|^{ 1 - \frac 2m }
= \& =
\left( \int_\Omega \left| \frac { \partial u }{ \partial x_i } \right|^m dx \right)^{ \frac 2m } |\Omega|^{ 1 - \frac 2m }
\leq \ & \leq
\left\lVert \frac { \partial u }{ \partial x_i } \right\rVert_{ L^m (\Omega) }^2
|\Omega|^{ 1 - \frac 2m } \leq C^2 \cdot |\Omega|^{ 1 - \frac 2m } .
\end{align*}
For the $\ell^2$-norm of the gradient, I believe we have simply
[
\lVert \nabla u \rVert_{ \ell^2 }^2 = |\nabla u|^2 = \sum_{i=1}^N \left| \frac {\partial u}{\partial x_i} \right|^2
]
This I can certainly integrate term by term and bound upwards, but it seems like that leads us in the wrong direction.
For the $L^m$-norm of the vector $\nabla u$, I believe we have the natural definition:
[
\lVert \nabla u \rVert_{ L^m }^m = \int_\Omega |\nabla u|^m dx
]
But I fail to see now how exactly to implement the suggested "Fubini-maneuver" with the norms, where the $\ell^2$-norm $|\nabla u| = \sqrt{ \sum_{i=1}^N \left| \frac { \partial u }{ \partial x_i } \right|^2 }$ is buried inside the integral and moreover we have a pesky square root.
hardisc
Moreover, will this really ensure that we obtain $\int_\Omega |\nabla u|^m dx \leq C^m $ from $ \int_\Omega \left| \frac{\partial u}{\partial x_i} \right|^m dx \leq C^m $? It seems like a constant $N$, the dimension of the ambient space, manages to emerge in the sought inequality, but maybe I am just failing to see if and how it vanishes later.
hardisc
thanks, and happy holidays to everyone
I meant change l2 of gradient into lm then you can interchange Lm with lm
is b matrix like a matrix of fourier coefs? kinda like a matrix of sin and cos and the highest value at the top is associated with the lowest freq while the bottom v is associated with the highest frequence?
Yes, that seems to be the case at first glance. Fourier coefficients are sometimes viewed just as a complex exponential as working with exponential tends to be cleaner
Absolute Fourier coefficients, there is an absolute value on it
rgr, yeah i see it. im self taught on these things so im just verifying my intution is correct 🙂
so this reimann lebeque lemma is essentially saying that as you go into the higher frequences (higher order of n in the fourier expansion) the signals (values) become zero right???
sorry this is a book about discreet inverse problems, so i think this the right place to ask, but im sure this is an analysis question im asking
its in relation to this part here
kinda beautiful how bessels/parsvaels inequalities come up
in a way this is similar to saying |bn| <= A/n^4
For an integrable function, yes
thank you very much 🙂
Because i before e except before c is an arbitrary rule
oh i didn't realise that lol cocat
but i think a lot of german names are unfortunately spelled wrong by english speakers lol
i didnt mean to disrepsect the legend. im just some dumb redneck 😛
thank you, I think I managed to put it together, but I do have a follow-up question. here is how I went about it.
Hölder's inequality (for series) yields:
\begin{align*}
|\nabla u|^2 = \lVert \nabla u \rVert_{\ell^2}^2 = \sum_{i=1}^N \left| \frac {\partial u}{\partial x_i} \right|^2 & \leq \left( \sum_{i=1}^N \left| \frac {\partial u}{\partial x_i} \right|^m \right)^{\frac 2m} \left( \sum_{i=1}^N 1 \right)^{ 1 - \frac 2m } \leq
\ & \leq
\lVert \nabla u \rVert^2_{\ell^m} \cdot N^{1 - \frac 2m}
\end{align*}
Thus, raising this to $\frac m2$, we have
[
|\nabla u|^m \leq \lVert \nabla u \rVert_{\ell^m}^m \cdot N^{\frac m2 - 1}
]
Integrating yields (here I switch order, but it is trivial, as the sum is finite):
[
\int_\Omega |\nabla u |^m dx \leq N^{\frac m2 - 1} \cdot \int_\Omega \left( \sum_{i=1}^N \left| \frac {\partial u}{\partial x_i} \right|^m \right) dx
= N^{\frac m2 - 1} \cdot \sum_{i=1}^N \left( \int_\Omega \left| \frac {\partial u}{\partial x_i} \right|^m dx \right)
]
Using $\int_\Omega \left| \frac {\partial u}{\partial x_i} \right|^m dx \leq C$, we get
[
\int_\Omega |\nabla u|^m dx \leq N^{\frac m2 - 1} \cdot \sum_{i=1}^N C^m = N^{\frac m2 - 1} \cdot C^m \cdot N = N^{\frac m2} \cdot C^m
]
Raising to $\frac 1m$, we get at last
[
\left( \int_\Omega |\nabla u|^m dx \right)^{\frac 1m} \leq \sqrt N \cdot C
]
So we did not quite get $ \int_\Omega |\nabla u|^m dx \leq C^m $, but rather the factor $\sqrt N$ appeared. But the sought goal was to go from $\int_\Omega |\nabla u_k |^m dx \leq C$ to $\int_\Omega |\nabla u|^m dx \leq C$.
Is this not possible, or am I just failing to see an additional argument?
hardisc
You will get something with N but that's just a determined constant so that can go inside C.
ok interesting, thanks! I should have been clearer in my first question, but the $C$ appearing in both inequalities was intended to represent one and the same constant. So the question was if and how to justify that e.g. $\displaystyle \int_\Omega |\nabla u_k|^m dx \leq 4$ will imply $ \displaystyle \int_\Omega |\nabla u|^m dx \leq 4 $, when $k \to \infty$. but I suppose that is not the case then?
hardisc
for context I am reading Julio Rossi's paper on tug-of-war games and pde:s, where he argues as follows:
it seems as if the upper bound stays the same, even when passing to the weak limit $u_\infty$, upon letting $p \to \infty$ in the inequality obtained for $\int_\Omega |\nabla u_p|^m$. I do not see why he does not change the upper bound, even if it is not all that important for the subsequent results
hardisc
That's just Fatou's lemma
I thought so too, but we only have weak convergence, not pointwise convergence, right? If we had pointwise convergence
[
\lim_{p\to \infty} |\nabla u_p|^m = |\nabla u_\infty|^m
]
then surely by Fatou
\begin{align*}
\int_\Omega |\nabla u_\infty|^m dx & = \int_\Omega \lim_{p \to \infty} |\nabla u_p|^m dx = \int_\Omega \liminf_{p \to \infty} |\nabla u_p|^m dx
\leq \ & \leq
\liminf_{p\to \infty} \int_\Omega |\nabla u_p|dx
\leq \liminf_{p\to \infty} C= C.
\end{align*}
All weak convergence tells us is for each $i$ that
[
\lim_{p \to \infty} \int_\Omega \frac {\partial u_p}{\partial x_i} \phi dx = \int_\Omega \frac {\partial u_\infty}{\partial x_i} \phi dx
]
for each $\phi$ in the space dual to $L^m (\Omega)$. I think this weak convergence for each partial derivative can be turned into a convergence in $\mathbb{R}^N$ of the gradient vectors, namely
[
\lim_{p \to \infty} \int_\Omega (\nabla u_p) \phi dx = \int_\Omega (\nabla u_\infty) \phi dx \in \mathbb{R}^N
]
Are you saying this can be adapted so that a Fatou lemma emerges and gets us where we want to go?
hardisc
Okay I thought you had pointwise convergence. Regardless, you can use the duality characterisation of norms and as test functions are dense in Lm' and you have convergence against these functions, you get that the norms converges
Is there any progress on 2 spatial and 1 time dimensional Inverse Scattering Transform for Solitons?
Hm okay, I am trying to unpack your suggestions here. By "duality characterization of norms", do you mean the following: for any $x$ in a normed vector space $(X, \lVert \cdot \rVert)$ we have (via Hahn-Banach theorem)
[
\lVert x \rVert = \sup \left{ |F(x)| : F \in X', \hspace{5pt} 0 < \lVert F \rVert_{op} \leq 1 \right}
]
Here $ \lVert F \rVert_{op} := \sup { |F(x)| : 0 < \lVert x \rVert \leq 1 } $.
So in that case, since the weak limit $u_\infty$'s each partial derivative lives in $L^m (\Omega)$, we have
[
\left \lVert \frac { \partial u_\infty }{ \partial x_i } \right \rVert_{ L^m (\Omega) } = \sup \left{ \left| \int_\Omega \frac { \partial u_\infty }{ \partial x_i } \phi , dx \right| : 0 < \lVert \phi \rVert_{ L^{m'}(\Omega) } \leq 1 \right}
]
We have
[
\left| \int_\Omega \frac { \partial u_\infty }{ \partial x_i } \phi , dx \right| \leq
\underbrace{\left| \int_\Omega \frac { \partial (u_\infty - u_p) }{ \partial x_i } \phi , dx \right|}{ \to , 0 \text{ as } p \to \infty, \text{ by weak conv.} }
+
\left|
\int\Omega \frac { \partial u_p }{ \partial x_i } \phi , dx
\right|
]
So Hölder's inequality gives us
[
\left| \int_\Omega \frac { \partial u_\infty }{ \partial x_i } \phi , dx \right| \leq
\left|
\int_\Omega \frac { \partial u_p }{ \partial x_i } \phi , dx
\right| \leq \left \lVert \frac { \partial u_p }{ \partial x_i } \right \rVert_{ L^m(\Omega) } \lVert \phi \rVert_{ L^{m'}(\Omega) } \leq C \cdot 1 = C
]
Thus [ \left\lVert \frac { \partial u_\infty }{ \partial x_i } \right\rVert_{ L^m (\Omega) } \leq C ]
This seems to work for each component, if this is what you had in mind that is. But how do we get the same inequality for the whole gradient $ \left( \int_\Omega |\nabla u_\infty|^m dx \right)^{\frac 1m} \leq C $?
hardisc
I have great trouble using the geometric method for inhomogenous variable coefficient linear pdes... I've encountered the Lagrange-Charpit equations, are there other good methods?
hello, I need to show that the billinear form a is coercieve. It is suggested to show the poincaré inequaility (on the first subspace V for example). Once I showed it, how the coercivity follows? Because we will have |Du|^2_L^2>= C|u|^2_L^2 and the lower bound is not the norm of u in V. How to correct this please?
I've got a question regarding uniqueness for the PDE
$$ \partial_t u + (-\Delta)^{1/2}u = u |d_{1/2} u|^2 $$
where
$$ |d_{1/2} u|^2 = \int_\mathbb{R} \frac{|u(x) - u(y)|^2}{|x-y|^2} dy. $$
Now, I have a weak solution in ( H^1(\mathbb{R};\mathbb{S} ^{n-1})) and in ( C^1([0,T];L^2) ), which is great, but for a robust uniqueness proof, you would typically need ( L^2([0,T];H^1(\mathbb{R})) ).
I already have this in ( L^2([s,T];H^1(\mathbb{R})) ) for all ( s > 0 ).
The problem is that the approaches I have tried all failed because of the pseudolocal behaviour of the fractional Laplacian and the complex combination of Sobolev-Slobodeckij and Bessel spaces, which are both contained in my PDE through ( d_{1/2} ) and the Laplacian. My general question, where I am open to any ideas, is: What methods exist to combine the behaviors of the Sobolev-Slobodeckij and Bessel potential integrals, i.e., the ( d ) and the ( -\Delta ) terms?
What are general approaches to achieving this kind of integrability (in a normal setting, ( H^2 ) would be sought instead)?
Are there other approaches to establishing uniqueness for these kinds of evolution equations?
Thanks in advance for any response; I just need more ideas!
KIl
Bessel and Sobolev-Soblodeckij spaces are the same over L²
I know that, its more about the inner part of the seminorms especially locally, like the |d_1/2 u|^2 and the (-Delta)^1/4 u, how are integrals over Omega similar to each other, if they even are
But you are on the whole line
other wise uniqueness in finite time
Oh sry not the line in time is tge problem, the line in space
Yes
I didn't mixed up
There is the maximal L^q(L^p) regularity property for the Poisson semigroup
Yes there is, the part which needs local behavior is the integrability of the function over time. The approach if you are looking at the normal harmonic heat flow leads to a localised look on the integrals and then a cover argument, a direct act on the whole space leads to problems,
The problem is that the fractional laplacian isn't a local operator only a pseudo local, which leads to a similar local estimate, but an estimate which is not suitable for covering arguments.
That's why I would like to switch to slobodeckji locally somehow with the fractional gradient as well to get some kind of local behavior, but the different norms and thus different scalar products makes it hard to do that
The maximal property was already used in the duhamels principle for getting a mild and then a weak solution
but you can also use it to prove uniqueness
Theorem 3.6 pages 7-8
Ok wait now I am confused I misread the property you meant, this looks like an idea I can try thank you!
Play with Sobolev embeddings, Holder and interpolation inequalities
How do you people always have some kind of paper which at least gives one always some ideas, I mean how much paper do you all read😂
Jup thats always the best to do
I am really use to this topic, so you have been just lucky there
Happy me
anyone have any suggestions? ive been on it for like 5 hours and gotten no here
did the previous two
What's the most general strategy for Linear PDEs? I suspect it's separation of variables, but what's the systematic method to determine the ansatz in that case?
I have trouble with this Green's function. Can someone help me?
daniil9274
you could try mirroring across the x-axis and the boundary of the circle
"linear PDEs" is a very large class of problems, I don't think there is any "general" technique.
Broadly they break down into elliptic, parabolic, and hyperbolic PDEs, and there are some standard techniques within each family that work fairly broadly.
One example is the method of characteristics for hyperbolic PDEs. It is a way of turning a PDE into an ODE along certain special curves, and those ODE solutions can be combined into a PDE solution.
https://en.m.wikipedia.org/wiki/Method_of_characteristics
PDE is kind of annoying in that there is no single winning technique, there are many, many different tricks, many different ansatz that work in different situations, and many, many PDEs that are not solvable exactly by pen and paper at all.
In mathematics, the method of characteristics is a technique for solving partial differential equations. Typically, it applies to first-order equations, although more generally the method of characteristics is valid for any hyperbolic partial differential equation. The method is to reduce a partial differential equation to a family of ordinary...
Im familiar with 2nd order method of characteristics, but as you mentioned it doesnt cover the elliptic case. Im also not particularly concerned with boundary conditions since the use case here is for solving the rather arbitrary pdes you encounter when solving the symmetry condition for a nonlinear equation.
There are things you can say about when separation of variables is possible. You can always search for your "separated" solution, the question is whether every solution can be written in terms of the special solutions you find, and you can probably imagine this is a question about whether a set of vectors spans a vector space (the equation is linear after all).
One sufficient (but maybe not necessary?) condition is that your differential operator be self-adjoint. In that case, the spectral theorem guarantees you a basis of eigenfunctions, and separation of variables is possible. There is a short discussion on the separation of variables page on Wikipedia.
So for a complex matrix A to be self adjoint, does that mean the real part of the matrix is symmetric and the imaginary part is anti-symmetric?
I don't typically think of operators on a space of functions in terms of a matrix because the space of functions is usually infinite-dimensional.
I would instead look at the inner product definition of self-adjoint. I believe the right inner product to use here is the L^2 inner product.
You can, the Heisenberg form of quantum mechanics uses matrices as linear operators instead of the schrodinger equation. Then each basis of the vector space corresponds to some linearly independent function in Hilbert space.
Yeah, but you can get matrices with infinitely many entries
in that case it doesnt matter since the higher eigenvalues correspond to energy levels that dont exist in any practical sense. SO you can just cut them off as they dont contribute much to the probability.
Physics gets away with a lot 😋
yeah... i think it took mathematicians a few decades to formalize and prove Path Integrals, by that time it was a standard method in physics.
They are still not rigorous except in some special cases believe it or not
We have one of the leading path formulation guys at our school
He worked at Cal Tech and would always run up to Feynman saying "we figured out such and such about the path formulation!". He would say "does it change the physical answers?"...."No..."...."then who cares!"
You know, I hadn't considered that functional integration might apply more broadly to the space of linear PDEs than the schrodinger equation, but there does appear to be ongoing work in that area.
https://www.amazon.com/Functional-Integration-Differential-Equations-Mathematics-ebook/dp/B088D73S5L
A complex matrix is self-adjoint if it's complex conjugate equals it
Yeah, I get that but I was trying to figure out what the conditions for that would be
also its the conjugate transpose
You can explicitly write down the condition elementwise if you write down the equality for a general self-adjoint matrix
Okay. Did you know of any particularly general approaches to linear PDEs? 2nd order is probably fine, havent run into much higher than that.
I know "completely general" doesnt exist, just like more general than they teach in Uni, and where the eigenfunctions arent in a table somewhere.
,help
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A somewhat general approach is method of characteristics.
If you're familiar with Fourier analysis, then that also works in a whole bunch of cases.
There's also semigroup theory and more generally the Duhamel's principle which helps you deal with evolution pdes
Fourier analysis relies on complex exponential or sin/cos eigenfunctions doesnt it?
Yes
if you wanted to use an integral transform on something that separates into Bessel functions you would need a Henkel transform etc.
I mean any linear operators solution "could" be represented by any set of orthogonal functions, but the preference is that they diagonalize the operator, or the known methods kind of break down
Yes this is how you can view Fourier transforms as well: an operation that diagonalises the convolution
I suppose its also important that these linear PDEs will always be homogeneous, so no need of greens functions or anything
does anyone know why our integral of convultion limits go from -00 to +00 and it changes to 0 to t
and we multiply our y(t) for u(t) which is the step function
i dont understand why can anyone help?
Hi everyone. Im working on a linear PDE right now that I realized has a strange form. It is variable coefficient(they are periodic) and I realized the operator actually decomposes into two parts, where one part is really just a coordinate rotated version of the other one. For example It can be written something like (L1 + L2)z = 0, where if I just had L1, I could change it to look like L2 by the change of coordinate u = x+y, v = x-y. I know how to solve the problem if I just have the single operator L1z=0 or L2z=0, since in essence they are the same type of operator after a coordinate rotation
Is there any literature on this type of problem? Where the differential operators have this relationship?
could you show the PDE?
(1+cos(x))cos(y)zxx + (1+cos(y))cos(x)zyy + 2sin(x)sin(y)zxy = 0, notice that I can write this as [(cos(y)zxx + cos(x)zyy)] + [cos(x)cos(y)(zxx + zyy) + 2sin(x)sin(y)zxy] = 0. The two parts in brackets are almost the same if you do a rotation and a scaling. So for example, if you take the second part and do a change of variables u = x+y, v = x-y, you'll get the form of the pde in the first bracket with a factor of two. So thats why I was thinking in essence these are kind of the same operator after a rotation and scaling. If you're just trying to deal with cos(y)zxx + cos(x)zyyy for example, you can easily do separation of variables to get a product of mathieu functions for your solution.
The main theme of this problem that is interesting but also extremely annoying is that it feels like there are 4 key directions, not 2. If I just had either operator, the directions would either be (x+y) and (x-y), or x and y. I've noticed this over and over again when I analyze the problem. The main insight I gained is that you can write this problem as ((1+cos(x)cos(y)zx + sin(x)sin(y)zy))x + (sin(x)sin(y)zx + (1+cos(y))cos(x)zy)y = 0, which helped me find its also derived from a lagrangian, and when I have the rewritten in the form I just wrote, it looks like the divergence of a vector field. I figured something in the vector field formulation could help me figure out whats going on with the solution.
so is zxx or zxy shorthand for ∂²z/∂x² and ∂²z/∂x∂y?
yes
The characteristic equation for that should be:
(1+cos(x))cos(y)(∂φ/∂x)² + 2sin(x)sin(y)(∂φ/∂x)(∂φ/∂y) + (1+cos(y))cos(x)(∂φ/∂y)² = 0
which can be solved by lagrange-charpit
(assuming you can figure out the integrals)
(also this only works if the equation is not elliptic, which I didnt check. The signs make it look like it might be elliptic, at least in some regions.)
I see. I was looking at that at one point, but these would be characteristics of the energy like function no, not the dependent variable z? That would still be a nice result. The discriminant is also mixed so it would only be valid in certain regions. The domain is thought of as periodic, with each unit cell being mostly elliptic, but the regions between them transitioning from hyperbolic to parabolic.
My understanding is hyperbolic, elliptic, parabolic classification is pointwise, so the characteristics might be valid in some places and invalid in others. Keep in mind that unlike first order characterists, second order characteristics are not solutions. They propagate boundary conditions over the region of the solution.
(z is constant along the characteristic)
(I used the variable φ to emphasize that the characteristic is not a solution)
I see. I appreciate the help. I am trying to work this out for the easier problem where I am just looking at cos(x)(cos(y))(zxx + zyy) + 2sin(x)sin(y)zxy = 0, because I do know at least one infinite family of solutions to it and then I can try to see how those might emerge from the lagrange charpit equations.
Is there any good interpretation of whats going on when my characteristics transition from regions where they are real in the hyperbolic regions to the complex in the elliptic regions? Because in my case, that will be happening periodically in this medium.
I havent finished reading it yet, but if you wanted to continue on your separation of variables direction I found this paper earlier
Separation of variables seems to be associated with point symmetries, though the symmetry condition is not useful for linear equations since the original equation recurs in the decomposition
Does anyone know the lowest energy solution (and preferably other solutions too) of the time-independent Schrödinger equation for a logarithmic potential in two dimensions?
this −(h²/2m)∇²ψ + ln(x)ψ = Eψ?
alternatively there is -∇²ψ + ln(y)ψ = Eψ or ∇²ψ + [ln(x) + ln(y)]ψ = Eψ
yeah, sorry there was some ambiguity in the question. Unfortunately standard separation of variables techniques are going to fail and you wont be able to find the eigenfunctions. Supposing there is an eigenfunction we don't know, can we predict the eigenvalues despite that? I need to go look in griffiths for a refresher.
I already have the solution for a -1/r potential in 2D (just a modified version of the 3D potential) but a real coulombic potential in 2D is ln(r), not -1/r
thats a well known problem though, the eigenfunctions in the 3d case are the associated legendre polynomials
(i think)
legendre polynomials multiplied by e^(-r)
if you found the eigenfunctions in some literature, Im not saying you're wrong, Im just saying I dont know them, and the R(r)O(θ) ansatz wont work.
right okay, the product of the two was the spherical harmonics
why not?
I mean I don't know if the logarithimic potential will have eigenfunctions based on the legendre polynomials, but the solutions should certainly still be decomposable into radial and angular components
So we talked about this a while back, but the condition for separability is the differential operator must be self-adjoint, once you know its separable, you still dont know the ansatz though.
(separation of variables does not work on every linear pde)
This paper may also be relevant to you since we are in 2 dimensions
can someone tell me if my understanding is right?
for burger's equation, a smooth solution will only stay smooth if the initial condition is monotonically increasing (so that no shock waves occur. instead it will form rarefaction waves), and discontinuous solutions will stay discontinuous unless they're monotonically increasing (where they will eventually become continuous as rarefaction waves).
Well technically speaking a discontinuous solution might become continuous and then discontinuous again if it is monotonically increasing in the neighborhood of the initial shock but decreasing somewhere else
interesting. so it should instead be that a solution that decreases anywhere will eventually stay discontinuous?
I don’t know
But if it’s decreasing anywhere I think it should become discontinuous at some point
I don’t know if that can later become continuous again
here is the symmetry condition for burgers equation
x̄ = ξ∂/∂x + τ∂/∂t + η∂/∂u + η_x(∂/∂u′) + η_t(∂/∂u̇) + η_xx(∂/∂u″)
η_x = Dη/dx - (∂u/∂x)Dξ/dx - (∂u/∂x)Dτ/dx = ∂η/∂x + ∂u/∂x(∂η/∂u) - (∂u/∂x)[ ∂ξ/∂x + ∂u/∂x(∂ξ/∂u) ] - (∂u/∂x)[ ∂ξ/∂x + ∂u/∂x(∂ξ/∂u) ]
η_t = Dη/dt - (∂u/∂t)Dξ/dt - (∂u/∂t)Dτ/dt = ∂η/∂t + ∂u/∂t(∂η/∂u) - (∂u/∂t)[ ∂ξ/∂t + ∂u/∂t(∂ξ/∂u) ] - (∂u/∂t)[ ∂ξ/∂t + ∂u/∂t(∂ξ/∂u) ]
η_xx = Dη_x/dx - (∂²u/∂x²)Dξ/dx - (∂²u/∂x²)Dτ/dx = ∂/∂x(∂η/∂x + ∂u/∂x(∂η/∂u) - (∂u/∂x)[ ∂ξ/∂x + ∂u/∂x(∂ξ/∂u) ] - (∂u/∂x)[ ∂ξ/∂x + ∂u/∂x(∂ξ/∂u) ]) + (∂u/∂x)∂/∂u(∂η/∂x + ∂u/∂x(∂η/∂u) - (∂u/∂x)[ ∂ξ/∂x + ∂u/∂x(∂ξ/∂u) ] - (∂u/∂x)[ ∂ξ/∂x + ∂u/∂x(∂ξ/∂u) ]) - (∂²u/∂x²)[ ∂ξ/∂x + ∂u/∂x(∂ξ/∂u) ] - (∂²u/∂x²)[ ∂ξ/∂x + ∂u/∂x(∂ξ/∂u) ]
x̄( ∂u/∂t + u∂u/∂x - ν∂²u/∂x²) = 0
-> (∂u/∂x)η + uη_x + η_t - νη_xx = 0
just need to substitute ∂²u/∂x² = ( ∂u/∂t + u∂u/∂x)/ν when ever it appears in the above
its linear in ξ, τ, and η, since those functions only depend on x, t, and u, you can make a decomposition on the derivatives of u into a really large system of usually trivial pdes
@mint canyon I looked at charpits method agian yesterday for the more simple case with cos(x)cos(y)(zx^2 + zy^2) + 2sxsyzxzy = 0. The equation reduces a lot because of the trig identitites and because these coefficients are related by derivatives. I feel like I should be able to get an exact integral here but I'm not seeing it
This is what I have.
I left out most previous steps because it's too long. But I feel like I'm overlooking something here.
did you try the parameter independent version?
well its easy to derive from the parametrized version
Not yet. I sort of have the parameter t in the beginning and then eliminate it through these reductions I guess. I initially thought after rearranging some of these, I could equate the symmetric equations again to integrate
What I mean is after I manipulate the first two and define new variables for u = sinx and v = siny, getting this relatinship dv/du = q/p, Id still be able to say dv/q = du/p = d(p^3)/u = d(q^3)/v, but I think thats not correct.
I mean, if its integrable, then integrate it and plug it in to the characteristic equation to see if its satisfied
look at equation 14
Okay I will look. I think I saw this paper earlier at one point. Maybe it will be a good read through
looking at the differentials I suspect a typo in that figure... my bad
I find this PDE strange because in its original form I showed you, I looked at coordinate transforms originally using characteristics to change it into a canonical form, for example eliminating the zuu or zvv coefficients in the new coordinate system. But doing so requires solving PDE
one should definitely be dq
solving these PDEs that have this quadratic form structure. and then I noticed this entire pde is actually derived from a lagrangian that has the exact same quadratic form structure.
you mean its an euler-lagrange equation?
yes
huh, I wonder if thats a general result or a coincidence
So for the equation cosxcosy(zxx + zyy) + 2sinxsinyzxy = 0, the corresponding lagrangian is L = (1/2)(cosxcosy)(zx^2 + zy^2) + sinxsinyzxzy. The class of PDES ive been studying are derived in a certain way so that the coefficients end up being derivatives of a similar functions. So in this PDE, they are second derivatives of a function cosxcosy. The general form of these equations are fyyzxx + fxxzyy - 2fxyzxy = 0, where f is a function you'd know that determines the coefficients. I think thats why it works out this way, but the derivations that leads to that equation doesnt use a lagrangian. The fact that it can also be derived from a lagrangian is just something I noticed the other day which helped a lott
The lagrangian for any of these is based off a quadratic form of the Hessian of the function f(which again we choose), and the "vector" formed by gradient of z(x,y).
Okay, you had me intrigued for the wrong reason, I thought you meant the characteristic equation was also an euler-lagrange equation. This is definitely specific to your problem
it would have been neat if there were some kind of variational description of the characteristic
Also I was thinking, when one uses characteristics to change coordinates for a second order PDE, they tend to have a standard procedure for eliminating these coefficients. So if you are doing a coordinate change from x,y to u,v, you can try to figure out what u and v have to be to say eliminate the coefficients on certain second derivatives in your new equation. So they have the standard form for parabolic, elliptic, etc. But when they go through this procedure, they usually do something like this.
So for example if the PDE we start with is Azxx + Bzxy + Czyy = 0, then the coefficient on zuu in the new equation would be Aux^2 + Buxuy + Cuy^2, and we would try to set that equation equal to zero and solve to determine u if we wanted. Usually when I see this done, they just divide through by uy or ux, demand that du = uxdx + uydy = 0, and then plug in the relationship for dy/dx and then use the quadratic formula to obtain some equations you need to integral dy/dx for to obtain the characteristics.
Okay my question is, if you get to the point of Aux^2 + Buxuy + Cuy^2 = 0, which you want to satisfy for your coordinate transform, why not just use the lagrange charpit method to figure out some expression, even if its implicit, for u. If I try the standard way of doing this problem where they end up with some step that says dy/dx = -B +- sqrtt(B^2 - 4AC)/2A, its totally impossible to do these integrals in some instances. If I use the lagrange charpit method there to solve that integral, am I gaining anything? The only thing I could think is it might implicitly give me an answer that relates u to x and y but Im not sure.
Ive seen the quadratic formula version of the second order method too, but it only works in the 2 variable case, so i just remember the generalized multivariable version
also, if you dont have constant coefficients, do you really want to deal with integration of the quadratic formula?
Yeah I agree. I'm just wondering why its so hammered into every second order linear pde approach I see. Like they never use the lagrange charpit method for solving those coordinate transform equations.
there may be some condition required for lagrange-charpit to work, but its the best method by far for fully nonlinear first order equations
Symmetry methods are a fallback and guaranteed to exist, but the condition for that can be intractable quite often
I haven't found a single example though where lagrange charpit was used on a nonlinear first order equation of my kind though, where its quadratic and has the mixed term zxzy in it. If I found more examples of that, it could help me.
What I mean is any example with azx^2 + bzy^2 + czxzy = something
I saw a paper where it was used on Hamilton-Jacobi, thats got quadratic derivatives
Though its actually really easy to solve with separation of variables despite being strongly nonlinear
Yeah I need to look more. I do see people use it for hamilton-jacobi which is pretty cool. Do you know any other good resources where I can read up on the lagrange charpit method and examples? I do have that one you sent me going over the rigor of it
I had a derivation memorized at one point, since its actually very close to Hamiltons equations of motion, except its in a 2n+1 dimensional "phase space"
(actual phase space is always 2n dimensional)
Prob time for me to go but I'll have to look up more resources on this for sure
Here's the starting point:
F(qᵢ, u, ∂u/∂qᵢ) = 0 -> F(qᵢ, u, pᵢ) = 0
qᵢ′ = dqᵢ/ds, u′ = ∑∂u/∂qᵢ(dqᵢ/ds), pᵢ′ = ∑∂pᵢ/∂qᵢ(dqᵢ/ds)
Then you choose qᵢ′ = ∂F/∂pᵢ
and substitute into the other equations
u′ = ∑∂u/∂qᵢ(∂F/∂pᵢ)
pᵢ′ = ∑ ∂pᵢ/∂qᵣ(∂F/∂pᵣ)
the pᵢ are an issue since F contains no derivatives of p, but if we look at DF/Dqᵢ expanded with the chain rule we get:
DF/Dqᵢ = ∑ ∂F/∂qᵢ + pᵢ∂F/∂u + ∑∑ ∂pᵢ/∂qᵣ(∂F/∂pᵣ) = 0
rearrange and you see that: ∑∑ ∂pᵢ/∂qᵣ(∂F/∂pᵣ) = - ∑ ∂F/∂qᵢ + pᵢ∂F/∂u
so pᵢ′ = - ∑ ∂F/∂qᵢ + pᵢ∂F/∂u
now get rid of the parameter:
dqᵢ/[ ∂F/∂pᵢ ] = du/[ ∑∂u/∂qᵢ(∂F/∂pᵢ) ] = dpᵢ/[- ∑ ∂F/∂qᵢ + pᵢ∂F/∂u ]
There are your first integrals
can we not remove the (4pi vt)^(-1/2) out of the log and neglect it since its constant wrt x?
supposed to derive that in my hw basically and i'm wondering if this step is ok or not (we used epsilon instead of nu)
it seems fine to me, but idk why they wouldn't simplify that further unless maybe something sketchy happens idk
This is the differential equation Im most interested in at the moment:
(½gᵢᵣgᵤᵥ - gᵢᵤgᵣᵥ)(δS/δgᵢᵣ)(δS/δgᵤᵥ) = 0
(½gᵢᵣgᵤᵥ - gᵢᵤgᵣᵥ)((∂S/∂gᵢᵣ - ∂/∂xₐ[∂S/∂gᵢᵣ,ₐ])(∂S/∂gᵤᵥ - ∂/∂xₐ[∂S/∂gᵤᵥ,ₐ]) = 0
(½gᵢᵣgᵤᵥ - gᵢᵤgᵣᵥ){(∂S/∂gᵢᵣ)(∂S/∂gᵤᵥ) - (∂S/∂gᵢᵣ)∂²S/(∂xₐ∂gᵤᵥ,ₐ) - ∂²S/(∂xₐ∂gᵢᵣ,ₐ)(∂S/∂gᵤᵥ) + ∂²S/(∂xₐ∂gᵢᵣ,ₐ)∂²S/(∂xₐ∂gᵤᵥ,ₐ)} = 0
27 independent variables 🧐
what's the equation for
its a single scalar equation for the Hamilton-Jacobi form of ADM
ADM is the canonical field equations for general relativity, if you want to represent it as a Cauchy problem
well, its the vacuum version, so no matter/sources
<@&268886789983436800>
did I break some kind of rule?
It's likely there was spam that was deleted
ahh I see
I have no idea whats covered in that book, but the book I used was "A First Course in Differential Equations" D Zill
also, there is another channel called odes-and-pdes for more intro questions
Suggest me a starter book for pde I tried 2,3 books but I find it hard to learn please help me I liked shepley l Ross book on ode I need book something like this
my pdes book for undergrad wasnt too amazing, but it was cheap (dover). let me get the title/author
"Fourier Series, Transforms, and Boundary Value Problems" JR Hanna, JH Rowland
There are better books, but it has the info in there and it doesn't get too bogged down in rigor/formalism
Contrary to the title it also has Bessel functions and Legendre polynomials in it
This is my syllabus
Yeah sorry, my book focuses entirely on boundary value problems, it has nothing on method of characteristics. Maybe grab a high rated math methods for physicists type book that covers all the pde stuff in the table of contents?
I need just a basic starter book
Which cover most of these topics
I am just doing for exam I hat pdes 🫣
yeah, thats why I recommended the math methods books, physicists dont care about rigor at all, it will be purely algorithmic discussions in those books
Oh! thank you so much
@mint canyon I made a little more progress on this general problem. I realized that there is another way you can formulate it even more simply that involves three linear first order pdes of 3 variables. The equivalent formulation is.
ux + fxzx = 0
vy+ fyzy = 0
uy + ux + fxzy + fyzx = 0
Where f is known. If you eliminate u and v from the equation, you get back
fyyzxx + fxxzyy - 2fxyzxy = 0
I like this simpler form better because uts first order and linear but im wondering if its too broad to draw results from. I think I should be able to get something from it, but I need to define new variables of some kind. I mean for example one clear thing is I can get new equations from adding and subtracting these, one being.
(u+v)(x+y) + f(x+y) * z_(x+y) = 0
Which looks very close to some sort of transport equation. In special cases the equations reduce nicely. What do you think? I feel like this set up is actually nicer and easier to draw results from as a starting point for a given f
you cant use method of characteristics on systems of equations unfortunately
also, I never know whether im looking at dependent or independent variables when you write your equations like that
Thats true. The general approach people use sometimes with systems of first order pdes is to solve for one of the variables. The point here is that that is exhausting and makes the problem harder. I want to keep it in this form with three independent variables and analyze it that way.
Similar to how with a state space form, its easier to draw conclusions frok that formulation instead of solving for one variable and looking at its higher order ode
My bad. u,v, and z are the dependent variables of x and y
is fx f*x or ∂f/∂x?
i dont remember coefficients of x in the original pde, so i dont think they would arise from simple coord transforms
unless its like x = arcsinx' or something
Yeah when Im writing fx or zx I mean the partials
This is a classic written by masters that is more explicit than Arnold
Though Arnold is awesome imo
Definitely gotta do some leg work to read it
Holy based
I recommended the same book to them in another channel
hirsch smale devaney!!!!!!!
Good taste lol
hi , how one can get the second inequality here $u \in W^{2,p}(B_{4} )$; $B_{4}={x\in R^{n},|x|<4 } $ , $\overline{\nabla u}=\int_{B_{4}}\frac{\nabla u}{|B_{4}|}$ and there is no assumption for n and $p>2$ , i tried to use Sobolev inequalities but i failed , any hint? okey i think that i solved that : i will apply mean value property for \nabla^{2} v since it is harmonic because v is
amani
I know this isn't really the place to ask so I apologise however I asked this a while ago in book recommendations and got no response. Does anyone know of any PDE books (preferably more applied) that cover coupled pdes or systems of pdes.
the one I read is Numerical Method for Conservation laws by LeVeque if you are interested in hyperbolic systems. do you have an idea of the applications you’re interested in?
is this substitution correct?
Ah, I am currently just doing a methods course so little to no theory at the moment. I think I found a section in some small dover book. The reason why I was interested is because I have a more theoretical course next year and thought since I have the time and I am interested, might aswell have an early look. Thanks though, I will keep that book in mind 🙂
iam not getting any reply there
this is the pde channel, we dont talk about odes here 
I need some help with this question
I introduced function h(x) and h'(x) that satisfy the needed conditions
then y + ah(x) and y' + ah'(x) are 1 parameter (a) functions at which K is stationary
But I never used the PDE anywhere in my answer
I dont think you need that EL pde to prove that right?
I think that is just a statement about the condition for stationarity.
The way I see it, I need to prove: EL pde holds => K is stationary w.r.t small variations
Ah you're right actually. I misread it
Are there any theorems on any analysis done on how the solution to a lagrangian, say L = 0, relates to the solution of its corresponding euler lagrange equation?
What I mean is L = 0 might be a pde/ode in its own right that one could solve, and the correspinding EL equation is a higher order equation thats typically harder to solve. Like when could I get away with saying the solution to L = 0 satisfies the corresponding euler lagrange equation
gonna be real, i have no idea what to do here. im reading the proof of the mean value formula in Evans (where the problem comes from) and i do not see at all how to get to this. are we supposed to use something like
u(0) = convolution of the fundamental solution with f = the average integral over a ball centered at 0
and then somehow manipulate it to get there? idk
In Evans, there should be something defined like
[\varphi(s) = \frac{1}{n\alpha(n)s^{n-1}}\int_{\partial B(0,s)}u(y)dS(y)] in the proof of the mean value formula. Look at $\int_{\epsilon}^r \varphi'(s)ds = \varphi(r)-\varphi(\epsilon)$. I think the motivation of this problem is to arrive to $u(0)$ independently from the fundamental solution
カービィ
epsilon here is set because phi(s) is clearly not defined at 0 so you need to be careful
I think the involved part here is calculation, and there should be enough information that pops out of this that you might be fine
What are the textbooks for beginning graduate students or advanced undergraduates who want to look into PDEs?
Evans' PDE
After finishing, I would be PDE master?
In front of highschool students? Sure
What comes after Evans?
Quite a lot of things, the book itself will inform you on that
If you want to learn about the important stuff that forms the backdrop for modern PDEs, I really recommend Distribution Theory and Fourier Analysis by Strichartz. Evans doesn't really get into that stuff, Evans is more traditional. Evans + Strichartz is a great foundation.
The most important parts of evans are probably chapters 2, 3, 5, 6, and 8? If you're looking for a subset to focus on
This is a Millenium Problem solution, right? https://arxiv.org/abs/2401.17147
We study the existence of strong solutions to the initial value problem for the incompressible Navier-Stokes equations in $\mathbb{R}^N, N\geq 3$. Our investigation shows that local in-time classical solutions do not develop singularity as long as the initial velocity lies in $(L^2(\mathbb{R}^N))^N\cap (L^\infty(\mathbb{R}^N))^N$.
what do you think
i think Dr. Xiangsheng Xu will be a millionaire if the proof is valid
not necessarily, the tax rate may be quite high
anyway it is very likely wrong
there are so many red flags
F
and i say this as someone with zero knowledge of navier stokes or fluids in general
so i imagine it will be retracted soon
like the single-author?
but who knows
no that is fine
but the big problem is
the claimed result is the opposite of what most of the community expects
also it is very short
i thought the community was expecting the existence of global smooth solutions 😶
for the zero viscosity limit, Euler, probably no, but i thought the extra laplacian term was expected to induce smoothness, as it does for the scalar case
idk
there is this though https://arxiv.org/abs/1402.0290
The Navier-Stokes equation on the Euclidean space $\mathbf{R}^3$ can be expressed in the form $\partial_t u = Δu + B(u,u)$, where $B$ is a certain bilinear operator on divergence-free vector fields $u$ obeying the cancellation property $\langle B(u,u), u\rangle=0$ (which is equivalent to the energy identity for the Navier-Stokes equation). In th...
so i know that generally solution operator for linear dispersive PDEs doesn't have bounded L^1 operator norm, but are there cases where S(t)u_0 is not even in L^1 for u_0 in L^1?
yeah so in class we sorta did that defining it as the average integral which is exactly that. but we showed that its derivative is actually zero for a harmonic function. so wont phi(r)-phi(ep)=0 for all epsilon>0?
You should be able to get this via the solution operator for the linear Schrodinger. Your S_t looks like e^i|x|^2 with something and then taking L1 norm of S_tu_0 an infinite upper bound via Young's inequality.
your question was not about a harmonic function?
oh my god you're right asudhsdsa
Hi guys, I’m extremely sorry if I’m asking dumb question but let me ask.
How to start understanding characteristic curves of first order linear PDE? Like any good recommendations like articles/blogs/links?
Check this out
Oh okay thanks
unstable-like
@tired hollow The implicit form of a solution surface is u - u(x,y) = 0, from vector calc we know the normal vector field to that surface is the gradient (∂u/∂u)k - (∂u/∂x)i - (∂u/∂y)j = 0. The vector field Ai + Bj + Ck is a tangent vector on the surface if its dot product with the gradient is C(∂u/∂u) - A(∂u/∂x) - B(∂u/∂y) = 0. A tangent vector field on the surface will have integral curves on the surface specified by the parametric equations du/dt = C, dx/dt = A, dy/dt = B.
Uh oh, let me read this and understand what you’re saying
tangent vectors and normal vectors would always be orthogonal right?
Yes, true
quasilinear first order pdes ARE the condition for orthogonality then
Uh so implicit function I understand
an integral curve is just the name of the associated parametric curve to some tangent vectors of that curve.
Okay I understood why u said implicit function = 0 can be represented as surface
But I didn’t get why u said the expression u mentioned is normal of surface?
you should have learned that in vector calc
At least I know partial derivative, directional derivative and freshet derivative. But I’m surprised about your expression on normal of a surface, I’ll check it out in vector calculus, no issues.
In geometry, a normal is an object (e.g. a line, ray, or vector) that is perpendicular to a given object. For example, the normal line to a plane curve at a given point is the line perpendicular to the tangent line to the curve at the point.
A normal vector of length one is called a unit normal vector. A curvature vector is a normal vector whose...
well in principle yes this is what would motivate the existence of such a solution but I'm not sure that it actually exists
we could for example just have that the L^1 norm of some solution grows very fast
Has anyone here read about Order Completion methods?
would a first course in fourier series and such go in here or better suited for the other chat?
odes and pdes in early university
If it's at the undergraduat elevel, most likely the odes & pdes channel
Or the advanced analysis channel if you're brave/if it's appropriate
i need to compute the wave breaking time for a general convex flux function $f(x)$
$$u_t+\paren{f(u)}_x=0,\quad u(x,0)=u_0(x)$$
eigentaylor
but i'm having a hard time understanding the process
my understanding is to look at the characteristics, but i never really learned how to find them lol
would a general characteristic curve be something like
$$x=x_0+f'(u_0(x_0))t$$
eigentaylor
if so then i think i get
$$t=-\frac{1}{f''(u_0(x_0))u_0'(x_0)}$$
and then i pick the minimum of that. which i think is consistent with the result for burger's equation but it seems a bit... sus lol
eigentaylor
the pure mathematician in me wants to be like "what about when its not defined or if f' isn't continuous etc."
but this is for a numerical PDEs class so maybe i should just be like "yep definitely works no problems to consider here"
and IF i'm on the right track, should it be
$$T_b=\min\paren{-\frac{1}{f''(u_0(x_0))u_0'(x_0)}}$$
or $$T_b=-\frac{1}{\min\paren{f''(u_0(x_0))u_0'(x_0)}}$$
eigentaylor
Uh, latex typing here is interesting though. Some features are not working…
hi i have some questions about Vlasov-poisson equation , can someone help me?
Not sure, u can post the qn here I guess
Yeah it makes sense, generally we assume that the solution exists $u(x,t)$ and upon solving ODE $dx/dt = f’(u)$, we expect that the characteristic curves $x(t)$ exists. So the existence of characteristic curve depends on f(u) function. And doing the whole process, I guess u correctly stated the characteristics equation (straight line). But the function f(u) dictates the slope, so it can cause rarefaction regions / shocks all that I guess.
Grand Duke
@eigentaylor that family contains equations fully nonlinear in ∂ₓu, you can only use method of characteristics on quasilinear equations. My understanding is Lagrange-Charpit (which would work in that case) is also a characteristic method, but I cant say if the characteristics you get from it have all the same properties as the quasilinear case.
You can also try appealing to the closed graph theorem.
Hi i'm currently working through M. Taylor P.D.E II, specifically on Pseudodifferential Operators. I'm trying to understand the lemma
My current try looks the following:
However im having a hard time understanding the requirement that $\delta<1$. Couldnt i just bound the $<\xi>^{m+\delta |\alpha|}$ term by some polynomial term of higher order?
hrbibbi
I think the 1 isn't important; just that you need some specific bound on delta so that you have a fixed seminorm to bound (20). But I might be wrong
but then the lemma itself doesn't really make sense to me, since $p(x,\xi)\in S_{\rho,\delta}^m$, and thus delta is already bounded
hrbibbi
The derivation is a bit hard to follow because it's seems bit inaccurate after line 17 -- for example, from (18) to (19) he seems to be trying to use the symbol bounds $p \in S^m_{\rho, \delta}$ without bringing the absolute values inside the (oscillating) integral. I would focus on (17).
Casey
$D\alpha_x (x^\beta pv)$ is a family of Schwartz functions in $x$, parametrized by $\xi$. So you want to see how the Schwartz seminorms depend on $\xi$.
Casey
How do you normally show that the Fourier transform of a Schwartz function is Schwartz? If $f(x)$ is Schwartz, then $\xi^\alpha \hat{f} = (-1)^\alpha \int[ (i \partial_x)^\alpha f (x)\ e^{-ix \xi} , dx$ which you can bound using a Schwartz seminorm of $f$ by a constant times $|f |_{\alpha, n+1}$ where $n$ is the dimension.
Casey
Now suppose $f$ actually depends on a parameter $\xi$. If $|f(\cdot, \xi)|\alpha \langle \xi \rangle^{\delta |\alpha|}$ and $\delta < 1$, then you can move the powers of $\xi$ on the right side to the left to obtain $ |\xi|^{(1-\delta) |\alpha|} |\hat{f}| \le M{\alpha}$ for all $\alpha$.
Casey
Now suppose $f$ actually depends on a parameter $\xi$. If \|f(\cdot, \xi)\|_\alpha \langle \xi \rangle^{\delta |\alpha|}$ and $\delta < 1$, then you can move the powers of $\xi$ on the right side to the left to obtain $ |\xi|^{(1-\delta) |\alpha|} |\hat{f}| \le M_{\alpha}$ for all $\alpha$.
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Sorry for the LateX errors I'm new to discord -- but hopefully you get the idea
thank you very much for the help. I was kind of suspecting that i had made some kind of error in my derivations, ill try to look from (17)
Just consider the estimate when $\beta=0 $.
You have $$|\xi^\alpha p_v(\xi)|\leq \int |D_x^\alpha (pv)|, dx .$$
This produces terms of the form
$$\int |D_x^{\gamma}p(x,\xi)||D_x^{\alpha-\gamma}v(x)| , dx $$
The symbolic estimates give the bound
$$|D_x^{\gamma}p(x,\xi)|\leq C_\gamma \langle \xi\rangle ^{m+\delta |\gamma|} $$
and the second factor is simply Schwartz, so certainly this integral in $x$ is finite, with the estimate
$$ |\xi^\alpha p_v(\xi)| \leq C_\gamma \langle \xi\rangle ^{m+\delta |\alpha|}$$
where I have redefined my constant.
We have this for every $\alpha$ so this implies
$$|p_v(\xi)|\leq C_\gamma \langle \xi\rangle ^{m+(\delta-1) |\alpha|}$$
To get that this is finite (no matter what $m$ is), we simply take this last estimate with $|\alpha|$ sufficiently large. This does not work if $\delta=1$.
grobmez
It is. ^
(replace "finite" with "bounded by <\xi>^(-N) for arbitrary N" in the last para.)
okay and in the case where $\beta\neq 0$ we just get the term
$$\int |D_x^{\gamma}p(x,\xi)||D_x^{\alpha-\gamma}(x^\beta v(x))| , dx $$
where the second term again is Schwartz and the argument holds again
hrbibbi
yep
great thank you
no problem
Guys, can anyone can pls throw some light on Monge cones?
My prof brought that up in PDE class, any helpful video/article or even an explanation would be very helpful!!
I guess I’m getting some understanding from this notes:
https://www.math.iitb.ac.in/~siva/ma515152022/3MA515Notes.pdf
We fix a point (x0, y0, z0) in R3 of a possible integral surface (integral surface = solution surface for nonlinear pde: f(x,y,u(x,y),ux,uy)=0)
(Don’t ask me how is that unknown z0 is fixed, I’m assuming that we assume it exists and fix it somewhere and let the other variables play 🤣) then we have
f(x0,y0,z0,ux,uy) = 0
My confusion is that we assume some solution z0 exists, can’t we assume that in same way it’s partial derivatives also exists? Like p0 & q0. Why do we have to assume that z0 is fixed and there we look at all possible tangent planes satisfying the eqn f(x0,y0,z0, ux,uy)=0?
(Maybe I’m not convinced that the solution to f exists in R5 plane not R3
)
I am trying to understand the following proof, which is necessary for e.g. proving weak derivatives are unique:
https://math.stackexchange.com/questions/3212146/two-proofs-of-the-fundamental-theorem-of-calculus-of-variations-one-correct-o
I understand every step, save for the statement that $u(x) \omega_\epsilon (x) $ converges to $u(x) w(x) $ as $\epsilon \to 0$, for almost every $x$. From Lebesgue's differentiation theorem it follows that the mollified $\omega_\epsilon$ converges to $\omega$ almost everywhere. But how is this passed on to the product $u \omega_\epsilon$? I understand it should suffice to look at $x$ that live in the support of $\omega_\epsilon$, but how do we control the value of $u(x)$? If $u(x)$ were bounded, we could simply just consider
[
| u(x) \omega_\epsilon(x) - u(x) \omega(x)| = |u(x)| |\omega_\epsilon(x) - \omega (x)|
]
$|u(x)|$ we could then bound, and the difference $|\omega_\epsilon(x) - \omega (x)|$ can be sent to zero due to almost everywhere convergence of $\omega_\epsilon \to \omega$.
hardisc
It seems like they prove for you that |uw(x)| ≤ |u(x)| so u is a majorant and hence DCT is applicable
yes the aim is eventually to deploy DCT. but the hypothesis remaining for DCT is pointwise convergence a.e., namely, $u \omega_\epsilon \to u \omega $ as $\epsilon \to 0$, so that we can pass to this limit in the integral $ \int u \omega_\epsilon $. And that pointwise convergence I do not see how to confirm
hardisc
Ah you don't understand how to get pointwise convergence?
If you get that we(x) converges to w(x) pointwisely, then for each fixed x, we(x) is just simply a sequence indexed by e converging to w(x). Now for a fixed x, u(x) is just some number so just recall the effect multiplication by a number have on a converging sequence
ah crap, was it really that simple?
we have that $N = { x : \omega_\epsilon(x) \not \to \omega(x) }$ has measure zero.
fix an arbitrary $x \not \in N$. then $u(x)$ is just some finite number. Then
[
|u(x)| | \omega_\epsilon (x) - \omega (x)| \leq |u(x)| \cdot \epsilon \to 0, \text{ as } \epsilon \to 0
]
Thus $u \omega_\epsilon \to u \omega$ fails only on a set of measure zero, so the convergence is almost everywhere.
like that? last question remaining is then what if $u(x)$ is not finite at a certain $x$? e.g. if $u(x) = + \infty$?
hardisc
You only care about almost sure convergence, so remove the zero-measure set of u = infinte (prove for integrable u, such sets have zero measure)
oh right. if the set of u = infinite had positive measure then we could integrate |u| over that set, getting an infinitely large integral, and that would contradict the integral of u over the entire space being finite. thus that set must have zero measure
huge thanks to you @lilac barn cocat, appreciate it so much
Yw!
I was recently attempting a problem from Evans' PDE text and I solved it, but I'm not sure my answer is correct since it looks a bit fishy. I was hoping someone could verify it and correct me if I'm wrong.
The problem goes as follows:
Let U = ${|x_1| < 1,|x_2| < 1}$ denote the open unit square in $R^2$ centered at the origin. Define the function $u:U \mapsto R$ as follows:
$$ u(x_1,x_2) = \begin{cases}
1-x_1 \text{ if} & |x_1| \leq |x_2|, x_1\geq 0, \
1+x_1 \text{ if} & |x_1| \leq |x_2|, x_1\leq 0, \
1-x_2 \text{ if} & |x_2| \leq |x_1|, x_2\geq 0, \
1+x_2 \text{ if} & |x_2| \leq |x_1|, x_2\leq 0 \
\end{cases}
$$
For which $1 \leq p \leq \infty$ does u lie in $W^{1,p}(U)?$
<br/><br/>
Solution:
My answer is that u lies in the Sobolev space for all $1\leq p\leq\infty.$
<br/>
Sketch of the argument:
First note that u is bounded on a set of finite measure so it lies in $L^{p}(U)$ for each $1 \leq p \leq \infty.$
Now it suffices to show that the weak first partials $u_{x_1}$ and $u_{x_2}$ also lie in $L^{p}(U)$ for each $1 \leq p \leq \infty.$ In particular first we show that these weak derivatives are actually functions and then we show that they are bounded.
To this extent we let $\phi$ be a test function on $U$ and consider the quantity:
$$\int_U{u \phi_{x_i}}$$
In order to simplify this quantity we divide the open unit square into 4 open regions $R_1,R_2,R_3, \text{ and } R_4$.
$$R_1 = {|x_1| < |x_2|, x_1 > 0}$$
$$R_2 = {|x_1| < |x_2|, x_1 < 0}$$
$$R_3 = {|x_1| > |x_2|, x_2 > 0}$$
$$R_4 = {|x_1| > |x_2|, x_2 < 0}$$
we orient each of these counter-clockwise and use Greens Theorem to simplify our integral as follows:
$$\int_{R_j} u \phi_{x_i} = \int_{\partial R_j} u \phi \nu_{i} dS - \int_{R_j} u_{x_i} \phi$$
Here {nu} denotes the outward pointing normal.
taco
We note that $\phi$ vanishes on the outer boundary of the unit square being smooth and compactly supported in u (it's a test function).
If we picture each of the regions to be triangles then u agrees on the shared boundary of any two regions (the boundaries are precisely $x_1 = x_2$ and $x_1 = -x_2$).
However note that for two regions sharing a boundary their corresponding normals point in precisely opposite directions (due to being oriented in opposite directions).
So we have that:
$$\sum_{j=1}^4 \int_{\partial R_j} u \phi \nu_{i} dS = 0$$
We are left with the expression:
$$ \int_U{u \phi_{x_i}} = \sum_{j=1}^4 (\int_{\partial R_j} u \phi \nu_{i} dS - \int_{R_j} u_{x_i} \phi) = - \sum_{j=1}^4 \int_{R_j} u_{x_i} \phi) $$
However, we see that u is differentiable on each of the $R_j$'s and we may plug in $u_{x_i}$ for each of the regions for $i=1,2$ to find the weak partial derivatives of u i.e.,
$$u_{x_1} = 1_{R_1} - 1_{R_2}$$
$$u_{x_2} = 1_{R_3} - 1_{R_4}$$
However, both these (weak) partial derivates are bounded on sets of finite measure. So we see that they are in $L^{p}(U)$ for each $1 \leq p \leq \infty.$
We can finally conclude that u lies in $W^{1,p}(U)$ for each $1 \leq p \leq \infty. : \square$
To reiterate, please let me know if this is correct or not, if not please let me know what the error is.
taco
I've made a corresponding stack exchange post if this is not readable: https://math.stackexchange.com/q/4861856/1289223
I'm in a numerical PDEs class and we have a section on numerical method for solving the advection equation $$\partial_tu = -a\partial_xu$$. I'm a little confused on why we'd need special methods to solve this, becaue if the initial data is given by $u_0(x)$ then the exact solution is just $u_0(x-at)$.
Lakshay
One way to think about it (but actual numerical/PDE analysts would answer better than me), it is because in interesting cases a=a(u) depends on the solution u itself, so that you need first to have sufficient knowledge on what happens in case were the coefficients are "frozen", to see what actually behaves well and to guess what could behave worse when trying to reach a nonlinear theory.
I'm going to post this here as well because I didn't see an ODE channel. Anyway, I'm wondering how to handle an equation of the form f(x)y" + y = 0, where f(x) is a periodic function that crosses zero. For example I'm looking at equations of the form y" + cos(x)/(1+sinx) y = 0. I can't get any solver to continue outside of the interval (0,2pi). Some of the solutions look nice inside of it, but outside of that, it basically brakes. I haven't seen a singularity like this covered in perturbation theory literature.
Removed the studying! role from you.
I'd like to solve a non-linear, coupled Klein-Gordon equation. Can someone lay out the techniques/approaches I need to study to achieve that?
I've found https://eqworld.ipmnet.ru/en/solutions/npde/npde2107.pdf In my particular case the non-linear function is a polynomial and I wonder if I can apply boundary conditions such that the function vanishes at infinity. Actually, I'd rather work with 3-dim space, too. And technically I have a system of 2 coupled equation, but I'm willing to simplify.
Any advice what I could read to do this task as I don't fully understand how to approach it?
For the pdf link I also wonder: Is the implicit traveling wave solution useful to do this task? And for the functional separable solution: why is xi quadratic in the variables x,t now? And why is the ODE for w(xi) of a different form and includes xi now?
@neon urchin have you tried a transformation group method to find a similarity variable?
I'm afraid I have only a very basic understand of PDEs and I'd need a book to learn that. Anything suitable for someone at physics undergrad level? Ideally to make me able to find a solution to a non-linear wave equation in a small timeframe.
If I assume my equation is w_tt = w_xx + w_yy + w_zz + b w^3, what would your suggestion mean? Is it related to point (3) in https://eqworld.ipmnet.ru/en/solutions/npde/npde2101.pdf ? I'm not sure what the F() means. Is it standard knowledge, free to chose, hard to express or does he just not write it out?
Is there a simple recipe to extend solutions from just w_xx as in the PDF to w_xx+w_yy+w_zz?
I read that paper and it doesnt really show any sort of method to solve the equation, it just kind of shows a solution
I'd be satisfied if I get a solution for something like a traveling wave 🙂 Should there be a single answer? Or are multiple forms possible?
There are many different methods for nonlinear pdes, the one Im most familiar with is transformation group methods (by Lie)
Lie sounds good. I always wondered how they are related. what's a modern introduction to learn that?
"symmetry methods for differential equations: a beginners guide" -P Hydon
do you want a brief overview?
If there is a way for have a short overview, I'd be very interested. It helps mapping out where the journey is going.
In particular I'm interested if it can help me find some kind of discrete spectrum for solutions which vanish at infinity in some way (like boundary conditions).
My main equation is just the wave equation with the d'Alembert operator. It can be a coupled system of equations and non-linear though
I've found papers about similar equation, but I don't understand what is going on there. Is it hard to write down a solution? Are there open questions?
So a Lie group can be thought of as a set of closed parametric curves called orbits
imagine these curves map points on a solution to a DE to points on other solutions uniquely
Then we say the differential equation is a differential invariant of the Lie group
that is, the group maps solutions to other solutions by way of some continuous parameter
The tangent vectors of the orbits are called "infinitesimal generators of the group"
is there a way that boundary conditions are included and then my solutions split into unconnected parts?
Im getting to that
ok, I'm reading 🙂
The condition for a differential invariant is that the infinitesimal generator acting on some expression is 0
(a vector is also an operator)
If there are derivatives in the expression, the infinitesimal generator must be "prolonged" (extended to a higher dimensional space, the space of derivatives)
You act on the differential equation and boundary conditions with the infinitesimal generator to figure out what the components of the vector field should be.
This condition is always linear
The similarity variable is then the solution to the invariant surface condition (which uses the infinitesimal generator). If you make a coordinate transform using the similarity variable, the number of independent variables is reduced by 1.
So a PDE with N independent variables and M order can be reduced to an algebraic equation by N+M symmetries (N similarity reductions and M order reductions)
sounds like an attractive method. for now I can only memorize and write down what you wrote and keep coming back to it while reading the book.
The infinitesimal generator (not prolonged) looks like this: χ = ξ(x,t,w)(∂/∂x) + τ(x,t,w)(∂/∂t) + η(x,t,w)(∂/∂w)
note a partial derivative here is the same as a coordinate basis vector
thanks! I'll try to imagine what this means and read the book. Hope it enables me to find some kind of discrete spectrum of solutions with boundary conditions
for your case the Lie group exists in the space of point transformations in x, t, and w, and maps every solution (point by point) to every other solution
could I have some conserved quantities which would take discrete values under some conditions?
X(x,t,w;ε), T(x,t,w;ε), W(x,t,w;ε) would be the orbits
like some integral over the whole space which for some conditions takes only discrete values
if you go to the space of contact transformations, you have Noethers Theorem....
I think I will get something conserved. I mainly wonder where to find the discreteness
for some boundary conditions
contact transformations are the generalization of canonical transformations in Hamiltonian mechanics
I'll get the book to understand these terms. Any additional book recommendation for beginners just in case it doesn't match my style?
they are transformations in the space of points and first derivatives of the dependent variables
yeah, I didnt want to burden you too much with contact transformations, but that is where conservation laws arise
I think I know what my conservation law will be. is there are chance that this conserved quantity takes discrete values if I impose additional constraints on my solution?
when I think of something as discrete or continuous, I usually think of a set. what set are you referring to here? the set of conserved quantities?
like {energy, momnetum, angular momentum} ?
some kind of real number which will take discrete values. for example the function value at zero. or the integral over the function over the whole space. or the conserved quantity. something that will need to be from a set of real numbers [E1,E2,...]. yes, like energy. like discrete energy levels
all this only if I impose some boundary conditions
or other kind of conditions on the solution
ahhh so you meant the set of possible eigenvalues for some observable
not sure if I can already relate this to observables. but naively speaking a real number in the solution which will be like discrete energy levels
like sine-waves in a box which can have only some wave lengths
the observable there corresponds to the Hamiltonian operator
(time-independent anyway)
maybe I need to get started with the book to understand better what I need
sorry, I shouldnt have used observable and operator interchangably. You're right that they are distinct
Klein-Gordan is for the relativistic quantum mechanics of a scalar field right?
yeah, they have a nonlinear schrodinger equation too
right, I saw papers about it. I need specifically $\Box w=f(w)$.
Gerenuk
well, if transformation groups end up being too big an undertaking, there is also generalized separation of variables, and method of constraints if your conservation law is valid. good luck
is that also mentioned in the book you suggested, or do you have another recommendation for this?
I have yet to find great resources on them, and Im still learning them unfortunately. They are narrower in scope, but just wanted to provide other options
ok, I'll take a note of these options
Im trying to understand proposition 2.1 from M. Taylor P.D.E II as shown in picture. However it is the first time I have encountered the notion of a distribution being $C^\infty$ does anyone have a resource or an explanation on what this means?
hrbibbi
Recall that function induce a natural distribution. The claim here is that there exists a smooth function which induces a distribution that equals this distribution
Ah okay makes sense. I must have overcomplicated it for myself…
When proving uniqueness of minimizers, one technique is to exploit strict convexity of the integrand of a functional. E.g. $F(u) = \int |u|^p$.
I have tried understanding how to prove $\mathbb{R}^n \ni x \mapsto |x|^p$ is strictly convex for $p > 1$. One can show $ |(1-t) x + t y|^p \leq (1-t) |x|^p + t |y|^p $ for arbitrary $x,y \in \mathbb{R}^n$ and $t \in (0,1)$ e.g. via Hölder inequality. Here is an argument for the one-dimensional case: https://math.stackexchange.com/a/2200275. This is convexity, and for strict convexity further analysis is required.
For strict convexity one has to check that equality forces the vectors $x$ and $y$ to be equal. The one-dimensional case is treated in the link above, and there one reaches $|x| = |y|$, where one can account for the signs of $x$ and $y$ being equal, it follows $x = y$.
The same argument leads one to $|x| = |y|$ in higher dimensions. But how would we obtain $x = y$ in higher dimensions from $|x| = |y|$? This is the gap I have not been able to bridge.
hardisc
I see, thank you!
i think sign is not the right way to think about the 1d case
in R^d, if x and y were not equal
then the convex combination would lie in the interior of the ball of radius |x|=|y|
the same argument works in 1d, but the boundary of the ball is two points so it is misleading
thanks for the response, I managed to solve it. we wind up having equality in the triangle inequality, which forces x = C*y for some non-negative constant C, and in tandem with |x| = |y|, we obtain x = y (assuming implicitly x and y are both non-zero).
I’m trying to derive the pde of the heat equation but cant find a resource that describes it step by step. Anyone who knows one or can help?
Boyce & Di Prima's book does this
Is there a soft copy?
Do you want the physical derivation?
Like, as in the physics behind it?
The physics and calculus behind it
Yeah
Conduction is the process by which heat is transferred from the hotter end to the colder end of an object. The ability of the object to conduct heat is known as its thermal conductivity, and is denoted k.
Heat spontaneously flows along a temperature gradient (i.e. from a hotter body to a colder body). For example, heat is conducted from the hotp...
Just scroll down to Fourier's Law midway down.
A typical example is when $K$ represents the identity map -- $K(x,y) = \delta(x-y)$ is smooth (identically 0) away from the diagonal $x=y$.
Casey
can anyone provide some insight as to where this comes from?
If you extremize that functional, with Euler Lagrange, you obtain the Poisson equation
The obstacle problem is a classic motivating example in the mathematical study of variational inequalities and free boundary problems. The problem is to find the equilibrium position of an elastic membrane whose boundary is held fixed, and which is constrained to lie above a given obstacle. It is deeply related to the study of minimal surfaces a...
Multiply the equation by w and integration by parts. You will get this functional. The admissible set is taken to account for the boundary
"what is the intuition behind this"
lobby scammer
this is from fritz john p. 65, but is there an actual name for this $$f \in C_{M,r}(y)$$ definition?
wciscnet
I am studying the p-laplace and in such contexts the following identity and the next two inequalities it implies are ubiquitous (see attached picture). I managed to verify the first identity. The middlemost inequality number one I also managed to obtain. But I have not at all been able to read off inequality number two. Judging from the author's presentation, it should perhaps be obvious, but I cannot see it.
The middlemost inequality number 1, I have shown as follows:
Suppose $|a| \leq |b|$ without loss of generality. Then $|a|^{p-2} \leq |b|^{p-2}$ and $|a|^2 \leq |b|^2$, so by the second term in the identity, inequality number one follows readily.
For inequality number two, my attempt only reached this far:
Supposing now strictly $|a| < |b|$ (we will soon divide by $|b-a|>0$), we then have $|a|^{p-2} < |b|^{p-2}$, and so
\begin{align*}
2^{-1} \left( |b|^{p-2} + |a|^{p-2} \right) |b-a|^2 > 2^{-1} \cdot \left(2 |a|^{p-2} \right) |b-a|^2 = \|a|^{p-2} |b-a|^{2-p} |b-a|^p = \left( \frac {|a|}{|b-a|} \right)^{p-2} |b-a|^p
\end{align*}
Unfortunately I do not see how to control $\frac {|a|}{|b-a|}$. If it is larger than $\frac 12$ then we are done, but I am not sure that holds for arbitrary $a$ and $b$ such that $|a| < |b|$. Perhaps my downward estimations have not been sufficiently sharp?
hardisc.
hm, interesting, how exactly? do we not need p -2 > 1 for convexity? e.g. $x \mapsto |x|^{\frac 12}$ is not convex I believe
hardisc.
There should be a (\mathbf{2^{-1}} 2^{2 - p} \lvert b - a \rvert^p) at the end in which case, the argument follows from ( p \geq 0 : )
[ \lvert a -b \rvert^p \leq \lvert 2 \max_{}, { \lvert a \rvert , \lvert b \rvert} \rvert^p = 2^p \max_{}, { \lvert a \rvert^p , \lvert b \rvert^p} \leq 2^p ( \lvert a \rvert^p + \lvert b \rvert^p).
]
To see a counterexample, set ( b = 3a) and (p = 2). It should give you a contradiction.
cocat
ah so it simply boiled down to $ |a + b| \leq 2 \max{ |a| , |b| }$, neat! big thanks.
however, I tried your example in the original inequalities number one and two (in my picture),
did not seem to produce a contradiction. or perhaps I have misunderstood?
just $p=2$ alone yields
[
2^{-1} (1 + 1) |b-a|^2 \geq 2^0 |b-a|^2
]
which certainly holds irrespective of $a$ and $b$.
hardisc.
Right, my bad. Try a = 0 and b =1, 0<p<2; this should give a contradiction
What happened in the statement of Marcinkiewicz interpolation theorem if I replace the condition of simple function class by schwartz class function? Then still the marcinkewicz interpolation is true?
I want to know this because while reading duoandixeta's book they have shown hilbert transform is weak (1,1) and strong(2,2) for schwartz class function. From there how they can concluded by interpolation it is strong (p,p) ?
@lilac barn can you help me in this case.
oh right, your hint a=0 helped with finding a counterexample. thank you so much
Interpolation does not depend on the choice of subspace as long as it is a dense one.
Don't ask the same question in multiple channels, you've been repeatedly told this in the past. I'm not really sure what you mean by simple function class here
And contained in both endpoint spaces.
I don't remember such things. Sorry I somehow did not access the group adv pde after posting. And in future if it happens again I don't care about reposting.
No marcinkewicz interpolation proof I have seen using only simple functions.
That shouldn't matter though, density should get you the same result
See this statement from the book of grafakos.
I don't see how this statement is valid for any dense class? Can you please provide me the general statement, I did not find it in any book at all. @astral vine @unborn quiver please.
Actually this is the main reason if the marcinkewicz statement is true for any dense class then, why did showing it for schwartz class , javier again proved it strong (p,p) nature for any L_p function from scratch? I did not get that. That's why I am caring about the general statement.
The statement I know is a subspace that's closed under truncation. I.e.
[f_t(x) = \begin{cases}
f(x) &|f|\le t\ 0 &|f|>t\end{cases}]
and $E$ (subset of measurable functions) is closed under truncation if $f\in E$ implies that $f_t\in E$ for all $t\in[0,\infty)$
MSC2020 49Qxx
What is it?
How is it connected to the interpolation theorem at all?
You asked about what you can do instead of simple functions
He proves the relevant Marcinkiewicz interpolation theorem at the start of the book
But that is not for schwartz class.
He proves for Lp iirc
How can he use marcinkewicz in the second page? In the first page they wrote marcinkewicz interpolation theorem?
Please see this. @lilac barn
What's your question here? Wdym by how can he use
Schwartz class functions are Lp for every p in [1,infty]
In the proof of statement of theorem 3.2 he showed (2,2) and weak (1,1) for schwartz class after that how he concluded it for scwartz class for p€(1,2) by interpolation ?
Just tell me this thing rigorously.
That I understood.
You consider an operator that is defined on L1+L2 mapping to the space of measurable functions.
Further impose that the restrictions to L1 (aka L1+0) is (1,1) and restriction to L2 (0+L2) is (2,2) bounded. Then Lp subset L1+L2 gets mapped to Lp
The problem is why it should be weak (1,1) for any L^1 function? I am asking this since where he proved it until that portion he only defined hilbert transformation for schwartz class function.
For L^2 it is fine by extension as a operator.
So your (1,1) does not make sense for L^1 function except the schwartz class. Please read it precisely.
It doesn't but then you use density
Then tell me how you can use density to this equation,
$\lvert Hf(x)>\lambda\rvert<= c|f|_1/\lambda$. How can you use density to prove this equation hold for $L^1$ function.
Vishnu das
From wealk boundedness you could not extend the definition from schwartz class to $L^1$ function.
Vishnu das
The biggest problem is you still do not know how hilbert transform is defined for $L^1$ function?
From wealk boundedness you could not extend the definition from schwartz class to $L^1$ function.
Vishnu das
You pick a Schwarz limit of a L1 function. The sequence is L1 Cauchy so their Hilbert transforms are Cauchy in measure, via the L1 weak bound. This implies there's an a.e limit. You define that to be the Hilbert transform of L1 function
Now prove that this transform is well-defined and the L1 limit still satisfies the (1,1) bound (it's simply triangle inequality)
this isn't 'advanced' relatively, but this was the closest channel i could find that mentioned pdes
i am trying to analytically derive a solution for poisson equation based on very simple ICs and BCs and 2nd and 3rd BCs
and then model it with FDA and FEA
and compare answers
is this the room for that stuff?
thank you
I think the closest thing would be the numerical analysis channel: https://discord.com/channels/268882317391429632/576514592725794816.
thank you for your response. for the analytical derivation would this still be the best channel for that? Just not the FDA and FEA stuff?
I think so, yes.
thanks
Not sure this is "advanced" PDEs for this #advanced-pdes chatroom but I'm trying to get intuition on the Poisson equation (ideally non physical) I made a question and just added a bounty
do you know any probability
not really
hmm
I mean a bit but probably not much more than a basic undergrad course
do you know what brownian motion is
yes
ok
consider for simplicity dim = 1
and consider a solution u to poisson eqn u'' = f on (0,1) with u(0)=u(1)=0
For good motivation in PDE perspective, you can look into Evan’s or Folland’s PDE book. For a statistical interpretation, Complex Made simple by David Ullrich provides a very nice motivation that isn’t very probability-theoretic, but suited for those without any stochastic background.
actually lets take a step back
first we can try to understand the green function
of the laplacian
-1/2|x-x0| I believe since dim is 1
let's define a "brownian bridge" to be a brownian motion B(t) started at B(0)=0, and conditioned to satisfy B(1)=0
(this is not obviously well-defined but just imagine a brownian motion joining the points (0,0) and (1,0))
I understand what this means but not sure why this is true
also if you view this identity as the definition of B, you can extend this to any dimension by just using the corresponding green function. in dim=2 the analogue of B looks like this (called a gaussian free field)
its just a computation
there is some reason why it should be true though
there are some other facts about harmonic functions
relating to brownian motion
like you can rephrase the mean value property as u(x) = E[u(B_T) | B_0=x] where B_T is brownian motion stopped when it first hits the boundary of the domain
not a particularly easy computation if you do not know how to define brownian bridge, though
iirc E[B(s)B(t)] = min(s,t)(1-max(s,t))
something like that
memorylessfunctor
so with that formula you can just compute
maybe the wrong place, but does anyone know much about 'solving' PDEs using neural networks? Has it seen much success recently?
neural networks are fundamentally approximations, whatever you get as a result will likely be equivalent to a numerical method, though I guess you could maybe train a really sophisticated neural network a known analytic method?
yo any idea for b)?
Try writing the usual characteristics
And what information can you deduce for the solution u(x(s),y(s))=z(s)?
that z(s) is a constant
Good so u(s) = z(s) = z_0. Now what do you know about z_0 and can you then write the resulting form in terms of x and y?
z=g(x0)=g(sqrt(x^2+y^2))?
What's g here?
sqrt(x^2+y^2)?
How's g defined? What's g(x)?
g(x)=u(x,0)
And what's u(x,0)?
Indeed so g(z) = z. Now plug this here
so sqrt(x^2+y^2)
Now verify if it does indeed solve the equation with the right initial condition
thats where i am a little fuzzy
