#advanced-pdes
1 messages · Page 6 of 1
Well check if it satisfies the PDE by calculating it's first partials and plugging them in, and then check if u(x,0)=x
it does not
It should satisfy the PDE, the question would be about the initial condition. Justifying the latter why should be sufficient then.
What about the initial condition? Is that satisfied?
i think they are
What should be u(-1,0) according to initial condition and according to your solution?
They're not
what result fo you get from initial condition?
The point is that since the curve (x,y)(s) can select the initial condition from either the positive side or the negative side, they either have to be both equal for a solution to exist (for example requiring u(x,0)=|x| or -|x|) or the solution wouldn't exist.
More precisely, as z(s) is constant in s
x₀ = u(x₀ , 0) = z(0) = z(π) = u(x(π), y(π)) = u(x₀ cos π , x₀ sin π) = u(−x₀, 0) = −x₀ which is a contradiction
I don't understand this. This is from Galtier's MHD book. b(y) = (bx(y), b0, 0) where bx is a function of y and b0 is a constant. The region is between 2 infinite plates parallel to the (x, z)-plane. "Insulating plates" imposes the boundary condition curl(b) = 0 on the top and bottom plates. Galtier is claiming this implies there's a potential that depends only on y. I'm not sure A. how you can get a potential from just having 0 curl on the boundary and B. why the potential couldnt vary linearly in x.
I suspect it's an error, because curl(b) = 0 immediately implies dbx/dy = 0 on the top and bottom plates (rather than bx = 0)
and getting both dirichlet and neumann conditions on the boundary seems ridiculous, but the resulting equation will be third order so maybe it turns out ok?
I could post more context but I dont think it's relevant
Ok given
$$(\partial_t + (-\Delta)^{1/2}) u \in L^2([0,T]\times\mathbb{R};\mathbb{R}^n)$$
Do i know if $\partial_t u$ and $(-\Delta)^{1/2} u$ exist and are also of the same integrability?
I already seached for energy bounds fitting this form, but couldnt find anything
KIl
Might be missing something but the vanishing of curl of b is equivalent to b being the gradient of a potential. This is just a general fact for vector-fields. Athough I might just be confused with the abuse of notation of mathbf(b) and b.
This is just a boundary condition, though
The curl doesnt vanish everywhere
Only on the plates
I imagine you can write down the Duhamel's formula for this PDE and then do Fourier transform to obtain some estimates.
Follow the same strategy as for heat equation.
So is the claim that b = grad phi not just on the boundary?
No, just on the boundary. But is it true that if the curl of a vector field vanishes on a plane, its restriction to the plane comes from a potential? i guess what you do is use stokes on curves in the plane?
But you'd only get that the gradient matches the vector field in directions parallel to the plane i think. but i guess that's enough for me here
i added 3d but then i removed it, idk why i think i need phi to be 3d
hmm
yeah ok i understand
ty
The problem is that the derivatives are together as on operator, idk if one of them even exists on its own, thus duhamel's formulare is not directly applicable the same with Fourier
Still, it seems to me like if b is constant and nonzero on the boundary, the curl is just as easily 0 and the potential just depends on x.
I meant take the Fourier transform of the equation first and then solve it via Duhamel. This gives you a formula for the Fourier transform of u so you can then do Plancherel and usual tricks to get some estimates
I know, but taking Fourier is the problem on its own, you cant intercahnge the partial_t with eth FT because the partial_t and the Delta are together and cant be seperated, that is the problem
You can also do energy bounds by multiplying the equation by (Delta)^1/2u and then play around with integration by parts, Cauchy-Schwartz, Youngs etc.
Not sure what you mean by together? Cant you just write par_t u -(Delta)^1/2 u =f and then take the Fourier transform in x?
nop you cannot because they are apllied as on operator
they exist as a distributional dervative together in L^2
?
What's your definition then?
it is as distributional derivative of (\partial_t - Delta thing) no schwartz function what so ever u is only in L^2
of course the test function yeah they work there for sure, but i need infos about u
I mean in my stated definition u can be a distribution as well.
Unless your point is that the equality doesn't hold pointwisely merely in the sense of distributions then sure
Like yes that is correct but i want existence of those derivatives in L^2 like stated before the same integrability
derivatives will always exist for distributions no questions asked
The strategy for these things is that you first assume your u is Schwartz. You derive some estimates that only hold in L2 (or whatever you like). This tells you what estimates you should expect. Then you can prove in distributional sense by doing the necessary rigor required to make the statement sensible.
Ofc, this doesn't give you the existence of a solution or whatever; just some a-priori estimates.
Also this fact holds regardless of you view u distributionally or not. In the case of distributions, you will transfer the derivatives to the test function, split the sum and then transfer the derivatives back to u, to note that this equality does hold.
Yes Maximal reularity for the Poisson semigroup
More precisely here this is the L² maximal regularity in time
in fact
put
Functionanatolysis
Then you can write
Functionanatolysis
Up to consider the extension of F to be 0 on the whole real line, i.e. F(t) = F(t) if t>0, F(t)=0 otherwise.
You can build u as
Functionanatolysis
Similarly
each Fourier symbol is bounded by one in modulus
The Fourier Plancherel theorem yields the boundedness : it is in fact even better than that
Functionanatolysis
(in fact there should be an additional term if u is not in H^{1}_0 (R^{1+n}+), but the whole picture is correct)
Isn't it that I have L^2 maximal theory only in this case if I have minimum H^1 initial condition?
And do you have a good source for it, it's my last part of my master Thesis which I just couldn't get on my own🫠
But thank you a lot!
Just for clarity
My u is at most $L^2_{t,x}$
The operation
$(partial_t + Delta)$ are applied as on operator together
The general $L^P$ theory was already applied once for regularity, but at one point I differentiate and get the existence of
$$
\Delta^{s} ( \partial_t u + \Delta^{1/2} u) \in L^2_{t,x}
$$
Now because weak derivatives commute I just swapped the outer Delta inside and asked my self the former question, that's why I have the operator simultaneously, cause I interchanged it with the outer $\Delta$
If I wouldn't have lost that my initial condition is $H^1$, I would be fine from my point of view, because i only hav $L^2$ I dont know
KIl
\dot{H}^{1/2} for the initial data
In fact, start from the whole space case
R^{n+1}
Then use restriction and extension operators to show that both operator necessarily agrees
(d_t + |D_x|) and (d_t) + |D_x| on R^{n+1}
then on R^{n+1}_+ (once you have the R^n+1 case, this is then just Fubini)
The space you are looking for is L^{2}_t(\dot{H}^{2s}_x)
Concerning this part this is sharp, iff
H^{1} is stronger since it requires one half more derivative
and u_0 to be in L²
For u in L^2
I think there is no direct hope in general
Maximal regularity is an iff type property
Finally a full and definive answer to your question relies on the joint functional calculus of sectorial operators with commuting resolvents.
A.k.a the Dore-venni theorem and its variants
(Which also holds on Banach spaces more general than Hilbert spaces)
Is it possible to find a (shauder) basis for the harmonic functions in the space of all smooth functions on R^n?
I essentially want a way to project into the space of harmonic functions
and having an explicit basis sounds like the easiest way to do this
What sort of topology are you putting on the smooth functions? Harmonic functions (and all their derivatives) are constant or unbounded on R^n, and under most natural topologies, this space is uninteresting.
Why are unbounded functions uninteresting. My goal here is to do a hodge decomposition (which is initially proven only on compact manifolds without boundary)
And in particular, I want to see the "harmonic component" of my function
Does that help?
Would that be unique? Suppose f = g+h where g is the harmonic component. Then lap f = lap h as lap g = 0. But note
f = (g+c) + (h-c) is also a valid decomposition for any first order polynomial/harmonic c and it still satisfies lap f = lap h = lap(h-c).
Now if you somehow quotient out harmonic functions when you take h, then that might work but not sure if there's a decomposition like that
they aren't uninteresting, my point was that in most natural topologies (sobolev norms, for instance), we only topologize a subspace, which has a 0 or 1 dim subspace of harmonic functions
also, since you are asking about a schauder basis, you need to decide on a topology to use. Piggybacking off of cocat's answer, you might also want some way to 'force' the decomposition to be unique. In the compact manifold case, we are looking at L^2 of differential forms, which allows us to identify quotients (by closed subspaces) with subspaces of our vector space. In fact, you can do hodge decomposition for L^2 differential forms in R^n, but the subspace of square integrable harmonic k-forms in R^n is zero dimensional for all k
can yoz show me where you have this? I only found it for H^1 intial data, that would tbh solve the whole thing
This is the one i found which i was able to edit to H^1 initial data
Juste write down the quantities and play with Fourier transform
I don't have any references, except maybe two of my papers. But those treat the very general case
Its alright if it generel
I mean no L² spaces or anything just abstract Lp maximal regularity for class of Operators.
First construct the Projections on L²
A Projection on the closure of the range of d
A projection on the closure of the range of d*
I-P-P* is then a projection on the finite dimensional space of harmonic forms
How can I get the projection onto the closure of the range of d without first getting rid of the harmonic part
Here's my recipie for compact manifolds with no boundary:
From hodge decomp:
w = df + d*g + \xi
Where \xi is harmonic.
First solve:
\Delta u = 0
By hodge thm you know that there's going to be a finite basis for this space corresponding to the cohomology representatives.
You now have a finite basis for harmonic forms and can easily project and then subtract that off w.
So we can assume wlog that we have:
w = df + d*g
To project this we do:
d*w = d*df
d*w = \Delta f (assuming w is a 1-form here)
And this is just a poisson pde which can be solved using standard (Greens function) methods.
Solving this PDE gives me f. And so I can then I've finished my decomposition sice:
d*g = w - df.
What underpins this all is first erasing the harmonic component
otherwise you get something like d*\xi in your pde
NVM I AM STUPID
d*\xi is always zero
as is d\xi
🤦
I'm having trouble doing this in dimension higher than 2
In all dimensions, we get that d*d = \Delta when acting on 0-forms. This lets you solve a poisson pde to do the projection onto im d.
An easy special case is when we're in 2D because dd* in acts like \Delta. This lets you, again, just solve a poisson pde to project to im d*
In 3D I need to solve something like:
curl w = curl(curl w)
I feel like a fundamental step needs to be directly projecting onto the harmonic subspace. But it's really unclear how to do that.
[I can't use the trick I explained above, because I'm wanting to do this on R^n and not something compact]
IMO it's totally reasonable to think that a vector field on R^n could contain an unbounded harmonic component.
You can build the projector the way I did
However you won't get anything more than a finite dimensional subspace by De Rham Cohomology.
I can't do one of the first projections
In particular, the projection associated with the d* image
Why ?
What do you mean by "You can't" ?
You have closed Hilbert subspaces. Such projection operators always exists
Computationally how would I do the projection
For the image of d it's straightforward
Essentially you have to solve a poisson PDE
I think it's going to end up being a weird equation like:
Curl F = Curl Curl Phi
And you're given F and need to find a Phi satisfying this
(in 3d anyway)
I'm going to repeat this because I feel like my answer got buried: you can do the Hodge decomposition for L^2 k-forms on R^n.
The subspace of harmonic L^2 k-forms on R^n is zero dimensional for all k (by the mean value property).
If you want to do this not on the space of L^2 k-forms, then things may get more interesting. You also have to decide how to topologize your vector space, and then potentially deal with issues like uniqueness of decomposition.
So, if we restrict our attention to only L^2 forms on R^n then the hodge decomposition holds and is unique. "but" the components in the decomposition are also going to be L^2.
I guess the statement says nothing about the uniqueness of the decomposition if we allow for the components to be not in L^2.
For instance, writing an L^2 1-form as a sum w = df + d*g where df and d*g are not in L^2 could be possible (it's not ruled out by the theorem)
I think this is true since for instance: it's true that any nonzero harmonic thing must be not L^2
mm
actually im not sure
V5_
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Their images intersect at zero regardless of integrability
sorry I'm having trouble typing the * symbol
thats fiine lol
yes
okay, i might try to prove that. But there are so many deathtrap theorems here
it's sort of a statement about chain complexes over a field, for instance, on smooth k-forms, we have the de Rham complex, and each vector space of k-forms splits as a direct sum of the image of d (from k-1 forms), the cokernel of d, and the kernel of d mod the image of d
I'm not from pdes, and sometimes random theorems delve deep into like elliptic pde knowledge lol
this reminds me of when someone I know who does AG told me about having to learn pdes to read the proof of the index theorem
I did the Hodge decomposition on Rn and Rn+ in a paper
For any LP/Sobolev and Besov spaces
The main point is that the Laplacian is injective on Rn, once you forgot polynomials.
Then the result is a "trivial" (in L² at least) consequence of Fourier Analysis.
come read about psidos with me 
so glad the french are dealing with this for everyone's benefit
once my term ends
The so sad truth
- what is C_{s,p}?
- What does the "dot" mean over the spaces? From context, I'm guessing it means the closure
- So are you saying that harmonic polynomials are the "only" problematic things in the HHD?
Actually, maybe if you DM me the article I might be able to answer these things for myself
kind of lost on this
i think i got
$\casedef{v_t-v_{xx}=g'(t),&\bR_+\times(0,\infty)\
v=0,&[0,\infty)\times[0,\infty)}$
eigentaylor
but i don't really understand the odd reflection part
and i don't think this is right
$v(x,t)=\int_0^tg'(s)\int_\bR\Phi(x-y,t-s)\dx y\dx s$
eigentaylor
any help appreciated
Forget about the dot, this is just fancy stuff here
and if you can can for got about the point you can also remove the considition C_s,p
this is a condition that says "okay if the space is complete/Banach"
For me the closure is the overline
H^{s,p} is the Sobolev spaces of order s over L^p
(think s=k is an integer)
the dot stands for the homogeneous Sobolev spaces.
in the sense of the norms are left invariant by a dilation
somehow
so a lot not necessarily technicalities for you
get over it
s=0, gives you the L^p result
H^{0,p}=L^p
First, you want to check the sign of g’(t), I think it should be -g’(t).
Now, odd reflection of a function f is taking -f(-x).
Once you have a heat equation defined on all of R using odd reflection, you can use the formula for the nonhomogeneous heat equation in Evans.
From here, it should just be some amount of bashing of integrals to solve for v(x,t) in an integral form that looks like what you’re asked to find
One way to proceed : prove that there is at most one solution
then show that the given formula is indeed a solution.
Oh that’s fun
I think the issue is that the professor said derive
Rather than prove that this is the unique solution
I think following Evans computations is the point of that exercise
Although that is a cute & clever way of going about it
Yeah I've seen this after I did propose this solution.
right so would it just be
$\casedef{v_t-v_{xx}=-g'(t),&\bR\times(0,\infty)\
v=0,&\bR\times[0,\infty)}$?
eigentaylor
and we're saying v(x,t)=-v(-x,t) if x<0?
Yeah, I'd also recommend writing out the equation being solved on R_- explicitly
It will make it easier to write out explicitly because you'll get integrals on R_- and R_+
oh, and shouldn't it be v=0 on R x {0}
oh yes! that was a dumb mistake. yeah that's right.
yeah that might explain why my integral for v(x,t) ended up just being g(t) by itself. i will try that rn
||Yeah, there's a sign change of the g' on R-||
spoilered bc I just verified it but didn't want to give it away
ahhh so basically it should be
$\casedef{v_t-v_{xx}=-\opn{sign}(x)g'(t),&\bR\times(0,\infty)\
v=0,&\bR\times\bdef{t=0}}$
eigentaylor
thank you! i will try it again
Yeah, the hope is that you end up with v(x,t) = -g(t) + blah, where blah is the result you're anticipating
[
v(x,t)=
\int_0^t\frac{1}{\sqrt{4\pi(t-s)}}
\int_\bR e^{-\frac{(x-y)^2}{4(t-s)}}(-\opn{sign}(y)g'(s))\dx y\dx s
]
\begin{multline*}
v(x,t)=\int_0^tg'(s)\bigg[
\int_{-\infty}^0\frac{e^{-\frac{(x-y)^2}{4(t-s)}}}{\sqrt{4\pi(t-s)}}(-1)\dx y\
-\int_{0}^\infty\frac{e^{-\frac{(x-y)^2}{4(t-s)}}}{\sqrt{4\pi(t-s)}}(1)\dx y\bigg]\dx s
\end{multline*}
\begin{multline*}
v(x,t)=\int_0^tg'(s)\bigg[
\int_{-\infty}^{\frac{x}{\sqrt{4(t-s)}}}\frac{e^{-u^2}}{\sqrt{\pi}}\dx u
-\int_{\frac{x}{\sqrt{4(t-s)}}}^{\infty}\frac{e^{-u^2}}{\sqrt{\pi}}\dx u\bigg]\dx s\
=\int_0^tg'(s)\bigg[
\int_{-\infty}^{\frac{x}{\sqrt{4(t-s)}}}\frac{e^{-u^2}}{\sqrt{\pi}}\dx u
-\paren{1-\int_{-\infty}^{\frac{x}{\sqrt{4(t-s)}}}\frac{e^{-u^2}}{\sqrt{\pi}}\dx u}\bigg]\dx s\
=\int_0^tg'(s)\bigg[
2\int_{-\infty}^{\frac{x}{\sqrt{4(t-s)}}}\frac{e^{-u^2}}{\sqrt{\pi}}\dx u
-1\bigg]\dx s
\end{multline*}
eigentaylor
am i on the right track or did i mess up somewhere? i tried to leverage that the integral of the exponential integral is 1
i think it's right and that gives me
$\int_0^t g'(s)\erf\paren{\frac{x}{\sqrt{4(t-s)}}}\dx s=g(t)-\int_0^t\frac{e^{-\frac{x^2}{4(t-s)}}}{\sqrt{\pi(t-s)}}g(s)\dx s$
eigentaylor
i think
Yeah, I think it looks good at a glance
If not, it’s fine up to a sign change in the change of variables somewhere
but then i need to show that
$-\int_0^t\frac{e^{-\frac{x^2}{4(t-s)}}}{\sqrt{\pi(t-s)}}g(s)\dx s=\frac{x}{\sqrt{4\pi}} \int_{0}^{t} \frac{1}{(t - s)^{3/2}} e^{-\frac{x^2}{4(t-s)}} g(s) \dx s$
eigentaylor
but the RHS looks like the partial derivative of the LHS wrt x...
mhm
then are they equal? if so, why is the expression equal to its partial derivative wrt x?
Oh, I misread what you were doing
$F(s)=\int_{-\infty}^{-\frac{x}{\sqrt{4(t-s)}}} \frac{e^{-u^2}}{\sqrt{\pi}}du$
has $F'(s) = -\frac{x}{4\sqrt{\pi} (t-s)^{3/2}} e^{-\frac{x^2}{4(t-s)}}$
MSC2020 49Qxx
agagdhsh right we're integrating with respect to s not x. thank you for continuing to help me through my dumbery
No worries, these computational things can be annoying so I get it
This is a silly question I'm asking because it's been a while since I've done problems with laplacians, but if I am looking at the 2d laplacian on a square, with periodic boundary conditions, if the boundary conditions I choose are dirichlet and say the value on every side is the same constant, this implies the solution is just constant over that square domain correct?
Yeah, you can use the maximum principle
does anyone have any
relatively short expository papers or anything
to get me excited for reading evans
applications based btw
for example how can the theory of weak solutions and the sobolev space stuff be applied
smth historical could work too
financial applications, fluids, other physics, they all work for me
short read
thanks
oh, and if you're interested in numerical simulations, maybe play around with finite element software, for example https://ngsolve.org/, which is based on the theory of weak solutions and sobolev spaces
Hi, any references about evolution families that we use to solve evolution PDEs of the form $u_t(x)=A(t)u(x)$ when the operator $A$ is time dependent, please?
Mikahopff
if A is an elliptic operator for any time
look at Non-autonomous maximal regularity
e.g.
Thank you very much
Do you know anything about the other case please?
About the other cases ?
when the operator is not necessarily elliptic?
For hyperbolic systems
there is the theory of friedrichs Symmetrizers
See Guy Metivier's book
Mostly for first order type systems
Ok ,thank you. it is good to take a look but I am only ineterested in existence of week solutions..etc.
Thank you again.
One Parameter semigroups for linear evolution equations Chapter 6.9
it seems quite good
was not aware of it
thx
The book is so good, the authors wrote a baby version after publishing the book because students were getting put off by the breadth of the book xD
Hahaha
Thank you very much.
im not sure if this is the right section to ask but, why is the phasor domain of KVL/ KCL equations of a RC, RL, RCL circuit linear. Allowing for an easier approach at solving intergrodifferential equations
!!
Can anyone please refer to easy to understand book for symmetrization & rearrangement inequalities
does anyone know a good vector calculus review?
I just wanna speedrun the curl, grad, div, stuff
- green theorem + stokes in 3d + line integrals
for evans
holding on 
oh I also have like
0 intution on the leplacian
I see the appendices but there's no proofs for most theorems
- Mean value property of harmonic functions
- Heat equation to understand it's regulating properties
- Maybe complex analysis stuff to see it's other connections
I would say you don't particularly need any more review on this besides what he covers in the appendix. Even if you haven't covered the proofs, I would say skip them and get started with the book. You can revisit the proof anytime and the more important thing is how to use the statements which Evans will teach.
why you want to speedrun? are you in a hurry?
yea, I need to catch up to a group of people I'm reading evans with
I would do that if I could at the very least understand the theorem statements 
I think I'm missing a couple of definitions
which definitions?
I think the definitions and notation choices in Evans are pretty self-contained for the most part.
Feel free to ask them on the server but as Gomez said, you can find all the definitions at the back of book.
Is it an online group?
like this definition for example,
I can't just look at it and understand what it's saying
which tells me I should prolly read on this stuff somewhere first before going back to evans
will do, thankyu!
yes
the definition right after it too
like, what the heck is \nu?
is it just like, any vector field defined on \partial U?
surely that can't be true
coz otherwise this wouldn't be well defined!
also, what's the difference between dS and dx 
I just... don't understand any of it lmfao
this basically is saying that the boundary is C^k if at each point, if you zoom in far enough, the boundary just looks like the graph of a C^k function
at each point on the boundary, the unit normal vector is the uni vector which points orthogonally to the boundary in the 'outward' direction, might help to just look up a picture
but why does it exist
and is it well defined?
because the boundary is C1, its locally just like a graph of a C1 function
and this lets you define it explicitly more less
probably a good idea to read up on surface integrals though before diving into evans
Okay, so you mean that you are having trouble parsing some of the definitions, not that these definitions are not present in Evans?
In the first example you should think in small dimensions first like n=2. This definition means a region like: y > x^2 has smooth boundary, because the function f(x)=x^2 is smooth. It just looks a bit more complicated because you can only hope to represent the boundary of a domain locally as a graph. (E.g. with a disk you would have to use different functions to graph different pieces of the circular boundary, but the point is you can do it "locally" about any point).
For the second, once you understand tangent (hyperplanes) to graphs of functions of several variables, the well-definedness of normal vector fields is a matter of linear algebra. (The orthocomplement of a hyperplane is 1-dimensional) .

oh!
okay, that makes sense
Can I join? I’m re-reading Evans for grad school
ohhhh, so that's what evans meant by "relabeling and reorienting the coordinates axes"
you just reorient them so that U \cap ball looks like the graph of some function
you should ask @pulsar forge tbh, it's not my reading group
you can also look at his post in #events message
there are certain commitments you have to agree to before joining
the answer is yes to the first question btw
but not only that, when I see a theorem or a definition I don't even know if I'm missing something or if I'm just being dum lel
In 2 dimensions, relabelling and reorienting just means that either write y as a function of x or x as a function of y to describe the boundary as a graph locally.
hmm good to talk about it with others / try problems etc to figure out exactly what your gaps are if any.
sure i dont mind, more discussions to be had 
oki 
I think I'll read on that stuff seperately rq and see if I don't understand anything
surface measures basically, similar to polar coordinates and how you have a "measure" on the circle using arc-measurment , its just more generalized.
i think folland covers it iirc
If your surface is a graph say $f(x)$, then it is parametrised by $x$ and the surface measure is like $\sqrt{1+|\nabla f(x)|^2}, dx$ in these coords
grobmez
if you are reserving x to use as coordinates in the whole space, replace the x in the above formula with like a x' or whatever.
If you need more clarifications for definitions like and related to this, check out Folland PDE book. He is much more precise with preliminaries like this.
Also, it helps to know that one of the reasons we care about the smoothness of the boundary because we frequently use Generalized Stokes Theorem.
Does anyone know any good resources for asymptotic methods in PDEs? I am familiar with asymptotic methods for ODE's, but I am less certain how to apply my methods in cases where I cannot reduce my PDE to some ODE's through separation of variables. I want to use it to study mixed type linear PDE's so I can understand how the solution is changing with the introduction of a term that extends the discriminant from being purely elliptic/hyperbolic to a mixed type.
Not that much actually since one can reach lower the regularity at an absurd level and still have a Stokes theorem. Lipschitz, SKT domains etc.
The general idea on the whole space is to consider the pseudo-differential operator and to cut it out, in the Fourier side' in various operators that behaves at different regimes. Usually heavily used, if I am not mistaken In problems such as dispersive PDEs as in water-waves systems etc.
This relies generally on Harmonic Analysis methods such as the stationary phases and other related results
simple question, but is this enough to deduce the wave operator is not hypoelliptic?
(since it seems to imply u doesn't need to be always smooth)
Well this isn't telling you that the solutions cannot be smooth, merely that they're C2. But your conclusion is correct: the wave operator isn't hypoelliptic as it's solutions can be arbitrarily rough.
How normal is trying to find solutions using Sobolev spaces? Just for curiosity
Not sure what "using" means. If the question is how usually do Sobolev spaces arise in PDE theory then the answer is all the time. Sobolev spaces give a more flexible characterisation of your original PDE problem
I meant, when ordinary derivatives doesnt work and the "solution" dont satifies the restrictions
Because my thesis is PDE related and Im trying to understand what it motivated Hörmander to consider distribution theory to solve a problem
Then check this out https://math.stackexchange.com/questions/3314557/why-should-i-believe-in-weak-solutions-to-pdes
I will check it thanks
iirc what motivated thinking about them was wanting to have some notion of solutions depending continuously on parameters (such as initial conditions) among other things
Im also taking a course about Sobolev spaces so I will ask my teacher too. He motivated from where this spaces appears and why but Im still a bit confused
Smth similar our teacher told us. I really appreciate that he gave us a math context with dates
Hi everyone. I'm not sure if this is the best place to ask this question because it's not really PDEs, but I'm using it to perform analysis related to PDEs. Essentially, I'm trying to expand a solution to a PDE using Hermite series (sum_n a_n H_n(x) for H_n the physicist Hermite polynomials). For simplicity, let's say it's a stationary solution for a 1D PDE so there's no need to worry about tensor spaces right now. For the purpose of my analysis, I need a Banach algebra on the sequence space of coefficients. So if w = uv (all three Hermite series), I need |w|_X <= C |u|_X |v|_X (edit: these are norms, but double bars are behaving strangely) for some constant C and X a Banach space. With Fourier series, we usually use l^1 (or a weighted version of l^1) as C = 1, so you don't need to "think about C" in that sense. For Hermite, this isn't so obvious because the product is "weird" (i.e. not a convolution). I'm not necessarily looking for a proof right now, but I've been going at this for a while so I thought I'd see if anyone could provide some intuition here? I'm beginning to think it's not true for l^1, but I don't want to aimlessly try l^2, then l^3, etc. and keep hitting dead ends if I'm looking at it the wrong way. I can provide some work if that helps.
This is definitely not my area (I deal with Riesz spaces and I avoid norms as much as I can), but I'll soon be meeting with some experts in functional analysis (the people I'll see on Tuesday deal with pre-Riesz spaces, but they like Banach algebras and the people I'll see on the 25th of March are people who work in Banach algebras). If you don't mind waiting (and, probably until the 25th of March), if you remind me then I can pose your question to an expert in Banach algebras and send that response to you. Apologies that I can't be of any help and that it'll take a while until I'm with the appropriate people.
That would be great! I'm not in a rush to get an answer. I'll also let you know if I find an answer beforehand. I'll be in touch!
OK, I'll let you know who has what to say!
why does this inequality hold?
I'm confused, shouldn't the integral go to infinity?
\Phi is the fundamental solution of the leplace equation and f is a compactly supported C^2 function
use Polar Coordinates
then you just have to found 1-dimensional anti-derivative
What is L^p norm on distributions?
like W^(k,p) is the space of functions with kth weak derivatives in L^p
but what does it mean for kth weak derivatives to be in L^p?
There isn't one. There is a natural one for distributions that are representable by Lp functions.
That's the function representing the kth weak derivative is in Lp
i see ok so it has to genuinely reside in L^p, makes sense
like sin(|x|) is in W^(k,infty) for any k
An interesting convention is also to say that for distributions that are not identifiable with an Lp function the value is +\infty, as for measurable functions.
Think for instance about Triebel and Besov norms
Is there a simple relationship between the concepts of the characteristic variety, characteristic hypersurfaces and bicharacteristic curves/strips?
Say we are looking at an m-th order linear PDE on a smooth manifold X of dimension n.
The first is a single 2n-1 dimensional conic submanifold of the cotangent bundle T*X, defined by the vanishing of the principal symbol of P.
The second is a set of of n-1 dimensional hypersurfaces in X, defined by the property that the conormal bundle is contained in the characteristic variety.
The third is a set of 1d curves in the cotangent bundle T^*M, defined as the integral curves of the Hamilton vector field associated to the principal symbol of P.
My understanding:
-The third and first have a clear connection, in that through any point on the char. variety there is a "null" bicharacteristic that stays on the the char. variety. The importance of these curves is results like the propagation of singularities.
-The second is something that can be regarded as an obstruction to solving Cauchy problems. (It essentially means that the m-th normal derivative of a solution to Pu=0 is not determined by the first m-1 normal derivatives). There are further refinements such as the various forms of hyperbolicity that one can ask for that guarantee existence of Cauchy problem solutions, but a non-characteristic initial hypersurface is using imposed to begin with.
However the geometric link between the characteristic hypersurfaces and bicharacteristic curves (or their projections to the base manifold X) is unclear to me. Does anyone know of one beyond their links to the char. variety mentioned above?
Does it count as a "relationship" that the bicharacteristic curve is always on the characteristic hypersurface? I think the bicharacteristic is the result of taking the characteristic of the characteristic equation (in the average use case).
It counts as a relationship, but also one that I was aware of. (See first point under "my understanding"). What I am more interested in is the relationship between the second and third notion. That is, between the notion of a characteristic hypersurface (most relevant for the consideration of Cauchy problems and where to specify initial data) and bicharacteristic curves (most relevant when considering the propagation of regularity for solutions to PDE of real principal type).
Also, I don't really know what you mean in your second sentence.
I was referring the the specific case of the second order method of characteristics being solvable by way of Lagrange-Charpit (the fully nonlinear method of characteristics for first order equations)
Sure well I know how to solve nonlinear first order equations using characteristics, and that in the linear case the characteristics are just the projections of the bicharacteristics in the cotangent bundle onto physical space, and furthermore that the condition of an initial hypersurface being non-characteristic is precisely equivalent to these projected characteristic curves meeting the initial hypersurface transversally. (Which is of course desirable in order to make the method of characteristics work).
All of this is well and good, but all of this is also for first order equations in particular.
The heart of my question is that I am curious if there is an equally nice geometric picture for the relationship between these concepts in the setting of higher order linear equations.
The characteristic equation for Second order PDEs is first order
∑ᵢ,ᵣ Aᵢᵣ(∂φ/∂xᵢ)(∂φ/∂xᵣ) = 0
Im not certain if method of characteristics generalizes to higher than second order. I think the principle coefficients in that case dont fit in an NxN matrix
you could use a rank (order) "tensor" I guess
I don't think it does, but I am not really asking about the method of characteristics in any case. Whether or not one can use the notion of characteristics (in any sense of the term) to actually solve equations, one still cares about:
a) the solution of Cauchy problems (for which the notion of a non-characteristic initial hypersurface is important to solvability)
b) the propagation of singularities (which happens along bicharacteristic curves in the cotangent bundle)
Okay, the only context I have heard the word "bicharacteristic" is when you take the characteristic of the characteristic equation.
I dont know enough about geometric PDE theory to probably answer your question, but I do know what all those words mean for general relativity
in what sense do you mean "take the characteristic of" ?
what I said about using Lagrange-Charpit earlier
What you call the characteristic equation is the condition for the level set of a function being a characteristic hypersurface in the sense I mean it
ah okay sure, well then yes that coincides with what I call bicharacteristic (the integral curves of the hamilton vector field of the principle symbol)
So I guess I am not completely satisfied yet, but I do now see that the condition defining characteristic hypersurfaces for an operator P (this condition is a nonlinear first order PDE) has characteristics that coincide with the bicharacteristic curves of the initial operator P in the Hamiltonian sense. That is an interesting (but probably obvious from the right point of view) observation.
Yeah ofc I guess that is the equivalence between Hamiltonian dynamics and the Hamilton-JAcobi formulation
when you say Hamilton vector field, do you mean Hamiltonian vector field, or is it something else?
exactly that. both terminologies are used in diff sources.
isnt that supposed to exist on a symplectic manifold instead of a Riemmanian?
Yes, that is why I said that bicharacteristic curves live in the cotangent bundle, which has a canonical symplectic structure.
what you are calling characteristic curves are the projections of these onto the base space
ahhh, okay. I learned a bit about those in Classical mechanics
symplectic form is preserved under canonical transformations and such
yep
did you know second order characteristics can be generalized to the fully nonlinear case? I was pretty surprised by that.
still has to be hyperbolic/parabolic for the characteristics to exist, but feels like it should be mentioned more in the literature
yes, it is definitely surprising when you first see it!
Since you brought up Hamilton-jacobi, there is a particular equation I was attempting to analyze for characteristics
https://en.wikipedia.org/wiki/Hamilton–Jacobi–Einstein_equation#General_equation_(free_curved_space)
In general relativity, the Hamilton–Jacobi–Einstein equation (HJEE) or Einstein–Hamilton–Jacobi equation (EHJE) is an equation in the Hamiltonian formulation of geometrodynamics in superspace, cast in the "geometrodynamics era" around the 1960s, by Asher Peres in 1962 and others. It is an attempt to reformulate general relativity in such a way t...
How was this equation derived in the document?
in free space, you can drop the sqrt(g)R term
What should I do if the derivation in your paper cannot be extrapolated
will these also be equal to delta^(alpha+beta) F
\partial, not \delta, but yes.
oops yea
What is the deal with Method of Constraints? Are you just selecting a constraint equation and hoping there is a Union between the solutions of the original and constraint equations?
i'm totally stuck on part b. like i get we want to show the limit of the integral of uxx^2-utt^2 is zero, can we somehow say that ux-ut approaches zero as t goes to infinity?
its probably easiest to show it using the formula for the solution in terms of g and h
remember that you need to show k(t) = p(t) for all t > T for some finite T. Its not enough for k(t) to approach p(t) or something like that
I see. it does have to be in finite time.
do you mean d'Alemberts solution?
yeah exactly
so i did the whole computation and when i did ux^2-ut^2 i got a sum of products of like g'(x+-t)h(x-+t), and for large enough t, we can misalign the supports to get it to be zero for all x.
but i think it might be much easier to just write it as u(x,t)=F(x+t)+G(x-t). i think same thing but the computations not as horrible lol
because F and G will also have compact support right?
because we can set the lower bounds of the integral on h to be outside the support of both functions
yeah so these are not compactly supported
because of the integral of h
the thing you did originally sounds correct
Literally my test for PDE today lmao
Just had it
It was straight brutality
Omg the same thing but a little harder lol
but the derivatives [g'(x)+-h(x)]/2 will be, right? then i think it does work
ux=F'(x+t)+G'(x-t)
ut=F'(x+t)-G'(x-t)
both have compact support, so ux^2-ut^2=4F'(x+t)G'(x-t)
we can pick t large enough such that we knock them both off their support and F'(x+t)G'(x-t)=0 for all x.
does that pass the vibe check?
The product of uxut from negative infinity to infinity goes to zero
What exactly is sign(x) defined as?
1 if x>0, -1 if x<0
Yeah I think so
any help?
use separation of variables, U(x,t) = X(x)T(t)
potentially a silly question, suppose
\begin{align}
\lvert \int g(x) f(x), dx\rvert^2 = \lvert \int \tilde{g}(x) f(x), dx\rvert^2
\end{align}
for all nice (to a physicist's standards) functions $f$. By taking $f(x) = \delta(x-x_0)$, you can see that $\lvert \tilde{g}(x_0)\rvert = \lvert g(x_0) \rvert $ for all $x_0$, and so $\tilde{g}(x_0) = e^{i \theta} g(x_0)$. From this alone there is no reason to think that $\theta$ is independent of $x$, but I strongly suspect that it is, and that one can see this from taking $f$ to be other functions besides a delta function. \
My question is... is $\theta$ actually independent of $x$? If so, how do you show it, and if not, then why not?
nay
g is a function from R to R?
sorry should have specified, g and f are functions from R -> C
nay
sorry this has errors
corrected: From taking f to be a single delta function $f(x) = \delta(x-x_0)$, we know $\tilde{g}(x_0) = e^{i \theta(x_0)} g(x_0)$. Now we want to show $\theta(x) = \text{constant}$. Take $f(x) = \delta(x-x_a) + e^{i \phi} \delta(x-x_b)$ for some $\phi$ of our choosing. Then we have, upon substitution into the integral and using the result from taking f to be a single delta function:
\begin{align}
\lvert g(x_a) + e^{i\phi}g(x_b)\rvert &= \lvert g(x_a) e^{i\theta(x_a)} + e^{i\phi} e^{i\theta(x_b)} g(x_b)\rvert \
&= \lvert g(x_a) + e^{i\phi} e^{i (\theta(x_b) - \theta(x_a))} g(x_b)\rvert
\end{align}
and then geometrically this can only hold for all $\phi$ if $\theta(x_a) - \theta(x_b) = 0$.
nay
This might be a silly question, but Im looking at a boundar value problem(dirichlet) for the laplacian on a square. Once I have the solution, Im wondering how the boundary changes when I integrate the function with respect to x or y.
Suppose thr boundary condition for the solution at the right edge x = a is f(y). Im wondering how the function at that edge changes when I integrate with respect to x.
I figured there was a straightforward way to see what it becomes because if I integrated with respect to y, its obvious youd just integrate f(y), but when I integrate my solution z with respect to x and evaluate it at x = a, its changing the fourier coefficients if f(y).
my question is just about plotting the "exact" solution i'm going to be getting numerically. would we use a very small epsilon and the Cole-Hopf transformation (would that even work?) or is there a simpler way i'm not seeing using characteristics or something?
you should be able to calculate a formula for the solution using characterstics
ln|t| + a = (ln|x| + b)/u = c
I broke it up into two Riemann problems and got
$u(x,0.5)=\casedef{
-0.5,&0\leq x<0.25\
\frac{x-1/2}{0.5},&0.25< x<1\
1,&1<x<1.25\
0,&1.25<x<1.5
}$
does that seem reasonable?
eigentaylor
$u(x,0.5)=\casedef{
-\frac12,&0\leq x<0.25\
\frac{x-\frac12}{0.5},&0.25< x<0.75\
1,&0.75<x<1.25\
0,&1.25<x\le\frac32
}$
eigentaylor
that would be much appreciated. I think it should actually be the first one but having someone double check would be great
okay yep I think i agree with the first one
one sanity check is the bit between the solution changing from u=x-1/2 / 0.5 to u=1 should be continuous
yeah definitely
Hi. I have a question about the Laplacian on a square again. I am looking at the case where all of the boundary conditions are equal to a quadratic, something simple like x^2. By boundary conditions I mean dirichlet. I'm doing it just by adding 4 of the individual solutions that are zero on 3 sides besides 1. The basis functions for expressing the functions on the profile are something liike sin(pin(x-a)/L), and when I'm trying to find the fourier series for this function that is quadratic using these, and im looking at the partial approximations, it looks like the series is converging extremely slowly and I'm wondering if that is because the basis functions I am using.
Can I see it in equations???
@wind mortar Let me attach a pdf witht the plot profile and my short calculations attached.
Beautiful
@wind mortar
lmao nevermind, I got it. I had a typo in my code that was plotting this. It still takes so many terms to get a good approximation though. I needed 200 terms just to get this. It just seems weird to me to approximation functions that look like they are non-zero at the end points of the boundary by eigenfunctions that are zero at the end points of the boundary. I mean in the case of x^2 over the interval [-pi pi], I'm approximating it with these sin((x+pi)n/2) functions that are zero at those end points.
I have a question about weak solutions of the wave equation
suppose I have the wave equation $u_{tt} = u_{xx}$ on $\mathbb{R} \times \mathbb{R}^+$ with initial condition $u(x,0) = H(x)$ and $u_t(x,0) = 0$
At the moment, it seems to me that the solutions $u_1(x,t) = H(x-t)$ and $u_2(x,t) = \frac 12 \left( H(x-t) + H(x+t)\right)$ both satisfy the wave equation weakly and the initial conditions ae. What am I missing here?
jamiecjx
suppose H were not a heaviside function but something that approximates it smoothly, then only the second solution $u_2$ makes sense.
jamiecjx
I think i resolved it, if we are to have a weak solution that takes in to account the initial conditions, then our test function $\varphi$ will somemtimes need to have support containing $t=0$, in which case the integration yields extra terms that involve the initial conditions
jamiecjx
@wind mortar My bad, thanks though. I do have a technical question though about solutions of the laplacian. When solving the laplacian on a square in the problem I mentioned with dirichlet bc, the typical approach Ive seen is adding these 4 solutions that each contain one of the boundary condition.
Does this approach fail to capture any solutions? For example, what about a solution that is bilinear that I also know solves the equation, or constant? Granted I know fourier series can also represent those, but it seems almost like a hastle to write in that manner.
@grand garnet add Me, are you doing quantum mechanics ?
@wind mortar No, it's sort of hard to explain the problem I'm looking at. It's related to small bending of surfaces. The out of plane component of the deformation for the surface I'm looking at is governed by the laplacian over a square interval [-a a] x [-a a]
Is the problem you are concerned with well-posed?
i.e. the solution exists and its unique
If this is the case, the separation of variables method should give us the solution, assuming that the method works.
Yeah, the domain is a square, so with Dirichlet boundary conditions, it'll be fine to just use separation of variables/fourier series to get to a solution.
If this is a numerics problem, you're best to ask in #numerical-analysis
Something like $\Delta u(x,y)=0$ on $[0,1]^2$ with $u(x,y)=g(x,y)$ in $\partial ([0,1]^2)$ is fine
Kirby
They mention g is a quadratic, so it's smooth
I meant to reply to your first message with that bc I think that's what they're trying to solve, but yes

No worries, discord likes to drop replies for me for some reason, as in if I click reply, it forgets I clicked reply
When I leave and re-enter the app
@tired hollow yes I would say so. I am just looking at the case where each profile on the side is f(x) = x^2 or g(y) = y^2. When I am plotting this however, I am getting these very sharp peaks at the 4 corners of these solutions which I anticipate is due to the fact I'm using eigenfunctions that vanish at the corners where my function takes non-zero values. I figured the appropriate way to handle this is to have my solution be a sum of solutions, one defined on (-1,1)^2, which is my square minus the four corners, and the other solution being piecewise that defines the value of the solution at those 4 corners
Your boundary data lack smoothness at the corners
This affects the convergence rate of the series
Back to your original question, this is fine since for wellposedness if i remember correctly the boundary data has to be in H^(1/2)(Γ), where Γ is the boundary.
Since the problem is well-posed, the solution exists and its unique, so your method should lead to the one only solution.
@tired hollow Okay I figured. Would using different eigenfunctions like cos help my convergence? Because theyd be nonzero at the corners or would this make no difference. I just figured it would be more natural to choose for these boundary conditions.
Does anyone know any good literature on linear second order pdes with periodic coefficients? (in such a way that the discriminant is mixed and alternating between hyperbolic and elliptic periodically in the domain).
There is only two/three references about PDEs with periodic coefficients and this is mostly for elliptic/Parabolic and Schrodinger equation, like PDEs
Search for Bloch-Floquet Theory
Kuchment is a first but hard reference
but prolly the msot important one
If I have something written like
$\mathrm{tr}(D^2F(\grad w))D^2w)=0$ (in the case of strictly convex functionals $F$, with enough regularity on $w$). We can "ignore dependence of $D^2F$ on $\grad w$ and write $A(x) = D^2F(x)$ uniformly elliptic." I am curious of the motivation of when we can remove dependence like this when studying solutions
Kirby
I'm currently reading Vasseur's notes on De Giorgi's method for Hilbert's 19th problem
has anyone messed with semigroup methods for linear operators?
I'm involved with the topic
what are your questions
@astral vine The following link contains an integral formula that "exponentiates" the infinitesimal generator to the representation of the semigroup, but its kind of confusing what they mean by Inverse
In mathematics, an analytic semigroup is particular kind of strongly continuous semigroup. Analytic semigroups are used in the solution of partial differential equations; compared to strongly continuous semigroups, analytic semigroups provide better regularity of solutions to initial value problems, better results concerning perturbations of th...
Im assuming the operator is taken to be a vector field in the coordinate basis of the partial derivatives.... though Im not sure what that means if you have 2nd derivatives
I guess it would just be another vector, but Im not certain what it would be in terms of the coordinate basis
Idk why this got a thumbs up, it was a question about some formal calculations in these notes on page 4 https://web.ma.utexas.edu/users/vasseur/documents/preprints/DGPekin.pdf
I understand the method, I'm just curious on when we can ignore dependence like this
Ok so if I am correct : what is confusing you is definition of
Functionanatolysis
That's correct
Okay so the definition of such an operator is given if you can solve
Functionanatolysis
provided f is known and u is the known
if you have existence and uniqueness of such solution
then you set
I'm also not certain I understand what the identity vector is
This is not a vector
This the identity map
so for the Laplacian
you want to solve the (Helmholtz) equation
Functionanatolysis
I'm back on this part
such an unique solution allows to define
$$ (\lambda \mathrm{I} - A)^{-1}f := u $$
Functionanatolysis
because if you apply the operator
$$(\lambda \mathrm{I}-A) [(\lambda \mathrm{I}-A)^{-1}f]= (\lambda \mathrm{I}-A) [u] = \lambda u-Au = f$$
Functionanatolysis
Okay, I get that. The inverse in this case seems like it would be some kind of "integral operator", so Im guessing that cant be treated as a vector in the original formula?
What do you mean by vector
u and f are the vectors here
everything else is about linear operators in such setting
∂/∂x is the basis vector in the x direction, I was assuming the operator A was taken to be a vector field in that way
You are mixing geometry stuff and differential operators formalism in functional analysis
Both are denoted the same way
well, infinitesimal generators are vector fields in Lie Groups
but are distinct objects
Can be representend by*
I get that point but you are mixing up the different type of stuff
there is an identification made there
those ∂/∂x (from geometry) and ∂/∂x (from FA) are NOT exactly the same objects
But okay
what ever that was jsut confusing for me
well, the idea is if you have some parametric curve along coordinate curves, with parameter x, the derivative gives you the tangent vector which is the basis vector. Though it does have to ACT on something to be meaningful (a curve)
I know geometry a little bit
I hear you though, functional analysis is different, I'll keep that in mind
This is the same semigroup theory behind those evolution equations
When you want to say that a "vector field X" is the generator of a semigroup, you have to forgot (for a short time) the geometric POV somehow
So Im feeling like if you can invert $$ (\lambda \mathrm{I} - A)$$
x17
and you have a standard evolution equation, dont you already have a solution to the X separable part of the equation?
what do you mean by the "X separable part" ?
$$ \partial_t u = Au $$ is separable isnt it?
x17
Not really
does A have t dependence?
No but I don't really get what you mean by separable
However
Yes
having the good information on L*I-A
gives you the semigroup
then the unique solution to your linear Abstract PDE
provided you have some prescribed initial data
$$ \partial_t u = \lambda, Au = \lambda $$
x17
No you cannot do that
You forgot a u and the two right handsides, first.
And second, this assume that the time derivative or A at least do have eigen vectors and eigenvalues
(without the u's as you wrote, it the equation is not false but won't lead anywhere)
the u on the right comes after the initial separation and can vary a bit with the choice of ansatz
This won't work even for the basic equations
you might need to divide by some extra function to get separation for instance
Maybe in your super specific case
But otherwise
for general A
it doesnot really makes sense
Think about A a matrix acting in dimension 2.
say a rotation matrix
(since you deal with Lie Groups this should be familiar to you)
Okay, so because u isnt known to be separable in general, Au might have t dependence, and u_t might have x dependence, even though A has no t derivatives or coefficient functions in t
general separation of variables can get pretty complicated, you have R-separation and the general ansatz $$ \Sigma_i^N X_i(x)T_i(t) $$
x17
This may not happen even for the easiest linear equations
This very specific to A when it has spectrum made only of eigenvalues, whose eigenvectors forms a Basis of your space
Yeah true, even with some really exotic ansatz, most linear equations arent separable, which is why Im looking into semigroup
I got distracted, Im sorry
What does it mean to integrate over the inverse operator, you said I should think of it like a matrix?
if A is a matrix that's not a trouble right ?
if you are on a Banach space
the equality
is it correct to call $$(\lambda I - A)^{-1}$$ the resolvent in this casee?
x17
Yes
and applied to a fixed element of your Banahc space
this lead to an holomorphic function whose "poles" are the spectrum (eigenvalues or not)
so have do you translate the resolvent from its operator to the associated matrix?
Don't get what you mean
is it like in Quantum where operate the Hamiltonian on an eigenfunction and then left multiply by its adjoint eigenfunction, and the 2 indices give the matrix element?
Note really I was talking about matrices because semigroup theory contains exponential of amtrices
everything still hold true for matrices
instead of general linear operators
i did a bit of matrix exponentiation with generators of GL(n)
again back in Lie group stuff
So when a start with a linear PDE, A is a differential operator. The resolvent of a will be... something else maybe a Volterra operator??? but it wont be a matrix, how do I get the resolvent into a form where I can use the formula?
In general there are no explicit form for the resolvent
You can just show that the operator and its resolvent exists and that's all
There are even operators that CANNOT have integral representation of solutions
So what is the procedure for using the formula and generating a solution (in the cases where that is possible)?
I don't know
just the semigroup and the resolvent exist
and in general additional regularity properties from the operator A are sufficient for what people wants to achieve
bummer I was hoping I could use this to solve elliptic equations with arbitrary coefficient functions
The theory, if the coefficients are not too rough, is already known
is it the transformation to standard form using the characteristics?
Absolutely not
when I use Lie's transformation group method (differential invariants), I get a bunch of arbitrary linear pdes that need to be solved, most of the time they are easy, but some times not. So im trying to learn methods for as many linear PDEs as possible
wait... isnt the resolvent just Greens function of the operator $$(\lambda I - A)u = 0$$
x17
instead of 0
delta function, right. my bad
you should put the dirac mass
But It may not exist green functions in general
it does for elliptic oeprators with smooth coefficients
There is a slow converging method of fourier expanding the Green's function
this only works in the periodic setting, or on the whole space when you have smooth coefficients
again
There is still somesort of Fourier approximation methods if you can show that the spectrum of the operator is purely made of eigenvalues whose eigenvectors are Basis of L²
Which again may not happen
suppose you could get a closed form (not expanded) greens function, then you can directly compute the semigroup representation?
This is true is you have a closed form for the resolvent problem yes
This is still an integral formula
but
somewhat explicit
but in general to compute an explicit formula for resolvent problem may be a hard task
okay, thanks alot. i think I understand the procedure and limitations of the method now.
Im a physicist, so i tend to lean more toward algorithmic thinking, sorry if that was creating disconnects, im mostly looking at methods as tools.
I have a sequence of functions $u^n$ and strong convergence $u^n \rightarrow u$ in $L^2((0,T) \times \Omega)$ on $\Omega = [0,1]^2$. I also have a weak convergence $f(u^n) \rightharpoonup g$ in $L^2((0,T) \times \Omega)$. What criteria does function $f$ need to satisfy so that I have a weak convergence $f(u^n) \rightharpoonup f(u)$ in some $L^2((0,T) \times \Omega)$ and $f(u) = g$ a.e.?
Xilexio
This is equivalent to f being a closed mapping from this space endowed with strong topology to this space endowed with weak topology
Now you can look up for references dealing with your hypotheses to see whether they imply closeness of the operator. A fairly general condition is f is a continuous/linear-bounded operator between the strong topologies
Thank you for your response. I have C^1 f that scales quadratically. The problem is that while in this case I was able to prove a strong convergence because |f(u^n) - f(u)|_L1 is bounded by C * |u^n - u|_L2, I do not know a theorem or method to get weak convergence. And I have just L2 convergence of u, not pointwise, so I don't see why it couldn't explode to infinity in some points as long as it integrates. Can you advise on what am I missing?
I'm having trouble finding a specific theorem about weak convergence of mapping with strongly converging arguments. Would you be able to name a theorem I could look up? Continuous mapping theorem works only for continuous u.
This tells you that f(u^n) converges strongly to f(u) which implies weak convergence
L1 convergence does but do I absolutely need strong convergence of f(u^n) to get weak one but in better space? Note that now I'm searching for a more general principle because I can imagine some bounded f(u^n) that converge to something weakly but not converging strongly even in L1.
Specifically, if u^n converges strongly to u in L2 and f is continuous and nonlinear and f(u^n) is bounded in space L1 (so converges to g), is g = f(u) a.e.?
And is proof of boundedness of f(u^n) required or does strong convergence of u somehow circumvent that?
In what space is f continuous?
Let me write it down better.
I have $f \in C^1(\mathbb{R})$. I have strong convergence $u^n \rightarrow u$ in $L^2(\Omega)$. I have bounded $f(u^n)$ in $L^2(\Omega)$, which gives me existence of $g$ such that we have weak convergence $f(u^n) \rightharpoonup g$ in $L^2(\Omega)$. I also know that $f(u) \in L^1(\Omega)$. I wanted to ask how to prove that $f(u) = g$ a.e. or equivalently that we have weak convergence $f(u^n) \rightharpoonup f(u)$ in $L^2(\Omega)$ or possibly in other space. Using quadrating scaling of $f$ (extra property), I was able to prove that I have strong convergence $f(u^n) \rightarrow f(u)$ in $L^1(\Omega)$, but I'd like to learn if there is a way to prove any weak convergence of $f(u^n)$ to $f(u)$ without relying on additional properties of $f$ and instead relying just on previous info.
Xilexio
Hi,
I'm trying to study the discrete spectrum of a 1D Schrödinger operator on an interval, either by finding it explicitly or by finding asymptotics as the size of the interval goes to infinity. Basically the operator I'm looking at is $-\frac{d}{dx^2}+V$ where the potential $V$ is given by some nice symmetric "single-well" $L^2$ function like for instance $\tanh^2(x)-1$. Operator is acting on $H_2\cap H_1^0(-\frac1\varepsilon,\frac1\varepsilon)$ (acting on functions on that interval with Dirichlet boundary conditions).
upheaval
I know that the discrete spectrum of those operators will "converge" in some sense to the spectrum of the same operator on $H^2(\mathbb R)$, and I can get a basic description of this spectrum as the potential is in $L^2$ (I know that its point spectrum lies in $\mathbb R^-$ and 0 is the only possible accumulation point)
upheaval
but I'm kinda stuck as to how to get estimates on the eigenvalues
(I don't need anything really sharp, just asymptotics of the spectral gap would be enough)
apply semiclassical analysis techniques. For a potential $V(x) = \tanh^2(x) - 1$ and considering the operator on a finite interval with Dirichlet boundary conditions, the asymptotic behavior of the eigenvalues $\lambda_n$ as the interval size tends to infinity can be summarized by the formula:
[
\lambda_n \sim -\left(\frac{n\pi}{\log(\varepsilon^{-1})}\right)^2
]
for large $n$, where $\varepsilon$ characterizes the size of the interval.
aafd
If f is a compactly supported smooth function on R^n then show that its symmetric decreasing rearrangement f* is also a compactly supported smooth function.
anyone have a good reference for derivation of compressible navier stokes?
or i will settle for incompressible
compressibility comes from the equation of state and equation of continuity which relate pressure to temp and density and which relate change in density change to flux of momentum, in the incompressible case you just set the density to a constant parameter
What is the difference between these two definitions of the fractional sobolev space H^s?
f in H^s iff (1+|n|^s)|f^(n)| in L^2
f in H^s iff f in L^2 and (1+|n|^{2s}) f^(n) in L^2
Where are you getting these definitions? The second definition doesn’t have order s, is it missing a square root?
First is from evans pdes
Yeah you forgot a square root in the second one
Since when you take the L^2 norm the first term is squared
You need a square root around the factor (1 + |n|^2s)
Since you’re taking an L^2 norm
Then why doesnt that definition say that
What
Because that definition is phrased in terms of an integral
If you add the square root, yes
Doesnt the sqrt go on the integral though
Write out the integral which defines the L^2 norm of (1 + |n|^2s)f^(n) and compare it to the one in the paper
You said that (1+|n|^2s)f^(n) is in L2, which is not what this says
We’re saying that they’re equivalent if the (1+|n|^2s) term has a square root so that it’s order s
It’s effectively order s
Both are order 2s when squared
You have inequalities like C_1(1 + |x|^s)^2 <= (1 + |x|^2s) <= C_2(1 + |x|^s)^2 which is all you need to show the norms are equivalent
Yeah
The order of that scalar is all that’s important here. In some places, you’ll also see $(1+|\xi|^{2})^{s/2}$ (denoted as $\langle \xi\rangle^s$) instead
Kirby
@sick maple this is a good exercise to verify that they’re equivalent
$(1+|n|^s)\hat u(n)\in L^2 \Leftrightarrow \int (1+|n|^s)^2|\hat u(n)|^2 dn<\infty$
kevinhardy2
and youre saying that
ok
yeah
youre saying that the right side of that is basically $\int(1+|n|^{2s})|\hat u(n)|^2 dn$
?
kevinhardy2
Sure but I’m looking for details
what specific details?
also, the momentum transport equation is just F = ma when you volume integrate both sides
I have a book I read about the derivation in if thats what you want, let me find the amazon link
Yes, for the reasons frank mentioned. I’d recommend you work through why the norms are equivalent
Rudolf
nvm I figured it out
so i've seen how to derive the continuity equation from mass conservation but didnt get how balance of momentum leads to the momentum equation
the book im reading just says its basically the same argument but i dont see how
the (mass) density * the material derivative of the velocity is basically the total time derivative of the momentum density, you replace the dx/dt, dy/dt, dz/dt terms with the velocity components though
on the other side you have the divergence of the stress tensor, which is just the Force density
for a similar reason |n|^{2s}|\hat u(n)|^2 is also equivalent right
how does the red part follow from compactness here?
its not; it follows from the previous bit of the proof
I am out for lunch atm but the estimate should just be from interior approximation, (i.e. the previous part of the proof). the compactness gives you that there are only finitely many of these needed.
ah, i see it now 
If $f\in W^{1,p}(\Omega)\cap C(\overline{\Omega})$ then can we say that $\mu(\operatorname{supp}(f)-{f\ne 0})=0$? Assume $\Omega\subset \mathbb{R}$.
contrapositive
in one dimension, the boundary of an open set has lebesgue measure zero
for $f\in W^{1,p}(\Omega)\cap C(\overline{\Omega})$ with $\Omega\subset\mathbb{R}$
Nats
I think this is false, I think there are open sets whose boundary is a fat cantor set
Yeah, take the complement of a fat cantor set
yeah, it's not always the case that it has zero lebesgue measure, that's true
For open subsets $V \subset\subset U$, the standard elliptic estimate for an order $m$ elliptic operator $L$ looks like
$$
|u|{H^k(V)} \leq \mathrm{const}(|Lu|{H^{k - m}(U)} + |u|_{L^2(U)}).
$$
Is there any way to get such an estimate to hold with $V = U$? Possibly after shrinking the domains?
Frank
I don't have time to elaborate or confirm but I think that if u vanishes on the boundary of U then you can take a bunch of functions u_k that are given by taking u and making it go to 0 on smaller and smaller collars about the boundary of U which limit to u
Ah yes, I think in that case it works
But I think when u doesn’t vanish on the boundary you really can’t get anything :’(
$$ \int_0^1 dx x(2-x) sin( \frac{2m + 1}{2} \pi x) = B_n \int_0^1 dx sin( \frac{2n + 1}{2} \pi x) sin( \frac{2m + 1}{2} \pi x) $$
x17
it'll be zero unless n=m , so just do the right integral for that case to get the normalization constant and divide both sides by it
can i get a hint for showing this ? i tried to think of functions that "blow" up on the boundary like ln(|x|), such that there derivative involves some form of dirac delta to avoid them being in W^1,p, but im not able to see the conclusion, how would i show the trace cant exist, because im basically trying to show any extension of some L^p function wont be L^p on its boundary but i dont see where the issue will arrise.
maybe it has to do with its derivative being badly behaved ? but then again i dont see how the derivative behaving badly implies the function itself is not integrable on boundary after some extension (at least not explicitly)
actually i have a idea, what if in R i take ln(|x|+1/n) which is integrable on (0,1), then the L^1 norm on the boundary is ln(1/n)+ln(1+1/n) while its L^1 norm is finite, so passing to the limit the operator cant be bounded
and i guess in case of W^1,1, what makes sure these things dont happen is the norm of the derivative making the boundary norm "well behave"
if im right 
I think you are overcomplicating things.
Take some continuous compactly supported function f in the half-plane (x,y:x > 0) that is nonzero somewhere on the boundary {x=0}. Then consider the one-parameter family of functions g(x,y;t) := f(tx,y) for t large. What are the restrictions to the boundary? How are the L^p norms of the restriction and g itself related?
Then understand why this example captures the general situation.
(Whilst doing this you should also think about the derivatives of g to understand why it does not violate the actual trace theorem.)
A simple method would be to consider mollifications of the boundary which would have constant Lp(boundary) but vanishing Lp(U)
Even simply, linearly interpolating between 0 and 1 near the boundary of U will also be sufficient
the method I gave above needs no computation with explicit functions at all, you win simply from the jacobian. although it is similar in spirit to the linearly interpolated example.
I wanted to give the mollification example as it works in quite a lot of different situations but then realized the interpolating example would be good for motivation
so if i got this right. denote the half plane by $\Omega$ we have that $$||g||{L^{p}(\Omega)}^{p} = \int{\Omega} |f(tx,y)|^{p}dxdy$$ which goes to 0 as $t \to \infty$ (by for example LDCT) but on the boundary we have $||g||{L^{p}(\partial\Omega)}^{p}= \int{\partial \Omega} |f(0,y)|^{p}dy$ which we can make positive by our choice of $f$, violating continuity of trace if it exists, but the derivative saves us cause then we have $D_{t}g(x,y)=xf(tx,y)$ which also vanishes on the boundary
James Banach
i should say ||g(t)|| to be precise
First part yes. Second part careful, the relevant derivative is in x, not t.
ah, yeah i see the mistake
Also one should not be considering the derivative of g at the boundary. The point is that our example does not have derivatives going to zero in norm in the interior, although the Lp norms of the function themselves do.
so what happens to ||g(t)|| in W^1,p? i cant see why ||grad f||, or even just \D_{x}g would not go to zero, its just integral of tDf(tx,y) but Df(tx,y) still goes to zero as t gets very large
Write down the integral, then do a change of coordinates from tx = u so that a t will pop-out in the integral and that will help you
Hi. I'm trying to look for materials on the following system of two PDEs.
Consider $\Omega = (0,1) \times (0,1)$, and $T > 0$.
[
\begin{cases}
\partial_t u(t, x) = -u(t,x)v(t,x), & 0 < t \leq T, x \in \Omega;\
\partial_t v(t,x) = \Delta v(t,x) - u(t,x)v(t,x), & 0 < t \leq T, x \in
\Omega.
\end{cases}
]
Boundary conditions: $u(t,x) = v(t,x) = 0$ for $0 < t \leq T$ and
all $x \in \partial \Omega$.
Initial conditions: $u(0, x) = u_0(x), v(0, x) = v_0(x)$ for all
$x \in \Omega$. They ($u_0, v_0$) are all non-negative throughout $\Omega$.
The idea is that this is a reaction diffusion equation.
I was looking to understand the kinds of solutions for this equation. It seems intuitive to me that they'll all be bounded. Intuitively, it seems to me that: $0 \leq u \leq u_0$ everywhere, $0 \leq v$ everywhere. It also seems intuitive to me that there is a global upper bound for $v$.
Do you guys know where I can find stuff about these kinds of equations?
phao
I mean websites... books... a chapter on a book, etc.
The laplacian operator $\Delta$ is spacial, meaning: $\Delta v = \partial^2_x v + \partial^2_y v$ in here.
phao
this is literally how my professor gave this homework problem and i feel like an idiot because i can't parse it
this was my best guess but what the heck are v and V here? functions from Rn to R or vector valued functions?
is v grad v a row vector applied a matrix resulting in a row vector?
in GR thats a directional covariant derivative of a vector along itself. If it equals 0, then the integral curve of v would be a geodesic.
$$u^\mu \grad_\mu u^\nu = 0$$
x17
if you assume euclidean geometry (and carteesian coords), the connection goes to zero, and you just have partial derivatives. I would assume thats your case?
$$ (u^1 \partial_1 + u^2 \partial_2+ u^3 \partial_3) u^\nu$$
x17
The usual notation is to write ( v \cdot \nabla v) and is to be interpreted as the matrix (\nabla v) acting on the vector ( v). More precisely, ( (v \cdot \nabla v){i} = \sum_j v^j \partial_j v^i). An important consequence of this that gets routinely used is that if (v) vanishes on the boundary then
[ \langle v \cdot \nabla v, v \rangle{L^2} = \langle v , \tfrac{1}{2} \nabla |v|^2 \rangle_{L^2} = - \tfrac{1}{2} \langle \nabla \cdot v, |v|^2 \rangle_{L^2} = 0
]
cocat
V is some generic function and v is in terms of V. You would wanna plug in the form of v to obtain an equation for V.
i ended up with
$Dp=\frac{V,DV}{(1-t)^{2a+b}}-
a\frac{V}{(1-t)^{a+1}}
-
\frac{bx,D V}{(1-t)^{a+b+1}}$
eigentaylor
but i don't know what i'm supposed to know about p to determine a and b
i always thought "man it's so extra to have to always specify what every single function is a map between" but now i get it. this is so annoying
is p like a function of only x?
if i just say "we need the 1-t exponents to match", then that just gives me b=0 and a=1. which could be the answer but it seems... naive? what do i know though
this is what my classmate got though. ||but their PDE work has been a bit suspect in the past >.>||
For p, take the divergence of the first equation and use the divergence free condition of v
you mean of v D v - D p - v_t? what the heck is the div(vDv) 0_0
Actually, you may not have to solve for p. You just wanna balance out a and b. So use this equation and write one for div v in terms of V and try to balance out a and b using those
so you mean like div(v)=div(V(x/(1-t)^b))/(1-t)^a=0 and work that out?
i'm multivar calc stupid ngl. i never learned advanced multivar calc, which is probably why im so bad at PDEs
Yes, this combined with the one previous should give you two equations in a and b that u can work out provided u did the math correctly.
i don't see how calculating the divergence is going to help though. it seems like i'll just get something like div(V)/(1-t)^(some power)=0 which just tells me div(V) is also zero.
So from here, it tells you that your powers of (1-t) should balance out and so 2a+ b = a+1 implying a+b = 1.
@steel umbra Do you know the continuity equation? it reduces to div(V) = 0 if the density is constant.
not at all
okay so that was on the right track
wait doesn't 2a+b=a+1 also have to be equal to a+b+1 or why does that last term not matter?
x17
The last term doesn't matter because it comes with x as well. So ideally, you would multiply by (1-t)^a+1 the whole equation so that the first two (1-t) disappear and for the last one you have x/(1-t)^b which is precisely the same argument as contained in V. So then you would set y = x/(1-t)^b hoping that there isn't any x or t left in the equation
i'm not following why having an x makes it irrelevant. and are we assuming Dp=0 so that we can multiply everything by (1-t)^whatever?
the time change in density is and the flux of the density through some Gaussian surface is 0. So the total quantity is of whatever rho is, is conserved.
Because you will do the change of variable y = x/(1-t)^b and since your V only depend on y so your hope is that the resulting equation only depends on y and any other contributions (like of t) vanish out (due to cancellation of powers)
We aren't assuming Dp= 0. There is usually a similar self-similar form given for p but they haven't provided it to you. Ideally you would assume that p = P(x/(1-t)^b) 1/(1-t)^c and get a similar condition for c.
oh so basically because we have (x/(1-t)^b)*Dv/(1-t)^(a+1) like the other term
Idk what you mean
$Dp=\frac{V,DV}{(1-t)^{2a+b}}-
a\frac{V}{(1-t)^{a+1}}
-
\paren{\frac{x}{(1-t)^b}}\frac{b,D V}{(1-t)^{a+1}}$
eigentaylor
so if 2a+b=a+1 we can cancel the denominators besides having a y
Yes so the part in the bracket becomes y and the remaining non-y terms shouldn't be present so it becomes an PDE in terms of V which you can solve much easier
i'm still just confused what to do with Dp if we aren't given that form for it
Don't worry about it as they aren't asking you to find what p is. Just give the condition for the powers.
well i get that a+b=1, but it seems like i'm supposed to narrow it down to specific values
but idk where to go from
$(1-t)^{a+1}Dp=V,DV-aV-ybDV$
eigentaylor
You don't have to go anywhere as it would be for solving V and p. They're not asking you to solve V and p. That is highly non trivial
For now, you just need to suggest that a+b = 1 and that's it. This tells you that there is a full family of self-similar solution depending on some parameter. There are a bit more constraints but u won't be able to derive it without difficult analysis.
alright fair enough
For curiosity, check "On self similar solutions to the incompressible Euler equations" section 2
i do have another question. i was doing separation of variables on another problem and got
$\paren{\frac{X'}{X}}^2\paren{\frac{X''}{X}}
+2\paren{\frac{X'}{X}}^2\paren{\frac{Y'}{Y}}^2
+\paren{\frac{Y'}{Y}}^2\paren{\frac{Y''}{Y}}
=0$
but idk what to do with it since i can't actually separate them
eigentaylor
i did suppose exponentials X=e^(ax) and Y=e^(by) and i got (a^2+b^2)^2=0 so that doesn't really help
unless i'm allowed to use u=e^(x+iy) but i dont think so lol
i just need to find a nontrivial solution
original was $u_x^2u_{xx}+2u_xu_yu_{xy}+u_y^2u_{yy}=0$ in $\bR^2$
eigentaylor
@steel umbra Try the separation ansatz u = X(x) + Y(y), I think it'll make the cross term vanish
oh yeah that'll delete the u_xy. so then basically it's
(X')^2 X''=-(Y')^2 Y''=C
nice thanks
or i guess more simply, just a single variable function u=X(x) would work if we just need one solution (since it's symmetric in x and y)
ODEs should be solvable with reduction of order
or wait... that just leads to a trivial solution nvm. i think you need both
i think they're just separable in X' (or Y')
yeah pick A to be 0 for simplicity (we just need one solution)
i got x^(4/3)-y^(4/3) so imma just quickly check that's a solution
any idea on how we got this estimate?
sean
in this form of gronwall
i don't rlly understand how they got this estimate, or how the conditions for gronwall are satisfied
Note that each component of the Jacobian can be bounded by Linfty norm of nabla u, using Gronwall. Since this holds for each component, we can control the full Jacobian via the same bound, atleast up to a constant
They're using the differential form of Gronwall here, look up the statement on Wikipedia, or differentiate the assumption.
Btw the book is pretty good, stick with it even though it might get overwhelming with the huge emphasis on Fourier
ohh i see i get it now
ah alright thanks for the advice
i have a month to read the first chapter for a research project and its alright so far
wait just to make sure, the L infinity norm is this right
im not used to working w vector fields compared to scalar fields so
is this equivalent to the operator norm?
No
Operator norm is the largest singular value of A^TA I think this is something else
Yes, if you choose the maximum norm in the input and output space
if $U$ is bounded and $\partial U$ is $C^1$, is $f=1$ necessarily in $L^1(\partial U)$?
minitarrasque
(equivalently, does the boundary have finite arclength?)
are functions which are equal weakly necessarily also equal a.e.?
(on sufficiently nice domains, if necessary)
oh wait of course yes
since int (f-g) phi = 0 for all phi in C_c^infty
so f=g
Has anyone heard of a linear hamiltonian system?
If $U$ is bounded then isn't its boundary compact?
Casey
I don't think so, the function needs to be of bounded variation
consider a circle with a lot of oscilations
like a lot
the perimeter goes to infinity
but it bounds a domain
casey didn't say anything about finite length, merely that the boundary is compact. this is true (it is closed and bounded in R^n).
and in the original question, C^1 regularity of the boundary was assumed, which rules out the behaviour you mention.
it would be compact in R^n but not necessarily as a R^{n-1} manifold i think
Guys i have some questions with pde
u_t = u_xx + 1
can i ansatz that u = X(x)T(t) and find some solutions for u_t - u_xx = 0
and then find the fouriers series that is equal to 1 and them compare them?
thanks
Though... you could also use method of characteristics if you want. The characteristic equation would be:
$$ A_{\mu \nu } \frac{\partial \phi}{\partial x^\mu} \frac{\partial \phi}{\partial x^\nu} = 0 $$ where $$ A_{xx} = 1 $$ and all other components are 0
x17
so basically $$ \phi(x, t) = c $$
x17
green function is for x \in [0,1] right?
i am looking for the (0,1)
you need boundary conditions to evaluate the greens function if thats what you are asking
you need them to propagate values along the characteristics too
so method of characteristic is my best friend here?
more information on the problem is your best friend
I just mean you need boundary conditions, and defining boundary conditions on an open boundary is... not something Ive done, except in the asymptotic case
u(0,t)=u(1,t)=0 and u(x,0)= some fucntion
right, but 0 and 1 are not part of the solution
i was thinking as a diffusion equation,
with 1 constant
I guess you would use right and left limits for the conditions in that case?
was thinking you can use fourier to find a interval from 0 to 1
independent of any method, you still need to specify the boundary conditions. I guess like I said, you could use 1-way limits
thanks for the help. i am just realizing now im bad at maths.
(0,1) is an open interval, 0 and 1 are excluded from it
so saying u(0,t) or u(1,t) does not make sense, they arent in the the domain
maybe $$ lim_{h \rightarrow 0-} u(h,t) = 0 $$
x17
isnt the equation saying the partial u/ partial x (which is temperature gradient) is equal to the uxx + 1
okay, if you can assume its closed then your BC are fine
can i use for example uxx + uyy = delta u for divergence u or something
im going way off topic here my bad
the greens function would come from:
$$ (\frac{\partial }{\partial t} - \frac{\partial^2}{\partial x^2} ) G = \delta(x, x', t, t') $$
x17
I'll leave it as a research task to figure out how to solve that, there are plenty of online resources, and explaining it on discord would be messy
basically you split the solution in parts and make them agree where the delta spike is
thanks i will look into it more
Is there a way to solve an equation of the form $$a(t,x) \partial_t u + \partial_x(a^2 u) = 0,?$$
afqt
If a only depended on t or x, I guess it'd just be a case of method of characteristics
Does it not?
Looks like characteristics to me. A particularly simple version too, because this is just a linear transport equation.
you need to write it in a different form like: $$ a\partial_t u + \partial_x(a^2)u + a^2 \partial_x u = 0$$
x17
Yeah, I figured it out. We get something like $\frac{du}{u} = - 2 \partial_x a$ along the characteristic
afqt
Thanks
Yeah I was kinda obsessing with keeping a^2 u together instead of taking the \partial_x a term as a source
Basic question about Sobolev spaces:
I am reading about the fundamental solutions to the $p$-Laplace, which are constituted by $ |x|^{ \frac {p-n}{p-1} } $ where $n$ is the dimension of the ambient $\mathbb{R}^n$. I've read that it does not belong to $W^{1,p} (\Omega)$ when $\Omega$ contains the origin. In order for the fundamental solution to be defined at the origin we need $p > n$. By asking for $n \geq 2$, the fundamental solution gets a cusp at the origin.
How can one prove that it is not weakly differentiable at the origin? I tried my hand at a wee simpler example to try to grasp functions endowed with a cusp, like the one-dimensional $f(x) = \sqrt{|x|}$ for $x \in (-1,1)$, which certainly has a cusp at the origin. The absolute value $|x|$ is weakly differentiable at the origin surely, but it seems like $|x|^\lambda$ for $0 < \lambda < 1$ is not.
Anyway, weak differentiability of the fundamental solution would mean there is $f' \in L^p (-1,1)$ such that for each $\phi \in C^\infty_0 (-1,1)$ we have
[
\int_{(-1,1)} \sqrt{|x|} \phi ' (x) dx = - \int_{(-1,1)} f'(x) \phi (x) dx
]
I suppose one can assume that it is, and try to derive a contradiction by appropriately choosing a sequence of test functions and subsequently performing an appropriate limiting procedure. But I have not been successful with this
hardisc.
one possible way forward is to try to find its distributional derivative and show its not L^1_loc (typically by a dirac delta showing somewhere)
Isn't $f'(x)=\frac{\mathrm{sgn}(x)}{2\sqrt{|x|}}\in L^1(-1,1)$ a perfectly good weak-derivative for your function $f(x)=\sqrt{|x|}$?
4453
It should be negative exponents when things start to go bad.
(at least when one demands weak derivatives in L1, and is working in 1d)
When things are genuinely bad, a simple way you can show the distributional derivative is not in L^p_loc for whatever p you like is just to calculate the actual derivative as a smooth function away from 0, and test the integrability of the p-th power of this. For radial things like in your question, polar coordinates will be very fast.
Does anyone know where I can find information on convolution of a given function with a Hankel function of first kind ?
ah very nice, seems so! i guess it was simpler than i thought, thank you!
yes seems so, but in that case the function is not even defined at the origin, so it does not even possess a strong derivative, whence the question is moot, no?
What is the relevance of the existence of strong derivatives to your original question? A function does not need to be defined everywhere (we typically are working in L^p spaces if not distributionally, so pointwise evaluation does not even make sense) or have strong derivatives to talk about weak derivatives.
In fact even the sqrt function discussed above doesn't have a strong derivative at 0.
sure, but sqrt(|x|) is defined at $x = 0$, whereas $ |x|^\lambda$ for negative $\lambda$ is not defined at $x = 0$.
that was what i meant
hardisc.
yeah but we are talking about taking weak derivatives of some L^p_loc function, also living in some L^p_loc space. such things are not sensitive to individual points. E.g. the function f(x)=1/sqrt(|x|) is a perfectly good definition of a function in L^1(-1,1). Set its value at 0 to be whatever you like, this does not change it as an L^1 representative.
right my bad, the origin has lebesgue measure zero, and thus invisible in integration
and it still makes sense to ask if it has a weak derivative also in L^1, and indeed it doesn't
roughly because the obvious candidate will blow up like 1/|x|^(3/2) about 0, and thus fail to be integrable.
ah, right! i think it is much clearer now, thank you very much
no problem
assume u: Rⁿ → Rᵐ
often in PDEs we do a change of coordinates (diffeomorphism) in the domain to simplify the equations. For instance instead of u(x) we look at u(Φ(x))
but how about in the codomain, like looking at Φ(u(x)) instead
this seems to be very rarely done for PDEs because it often messes up the equation form. But it is done all the time in ODEs. Nevertheless, in which PDEs have you seen people "change the codomain" ? The ϕ I have in mind is the diffeomorphism between the open ball and Rⁿ.
Well, Fourier transform is a major example of this. And it appears a lot in PDEs, especially for dispersive and Navier-Stokes
But yes, not a diffeomorphism
yeah it seems like a rare operation in PDEs even though ODEs use it a lot
in this comment on the proof Evans has of the Lax-Milgram theorem, why is this true? Wouldn't we need to show that H is complete under the induced norm?
because you can prove the norms are comparable up to a constant
Not really. We don't argue via an induced norm. We just define a mapping A : B[u,v] = (Au,v) where A is well-defined due to boundedness of B and thus Riesz.
Moreover, A has closed dense range and injective due to coercivity of B.
As such, A is bijective so you're done.
Where is symmetry used here
Also "closed dense range"? That's just... full?
I am guessing you used symmetry to turn injectivity into dense range.
And then the linear map is bounded below so the range is closed?
If that's the argument, that works too, though I doubt that's what Evans intended. Since he mentioned Riesz with symmetry specifically and your argument didn't need symmetry for Riesz.
this is the argument he gave for proving the lax-milgram theorem, but this corollary afterwards i think is not supposed to use that route, i think it is trying to argue "call H' = H but with the new inner product ((u,v)), then by RRT since (f,.) is a bounded linear operator, there exists u such that ((u,v))=(f,v) and we're done"
but this only works if H' is actually a Hilbert space
i.e. it needs to be complete
but I think Delerik's argument works for this
Yep equivalent norms give the same topology. This is a fact so basic that in diff geo people only bother to define norms on tensor fields up to equivalent norms.
hey
hi?
sorry to bother you but can you maybe help me with a question that i wrote it in "real-complex-analysis", if you have a bit time im going to freak out
oh i litearlly just did it now thx anyway
Without symmetry, why should B be an inner product? This is needed for Riesz.
are you asking about my method or cocat
mine just uses symmetry -> inner product + riesz
cocat is bilinear form -> linear operator A via Riesz
The coercivity automatically implied closed range and injectivity. For density, pick v such that (Au,v) =0 for all u in H. Then v is 0 again by coercivity, (using the characterisation that a subspace is dense if any functional vanishing over it vanishes everywhere)
I think they just forgot to state they were using symmetry at that point. It doesn't make sense to invoke Riesz without having this.
Yes the point is that if you had symmetry then it's a trivial consequence of Riesz but since you don't have symmetry, it's remarkable that we still get the same resukt out.
I think the person was asking about why the so-called "trivial consequence of Riesz" holds
(not about lax-milgram without symmetry)
Ohh, I see. I thought they needed help in understanding the italicized statement. Then yes, equivalence of norms provided symmetry.
This is from the Lieb & loss Analysis book. They deduced $\chi_D = R_{\theta}\chi_D$ a.e. for all $\theta$.
From this they are saying that $D=F^$ , I didn't understand how they are getting $D=F^$. Can anyone please help
souravghosh0465
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I have sort of an open ended question here so bare with me.
L1(z(x,y)) = 0. Which I know exact solutions for(an infinite, orthogonal family), and Where L1 is a second order differential operator with variable coefficients.
Now say I am looking at the following pde.
L1(z) + L2(z) = 0, where L1 is the same linear operator as before, but L2 is a new operator defined in the following way.
Say I take my original equation L1(z) = 0 and coordinate transform it by the substitution x -> x+y and y->x-y. The resulting operator you get in this new equation is exactly L2.
So in essence, the equation (L1 + L2)z = 0 is sort of like L1 plus its rotated version by 45 degrees(with a small scaling factor).
An example of this time of equation would be zxx - zxy + zyy = 0, with L1z = zxx - zyy .
Is there any more general procedure to sort of tackle this problem (L1 + L2)z = 0 when I exactly know how to solve the easy case? Or even say something about possible solutions
@pine oriole any good reference on what’s going on in “parabolic” situations?
Hello,
Let $L$ be a sectorial operator, with a bounded inverse. then $D(A^\alpha)=[X, D(A)]\alpha$, where $X$ is a Hilbert space and $[X, D(A)]\alpha$ is the complex interpolation space between $X$ and $D(A)$
Anyone knows where I can find more details and the proof please?
Mikahopff
You can find this in One Parameter Semigroups for Linear Evolution Equations Chapter II.5
that's just the heat equation
any PDE book will teach you first elliptic (Laplacian) then parabolic (heat equation)
heat semigroup is born for such
I see
Hello,
Are injective sectorial operators invertible?
I know they have dense range but I am not sure if this can be used to derive the boundedness of the inverse ??
I have the PDE that becomes:
[\hat{u}(\xi,t)=\hat{f}(\xi)e^{-k\xi^4t},]
after taking Fourier transforms. I want to prove the inequality:
[ \lvert\lvert u(x,t)\rvert\rvert^2_{L^2(\mathbb{R})}\le \frac{\int_{\mathbb{R}}e^{-x^4}dx}{\sqrt[4]{2kt}}\lvert\lvert f(x)\rvert\rvert_{L^2(\mathbb{R)}}^2]
So I start with the LHS, I use plancherels theorem (ie. L2 is preserved under Fourier).
My next step is writing the norms in the integral definition. The problem is then splitting the integral into a product:
[\left(\int_\mathbb{R}\lvert \hat{f}(\xi)e^{-k\xi^4 t}\rvert^2d\xi\right)^2,]
then using inverse Fourier transforms to get to the result. Cauchy schwarz was my first idea but I get too high power inside the integral and too small of a power outside.
Max
