Conversation started Jun 30, 2019 at 0:54.
Jun 30, 2019 00:54
can someone explain to me the Laplace-Beltrami operator and why its spectrum is that important? Apparantly the Selberg trace formula is important for NT, but I never worked with the spectrum of a differential operator before
@Mathein: It starts with hearing the shape of a vibrating drum :)
@MatheinBoulomenos you can hear the euler characteristic of a closed surface
Sounds like a "kill your father" thing.
cleans out his ears
holds a plate to his ear and hears "... 1 1 1 1 1 1 1 1 1 1 ..."
Darn it's not closed.
emits a final cry before being devoured by geometers.
Jun 30, 2019 00:58
I think the same is only true when you have a boundary if you know that the boundary is totally geodesic
Hmmm, this sounds like a good thing for you to teach us, @Ryan.
@TedShifrin are you fond of Eliashberg?
right so the basic result is that on a surface $$\sum_{j=0}^\infty e^{-\lambda_jt}=\frac{V(M^2,g)}{4\pi t}+\frac{\chi(M)}{6}+O(t)$$
I don't know him personally, nor most of his work.
to no-one's surprise, the chi appears because of Gauss-Bonnet
Jun 30, 2019 01:01
what is $V(M^2,g)$?
volume
This sounds like classic heat equation stuff for Gauss-Bonnet.
yes the thing on the left is the trace of the heat kernel
@Mathein: $g$ is the metric and your Laplace-Beltrami is defined dependent upon $g$.
@MatheinBoulomenos do you know what the heat kernel is
Jun 30, 2019 01:03
it's the kernel of the heat operator
no, I have no idea
kernel ≠ kernel
equality is't reflexive anymore?
ok you probably know functional analysis so if we want to solve some abstract problem like $x'(t)=Ax(t)$ where $x(t)$ is a curve in some Banach space and $A$ is a linear operator then we can write $x(t)=e^{At}x_0$, where $x_0$ is the "initial condition"
yeah I know functional analysis
LOL, that's freshman linear algebra :P
Jun 30, 2019 01:05
to make this rigorous you need some conditions on $A$ of course
@TedShifrin tbh never learned this in linear algebra
so we want to study the solutions of $(\partial_t-\Delta)u=0$ (heat equation) on a Riemannian manifold
I had to read it in Hirsch & Smale
I might call such a $u$ a caloric function
should have been in our ODE course, but it is a WASTE.
Jun 30, 2019 01:06
I taught it my linear algebra courses and, of course, it's in my books, @anakhro.
so we want to solve this for $u(x,t)$ where $(x,t)\in M\times[0,\infty)$ and $\Delta$ is taken wrt a fixed metric $g$ on $M$
and we have some initial condition $u_0\in C^\infty(M)$, which means we want $u(\cdot,0)=u_0$
@TedShifrin one day I will be like you and write a book I can reference.
I hope so, @anakhro.
See Anakhro [2].
now using the functional calculus we can write $u(t)=e^{t\Delta}u_0$
Jun 30, 2019 01:08
Now, that's more obnoxious than necessary :D
this can be made rigorous because $\Delta$ is essentially self-adjoint on $C^\infty(M)$
the "heat kernel" is the operator $e^{t\Delta}$
notes that Ryan is doing a splendid job so far
5
I was expecting a fundamental solution type of kernel, @Ryan.
i was going to write an integral kernel in a second
now $e^{t\Delta}:L^2\to L^2$ is actually a trace-class operator for $t>0$
and we have the nice formula $$\mathrm{tr}\,e^{t\Delta}=\sum_{j=0}^\infty e^{-t\lambda_j}$$
now the problem is that actually computing the RHS is kind of impossible from what I just said, so we have to consider another representation of the heat kernel
To fix notation let $\{\phi_j,\lambda_j\}_{j=0}^\infty$ be the spectral resolution for the Laplacian (on a closed Riemannian manifold)
this means that $\Delta \phi_j+\lambda_j\phi_j=0$, $\phi_j\in C^\infty$, $\{\phi_j\}$ is an orthonormal basis for $L^2$, and $0=\lambda_0<\lambda_1\le \lambda_2\le\cdots\to \infty$
this means that $\phi_j$ are eigenvectors and $\lambda_j$ are eigenvalues, right?
sniped
@TedShifrin If you're familiar with quantum mechanics you'll see that I've taken the following from my QM course
we have the identity $$\sum_{j=0}^\infty\phi_j\otimes \phi_j=id_{L^2}$$
the tensor means the following: if $f,g,h\in L^2$, then $$(f\otimes g)h=(g,h)_{L^2}f$$
Jun 30, 2019 01:17
(using $L^2 \cong (L^2)^*$?)
oh yeah
yeah, I assumed as much
this all works for a Laplacian on a complex vector bundle in which case one needs to add some transposes and whatnot
here it's simple
ok so we take $u(t)=e^{t\Delta}u_0$ and expand $u_0=\sum a_j\phi_j$
now we can just compute that $e^{t\Delta}\phi_j=e^{-\lambda_jt}\phi_j$
so by "linearity" (this part needs to be checked), $u(t)=\sum e^{-\lambda_jt}a_j\phi_j$
but we can rewrite this as $u(t)=(\sum_{j}e^{-\lambda_jt}\phi_j\otimes\phi_j)u_0$
so, at least formally, $e^{t\Delta}=\sum e^{-\lambda_jt}\phi_j\otimes \phi_j$
good so far?
yeah, I'm following
thanks a lot for the great exposition
Let's go back to the tensor product. With everything written out we have $$(f\otimes g)h(x)=\int_M f(x)g(y)h(y)\,dy$$
so we can represent the tensor product of two functions as an integral operator
so the key to bringing PDE back into the fold is writing: $$u(x,t)=e^{t\Delta}u_0(x)=\int_MH(x,y,t)u_0(y)\,dy$$
where $$H(x,y,t)=\sum_{j=0}^\infty e^{-\lambda_jt}\phi_j(x)\phi_j(y)$$
Jun 30, 2019 01:27
So is $H(x,y,t)$ the heat kernel?
yeah
it turns out that $H$ is smooth on $M\times M\times (0,\infty)$
and it blows up along the diagonal as $t\searrow 0$
so on R^n we can actually write down the heat kernel explicitly
I know that's not a compact manifold but the same ideas work
The answer is $$e(x,y,t)=(4\pi t)^{-n/2}e^{-|x-y|^2/4t}$$
And that's the classic fundamental solution.
If you compute Laplacian of that, you get $\delta_y$.
right so this thing satisfies $$(\partial_t-\Delta_x)e(x,y,t)=\delta_y(x)$$
So ... think convolution and what Ryan's been doing.
where $\delta_y$ is the Dirac mass at $y$
Jun 30, 2019 01:31
this is a weak derivative, right?
er sorry that's slightly wrong
it satisfies the heat equation, i.e. $(\partial_t-\Delta_x)e(x,y,t)$ for $t>0$
and $e(\cdot,y,t)\to \delta_y$ as $t\searrow 0$
in various senses, let's keeps this informal haha
You're doing great.
Jun 30, 2019 01:34
Ted and I both mixed this up with the Laplace equation
well, not with $t$ in there :P
@MatheinBoulomenos So the derivatives here are classical ones
Yeah, when I said "compute Laplacian" I was an idiot.
$e$ is a smooth function for $t>0$
ok so the story continues with Minakshisundaram and Pleijel
Wow ... what a name to have to type!
Jun 30, 2019 01:36
I think I did it correctly
I don't know it/him/her.
They asked to what extent does $H(x,y,t)$ look like $e(x,y,t)$ as $x\to y$ and $t\searrow 0$
Recall that on a Riemannian manifold we have a distance function $d$. So we consider the "naive heat kernel" $$\mathcal E(x,y,t)=(4\pi t)^{-n/2}e^{-d(x,y)^2/4t}$$
their idea is that we should be able to add correction terms to this and obtain the real heat kernel
since this thing obviously is like $e$ for short distances and times, and if the correction terms are small, then $H$ looks like $e$ too
it turns out the right thing to look at is $$H_k(x,y,t)=\mathcal E(x,y,t)\sum_{j=0}^kt^ju_j(x,y)$$
and we want to compute $u_j$ so that they satisfy $$(\partial_t-\Delta_x)H_k=-\mathcal Et^k\Delta_x u_k$$
I don't have a great reason for why this equation, but it works out in the end
This looks like classic perturbation theory, I guess.
it's definitely motivated by that
there's probably rules for doing this stuff for ODEs and just just made it work in this setting
so you can compute the $u_j$'s from this, at least in principle.
it gives a recursion relation and you start with $u_0= 0$ on the diagonal
this turns out to be enough to determine all the others, but actually computing them is very hard
it involves the metric determinant in polar coordinates in a neighborhood of the diagonal, kind of nasty
now what is particularly interesting are the numbers $$a_j=\int u_j(x,x)\,dx$$
because these give the coefficients in the $t$-expansion of $$\mathrm{tr}\,e^{t\Delta}=\int H(x,x,t)\,dx$$
it turns out that $u_1(x,x)=R(x)/6$, where $R$ is the scalar curvature
so by the Gauss--Bonnet formula, $$a_1=\frac 46\pi\chi$$ when $n=2$
I hate to leave in the middle of this lecture, but I have to cook dinner. I'll catch up later :) Thanks, Ryan.
Jun 30, 2019 01:49
cheers
it's basically done anyway
one can show that for $k$ sufficiently large, $H_k$ approximates $H$ very well and we have $$\sum e^{-\lambda_jt}=(4\pi t)^{-n/2}\left(\sum_{j=0}^k t^j\int u_j(x,x)\,dx\right)+O(t^\alpha),$$
where $\alpha$ is some power
I actually wanted $u_0(x,x)=1$ haha
so the first term gives the volume, always
and when $n=2$ you get the Euler characteristic in the second term
wow, really cool
thanks a lot
np
@BalarkaSen there might be something interesting to you above
the heat kernel is one of the main tools in geometric analysis
the relationship to the Poincare conjecture is particularly mysterious
 
Conversation ended Jun 30, 2019 at 1:57.