Determine the function from a simple condition on its Jacobian matrix.

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Discussion Overview

The discussion revolves around determining a function from a condition imposed on its Jacobian matrix, specifically in the context of isometries in Minkowski spacetime. Participants explore the implications of the Jacobian condition and its relation to the structure of isometries, touching on concepts from differential geometry and the properties of pseudo-Riemannian manifolds.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant proposes that the condition on the Jacobian matrix implies the existence of a linear function and a constant vector, suggesting a form for the function in terms of affine transformations.
  • Another participant introduces the concept of viewing the problem through the lens of pseudo-Riemannian manifolds and the exponential map, arguing that the function behaves as an isometry.
  • A later reply expresses uncertainty about the exponential map and its application, indicating a need to refresh knowledge on the topic.
  • One participant suggests an alternative approach by analyzing the Killing vector fields of Minkowski spacetime, proposing that this could lead to a proof of the isometry group being the Poincaré group.
  • Another participant questions the assumptions necessary for applying certain theorems related to the exponential map, particularly in the context of Lie groups.
  • One participant expresses a preference for a more straightforward approach that minimizes the need for advanced differential geometry knowledge, while also reflecting on their past experiences with similar proofs.

Areas of Agreement / Disagreement

Participants present multiple competing views on how to approach the problem, with no consensus reached on a single method or solution. There is ongoing debate regarding the relevance and application of differential geometry concepts versus more elementary approaches.

Contextual Notes

Some participants note limitations in their understanding of certain concepts, such as the exponential map and Killing vector fields, which may affect their arguments. There are also discussions about the assumptions required for applying specific theorems, indicating a potential gap in the foundational knowledge necessary for the proofs being considered.

  • #31
With some assumptions the inverse \phi^{-1} can be assumed differentiable too. Then

<br /> (\nabla\phi)^T(\nabla\phi)=\textrm{id}<br />

will imply

<br /> \textrm{id} = (\nabla\phi^{-1})^T(\nabla\phi^{-1})<br />

I think the necessary pieces of puzzle are starting to be around now...
 
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  • #32
jostpuur said:
This condition seems to imply

<br /> \|\phi(x)-\phi(y)\|\leq \|x-y\|<br />

for all x,y.

In proof of this I used a triangle inequality that will not hold in Minkowski space. Damned thing...

Anyway, I would like to point out that the proof that micromass wrote in Hilbert spaces will also work in Minkowski type spaces. Assume that \eta is some N\times N symmetric matrix such that zero is not its eigenvalue (but the eigenvalues can be both positive and negative). If \phi:\mathbb{R}^N\to\mathbb{R}^N is a bijection that satisfies

<br /> \big(\phi(x)-\phi(y)\big)^T\eta \big(\phi(x)-\phi(y)\big) = (x-y)^T\eta (x-y),<br />

then the \phi will be an affine mapping \phi(x)=Ax+a. At least I didn't see anything that wouldn't work in these steps when they are modified: https://www.physicsforums.com/showpost.php?p=4417877&postcount=4
 
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  • #33
jostpuur said:
Continuity of the derivative should be enough to imply the approximation

<br /> \|\phi(x)-\phi(y)\|^2 = \|x-y\|^2 + o(\|x-y\|^2)<br />

in the limit \|x-y\|\to 0. Perhaps this infinitesimal isometry property can be extended some how.

I was doing things complicatedly here. The continuity of derivative is not needed. The result also generalizes.

Assume that \eta is some N\times N symmetric matrix. If \phi:\mathbb{R}^N\to\mathbb{R}^N is a differentiable mapping such that

<br /> (\nabla\phi(x))^T\eta (\nabla\phi(x)) = \eta<br />

for all x\in\mathbb{R}^N, then

<br /> \big(\phi(x)-\phi(y)\big)^T\eta\big(\phi(x)-\phi(y)\big) = (x-y)^T\eta (x-y) + o(\|x-y\|^2)<br />

in the limit \|x-y\|\to 0 (can be the Euclidian norm here, but it shouldn't matter). (To be rigorous, I think the limit must be interpreted so that other one of the parameters is constant in the limit.)

So the final critical gap is that how do you extend the infinitesimal isometry property to the whole space? That's something I didn't get yet.
 
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  • #34
Fredrik said:
Maybe I should have mentioned what I'm really trying to do. I want to prove rigorously that the isometry group of Minkowski spacetime (defined as ##\mathbb R^4## with the Minkowski metric) is the Poincaré group, defined as the set of all affine maps ##x\mapsto \Lambda x+a## such that ##\Lambda^T\eta\Lambda=\eta##.

So this problem became solved in the other Mazur-Ulamn thread.

But this discussion also introduced a new problem which is that if the mapping has an infinitesimal isometry property, then the isometry property extends to finite regions and possibly the whole space. Did this become solved too? I didn't understand how it happened.

The problem I asked about came up after I proved that ##\phi## is an isometry if and only if its Jacobian ##J_\phi(x)## satisfies ##J_\phi(x)^T\eta J_\phi(x)=\eta## for all x.

This sounds like the precise problem I got stuck with. Are you sure you accomplished this?
 
  • #35
jostpuur said:
Are you sure you accomplished this?
Yes, but keep in mind that I was talking about isometries in the sense of differential geometry, not in the sense of normed vector spaces. I included the proof in post #21.

jostpuur said:
So this problem became solved in the other Mazur-Ulamn thread.
Unfortunately no. Micromass' suggestion to use spacetime's exponential map is still the most promising approach. I haven't verified the details yet. I still don't even know how to define the exponential map of a Lorentzian manifold like Minkowski spacetime.

The technique that micromass suggested for Hilbert spaces works for Minkowski spacetime as well. It can be used to prove things like this: If ##\Lambda:\mathbb R^4\to\mathbb R^4## is a surjective map such that ##g(\Lambda(x),\Lambda(y))=g(x,y)## for all ##x,y\in\mathbb R^4##, then ##\Lambda## is linear and its matrix representation with respect to the standard basis satisfies ##\Lambda^T\eta\Lambda=\eta##. But that's not the problem I was having difficulties with.

If I could prove that "##\phi## is an isometry" implies something like the assumption in the theorem I just stated, then I'm pretty much done. Unfortunately all I was able to prove by using the definitions in a straightforward way was that the Jacobian satisfies a condition like the one I want the function itself to satisfy.

jostpuur said:
But this discussion also introduced a new problem which is that if the mapping has an infinitesimal isometry property, then the isometry property extends to finite regions and possibly the whole space. Did this become solved too? I didn't understand how it happened.
I don't understand what you're referring to here, or what an infinitesimal isometry property is. Hm, "infinitesimal" often refers to things related to the tangent space. So maybe you meant something like an isometry in the sense of normed vector spaces, i.e. a condition like ##g(\Lambda(x)-\Lambda(y),\Lambda(x)-\Lambda(y))=g(x-y,x-y)##? The problem I asked about in #1 doesn't start with a condition like that. It starts with the condition that ##\phi:\mathbb R^4\to\mathbb R^4## is such that ##\phi^*g=g##, where ##\phi^*## denotes the pullback map. It's defined by ##\phi^*g_{\phi(p)}(u,v)=g_p(\phi_*u,\phi_*v)##, where ##\phi_*## is the pushforward map, defined by ##\phi_*v(f)=v(f\circ\phi)##. I'm using all these definitions in post #21.
 
  • #36
Here's a summary of what I know and don't know. I assume that \eta is some N\times N symmetric matrix, which does not have zero as its eigenvalue. The mapping \phi always means some mapping \mathbb{R}^N\to\mathbb{R}^N.

Definition: The mapping \phi has a property AFF if it can be written in form \phi(x)=Ax+a with some matrix A and a vector a, and also
<br /> A^T\eta A = \eta.<br />

Definition: The mapping \phi has a property ISO if it satisfies
<br /> \big(\phi(x)-\phi(y)\big)^T\eta \big(\phi(x)-\phi(y)\big) = (x-y)^T\eta (x-y)<br />
for all x,y.

Definition: The mapping \phi has a property INF if it satisfies
<br /> \big(\phi(x+h)-\phi(x)\big)^T \eta\big(\phi(x+h)-\phi(x)\big) = h^T\eta h+o(\|h\|^2)<br />
in the limit h\to 0 for all x.

Definition: The mapping \phi has a property PDE if it satisfies
<br /> \big(\nabla\phi(x)\big)^T\eta\big(\nabla\phi(x)\big) = \eta<br />
for all x.

I know that AFF\LongleftrightarrowISO.

I know that INF\LongleftrightarrowPDE.

Also ISO\LongrightarrowINF is obvious.

So to summarise, we have \Big(AFF\LongleftrightarrowISO\Big)\underset{!}{\Longrightarrow}\Big(INF\LongleftrightarrowPDE\Big).

The final mystery to me is that how to replace the arrow marked with exclamation marks into an equivalent symbol, pointing in both directions.
 
  • #37
So there was some confusion about the precise meaning of isometry. But I guess we are still wondering the same problem.

Let \Omega\subset\mathbb{R}^2 be some bounded open set containing the origin.

Suppose \mathcal{L}_0 is a collection of lines such that none of the lines in this collection intersect each other in \Omega, and also for every point x\in\Omega, there exists some line going through it.

In other words L_1,L_2\in\mathcal{L}_0, L_1\neq L_2 implies L_1\cap L_2\cap \Omega = \emptyset, and \forall x\in\Omega\;\exists L\in\mathcal{L}_0 such that x\in L.

First question. Are all lines in \mathcal{L}_0 parallel to each other neccessarily? The answer is no. For example, the lines could be of the form \{(R-t\cos(\theta),t\sin(\theta))\;|\;t\in\mathbb{R}\} with some constants R (large) and \theta. The lines intersect in point (R,0), but it is outside \Omega.

Suppose \mathcal{L}_1 is collection of curves such that for every point in \Omega there exists a curve in \mathcal{L}_1 such that the curve goes through the point, and also that the curves do not intersect each other inside \Omega. Also let's assume that when a curve of \mathcal{L}_1 intersects a line of \mathcal{L}_0 the intersection is always perpendicular.

Continuing the previous example, the curves of \mathcal{L}_1 would need to be of the form \{(R-t\cos(\theta),t\sin(\theta))\;|\;\theta\in\mathbb{R}\} with some constants t. So inside \Omega these curves are pieces of circles, with center in (R,0).

Final piece: Let's insist, that the curves of \mathcal{L}_1 must be straight lines too. Is it now necessary, that lines in \mathcal{L}_0 are parallel to each other, and also lines in \mathcal{L}_1 are parallel to each other? I think the answer is yes. But how do you prove this?
 

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