Power Series for Volume of Balls in Riemannian Manifold

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Discussion Overview

The discussion revolves around finding the power series expansion for the volume of a ball of radius r centered at a point p in a Riemannian manifold of dimension n. Participants explore the mathematical formulation and calculations involved, particularly focusing on the first two non-zero terms of the expansion.

Discussion Character

  • Technical explanation
  • Mathematical reasoning
  • Debate/contested

Main Points Raised

  • One participant presents the integral formula for the volume of the ball and notes that the constant term is zero, suggesting the need to find the first two non-zero terms.
  • Another participant asserts that the differential of the exponential map at zero is the identity, leading to a determinant of one for the first non-zero term, and mentions the integration over the surface area of a sphere.
  • A different participant proposes that the derivative of the exponential map at a point may relate to the Ricci curvature, suggesting that integrating this over the ball could yield the scalar curvature.
  • One participant references external material, specifically Wikipedia, to find relevant formulas regarding the Taylor expansion of the volume element in geodesic normal coordinates, indicating a potential source for further insights.

Areas of Agreement / Disagreement

Participants express differing views on the nature of the second term in the expansion and the role of curvature, indicating that multiple competing perspectives remain unresolved.

Contextual Notes

Participants acknowledge the complexity of differentiating the determinant of the differential of the exponential map and the potential influence of curvature on the second term, but do not resolve these mathematical challenges.

tornado28
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I'm trying to work out the following problem: Find the first two terms of the power series expansion for the volume of a ball of radius r centered at p in a Riemannian Manifold, M with dimension n. We are given that

Vol(B_r(p)) = \int_S \int_0^r \det(d(exp_p)_{tv})t^{n-1}\mathrm{d}t \mathrm{d}v

(I'm ignoring the cut locus distance because we are only interested in small r anyway.) I assume that S = S^{n-1} = \{v \in T_pM : |v| = 1 \}. Clearly the constant term is 0, because a ball of radius 0 has no area in any manifold, so I think that they are really asking for the first two non-zero terms. To find the next term we need to calculate the derivative of Vol(B_r(p)) wrt r.

\frac{\mathrm{d}}{\mathrm{d}r} Vol(B_r(p)) =<br /> \frac{\mathrm{d}}{\mathrm{d}r}\int_S \int_0^r \det(d(exp_p)_{tv})t^{n-1}\mathrm{d}t \mathrm{d}v = \int_S \frac{\mathrm{d}}{\mathrm{d}r} \left(\int_0^r \det(d(exp_p)_{tv})t^{n-1}\mathrm{d}t\right) \mathrm{d}v = \int_S \det(d(exp_p)_{rv})r^{n-1} \mathrm{d}v

I can pass the derivative under the integral sign because S is compact and the inner integral is a continuous function of v. (Right?) So the second term is 0 also, unless n=1. Here's where I run into trouble. I'm not sure how to differentiate \det(\mathrm{d}(exp_p)_{rv}). I do know that \mathrm{d}(exp_p)_{tv} \cdot tw = J(t) where J(t) is the Jacobi Field along \gamma_v defined by J(0)=0 and J&#039;(0)=w. My guess is that the solution uses this along with some linear algebra trick to find the derivative.

Thanks in advance for your help!
 
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My notation might be a bit rusty, but the differential of the exponential at 0 is the identity. So d(exp)(rv)= I + O(r).

So the first non zero term will come from that I, which has determinant 1. You integrate over v to get the usual surface area of a (Euclidean) sphere. Since you are looking at the derivative of V, the antiderivative gives the volume of the euclidean ball.

To get the second term, you'll need the next term in the differential of that exponential. It will have to involve curvature somehow. From your formula, it looks like you might take J(w,t)/t and find the second non zero term in its expansion. (The first non zero term is w, which is why d(exp)(0) = I.
 
Thanks. That gets me the first term, and at least gives me an educated guess for the second term. I'm guessing that \frac{d}{dr} \left( d(\exp_p)_{rv} \right) = ric_p(v). When you integrate this over the whole ball you end up getting the scalar curvature which is what was supposed to happen.
 
Since you mentioned the Ricci tensor, I looked it up on Wikipedia. They have formulas there that look relevant. In particular, under the heading "direct geometric meaning", they have the first two nonzero terms in the Taylor expansion of the volume element in geodesic normal coordinates.

http://en.wikipedia.org/wiki/Ricci_curvature
 

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