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An improved volume bound under Ricci and scalar curvature lower bounds

Published 19 Aug 2026 in math.DG and math.MG | (2608.19196v1)

Abstract: We study volume comparison for closed Riemannian manifolds satisfying a positive Ricci curvature lower bound together with an improved scalar curvature lower bound. Using an integral extension of the finite shuffling comparison for scalar Jacobi solutions due to Brown and Freedman \cite{BrownFreedman2022}, we prove that if a closed Riemannian manifold (N<sup>n,</sup>g)(N<sup>n,</sup> g) satisfies Ricg(n1)g\operatorname{Ric}_g\ge (n-1)g and the scalar curvature Rgn(n1)(1+ε)R_g\ge n(n-1)(1+\varepsilon), then its volume satisfies Ng11+nεS<sup>n.</sup>\lvert N\rvert_g \le \frac{1}{\sqrt{1+n\varepsilon}}\lvert\mathbb S<sup>n\rvert.</sup> In fact, assuming only Ricg(n1)g\mathrm{Ric}_g\ge(n-1)g, we can prove that NgS<sup>n</sup>1NgN(Rgn1(n1))<sup>12</sup>dvolg.\frac{|N|_g}{\left|\mathbb{S}<sup>n\right|}</sup> \le \frac{1}{|N|_g} \int_N\left(\frac{R_g}{n-1}-(n-1)\right)<sup>{-\frac{1}{2}}</sup> d \mathrm{vol}_g. The equality holds if and only if NN is isometric to the unit sphere. The proof combines a coefficient-adapted Jacobian comparison with the integral shuffling comparison. This yields an estimate that retains the full Ricci spectrum. The resulting volume bound agrees to first order in ε\varepsilon with the factor predicted by Bray's conjecture. A further consequence of the argument is an averaged volume comparison for metric balls involving the scalar curvature.

Authors (1)

Summary

  • The paper proves that a closed n-manifold with Ricci curvature at least (n−1)g and scalar curvature at least n(n−1)(1+ε) has volume ratio at most (1+nε)^−1/2, with equality only for the unit sphere when ε=0.
  • The paper develops coefficient-adapted Jacobian comparison and an integral shuffling theorem over the geodesic flow to retain directional Ricci information and derive sharper scalar-curvature and Ricci-spectrum volume estimates.
  • The paper improves Bishop’s bound in every dimension n≥3 but does not resolve Bray’s conjecture for n≥4, leaving an order-ε² gap between its bound and Bray’s predicted factor.
  • follow_up_questions

Overview and main results

This paper by Kwok-Kun Kwong establishes a quantitative improvement of Bishop's volume comparison theorem for closed Riemannian manifolds satisfying a Ricci curvature lower bound together with an improved scalar curvature lower bound. The main theorem states that if a closed nn-manifold (n3n \ge 3) satisfies Ricg(n1)g\operatorname{Ric}_g \ge (n-1)g and Rgn(n1)(1+ε)R_g \ge n(n-1)(1+\varepsilon) for some ε0\varepsilon \ge 0, then

NgSn(1+nε)1/2,\frac{|N|_g}{|\mathbb S^n|} \le (1+n\varepsilon)^{-1/2},

with equality if and only if NN is isometric to the unit sphere and ε=0\varepsilon = 0. For every ε>0\varepsilon > 0, the right-hand side is strictly less than one, so the result gives a strict improvement over Bishop's bound in all dimensions, without any symmetry, C2C^2-closeness, or upper Ricci bound assumptions.

The uniform estimate follows from a stronger, pointwise-in-scalar-curvature statement: assuming only n3n \ge 30,

n3n \ge 31

This averaged form retains the full scalar curvature distribution rather than only its infimum. A still sharper intermediate result bounds the volume by the average of n3n \ge 32, which involves the full spectrum of the Ricci tensor.

Relation to Bray's conjecture

The motivation is a conjecture of Bray from his thesis on the Riemannian Penrose inequality: for each n3n \ge 33 there should exist n3n \ge 34 such that n3n \ge 35 and n3n \ge 36 imply n3n \ge 37. In dimension three this is essentially settled: Bray's football theorem provides a sharp function n3n \ge 38, Gursky–Viaclovsky proved rigorously that n3n \ge 39, and Brendle established the rigidity case using the Gauss equation and Gauss–Bonnet on two-dimensional isoperimetric surfaces — a step that does not extend to higher dimensions.

The paper's estimate compares to Bray's predicted factor as follows. By Bernoulli's inequality, Ricg(n1)g\operatorname{Ric}_g \ge (n-1)g0 for Ricg(n1)g\operatorname{Ric}_g \ge (n-1)g1, so the new bound does not reach Bray's conjectured volume factor. However, binomial expansion shows

Ricg(n1)g\operatorname{Ric}_g \ge (n-1)g2

so the two factors agree to first order in Ricg(n1)g\operatorname{Ric}_g \ge (n-1)g3 and differ only at order Ricg(n1)g\operatorname{Ric}_g \ge (n-1)g4. The paper is explicit that Bray's conjecture under only its two lower curvature bounds remains open in dimensions Ricg(n1)g\operatorname{Ric}_g \ge (n-1)g5; the present result is a step toward it rather than a resolution.

Proof ingredients

The argument combines three components.

Coefficient-adapted Jacobian comparison. For Ricg(n1)g\operatorname{Ric}_g \ge (n-1)g6, let Ricg(n1)g\operatorname{Ric}_g \ge (n-1)g7 solve the scalar Jacobi equation Ricg(n1)g\operatorname{Ric}_g \ge (n-1)g8 with Ricg(n1)g\operatorname{Ric}_g \ge (n-1)g9, Rgn(n1)(1+ε)R_g \ge n(n-1)(1+\varepsilon)0. Via a refined Riccati analysis tracking the traceless shape operator Rgn(n1)(1+ε)R_g \ge n(n-1)(1+\varepsilon)1, the paper proves that before the first conjugate time,

Rgn(n1)(1+ε)R_g \ge n(n-1)(1+\varepsilon)2

where Rgn(n1)(1+ε)R_g \ge n(n-1)(1+\varepsilon)3 is the polar Jacobian. Notably, this comparison requires no curvature lower bound. An exact identity expresses Rgn(n1)(1+ε)R_g \ge n(n-1)(1+\varepsilon)4 as a double integral of Rgn(n1)(1+ε)R_g \ge n(n-1)(1+\varepsilon)5, giving both the inequality and the equality characterization.

Integral shuffling comparison. Brown and Freedman proved a finite-family comparison: rearranging coefficients of stopped Jacobi solutions in nondecreasing order at each time can only increase the sum of Rgn(n1)(1+ε)R_g \ge n(n-1)(1+\varepsilon)6-th powers of terminal values. The paper extends this to a continuum via measure-preserving flows. The key technical work is a continuity lemma showing that stopped solutions depend continuously on their coefficients in Rgn(n1)(1+ε)R_g \ge n(n-1)(1+\varepsilon)7 (handled case-by-case according to whether the first zero lies beyond, before, or exactly at time Rgn(n1)(1+ε)R_g \ge n(n-1)(1+\varepsilon)8), followed by finite-rational approximation and dominated convergence. The resulting theorem states that for a continuous measure-preserving flow Rgn(n1)(1+ε)R_g \ge n(n-1)(1+\varepsilon)9 on a compact probability space ε0\varepsilon \ge 00 and continuous ε0\varepsilon \ge 01,

ε0\varepsilon \ge 02

where ε0\varepsilon \ge 03 solves ε0\varepsilon \ge 04 and ε0\varepsilon \ge 05 is the stopped constant-coefficient solution.

Liouville measure preservation. Applying the integral shuffling theorem to the geodesic flow ε0\varepsilon \ge 06 on ε0\varepsilon \ge 07 with normalized Liouville measure ε0\varepsilon \ge 08 and ε0\varepsilon \ge 09 converts estimates along individual geodesics into averaged estimates over the unit tangent bundle. Measure preservation ensures that although NgSn(1+nε)1/2,\frac{|N|_g}{|\mathbb S^n|} \le (1+n\varepsilon)^{-1/2},0 varies along each geodesic, the distribution of its values over NgSn(1+nε)1/2,\frac{|N|_g}{|\mathbb S^n|} \le (1+n\varepsilon)^{-1/2},1 is fixed in time — precisely the continuous analogue of the equal-level-measure condition in the finite lemma.

Consequences for metric balls and the Ricci spectrum

Two further results follow from the same machinery. First, an averaged volume comparison for metric balls incorporating scalar-curvature excess: under NgSn(1+nε)1/2,\frac{|N|_g}{|\mathbb S^n|} \le (1+n\varepsilon)^{-1/2},2, writing NgSn(1+nε)1/2,\frac{|N|_g}{|\mathbb S^n|} \le (1+n\varepsilon)^{-1/2},3,

NgSn(1+nε)1/2,\frac{|N|_g}{|\mathbb S^n|} \le (1+n\varepsilon)^{-1/2},4

where NgSn(1+nε)1/2,\frac{|N|_g}{|\mathbb S^n|} \le (1+n\varepsilon)^{-1/2},5 is the double-integral kernel introduced in Kwong's earlier work and NgSn(1+nε)1/2,\frac{|N|_g}{|\mathbb S^n|} \le (1+n\varepsilon)^{-1/2},6 is a decreasing function defined by a spherical integral. This refines the Bishop–Gromov bound quantitatively whenever the scalar excess is not identically zero. The proof uses a convexity argument showing that spherical averages of exponentials of quadratic forms are maximized when the form has rank one.

Second, when NgSn(1+nε)1/2,\frac{|N|_g}{|\mathbb S^n|} \le (1+n\varepsilon)^{-1/2},7, letting NgSn(1+nε)1/2,\frac{|N|_g}{|\mathbb S^n|} \le (1+n\varepsilon)^{-1/2},8 yields the spectral bound

NgSn(1+nε)1/2,\frac{|N|_g}{|\mathbb S^n|} \le (1+n\varepsilon)^{-1/2},9

The exponent NN0 is critical here: Jensen's inequality would give only a lower bound for general exponents, but for this special exponent the spherical average evaluates exactly, via a Gaussian integral computation, to NN1 where NN2. This yields the determinant bound

NN3

Equality forces umbilic small geodesic spheres, hence NN4 on NN5 for all unit NN6; combined with Schur's lemma and a quotient-manifold volume count, this gives rigidity to round spheres. The final step to the main theorem uses the elementary inequality NN7 for NN8, applied to eigenvalues of NN9, replacing the determinant by the scalar-curvature expression.

Limitations and open questions

Several qualifications are stated plainly in the paper. The uniform bound ε=0\varepsilon = 00 falls short of Bray's conjectured factor ε=0\varepsilon = 01 by a term of order ε=0\varepsilon = 02, so Bray's conjecture remains open in dimensions ε=0\varepsilon = 03 under only the two curvature lower bounds. The averaged ball comparison holds for almost every radius, since metric spheres may meet cut loci in positive ε=0\varepsilon = 04-measure at exceptional radii, though the volume estimate itself holds for every radius. The total-volume estimate requires positive Ricci curvature; the passage from the determinant bound to the scalar bound discards information from higher elementary symmetric functions ε=0\varepsilon = 05 of the nonnegative tensor ε=0\varepsilon = 06, and whether exploiting these could close the order-ε=0\varepsilon = 07 gap to Bray's factor is a natural open question left unaddressed.

Conclusion

The paper proves that a scalar curvature excess above ε=0\varepsilon = 08 yields an explicit, quantitative improvement of Bishop's volume bound in all dimensions ε=0\varepsilon = 09, without auxiliary hypotheses, and identifies the equality cases completely. Methodologically, it demonstrates that the shuffling principle of Brown and Freedman, extended to integral form over the geodesic flow, allows volume comparison to retain directional Ricci data rather than collapsing to a common lower bound. The first-order agreement with Bray's conjectured volume factor makes the remaining second-order gap a concrete target for further work.

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