Published March 2025 | Version Published
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Spectral Bounds on Hyperbolic 3-Manifolds: Associativity and the Trace Formula

  • 1. ROR icon University of Mississippi
  • 2. ROR icon Institute for Advanced Study
  • 3. ROR icon California Institute of Technology

Abstract

We constrain the low-energy spectra of Laplace operators on closed hyperbolic manifolds and orbifolds in three dimensions, including the standard Laplace--Beltrami operator on functions and the Laplacian on powers of the cotangent bundle. Our approach employs linear programming techniques to derive rigorous bounds by leveraging two types of spectral identities. The first type, inspired by the conformal bootstrap, arises from the consistency of the spectral decomposition of the product of Laplace eigensections, and involves the Laplacian spectra as well as integrals of triple products of eigensections. We formulate these conditions in the language of representation theory of PSL₂(ℂ) and use them to prove upper bounds on the first and second Laplacian eigenvalues. The second type of spectral identities follows from the Selberg trace formula. We use them to find upper bounds on the spectral gap λof the Laplace--Beltrami operator on hyperbolic 3-orbifolds, as well as on the systole length of hyperbolic 3-manifolds, as a function of the volume. Further, we prove that the spectral gap  of the Laplace--Beltrami operator on all closed hyperbolic 3-manifolds satisfies λ₁ < 47.32. Along the way, we use the trace formula to estimate the low-energy spectra of a large set of example orbifolds and compare them with our general bounds, finding that the bounds are nearly sharp in several cases.

Copyright and License

© The Author(s) 2024. This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/.

Acknowledgement

We would like to thank Peter Sarnak and Akshay Venkatesh for useful discussions and Petr Kravchuk for useful discussions and collaboration on related ideas.

Funding

DM acknowledges funding provided by Edward and Kiyomi Baird as well as the grant DE-SC0009988 from the U.S. Department of Energy. SP acknowledges the support by the U.S. Department of Energy, Office of Science, Office of High Energy Physics, under Award Number DE-SC0011632 and by the Walter Burke Institute for Theoretical Physics.

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Additional details

Related works

Describes
Journal Article: https://rdcu.be/eBhls (ReadCube)
Is new version of
Discussion Paper: arXiv:2308.11174 (arXiv)

Funding

Edward and Kiyomi Baird
United States Department of Energy
DE-SC0009988
United States Department of Energy
DE-SC0011632
California Institute of Technology

Dates

Accepted
2024-12-20
Available
2025-02-17
Published online

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Caltech groups
Walter Burke Institute for Theoretical Physics, Division of Physics, Mathematics and Astronomy (PMA)
Publication Status
Published