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Bounds on spectral gaps of Hyperbolic spin surfaces

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arxiv 2311.13330 v1 pith:CH7MFHNI submitted 2023-11-22 math.SP hep-thmath-phmath.DGmath.MPmath.NT

classification math.SPhep-thmath-phmath.DGmath.MPmath.NT
keywords spectralboundslaplacianspinhyperbolicidentitiesnearlycompact
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abstract

We describe a method for constraining Laplacian and Dirac spectra of two dimensional compact orientable hyperbolic spin manifolds and orbifolds. The key ingredient is an infinite family of identities satisfied by the spectra. These spectral identities follow from the consistency between 1) the spectral decomposition of functions on the spin bundle into irreducible representations of $\mathrm{SL}(2,\mathbb{R})$ and 2) associativity of pointwise multiplication of functions. Applying semidefinite programming methods to our identities produces rigorous upper bounds on the Laplacian spectral gap as well as on the Dirac spectral gap conditioned on the former. In several examples, our bounds are nearly sharp; a numerical algorithm based on the Selberg trace formula shows that the $[0;3,3,5]$ orbifold, a particular surface with signature $[1;3]$, and the Bolza surface nearly saturate the bounds at genus $0$, $1$ and $2$ respectively. Under additional assumptions on the number of harmonic spinors carried by the spin-surface, we obtain more restrictive bounds on the Laplacian spectral gap. In particular, these bounds apply to hyperelliptic surfaces. We also determine the set of Laplacian spectral gaps attained by all compact orientable two-dimensional hyperbolic spin orbifolds. We show that this set is upper bounded by $12.13798$; this bound is nearly saturated by the $[0;3,3,5]$ orbifold, whose first non-zero Laplacian eigenvalue is $\lambda^{(0)}_1\approx 12.13623$.

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  1. Moduli Bounds from Spin-2 Sum Rules

    hep-th 2026-08 accept novelty 6.0 of 10

    The paper proves, from massive spin-2 scattering sum rules, that the lightest KK graviton must couple to a scalar with (m_sc/m_1)^2 ≤ 4/3, and every KK graviton m_n to a scalar with (m_sc/m_n)^2 < 36/25.

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