2021
DOI: 10.48550/arxiv.2109.09219
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A Gutzwiller Trace formula for Dirac Operators on a Stationary Spacetime

Abstract: A Duistermaat-Guillemin-Gutzwiller trace formula for Dirac-type operators on a globally hyperbolic spatially compact standard stationary spacetime is achieved by generalising the recent construction by A. Strohmaier and S. Zelditch [Adv. Math. 376, 107434 (2021)] to a vector bundle setting. We have analysed the spectrum of the Lie derivative with respect to the Killing vector field on the solution space of the Dirac equation and found that it consists of discrete real eigenvalues. The distributional trace of … Show more

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Cited by 1 publication
(5 citation statements)
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“…This involves understanding the distribution of the frequency spectrum for the wave equation on a Kaluza-Klein spacetime when restricted to the isotypic subspace of an irreducible representation of the structure group, in the limit that the weight of the representation approaches infinity in the Weyl chamber. This is a direct generalization of the results from [23] and is closely related to [22], [14]. Furthermore we show how to apply these results to frequency asymptotics for the massive Klein-Gordon equation on vector bundles as one takes the representation defining the vector bundle to infinity.…”
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confidence: 62%
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“…This involves understanding the distribution of the frequency spectrum for the wave equation on a Kaluza-Klein spacetime when restricted to the isotypic subspace of an irreducible representation of the structure group, in the limit that the weight of the representation approaches infinity in the Weyl chamber. This is a direct generalization of the results from [23] and is closely related to [22], [14]. Furthermore we show how to apply these results to frequency asymptotics for the massive Klein-Gordon equation on vector bundles as one takes the representation defining the vector bundle to infinity.…”
supporting
confidence: 62%
“…Since we allow for a potential (as long as it is constant along the fibers of P and independent of t) the energy quadratic form on the space of solutions ker ω need not be positive definite, but we use standard results from harmonic analysis together with some results on Krein and Pontryagin spaces to show that it is positive definite on the isotypic subspace H m for m sufficiently large. In Section 3.1 we apply a result from [14] to obtain that µ(E, m, −) is tempered and then we provide a proof of Corollary 1.4 given Theorems 1.1,1.2,1.3. Finally, in Section 4 we simply combine the techniques from [22] and [11] to obtain our main theorems.…”
Section: Questionmentioning
confidence: 99%
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