Abstract
The heat kernel and quasinormal mode methods of computing 1-loop partition functions of spin fields on hyperbolic quotient spacetimes are related via the Selberg zeta function. We extend that analysis to thermal backgrounds, with quotient structure . Specifically, we demonstrate the zeros of the Selberg function encode the normal mode frequencies of spin fields upon removal of non-square-integrable modes. With this information we construct the 1-loop partition functions for symmetric transverse traceless tensors in terms of the Selberg zeta function and find exact agreement with the heat kernel method.
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