Spectral form factors for curved spacetimes with horizon
Dmitry S. Ageev, Vasilii V. Pushkarev, Anastasia N. Zueva

TL;DR
This paper investigates the spectral form factor in curved spacetimes with horizons, extending previous models to include massive fields and de Sitter space, and compares the results with random matrix theory to explore chaos indicators.
Contribution
It extends the analysis of spectral form factors in black hole and de Sitter backgrounds to massive fields and compares with integrable systems, questioning the link to quantum chaos.
Findings
BTZ and de Sitter models show dip-ramp-plateau structure
Spectral form factors differ from random matrix predictions
Models are highly distinct integrable systems
Abstract
The spectral form factor is believed to exhibit a special type of behavior called ``dip-ramp-plateau'' in chaotic quantum systems that originates from random matrix theory. This suggests that the shape of the spectral form factor could serve as an indicator of chaos in various quantum systems. It has been shown recently that the dip-ramp-plateau structure appears in the spectral form factor when the normal modes of a massless scalar field theory in the brick-wall model of the BTZ black hole are treated as eigenvalues of a quantum Hamiltonian. At the same time, the level spacing distribution of these normal modes differs from that associated with random matrix theory ensembles. In this paper, we extend the results for BTZ background to the case of non-zero mass of the field, study the generalized spectral form-factor, and consider the same context for another non-trivial background -- de…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Astrophysical Phenomena and Observations
