Time Evolution of Temperature and Entropy of a Gravitationally Collapsing Cylinder
Evan Halstead, Peng Hao

TL;DR
This paper studies the time evolution of temperature and entropy during gravitational collapse of a cylindrical domain wall, revealing that entropy approaches a constant near Hawking entropy but decreases over time, preventing spontaneous collapse.
Contribution
It extends previous spherical collapse models to a cylindrical topology using a (3+1) BTZ metric, analyzing radiation spectrum and thermodynamics during collapse.
Findings
Spectrum is quasi-thermal with increasing thermality near the horizon.
Late-time temperature closely matches Hawking temperature.
Entropy approaches a constant close to Hawking entropy but decreases over time.
Abstract
We investigate the time evolution of the temperature and entropy of a gravitationally collapsing cylinder, represented by an infinitely thin domain wall, as seen by an asymptotic observer. Previous work has shown that the entropy of a spherically symmetric collapsing domain approaches a constant, and we follow this procedure using a (3+1) BTZ metric to see if a different topology will yield different results. We do this by coupling a scalar field to the background of the domain wall and analyzing the spectrum of radiation as a function of time. We find that the spectrum is quasi-thermal, with the degree of thermality increasing as the domain wall approaches the horizon. The thermal distribution allows for the determination of the temperature as a function of time, and we find that the late time temperature is very close to the Hawking temperature and that it also exhibits the proper…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Astrophysics and Star Formation Studies
