史瓦西黑洞的Unruh熵

Maksym Teslyk, Olena Teslyk, Larissa Bravina, Evgeny Zabrodin
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引用次数: 0

摘要

估计了Unruh辐射产生的熵,并将其与史瓦西黑洞的熵进行了比较。我们通过一组Unruh视界模拟了一个质量为M的球形系统,并估计了出射辐射的总熵。对发射粒子的质量和自旋的依赖被考虑在内。所得结果可以很容易地推广到出射粒子的任何其他固有自由度。Unruh熵与史瓦西黑洞熵的比值以精确的解析形式导出。对于大型黑洞,该比率对发射量子的量子数(如自旋s)表现出很高的敏感性,在s=0时为0%,在s=5/2时为19.0%。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Unruh Entropy of a Schwarzschild Black Hole
The entropy produced by Unruh radiation is estimated and compared to the entropy of a Schwarzschild black hole. We simulate a spherical system of mass M by a set of Unruh horizons and estimate the total entropy of the outgoing radiation. Dependence on the mass and spin of the emitted particles is taken into account. The obtained results can be easily extended to any other intrinsic degrees of freedom of outgoing particles. The ratio of Unruh entropy to the Schwarzschild black hole entropy is derived in exact analytical form. For large black holes, this ratio exhibits high susceptibility to quantum numbers, e.g., spin s, of emitted quanta and varies from 0% for s=0 to 19.0% for s=5/2.
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