The generalised second law and the black hole evaporation in an empty space as a nonequilibrium process
Hiromi Saida

TL;DR
This paper demonstrates that during black hole evaporation in empty space, the total entropy increases due to the black hole's temperature rise, even without self-interactions in the Hawking radiation, using nonequilibrium thermodynamics.
Contribution
It applies nonequilibrium thermodynamics to show entropy increase in non-self-interacting Hawking fields during black hole evaporation, extending understanding of the generalized second law.
Findings
Entropy emission rate grows faster than black hole entropy decrease.
Black hole temperature increase drives the entropy increase of Hawking radiation.
Total entropy increases despite absence of self-interactions in Hawking field.
Abstract
When a black hole is in an empty space on which there is no matter field except that of the Hawking radiation (Hawking field), then the black hole evaporates and the entropy of the black hole decreases. The generalised second law guarantees the increase of the total entropy of the whole system which consists of the black hole and the Hawking field. That is, the increase of the entropy of the Hawking field is faster than the decrease of the black hole entropy. In naive sense, one may expect that the entropy increase of the Hawking field is due to the self-interaction among the composite particles of the Hawking field, and that the "self"-relaxation of the Hawking field results in the entropy increase. Then, when one consider a non-self-interacting matter field as the Hawking field, it is obvious that the self-relaxation does not take place, and one may think that the total entropy does…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
