Thermodynamics of acoustic black holes in two dimensions release_xy4pk3dovrdkvafqny4fagsq3q

by Baocheng Zhang

Released as a article .

2016  

Abstract

It is well-known that the thermal Hawking-like radiation can be emitted from the acoustic horizon, but the thermodynamic-like understanding for acoustic black holes was rarely made. In this paper, we will show that the kinematic connection can lead to the dynamic connection at the horizon between the fluid and gravitational models in two dimension, which implies that there exists the thermodynamic-like description for acoustic black holes. Then, we discuss the first law of thermodynamics for the acoustic black hole via an intriguing connection between the gravitational-like dynamics of the acoustic horizon and thermodynamics. We obtain a universal form for the entropy of acoustic black holes, which has an interpretation similar to the entropic gravity. We also discuss the specific heat, and find that the derivative of the velocity of background fluid can be regarded as a novel acoustic analogue of the two-dimensional dilaton potential, which interprets why the two-dimensional fluid dynamics can be connected to the gravitational dynamics but difficult for four-dimensional case. In particular, when a constraint is added for the fluid, the analogue of a Schwarzschild black hole can be realized.
In text/plain format

Archived Files and Locations

application/pdf  195.6 kB
file_q5k43owa2rh7pfflfjzq2hetke
arxiv.org (repository)
web.archive.org (webarchive)
Read Archived PDF
Archived
Type  article
Stage   submitted
Date   2016-06-02
Version   v1
Language   en ?
arXiv  1606.00693v1
Work Entity
access all versions, variants, and formats of this works (eg, pre-prints)
Catalog Record
Revision: 7e3704eb-2659-4e0a-857d-ff00de211c7b
API URL: JSON