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Entropy 2016, 18(11), 415; doi:10.3390/e18110415

Simple Harmonic Oscillator Canonical Ensemble Model for Tunneling Radiation of Black Hole

Center for Astrophysics, Guangzhou University, GuangZhou 510006, China
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Academic Editor: Remo Garattini
Received: 30 August 2016 / Revised: 26 October 2016 / Accepted: 10 November 2016 / Published: 23 November 2016
(This article belongs to the Special Issue Black Hole Thermodynamics II)
View Full-Text   |   Download PDF [225 KB, uploaded 23 November 2016]

Abstract

A simple harmonic oscillator canonical ensemble model for Schwarzchild black hole quantum tunneling radiation is proposed in this paper. Firstly, the equivalence between canonical ensemble model and Parikh–Wilczek’s tunneling method is introduced. Then, radiated massless particles are considered as a collection of simple harmonic oscillators. Based on this model, we treat the black hole as a heat bath to derive the energy flux of the radiation. Finally, we apply the result to estimate the lifespan of a black hole. View Full-Text
Keywords: PW tunneling; canonical ensemble; energy flux of Hawking radiation PW tunneling; canonical ensemble; energy flux of Hawking radiation
This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. (CC BY 4.0).

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Yang, J.; He, T.; Zhang, J. Simple Harmonic Oscillator Canonical Ensemble Model for Tunneling Radiation of Black Hole. Entropy 2016, 18, 415.

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