Open AccessHawking radiation from the dynamical spherical symmetrically Einstein-Yang-Mills-Chern-Simons black hole
Author(s) -
杨树政,
林恺
Publication year - 2013
Publication title -
wuli xuebao
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.199
H-Index - 47
ISSN - 1000-3290
DOI - 10.7498/aps.62.060401
Subject(s) - hawking radiation , physics , black hole (networking) , event horizon , sonic black hole , black hole thermodynamics , micro black hole , chern–simons theory , mathematical physics , horizon , quantum electrodynamics , scalar field , white hole , quantum mechanics , classical mechanics , gravitational collapse , gravitational wave , gauge theory , computer network , routing protocol , routing (electronic design automation) , computer science , link state routing protocol , astronomy
Using Hamilton-Jacobi method, the Hawking tunneling radiation and temperature are investigated near the event horizon of the Einstein-Yang-Mills-Chern-Simons black hole. The results show that the temperature and tunneling rate depend on the charge and horizon of black holes, and the conclusion is significant for investigating other dynamical black holes. What is more, we also prove that this method can be used to study Hawking radiation in the scalar, vector, Dirac field and gravitational wave cases.