Open AccessStefan-Boltzmann's law of the Dirac field of static spherically symmetric black holes
Author(s) -
Meng Qing-miao
Publication year - 2003
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.52.2102
Subject(s) - physics , event horizon , black hole (networking) , boltzmann constant , quartic function , nonsingular black hole models , entropy (arrow of time) , extremal black hole , mathematical physics , classical mechanics , charged black hole , quantum mechanics , spacetime , mathematics , computer network , routing protocol , routing (electronic design automation) , computer science , pure mathematics , link state routing protocol
Using the statistical entropy of the Dirac field of static spherically symmetric black hole, the Stefan-Boltzmann's law of static spherically symmetric black ho les is calculated, and we obtain a conclusion that the radiant emittance of a bl ack hole is proportionate to quartic power of temperature of the event horizon o f the black hole. It is found that the value of Stefan-Boltzmann constant in curved space-time is different from that in Euclidean space-time, and the constant has different value in different space-time.