Open AccessTHE QUANTUM THERMAL EFFECT OF THE CHARGED, AXIALLY SYMMETRIC NONSTATIONARY BLACH HOLE
Author(s) -
MaoWang Lu
Publication year - 2000
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.49.1035
Subject(s) - physics , axial symmetry , hawking radiation , black hole (networking) , event horizon , thermal radiation , charged black hole , thermal , charge (physics) , horizon , quantum electrodynamics , extremal black hole , classical mechanics , quantum mechanics , event (particle physics) , thermodynamics , computer network , routing protocol , routing (electronic design automation) , astronomy , computer science , link state routing protocol
The Hawking radiation for a charged axially symmetric nonstationary black hole is studied. We obtain the event horizon equation and the Hawking thermal spectrum formula. Both the shape and the temperature of the black hole depend on the time and the angle. They can reduce to the well-known results when there is no electric charge.