Hawking radiation from a dynamical Kerr–Newman black hole
Keyword(s):
After Hawking radiation from a Schwarzschild black hole is calculated using the Damour–Ruffini method, the tortoise coordinate transformation in a static black hole is extended to a dynamical axisymmetric black hole, such as a dynamical Kerr–Newman black hole. Under the generalized tortoise coordinate transformation, Hawking radiation from a dynamical Kerr–Newman black hole is obtained successfully. Moreover, it also seems to occur on the apparent horizon instead of the event horizon.
2012 ◽
Vol 12
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pp. 358-367
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2012 ◽
Vol 51
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pp. 3214-3221
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2013 ◽
Vol 52
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pp. 1682-1687
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2011 ◽
Vol 51
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pp. 518-525
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2011 ◽
Vol 51
(4)
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pp. 1195-1203
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Keyword(s):
2009 ◽
Vol 24
(22)
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pp. 1775-1783
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2004 ◽
Vol 36
(11)
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pp. 2511-2523
2014 ◽
Vol 54
(2)
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pp. 604-613
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