GENERAL: The generalized Stefan-Boltzmann law of a rectilinear non-uniformly accelerating Kinnersley black hole

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

3

Scientific paper

Using entropy density of Dirac field near the event horizon of a rectilinear non-uniformly accelerating Kinnersley black hole, the law for the thermal radiation of black hole is studied and the instantaneous radiation energy density is obtained. It is found that the instantaneous radiation energy density of a black hole is always proportional to the quartic of the temperature on event horizon in the same direction. That is to say, the thermal radiation of a black hole always satisfies the generalized Stefan-Boltzmann law. In addition, the derived generalized Stefan-Boltzmann coefficient is no longer a constant, but a dynamic coefficient related to the space-time metric near the event horizon and the changing rate of the event horizon in black holes.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

GENERAL: The generalized Stefan-Boltzmann law of a rectilinear non-uniformly accelerating Kinnersley black hole does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with GENERAL: The generalized Stefan-Boltzmann law of a rectilinear non-uniformly accelerating Kinnersley black hole, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and GENERAL: The generalized Stefan-Boltzmann law of a rectilinear non-uniformly accelerating Kinnersley black hole will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-915328

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.