Radiation spectrum of a high-dimensional rotating black hole

Details Radiation spectrum of a high-dimensional rotating black hole Radiation spectrum of a high-dimensional rotating black hole

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010scchg..53..504z&link_type=abstract

Science China Physics, Mechanics and Astronomy, Volume 53, Issue 3, pp.504-507

Astronomy and Astrophysics

Astronomy

Damour-Ruffini Method, Hawking Radiation, Tortoise Coordinate Transformation, High-Dimensional Rotating Spacetime

Scientific paper

This study extends the classical Damour-Ruffini method and discusses Hawking radiation in a ( n + 4)-dimensional rotating black hole. Under the condition that the total energy and angular momentum of spacetime are conservative, but angular momentum a = J/ M of unit mass of the black hole is variable, taking into consideration the reaction of the radiation of the particle to the spacetime, a new Tortoise coordinate transformation and discuss the black hole radiation spectrum is discussed. The radiation spectrum that satisfies the unitary principle in the general case is derived.

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