Hawking Radiation of Dirac Particles in a Nonuniformly Rectilinearly Accelerating Black Hole

Details Hawking Radiation of Dirac Particles in a Nonuniformly Rectilinearly Accelerating Black Hole Hawking Radiation of Dirac Particles in a Nonuniformly Rectilinearly Accelerating Black Hole

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003gregr..35..595z&link_type=abstract

General Relativity and Gravitation, v. 35, Issue 4, p. 595-603 (2003).

Physics

Scientific paper

The Hawking radiation of Dirac particles on the event horizon of a nonuniformly rectilinearly accelerating black hole is studied in this paper. First, we construct the symmetrized null tetrad from which the spin coefficients and Dirac equation are derived. Next, by proposing generalized tortoise coordinate transformation, the decoupling problem of the Dirac equation with nonzero rest mass is solved. Finally, by analytic continuation, the Hawking thermal spectrum formula of Dirac particle for nonuniformly rectilinearly accelerating black hole is obtained.

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