Quantum Thermal Effect of Dirac Particles in a Non-uniformly Rectilinearly Accelerating Kinnersley Black Hole

Details Quantum Thermal Effect of Dirac Particles in a Non-uniformly Rectilinearly Accelerating Kinnersley Black Hole Quantum Thermal Effect of Dirac Particles in a Non-uniformly Rectilinearly Accelerating Kinnersley Black Hole

2001-09-22

arxiv.org/abs/gr-qc/0109080v2

Chin.Phys.Lett. 19 (2002) 141-143

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

revtex, 3 pages, no figure, typos corrected, references added, version to appear in journal (CPL)

Scientific paper

10.1088/0256-307X/19/1/344

The Hawking radiation of Dirac particles in an arbitrarily rectilinearly accelerating Kinnersley black hole is studied by using a method of the generalized tortoise coordinate transformation. Both the location and the temperature of the event horizon depend on the time and polar angle. The Hawking thermal radiation spectrum of Dirac particles is also derived. PACS numbers: 97.60.Lf, 04.70.Dy

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