Hawking Radiation of Dirac Particles in 1+1 Dimensional Nonstatic Black Hole
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Abstract
This letter is devoted to the discussion of the Hawking radiation of Dirac particles in 1 + 1 dimensional space-time. The general nonstatic 1 + 1 dimensional metric is used to calculate the radiant spectrum and the expression of radiation temperature, which, as an example, verifies the quantum-mechanical instability in black hole due to Hawking radiation.
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Cite this article:
CHEN Da-ming, SHEN You-gen, SONG Guo-xuan. Hawking Radiation of Dirac Particles in 1+1 Dimensional Nonstatic Black Hole[J]. Chin. Phys. Lett., 1996, 13(8): 633-636.
CHEN Da-ming, SHEN You-gen, SONG Guo-xuan. Hawking Radiation of Dirac Particles in 1+1 Dimensional Nonstatic Black Hole[J]. Chin. Phys. Lett., 1996, 13(8): 633-636.
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CHEN Da-ming, SHEN You-gen, SONG Guo-xuan. Hawking Radiation of Dirac Particles in 1+1 Dimensional Nonstatic Black Hole[J]. Chin. Phys. Lett., 1996, 13(8): 633-636.
CHEN Da-ming, SHEN You-gen, SONG Guo-xuan. Hawking Radiation of Dirac Particles in 1+1 Dimensional Nonstatic Black Hole[J]. Chin. Phys. Lett., 1996, 13(8): 633-636.
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