The Hawking radiation of the charged particle via tunnelling from the axisymmetric Sen black hole

蒋青权,; 杨树政,; 陈德友,

doi:10.1088/1009-1963/15/8/013

Cited by 7 publications

(1 citation statement)

References 17 publications

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“…因此, 有必要将先前对Kerr-Newman 黑洞的隧穿辐射研究 [14,16] 推广到Kerr-Sen黑洞情形. 先前的工作 [10][11][12] 对此类转动黑洞隧穿辐射的研究不仅采用群速度与相速度的关系式v p = v g /2推导有质量粒子的测地线方程, 而且需要在拖曳坐标系中完成相关的计算. 需要指出的是, 这些工作也没有给出Kerr-Sen黑洞解的正确的类Painlevé-Gullstrand坐标表示.…”

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An improved research on tunneling radiation from the Kerr-Sen black hole

Zhao

2018

Sci. Sin.-Phys. Mech. Astron.

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An improved research on tunneling radiation from the Kerr-Sen black hole

Zhao

2018

Sci. Sin.-Phys. Mech. Astron.

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Fermions tunneling from the Horowitz-Strominger Dilaton black hole

Zeng

2009

Sci. China Ser. G-Phys. Mech. Astron.

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Based on the work of Kerner and Mann, fermions tunneling from the Horowitz-Strominger Dilaton black hole on the membrane is studied. Owing to the coupling among electromagnetic field, matter field and gravity field, the Dirac equation of charged particles is introduced, and according to that, the expected emission temperature is obtained. After the self-gravitational interaction is considered, it is found that the tunneling rate of fermions also satisfies the underlying Unitary theory as the case of scalar particles.Hawking radiation, fermions tunneling, Horowitz-Strominger Dilaton black hole Thirty years ago, Hawking [1,2] proposed and proved that a black hole is not fully black but may emit radiation by calculating the Bogoliubov transformation coefficients between in and out states for a body collapsing to form a black bole. Then Damour and Ruffini [3] introduced another method, which does not depend on the second quantization but adopts the relativistic quantum mechanics in curved background space time, to prove Hawking radiation. In 1988, Sannan [4] improved their work by making use of the idea of quantum field theory and quantum statistics. At the same time, people also proved Hawking radiation from the viewpoint of Temperature Green Function [5] , Path Integral [6] , Action Euclidean Integral [7] , Boulware Second Quantization [8]

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Tunnelling effect of the non-stationary Kerr black hole

Yang

Chen

2008

Chinese Phys. B

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Extending Parikh and Wilczek's work to the non-stationary black hole, we study the Hawking radiation of the non-stationary Kerr black hole by the Hamilton-Jacobi method. The result shows that the radiation spectrum is not purely thermal and the tunnelling probability is related to the change of Bekenstein-Hawking entropy, which gives a correction to the Hawking thermal radiation of the black hole.

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The Hawking radiation of the charged particle via tunnelling from the axisymmetric Sen black hole

Cited by 7 publications

References 17 publications

An improved research on tunneling radiation from the Kerr-Sen black hole

An improved research on tunneling radiation from the Kerr-Sen black hole

Fermions tunneling from the Horowitz-Strominger Dilaton black hole

Tunnelling effect of the non-stationary Kerr black hole

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