Dirac Particles Emission from Reissner-Nordstrom-Vaidya Black Hole

6th Asian Physics Symposium

Tiandho, Yuant^1 ; Triyanta^1

Theoretical High Energy Physics and Instrumentation Division, Faculty of Mathematics and Natural Sciences, Institut Teknologi Bandung, Jl. Ganesha No. 10, Bandung

40132, Indonesia^1

关键词: Black holes;    Curved spacetime;    Dirac equations;    Dirac particles;    Emission process;    Hamilton-Jacobi;    Tunneling effects;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/739/1/012146/pdf
DOI  :  10.1088/1742-6596/739/1/012146

来源: IOP

【 摘 要 】

Using Hamilton-Jacobi method, we study the Dirac particles emission from Reissner-Nordstrom-Vaidya (RNV) black hole. The Dirac particles are described by Dirac equation in curved spacetime and emission process is defined as tunneling effect. The probability of Dirac particles emission is related to the Hawking temperature and we obtain that this temperature is equal to temperature that derived through spinless particles emission. Furthermore, we also show that the mass of Dirac particles does not affect to the Hawking temperature.