2006/06/15 by Jun Ren, Jingyi Zhang, Zhang Jing-Yi +2 · 1 citation
Physics and Astronomy · #Black Holes and Theoretical Physics #Black hole (networking) #Computer science #Cosmology and Gravitation Theories #Event (particle physics) #Event horizon #Hawking #Hawking radiation #Horizon #Micro black hole #Noncommutative and Quantum Gravity Theories #Physics #Quantum mechanics #Quantum tunnelling #Work (physics) #gr-qc
paper · pdf · doi:10.1088/0256-307x/23/8/016
published as Chin.Phys.Lett. 23 (2006) 2019-2022
arxiv created 2006/06/15 · openalex publication_date 2006/07/21 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We extend Parikh's study to the non-stationary black hole. As an example of the non-stationary black hole, we investigate the tunnelling effect and Hawking radiation from a Vaidya black hole whose Bondi mass is identical to its mass parameter. The Hawking radiation is considered as a tunnelling process across the event horizon and we calculate the tunnelling probability. It is found that the result is different from Parikh's study because dr H / dv is the function of Bondi mass m ( v ).