Accurate correction of arbitrary spin fermion quantum tunneling from non-stationary Kerr-de Sitter black hole based on corrected Lorentz dispersion relation  

作　　者：Bei Sha Zhi-E Liu Yu-Zhen Liu Xia Tan Jie Zhang Shu-Zheng Yang 沙贝;刘志娥;刘玉真;谭霞;张洁;杨树政(School of Physics and Electronic Engineering,Qilu Normal University,Jinan 250200,China;College of Physics and Space Science,China West Normal University,Nanchong 637002,China)

机构地区：[1]School of Physics and Electronic Engineering,Qilu Normal University,Jinan 250200,China [2]College of Physics and Space Science,China West Normal University,Nanchong 637002,China

出　　处：《Chinese Physics C》2020年第12期226-233,共8页中国物理C（英文版）

基　　金：Supported by National Natural Science Foundation of China(11573022);National Natural Science Foundation of China(11273020);Natural Science Foundation of Shandong Province,China(ZR2019MA059)。

摘　　要：According to a corrected dispersion relation proposed in the study on the string theory and quantum gravity theory,the Rarita-Schwinger equation was precisely modified,which resulted in the Rarita-Schwinger-Hamilton-Jacobi equation.Using this equation,the characteristics of arbitrary spin fermion quantum tunneling radiation from non-stationary Kerr-de Sitter black holes were determined.A number of accurately corrected physical quantities,such as surface gravity,chemical potential,tunneling probability,and Hawking temperature,which describe the properties of black holes,were derived.This research has enriched the research methods and enabled increased precision in black hole physics research.

关 键 词：black hole rermions tunneling radiation Lorentz dispersion relation 

分 类 号：O412.1[理学—理论物理] O413[理学—物理]