2020/02/09 by Bei Sha, Zhi-E Liu, Yu-Zhen Liu +3 · 9 citations
Physics and Astronomy · #Black hole (networking) #Dispersion relation #Extremal black hole #Hawking radiation #Micro black hole #Noncommutative and Quantum Gravity Theories #Quantum Electrodynamics and Casimir Effect #Quantum and Classical Electrodynamics #Quantum gravity #Quantum tunnelling #Spin (aerodynamics) #String theory #gr-qc #hep-th #quant-ph
paper · pdf · doi:10.1088/1674-1137/abb4d6
published in Chinese Physics C 44(12), 125104 (IOP Publishing) · 8 pages
arxiv created 2020/02/09 · openalex created_date 2020/02/14 · openalex publication_date 2020/09/03 · arxiv updated 2020/12/30 · openalex updated_date 2026/08/06
Abstract 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.