| Issue |
EPL
Volume 139, Number 5, September 2022
|
|
|---|---|---|
| Article Number | 59001 | |
| Number of page(s) | 7 | |
| Section | Gravitation, cosmology and astrophysics | |
| DOI | https://doi.org/10.1209/0295-5075/ac8610 | |
| Published online | 19 August 2022 | |
Modification method of NUT-Kerr-Newman-de Sitter black hole entropy by Lorentz symmetry breaking and beyond the semi-classical approximation
School of Physics and Astronomy, China West Normal University - Sichuan Nanchong, 637002, PRC
(a) 1392600876@qq.com
(b) 1847372937@qq.com
(c) szyangcwnu@126.com (corresponding author)
Received: 12 June 2022
Accepted: 2 August 2022
According to Lorentz symmetry breaking and black hole quantum tunneling radiation theory, aether-like field is correctly introduced into the general stationary black hole space-time, and the modified boson dynamic equation is obtained. On this basis, the Hawking temperature and black hole entropy of NUT-Kerr-Newman-de Sitter black hole with general stationary characteristics are modified, and the method used in this paper and the significance of the conclusions are deeply discussed.
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