Perturbation analysis for massless spin fields in accelerating Kerr-Newman-(anti-)de Sitter black holes
DOI10.1142/S0217732321501753zbMath1487.83107OpenAlexW3195297313MaRDI QIDQ5067277
Zhong-heng Li, Zai-Dong Wang, Haibo Wei, Yi-Gu Chen, Hui Zheng, Liqin Mi
Publication date: 1 April 2022
Published in: Modern Physics Letters A (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1142/s0217732321501753
Black holes (83C57) Spinor and twistor methods applied to problems in quantum theory (81R25) Perturbations in context of PDEs (35B20) Equations of motion in general relativity and gravitational theory (83C10) Numerical radial basis function approximation (65D12) Particle exchange symmetries in quantum theory (general) (81V72)
Uses Software
Cites Work
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- Stability of a Schwarzschild Singularity
- An Approach to Gravitational Radiation by a Method of Spin Coefficients
- Spin-weighted angular spheroidal functions
- Integrability conditions for the coupled electromagnetic- gravitational perturbation equations of the Kerr-Newman spacetime
- On Litvin's lemma
- Exact Space-Times in Einstein's General Relativity
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