Radiating charged rotating metric in de Sitter space in retarded time coordinates and the energy-momentum tensor

DOI10.1088/0264-9381/15/1/011zbMath0925.53031OpenAlexW2066250592MaRDI QIDQ4399354

Dianyan Xu

Publication date: 18 March 1999

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1088/0264-9381/15/1/011

zbMATH Keywords

charged rotating metric in de Sitter spaceEinstein-Maxwell equations with cosmological termradiating energy-momentum tensor

Mathematics Subject Classification ID

Applications of differential geometry to physics (53Z05) Exact solutions to problems in general relativity and gravitational theory (83C15) Einstein-Maxwell equations (83C22)

Related Items (6)

New tortoise coordinate and Hawking radiation of Dirac particles in a non-stationary Kerr-Newman black hole ⋮ NON-STATIONARY ROTATING BLACK HOLES: ENTROPY AND HAWKING'S RADIATION ⋮ Rotating metrics admitting non-perfect fluids ⋮ Modified Hawking radiation of stationary and nonstationary Kerr-Newman-de Sitter black hole ⋮ CHARACTERISTICS OF QUANTUM RADIATION OF SLOWLY VARYING NONSTATIONARY KERR–NEWMAN BLACK HOLES ⋮ Hawking radiation of a non-stationary Kerr-Newman black hole: Spin-rotation coupling effect

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