Energy in the spacetime field of the charged rotating BTZ black hole via approximate Lie symmetries

DOI10.1088/0031-8949/83/05/055002zbMath1262.83030OpenAlexW2019397723MaRDI QIDQ4911635

Ibrar Hussain

Publication date: 20 March 2013

Published in: Physica Scripta (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1088/0031-8949/83/05/055002

zbMATH Keywords

black holegeodesic equationsLie approximate symmetry

Mathematics Subject Classification ID

Black holes (83C57) Gravitational energy and conservation laws; groups of motions (83C40) Analogues of general relativity in lower dimensions (83C80) Lie algebras of linear algebraic groups (17B45) Equations of motion in general relativity and gravitational theory (83C10) Einstein-Maxwell equations (83C22)

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2nd order approximate Noether and Lie symmetries of Gibbons-Maeda-Garfinkle-Horowitz-Strominger charged black hole in the Einstein frame ⋮ BLACK HOLES AND COLLISION ENERGY IN THE CENTER-OF-MASS FRAME ⋮ Effect of a quintessence model on the energy of the Reissner-Nordstrom black hole

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