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- W2811462419 abstract "The evaluation of the energy-momentum distribution for a new four-dimensional, spherically symmetric, static and charged black hole spacetime geometry with constant nonzero topological Euler density is performed by using the energy-momentum complexes of Einstein and Møller. This black hole solution was recently developed in the context of the coupled Einstein–nonlinear electrodynamics of the Born-Infeld type. The energy is found to depend on the mass <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M1><mml:mrow><mml:mi>M</mml:mi></mml:mrow></mml:math> and the charge <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M2><mml:mrow><mml:mi>q</mml:mi></mml:mrow></mml:math> of the black hole, the cosmological constant <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M3><mml:mrow><mml:mi mathvariant=normal>Λ</mml:mi></mml:mrow></mml:math>, and the radial coordinate <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M4><mml:mrow><mml:mi>r</mml:mi></mml:mrow></mml:math>, while in both prescriptions all the momenta vanish. Some limiting and particular cases are analyzed and discussed, illustrating the rather extraordinary character of the spacetime geometry considered." @default.
- W2811462419 created "2018-07-10" @default.
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- W2811462419 date "2018-10-25" @default.
- W2811462419 modified "2023-09-23" @default.
- W2811462419 title "Localization of Energy-Momentum for a Black Hole Spacetime Geometry with Constant Topological Euler Density" @default.
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- W2811462419 doi "https://doi.org/10.1155/2018/5212696" @default.
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