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- W2950903550 abstract "The evaluation of the energy-momentum distribution for a new four-dimensional, spherically symmetric, static and charged black hole spacetime geometry with constant non-zero topological Euler density is performed by using the energy-momentum complexes of Einstein and Moller. This black hole solution was recently developed in the context of the coupled Einstein--non-linear electrodynamics of the Born-Infeld type. The energy is found to depend on the mass $M$ and the charge $q$ of the black hole, the cosmological constant $Lambda$ and the radial coordinate $r$, while in both prescriptions all the momenta vanish. Some limiting and particular cases are analyzed, illustrating the rather extraordinary character of the spacetime geometry considered." @default.
- W2950903550 created "2019-06-27" @default.
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- W2950903550 date "2018-07-01" @default.
- W2950903550 modified "2023-09-23" @default.
- W2950903550 title "Localization of Energy-Momentum for a Black Hole Spacetime Geometry with Constant Topological Euler Density" @default.
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