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• W2963883449 abstract "The energy-momentum of a new four-dimensional, charged, spherically symmetric, and nonsingular black hole solution constructed in the context of general relativity coupled to a theory of nonlinear electrodynamics is investigated, whereby the nonlinear mass function is inspired by the probability density function of the continuous logistic distribution. The energy and momentum distributions are calculated by use of the Einstein, Landau-Lifshitz, Weinberg, and Møller energy-momentum complexes. In all these prescriptions, it is found that the energy distribution depends 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, an additional parameter <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M3><mml:mrow><mml:mi>β</mml:mi></mml:mrow></mml:math> coming from the gravitational background considered, 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>. Further, the Landau-Lifshitz and Weinberg prescriptions yield the same result for the energy, while, in all the aforesaid prescriptions, all the momenta vanish. We also focus on the study of the limiting behavior of the energy for different values of the radial coordinate, the parameter <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M5><mml:mrow><mml:mi>β</mml:mi></mml:mrow></mml:math>, and the charge <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M6><mml:mrow><mml:mi>q</mml:mi></mml:mrow></mml:math>. Finally, it is pointed out that, for <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M7><mml:mi>r</mml:mi><mml:mo>→</mml:mo><mml:mi mathvariant=normal>∞</mml:mi></mml:math> and <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML id=M8><mml:mi>q</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant=normal>0</mml:mn></mml:math>, all the energy-momentum complexes yield the same expression for the energy distribution as in the case of the Schwarzschild black hole solution." @default.
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• W2963883449 date "2017-01-01" @default.
• W2963883449 modified "2023-09-23" @default.
• W2963883449 title "Energy-Momentum for a Charged Nonsingular Black Hole Solution with a Nonlinear Mass Function" @default.
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• W2963883449 doi "https://doi.org/10.1155/2017/7656389" @default.
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