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Schwarzschild’s Solution and Black Holes
2019In Chap. 14 we showed that the exterior Schwarzschild solution of Einstein’s equation describes the gravitational field outside a static spherical mass with constant mass density. This solution has the peculiar characteristic that some components of the metric tensor became infinite at the Schwarzschild radius \(r_{s}=2m\) and at \(r=0\).
Antonio Romano, Mario Mango Furnari
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Cosmological dynamical black hole solutions
International Journal of Modern Physics AWe find new classes of the dynamical black hole solutions in five- or higher-dimensional Einstein–Maxwell-dilaton theory, in which the dilaton field interacts nontrivially with the Maxwell field, and the cosmological constant, with two arbitrary coupling constants.
Bardia H. Fahim, A. M. Ghezelbash
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Black hole solutions with torsion
2009Classical general relativity theory is torsion free. However, since general relativity and general relativity with torsion are experimentally indistinguishable at this time, it is important to explore the consequences of torsion through its physical effects.
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Electromagnetic counterparts to massive black-hole mergers
Living Reviews in Relativity, 2022Tamara Bogdanovic +2 more
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