“Golden Oldie”: On the Gravitational Field of a Mass Point According to Einstein's Theory

By K. Schwarzschild. 2003

607 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/21efb6b9e9279153022dd5f014ca5f9e58c63fc2

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In Astronomy and Astrophysics

Citations in the corpus

Testing the nature of dark compact objects: a status report (2019, background): “Even though the first nontrivial regular, asymptotically flat, vacuum solution to the field equations describing BHs were written already in 1916 [2, 3], several decades would elapse until such solutions became accepted and understood.”
Dilaton gravity in two-dimensions (2002, background): “For example, a singularity like the one in the Schwarzschild metric [386] can be reached by at least one (time- or light-like) geodesic with finite affine parameter (i.”
Magnetically charged black holes from non-linear electrodynamics and the Event Horizon Telescope (2019, background): “A generic prediction of General Relativity (GR) [1–3], BHs are understood to constitute the end state of gravitational collapse of matter.”
Gravitation (2019, background): “The Schwarzschild solution In January 1916, about one month after Einstein published his field equation, the German physicist Karl Schwarzschild found its very first exact solution [22], describing space-time surrounding a static and spherically symmetric massive object3.”
Black hole stereotyping: induced gravito-static polarization (2011, background): “Even though black hole Love numbers could have been defined following Schwarzschild’s discovery of the black hole metric [6] it was only rather recently that works on the subject appeared.”
Black holes with scalar hair in light of the Event Horizon Telescope (2020, background): “At the same time, we have been unable to test that which is the very defining property of BHs, the existence of an event horizon (EH) [84, 85].”
Thermodynamics of black holes in two (and higher) dimensions (2007, neutral): “Schwarzschild − 1 2X − 1 2G4 √ G4 2X √ 2X G4 [70]”
Superradiance (2015, background): “1916 Shortly afterwards, Schwarzschild [23] and Droste [24] derive the first solution of Einstein’s equations, describing the gravitational field generated by a point mass.”
Numerical methods for finding stationary gravitational solutions (2015, methodology): “[176] K.”
Tests for the existence of black holes through gravitational wave echoes (2017, background): “Even though Schwarzschild and Droste wrote down the first nontrivial regular, asymptotic flat, vacuum solution to the field equations already in 1916 [2, 3], several decades would elapse until such solutions became accepted.”
Superradiance: Energy Extraction, Black-Hole Bombs and Implications for Astrophysics and Particle Physics (2015, background): “1916 Few months later, Schwarzschild derives the first solution of Einstein’s equations, describing the gravitational field generated by a mass point [22].”
Testing the rotational nature of the supermassive object M87* from the circularity and size of its first image (2019, background): “They are a fundamental prediction of General Relativity (GR) [1–3], and are believed to hold the key for the unification of GR and quantum mechanics [4, 5].”
Islands in Schwarzschild black holes (2020, background): “Needless to say, the asymptotically flat four-dimensional Schwarzschild black hole is the first solution historically [29] and the simplest and the most interesting black hole.”
Wormholes as black hole foils (2007, methodology): “This metric differs from the standard Schwarzschild metric [1] only through the presence of the dimensionless parameter λ.”