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Astrophysical Black Holes: A Review

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arxiv 1906.03871 v1 pith:7F55INGN submitted 2019-06-10 astro-ph.HE gr-qc

classification astro-ph.HEgr-qc
keywords blackholesastrophysicalmassobjectsreviewstartedaccording
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In this review, I have tried to focus on the development of the field, from the first speculations to the current lines of research. According to Einstein's theory of general relativity, black holes are relatively simple objects and completely characterized by their mass, spin angular momentum, and electric charge, but the latter can be ignored in the case of astrophysical macroscopic objects. Search for black holes in the sky started in the early 1970s with the dynamical measurement of the mass of the compact object in Cygnus X-1. In the past 10-15 years, astronomers have developed some techniques for measuring the black hole spins. Recently, we have started using astrophysical black holes for testing fundamental physics.

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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Constraints and Consistency of Rotating Regular Black Hole Thermodynamics

    gr-qc 2026-01 reject novelty 6.0 of 10

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  3. The Case for Astrons

    gr-qc 2026-05 unverdicted novelty 4.0 of 10

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  4. Astrons: Reissner-Nordstr\"om Primordial Naked Singularities

    astro-ph.HE 2026-05 unverdicted novelty 3.0 of 10

    Constraints on primordial charged naked singularities (astrons) show charge saturation and plasma screening limit their viability, with homogeneous energy density scaling as a^{-4} providing no late-time acceleration.

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