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Accreting Black Holes

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arxiv 1810.07041 v3 pith:3JUTSTHP submitted 2018-10-16 astro-ph.HE gr-qc

Sourabh Nampalliwar , Cosimo Bambi This is my paper
classification astro-ph.HEgr-qc
keywords blackholesclassificationholemodelsobservationsaccretingaccretion
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This chapter provides a general overview of the theory and observations of black holes in the Universe and on their interpretation. We briefly review the black hole classes, accretion disk models, spectral state classification, the AGN classification, and the leading techniques for measuring black hole spins. We also introduce quasi-periodic oscillations, the shadow of black holes, and the observations and the theoretical models of jets.

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Cited by 1 Pith paper

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

  1. Null geodesics, causal structure, and matter accretion in Lorentzian-Euclidean black holes

    gr-qc 2025-07 reject novelty 5.0 of 10

    In the Lorentzian-Euclidean black hole, photons and massive particles are claimed to be unable to cross the event horizon, making the spacetime geodesically complete and avoiding the central singularity.

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