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Dark energy accretion onto black holes in a cosmic scenario

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Abstract

In this paper we study the accretion of dark energy onto a black hole in the cases that dark energy is equipped with a positive cosmological constant and when the space-time is described by a Schwarzschild-de Sitter metric. While the first case is the same as the usual accretion procedure for a more complicated fluid, the second one give rise to a consistent cosmic scenario for the mentioned phenomenon.

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Authors and Affiliations

  1. Colina de los Chopos, Instituto de Matemáticas y Física Fundamental, Consejo Superior de Investigaciones Científicas, Serrano 121, 28006, Madrid, Spain

    Prado Martín-Moruno, Salvador Robles-Pérez & Pedro F. González-Díaz

  2. Laboratoire de Physique Théorique et Appliquée, Faculté des Sciences, Dhar El Mahraz, Université Sidi Mohamed Ben Abdellah, B.P. 1796, Fés-Atlas, Fés, Morocco

    Az-Eddine L. Marrakchi

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  1. Prado Martín-Moruno
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  2. Az-Eddine L. Marrakchi
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  3. Salvador Robles-Pérez
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  4. Pedro F. González-Díaz
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Correspondence to Prado Martín-Moruno.

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Martín-Moruno, P., Marrakchi, AE.L., Robles-Pérez, S. et al. Dark energy accretion onto black holes in a cosmic scenario. Gen Relativ Gravit 41, 2797–2811 (2009). https://doi.org/10.1007/s10714-009-0808-8

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  • DOI: https://doi.org/10.1007/s10714-009-0808-8

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