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Dark energy effects on charged and rotating black holes

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Abstract.

Using the canonical typicality method, we reconsider the study of dark energy effects on four-dimensional black holes. Concretely, we investigate the associated influences on the spectrum of various black hole backgrounds including the charged and the rotating ones. For such black hole solutions, we first elaborate analytically the corresponding radiation spectrum, the Hawking temperature and the dark information. Then, we discuss and analyze the corresponding findings. This work, recovering the results of the Schwarzschild black hole, confirms that dark energy can be considered as a cooling system surrounding the black holes providing a colder radiation and a slower Hawking radiation process.

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Author information

Authors and Affiliations

  1. Equipe des Sciences de la Matière et du Rayonnement, ESMAR, Département de Physique Faculté des Sciences, Université Mohammed V, Rabat, Morocco

    A. Belhaj

  2. Département de Physique, LabSIMO, Faculté des Sciences, Université Ibn Tofail, Kénitra, Morocco

    A. El Balali, W. El Hadri & M. B. Sedra

  3. High Energy and Astrophysics Laboratory, FSSM, Cadi Ayyad University, P.O.B. 2390, Marrakesh, Morocco

    H. El Moumni

  4. LMTI, Faculty of Sciences, Ibn Zohr University, B.P 8106, Agadir, Morocco

    H. El Moumni

Authors
  1. A. Belhaj
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  2. A. El Balali
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  3. W. El Hadri
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  4. H. El Moumni
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  5. M. B. Sedra
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Correspondence to A. Belhaj.

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Belhaj, A., El Balali, A., El Hadri, W. et al. Dark energy effects on charged and rotating black holes. Eur. Phys. J. Plus 134, 422 (2019). https://doi.org/10.1140/epjp/i2019-12803-y

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