Black hole evaporation in conformal gravity

doi:https://doi.org/10.1088/1475-7516/2017/09/033

Title: Black hole evaporation in conformal gravity

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Abstract

We study the formation and the evaporation of a spherically symmetric black hole in conformal gravity. From the collapse of a spherically symmetric thin shell of radiation, we find a singularity-free non-rotating black hole. This black hole has the same Hawking temperature as a Schwarzschild black hole with the same mass, and it completely evaporates either in a finite or in an infinite time, depending on the ensemble. We consider the analysis both in the canonical and in the micro-canonical statistical ensembles. Last, we discuss the corresponding Penrose diagram of this physical process.

Authors:

Bambi, Cosimo; Rachwał, Lesław ^[1]; Modesto, Leonardo ^[2]; Porey, Shiladitya ^[3]

Center for Field Theory and Particle Physics and Department of Physics, Fudan University, 220 Handan Road, 200433 Shanghai (China)
Department of Physics, Southern University of Science and Technology, 1088 Xueyuan Road, Shenzhen 518055 (China)
Department of Physics, Indian Institute of Technology, 208016 Kanpur (India)

Publication Date:: 2017-09-01

OSTI Identifier:: 22667677

Resource Type:: Journal Article

Journal Name:: Journal of Cosmology and Astroparticle Physics

Additional Journal Information:: Journal Volume: 2017; Journal Issue: 09; Other Information: Country of input: International Atomic Energy Agency (IAEA); Journal ID: ISSN 1475-7516

Country of Publication:: United States

Language:: English

Subject:: 79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; BLACK HOLES; EVAPORATION; GRAVITATION; MASS; SCHWARZSCHILD RADIUS; SINGULARITY; SPHERICAL CONFIGURATION; SYMMETRY

Citation Formats


                    Bambi, Cosimo, Rachwał, Lesław, Modesto, Leonardo, and Porey, Shiladitya. Black hole evaporation in conformal gravity.  United States: N. p., 2017. 
        Web.  doi:10.1088/1475-7516/2017/09/033.

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                    Bambi, Cosimo, Rachwał, Lesław, Modesto, Leonardo, & Porey, Shiladitya. Black hole evaporation in conformal gravity.  United States.  https://doi.org/10.1088/1475-7516/2017/09/033

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                    Bambi, Cosimo, Rachwał, Lesław, Modesto, Leonardo, and Porey, Shiladitya. Fri .  
        "Black hole evaporation in conformal gravity".  United States.  https://doi.org/10.1088/1475-7516/2017/09/033.

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@article{osti_22667677,

  title        = {Black hole evaporation in conformal gravity},

  author       = {Bambi, Cosimo and Rachwał, Lesław and Modesto, Leonardo and Porey, Shiladitya},

  abstractNote = {We study the formation and the evaporation of a spherically symmetric black hole in conformal gravity. From the collapse of a spherically symmetric thin shell of radiation, we find a singularity-free non-rotating black hole. This black hole has the same Hawking temperature as a Schwarzschild black hole with the same mass, and it completely evaporates either in a finite or in an infinite time, depending on the ensemble. We consider the analysis both in the canonical and in the micro-canonical statistical ensembles. Last, we discuss the corresponding Penrose diagram of this physical process.},

  doi          = {10.1088/1475-7516/2017/09/033},

  url          = {https://www.osti.gov/biblio/22667677},
  journal      = {Journal of Cosmology and Astroparticle Physics},

  issn         = {1475-7516},

  number       = 09,

  volume       = 2017,

  place        = {United States},

  year         = {2017},

  month        = {9}

}

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