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Hawking radiation from quasilocal dynamical horizons

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Abstract

In completely local settings, we establish that a dynamically evolving spherically symmetric black hole horizon can be assigned a Hawking temperature and with the emission of flux, radius of the horizon shrinks.

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Acknowledgement

This article is based on a work done by the author in collaboration with A Ghosh and B Chatterjee. The author is partially supported through the UGC BSR start-up grant vide their letter No. F. 20-1(30)/2013(BSR) /3082.

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Authors and Affiliations

  1. Department of Physics and Astronomical Science, Central University of Himachal Pradesh, Kangra, 176 215, India

    AYAN CHATTERJEE

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  1. AYAN CHATTERJEE
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Correspondence to AYAN CHATTERJEE.

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CHATTERJEE, A. Hawking radiation from quasilocal dynamical horizons. Pramana - J Phys 86, 307–314 (2016). https://doi.org/10.1007/s12043-015-1150-1

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  • DOI: https://doi.org/10.1007/s12043-015-1150-1

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