Radiación de Hawking

Authors

  • J. M Fernández Cristóbal

Keywords:

Quantization on curved spacetime, Hawking radiation, tunneling method, apparent horizon

Abstract

The aim of this article is to provide a general analysis of the so-called Hawking radiation in black holes from a didactic perspective, including a brief introduction to quantization in curved spacetime. Two main methods for obtaining the radiation spectrum are explained: the original one due to Hawking and the tunneling method. Also, it is shown how the second mechanism can be extended to obtain the radiation spectrum in a different kind of horizon, that associated to the Friedmann-Robertson-Walker metric. Finally, some recent objections to the derivation by the tunneling method are mentioned.

Downloads

Published

2010-01-01

How to Cite

[1]
J. M Fernández Cristóbal, “Radiación de Hawking”, Rev. Mex. Fis. E, vol. 56, no. 2 Jul-Dec, pp. 213–226, Jan. 2010.

Issue

Vol. 56 No. 2 Jul-Dec (2010): Revista Mexicana de Física E

Section

Artículos

License

Copyright (c) 2019 Revista Mexicana de Física E

Creative Commons License

This work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.

Authors retain copyright and grant the Revista Mexicana de Física E right of first publication with the work simultaneously licensed under a CC BY-NC-ND 4.0 that allows others to share the work with an acknowledgement of the work's authorship and initial publication in this journal.