Black holes in anti-de Sitter (AdS) spacetime
DOI:
https://doi.org/10.15381/rif.v25i1.21966Keywords:
Black holes, anti de Sitter, Hawking temperatureAbstract
The space-time metric AdS will be determined and based on it the cosmological constant will be calculated as a function of the radius of the space AdS, using this cosmological constant the Einstein equations will be solved in order to find a metric based on from the radial coordinate of the event horizon, then some thermodynamic properties of black holes in spacetime AdS such as temperature, area and entropy will be calculated.
Downloads
Published
Issue
Section
License
Copyright (c) 2022 Fulgencio Villegas
This work is licensed under a Creative Commons Attribution 4.0 International License.
THE AUTHORS RETAIN THEIR RIGHTS:
a. The authors retain their trademark and patent rights, as well as any process or procedure described in the article.
b. The authors retain the right to share, copy, distribute, perform and publicly communicate the article published in the Revista de Investigación de Física (for example, place it in an institutional repository or publish it in a book), with an acknowledgment of its initial publication in the Revista de Investigación de Física.
c. The authors retain the right to make a subsequent publication of their work, to use the article or any part of it (for example: a compilation of their works, notes for conferences, thesis, or for a book), provided that they indicate the source. of publication (authors of the work, journal, volume, number and date).
