The entropy of an acoustic black hole in neo-Newtonian theory

Author:

Anacleto M. A.1,Salako Ines G.23,Brito F. A.14,Passos E.15

Affiliation:

1. Departamento de Física, Universidade Federal de Campina Grande, Caixa Postal 10071, 58429-900 Campina Grande, Paraíba, Brazil

2. Ecole de Machinisme Agricole et de Construction Mécanique, Université d’Agriculture de Kétou, BP: 43 Kétou, Bénin

3. Institut de Mathématiques et de Sciences Physiques (IMSP), 01 BP 613 Porto-Novo, Bénin

4. Departamento de Física, Universidade Federal da Paraíba, Caixa Postal 5008, 58051-970 João Pessoa, Paraíba, Brazil

5. Instituto de Física, Universidade Federal do Rio de Janeiro, Caixa Postal 21945, Rio de Janeiro, Brazil

Abstract

In this paper, we consider the metric of a (2[Formula: see text]+[Formula: see text]1)-dimensional rotating acoustic black hole in the neo-Newtonian theory to compute the Hawking temperature, and applying the quantum statistical method, we calculate the statistical entropy using a corrected state density due to the generalized uncertainty principle (GUP). In our calculations, we have shown that the obtained entropy is finite and correction terms are generated. Moreover, the computation of the entropy for this method does not present logarithmic corrections.

Publisher

World Scientific Pub Co Pte Lt

Subject

Astronomy and Astrophysics,Nuclear and High Energy Physics,Atomic and Molecular Physics, and Optics

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