On Regular Black Holes at Finite Temperature

Author:

Ulhoa S. C.12ORCID,Spaniol E. P.3ORCID,Gomes R.4,Santos A. F.5ORCID,Santana A. E.1

Affiliation:

1. International Center of Physics, Instituto de Física, Universidade de Brasília, 70910-900 Brasília, DF, Brazil

2. Canadian Quantum Research Center, 204-3002 32 Ave, Vernon, BC, V1T 2L7, Canada

3. UDF Centro Universitário and Centro Universitário de Brasília UniCEUB, Brasília, DF, Brazil

4. Instituto de Física, Universidade de Brasília, 70910-900 Brasília, DF, Brazil

5. Instituto de Física, Universidade Federal de Mato Grosso, 78060-900, Cuiabá, Mato Grosso, Brazil

Abstract

The Thermo Field Dynamics (TFD) formalism is used to investigate the regular black holes at finite temperature. Using the Teleparalelism Equivalent to General Relativity (TEGR), the gravitational Stefan-Boltzmann law and the gravitational Casimir effect at zero and finite temperature are calculated. In addition, the first law of thermodynamics is considered. Then, the gravitational entropy and the temperature of the event horizon of a class of regular black holes are determined.

Funder

Conselho Nacional de Desenvolvimento Científico e Tecnológico

Publisher

Hindawi Limited

Subject

Nuclear and High Energy Physics

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