%0 Journal Article
%T Thermodynamics and evaporation of a modified Schwarzschild black hole in a non-commutative gauge theory
%A Araujo Filho, A. A.
%A Zare, S.
%A Porffrio, P. J.
%A Kriz, J.
%A Hassanabadi, H.
%J Physics Letters B
%D 2023
%V 838
%I Elsevier
%@ 0370-2693
%G English
%F AraujoFilho_etal2023
%O WOS:000935398000001
%O exported from refbase (https://references.ific.uv.es/refbase/show.php?record=5483), last updated on Mon, 13 Mar 2023 08:13:37 +0000
%X In this work, we study the thermodynamic properties on a non-commutative background via gravitational gauge field potentials. This procedure is accomplished after contracting de Sitter (dS) group, SO(4, 1), with the Poincare group, ISO(3, 1). Particularly, we focus on a static spherically symmetric black hole. In this manner, we calculate the modified Hawking temperature and the other deformed thermal state quantities, namely, entropy, heat capacity, Helmholtz free energy and pressure. Finally, we also investigate the black hole evaporation process in such a context.
%K Thermodynamic properties
%K Black hole
%K Non-commutative gauge theory
%K Evaporation process
%R 10.1016/j.physletb.2023.137744
%U https://arxiv.org/abs/2212.03134
%U https://doi.org/10.1016/j.physletb.2023.137744
%P 137744-9pp