GUP black hole remnants in quadratic gravity

Autor(es)

Kuntz, Ibere ^{[1, 2]} ; da Rocha, Roldao ^{[3, 1]}

Afiliação do(s) autor(es)

^[1] Fed Univ ABC, Ctr Math, BR-09580210 Santo Andre, SP - Brazil

^[2] Fed Univ ABC, Ctr Phys, BR-09580210 Santo Andre, SP - Brazil

^[3] Abdus Salaam Int Ctr Theoret Phys, Str Costiera 11, I-34151 Trieste - Italy

• Tipo de documento: Artigo Científico
• Fonte: EUROPEAN PHYSICAL JOURNAL C; v. 80, n. 5 MAY 27 2020.
• Citações Web of Science: 0

Resumo

The Hawking radiation of static, spherically symmetric, asymptotically flat solutions in quadratic gravity is here scrutinized, in the context of the generalized uncertainty principle (GUP). Near-center and near-horizon Frobenius expansions of these solutions are studied. Their Hawking thermal spectrum is investigated out of the tunnelling method and the WKB procedure. Computing the Hawking flux of these black hole solutions shows that, for small black holes and for a precise combination of the GUP parameter and the parameters that govern the gravitational interaction in quadratic gravity, the black hole luminosity can vanish. This yields absolutely stable mini black hole remnants in quadratic gravity. (AU)

• Processo FAPESP: 17/18897-8 - Correspondência fluido/gravidade, setores fermiônicos e suas ramificações
• Beneficiário: Roldão da Rocha
• Modalidade de apoio: Auxílio à Pesquisa - Regular