Abstract
AbstractWe study the quantum hair associated with coherent states describing slowly rotating black holes and show how it can be naturally related with the Bekenstein–Hawking entropy and with 1-loop quantum corrections of the metric for the (effectively) non-rotating case. We also estimate corrections induced by such quantum hair to the temperature of the Hawking radiation through the tunnelling method.
Funder
Conselho Nacional de Desenvolvimento Científico e Tecnológico
Chinese Scholarship Council
Coordenação de Aperfeiçoamento de Pessoal de Nível Superior
Instituto Nazionale di Fisica Nucleare
Fundação de Amparo à Pesquisa do Estado de São Paulo
Publisher
Springer Science and Business Media LLC
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