Zero Mass Remnant as an Asymptotic State of Hawking Evaporation
classification
🌀 gr-qc
hep-th
keywords
remnantachieveallowsalthoughamountasymptoticblackcompletely
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We show that although generalized uncertainty principle with negative parameter allows black holes to evaporate completely, this process takes an infinite amount time to achieve, resulting in a metastable remnant.
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Cited by 1 Pith paper
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Kiselev black hole and the ultra-slow evaporating behavior
Lowering the quintessence state parameter w_q in Kiselev black holes produces ultra-slow evaporation distinct from PFDM and Horndeski cases, offering a possible constraint on w_q.
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