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arxiv: 1806.03691 · v1 · pith:F3VFB6NCnew · submitted 2018-06-10 · 🌀 gr-qc · hep-th

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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  1. Kiselev black hole and the ultra-slow evaporating behavior

    gr-qc 2026-06 unverdicted novelty 4.0

    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.