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White holes as the asymptotic limit of evaporating primordial black holes

Early Universe Cosmology and Strings Group, Center for Astrophysics, Space Physics, and Engineering Research, Baylor University, One Bear Place, Waco, TX 76706, USA

E-mail Address: Jeff_Lee@Baylor.edu

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and

Gerald B. Cleaver

http://orcid.org/0000-0001-8528-285X

Early Universe Cosmology and Strings Group, Center for Astrophysics, Space Physics, and Engineering Research, Baylor University, One Bear Place, Waco, TX 76706, USA

Department of Physics, Baylor University, One Bear Place, Waco, TX 76706, USA

E-mail Address: Gerald_Cleaver@Baylor.edu

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https://doi.org/10.1142/S0217751X16501621Cited by:0 (Source: Crossref)

Abstract

This paper examines the interaction of an intense fermion field with all of the particle species of an attometer primordial black hole’s (PBH) high energy Hawking radiation spectrum. By extrapolating to Planck-sized PBHs, it is shown that although Planck-sized PBHs closely simulate the zero absorption requirement of white holes, the absorption probability is not truly zero, and therefore, thermodynamically, Planck-sized primordial black holes are not true white holes.

Keywords:

PACS: 04.70.-s, 04.70.-Dy

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