Casadio, R., Giugno, A., Micu, O. and Orlandi, A. (2015) Thermal BEC Black Holes. http://arxiv.org/abs/1511.01279
has been cited by the following article:
TITLE: Why and How Do Black Holes Radiate?
AUTHORS: Risto Raitio
KEYWORDS: Quantum Black Hole, Hawking Radiation, Standard Model, Grand Unified Theory
JOURNAL NAME: Open Access Library Journal, Vol.2 No.12, December 18, 2015
ABSTRACT: The phenomenological model proposed in this note indicates that the black hole radiation consists of two components: the standard thermal Hawking radiation and an additional non-thermal baryonic/leptonic component due to quantum number neutralization by the no-hair theorem. The particle radiation grows relatively stronger than the Hawking radiation with increasing black hole mass, and it can be tested in principle.