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Title: Observing remnants by fermions' tunneling

The standard Hawking formula predicts the complete evaporation of black holes. In this paper, we introduce effects of quantum gravity into fermions' tunneling from Reissner-Nordstrom and Kerr black holes. The quantum gravity effects slow down the increase of Hawking temperatures. This property naturally leads to a residue mass in black hole evaporation. The corrected temperatures are affected by the quantum numbers of emitted fermions. Meanwhile, the temperature of the Kerr black hole is a function of θ due to the rotation.
Authors:
 [1] ; ;  [2]
  1. College of Physics and Electronic Information, China West Normal University, Nanchong, 637009 China (China)
  2. Center for Theoretical Physics, College of Physical Science and Technology, Sichuan University, Chengdu, 610064 China (China)
Publication Date:
OSTI Identifier:
22370616
Resource Type:
Journal Article
Resource Relation:
Journal Name: Journal of Cosmology and Astroparticle Physics; Journal Volume: 2014; Journal Issue: 03; Other Information: Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; 71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; BLACK HOLES; EMISSION; EVAPORATION; FUNCTIONS; MASS; QUANTUM GRAVITY; QUANTUM NUMBERS; ROTATION; TUNNEL EFFECT