Mini Black Holes

2018 ◽  
pp. 95-103
Author(s):  
Yasunori Nomura ◽  
Bill Poirier ◽  
John Terning
Keyword(s):  
Black Holes ◽  
Mini Black Holes

Upper limits on micro-mini black holes

1981 ◽  
Vol 75 (2) ◽  
pp. 229-236 ◽  
Author(s):  
Tony Rothman ◽  
Richard Matzner
Keyword(s):  
Black Holes ◽  
Upper Limits ◽  
Mini Black Holes

scholarly journals The progress of mini black holes: principles and analytical astronomical observation techniques

2021 ◽  
Vol 2083 (2) ◽  
pp. 022040
Author(s):  
Jiatong Tan
Keyword(s):  
Black Holes ◽  
General Relativity ◽  
Black Hole ◽  
Astronomical Observation ◽  
Quantum Field ◽  
Prospective Development ◽  
Stephen Hawking ◽  
Mini Black Holes ◽  
Background Models ◽  
Shed Light

Abstract Mini-black hole (MBH) is a concept first proposed by Stephen Hawking in the 1970s. Normally, exploring MBHs will enhance the understanding of quantum theory and gravity theory as well as be helpful in predicting the configuration of the early universe. Based on information retrieval, this paper summarizes the progress of MBHs and takes three major aspects: background, models, practical methods for observations, and analysis. Specifically, the descriptive equations are derived, and different models are discussed separately. These results shed light on the prospective development of quantum field theorem, general relativity, and string theory.

Mini Black Holes Decay in the Atmosphere

2010 ◽  
Author(s):  
S. Lamri ◽  
S. Kalli ◽  
J. Mimouni ◽  
N. Mebarki ◽  
J. Mimouni
Keyword(s):  
Black Holes ◽  
Mini Black Holes

Thermal relativity, modified Hawking radiation, and the generalized uncertainty principle

2019 ◽  
Vol 16 (10) ◽  
pp. 1950156
Author(s):  
Carlos Castro Perelman
Keyword(s):  
Black Holes ◽  
Black Hole ◽  
Hawking Radiation ◽  
Uncertainty Relation ◽  
Generalized Uncertainty Principle ◽  
Black Hole Entropy ◽  
The Novel ◽  
Black Hole Information ◽  
The One ◽  
Mini Black Holes

After a brief review of the thermal relativistic corrections to the Schwarzschild black hole entropy, it is shown how the Stefan–Boltzman law furnishes large modifications to the evaporation times of Planck-size mini-black holes, and which might furnish important clues to the nature of dark matter and dark energy since one of the novel consequences of thermal relativity is that black holes do not completely evaporate but leave a Planck size remnant. Equating the expression for the modified entropy (due to thermal relativity corrections) with Wald’s entropy should, in principle, determine the functional form of the modified gravitational Lagrangian [Formula: see text]. We proceed to derive the generalized uncertainty relation which corresponds to the effective temperature [Formula: see text] associated with thermal relativity and given in terms of the Hawking ([Formula: see text]) and Planck ([Formula: see text]) temperature, respectively. Such modified uncertainty relation agrees with the one provided by string theory up to first order in the expansion in powers of [Formula: see text]. Both lead to a minimal length (Planck size) uncertainty. Finally, an explicit analytical expression is found for the modifications to the purely thermal spectrum of Hawking radiation which could cast some light into the resolution of the black hole information paradox.

The signature of superstring balls near mini black holes at LHC

2012 ◽  
Vol 344 (1) ◽  
pp. 79-86 ◽  
Author(s):  
A. Sepehri ◽  
S. Shoorvazi ◽  
S. J. Fatemi ◽  
S. Doostmohammadi
Keyword(s):  
Black Holes ◽  
Mini Black Holes
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