On Limiting Eigenvalue Distribution Theorems in Semiclassical Analysis

2012 ◽  
pp. 221-252 ◽  
Author(s):  
Daisy Ojeda-Valencia ◽  
Carlos Villegas-Blas
Keyword(s):  
Eigenvalue Distribution ◽  
Semiclassical Analysis

scholarly journals Domination number and Laplacian eigenvalue distribution

2016 ◽  
Vol 53 ◽  
pp. 66-71 ◽  
Author(s):  
Stephen T. Hedetniemi ◽  
David P. Jacobs ◽  
Vilmar Trevisan
Keyword(s):  
Domination Number ◽  
Eigenvalue Distribution ◽  
Laplacian Eigenvalue

scholarly journals Quantum versus semiclassical analysis of the conductivity of two-dimensional electrons in a magnetic field

1997 ◽  
Vol 56 (16) ◽  
pp. 10446-10452 ◽  
Author(s):  
M. Hayne ◽  
A. Usher ◽  
J. J. Harris ◽  
C. T. Foxon
Keyword(s):  
Magnetic Field ◽  
Two Dimensional ◽  
Semiclassical Analysis

Unimolecular dissociation rates by a semiclassical analysis of quantum resonance lifetimes

1987 ◽  
Vol 133 (6) ◽  
pp. 531-537 ◽  
Author(s):  
Vincenzo Aquilanti ◽  
Simonetta Cavalli ◽  
Gaia Grossi
Keyword(s):  
Unimolecular Dissociation ◽  
Semiclassical Analysis ◽  
Quantum Resonance

scholarly journals A Novel similarity measure based on eigenvalue distribution

2016 ◽  
Vol 170 (3) ◽  
pp. 352-362 ◽  
Author(s):  
Xu Huang ◽  
Mansi Ghodsi ◽  
Hossein Hassani
Keyword(s):  
Similarity Measure ◽  
Eigenvalue Distribution

Semiclassical analysis of post collision interaction phenomena

1976 ◽  
Vol 9 (12) ◽  
pp. L363-L367 ◽  
Author(s):  
R Morgenstern ◽  
A Niehaus ◽  
U Thielmann
Keyword(s):  
Semiclassical Analysis ◽  
Interaction Phenomena

scholarly journals Black Hole Interior from Loop Quantum Gravity

2008 ◽  
Vol 2008 ◽  
pp. 1-12 ◽  
Author(s):  
Leonardo Modesto
Keyword(s):  
Black Hole ◽  
Quantum Gravity ◽  
Event Horizon ◽  
Loop Quantum Gravity ◽  
Planck Scale ◽  
Semiclassical Analysis ◽  
Schwarzschild Solution ◽  
Quantum Black Hole ◽  
Minimum Value ◽  
Black Hole Interior

We calculate modifications to the Schwarzschild solution by using a semiclassical analysis of loop quantum black hole. We obtain a metric inside the event horizon that coincides with the Schwarzschild solution near the horizon but that is substantially different at the Planck scale. In particular, we obtain a bounce of theS2sphere for a minimum value of the radius and that it is possible to have another event horizon close to ther=0point.

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