Semiclassical analysis of driven-dissipative excitonic condensation

2021 ◽  
Author(s):  
R. Imai ◽  
J. Takahashi ◽  
T. Oyama ◽  
Y. Yamanaka
1997 ◽  
Vol 56 (16) ◽  
pp. 10446-10452 ◽  
Author(s):  
M. Hayne ◽  
A. Usher ◽  
J. J. Harris ◽  
C. T. Foxon

1987 ◽  
Vol 133 (6) ◽  
pp. 531-537 ◽  
Author(s):  
Vincenzo Aquilanti ◽  
Simonetta Cavalli ◽  
Gaia Grossi

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

2008 ◽  
Vol 2008 ◽  
pp. 1-12 ◽  
Author(s):  
Leonardo Modesto

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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