Prediction of the Thermodynamic Behavior of Aqueous Silica in Aqueous Complex Solutions at Various Temperatures

Author(s):  
Jacques Schott ◽  
Jean-Louis Dandurand
1993 ◽  
Vol 66 (2) ◽  
pp. 125-125
Author(s):  
C. Bandy
Keyword(s):  

1978 ◽  
Vol 9 (4) ◽  
Author(s):  
F. SOMMER ◽  
B. PREDEL ◽  
D. ESCHENWECK ◽  
G. OEHME

2017 ◽  
Vol 26 (12) ◽  
pp. 1743024 ◽  
Author(s):  
Pablo Bueno ◽  
Pablo A. Cano

We argue that, when certain higher-curvature corrections are added to the four-dimensional Einstein–Hilbert action, black holes become stable below certain mass. We show this to be the case for an infinite family of ghost-free theories involving terms of arbitrarily high order in curvature. The thermodynamic behavior of the new black holes is universal for arbitrary values of the couplings, with the only exception of the Schwarzschild solution itself, which is recovered when all the couplings are set to zero. For this class of theories, the issue of non-unitary evolution is inexistent, as black holes never evaporate completely.


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