$49.00 (cloth), 172 ppMichael C. Mackey, Time's Arrow: The Origins of Thermodynamic Behavior, Springer, Boca Raton, FL (1992).

1994 ◽  
Vol 56 (1) ◽  
pp. 166-168
Author(s):  
W HORSTHEMKE
Physics Today ◽  
1992 ◽  
Vol 45 (9) ◽  
pp. 72-72 ◽  
Author(s):  
Michael C. Mackey ◽  
Ronald F. Fox

1997 ◽  
Author(s):  
Elke E. van der Meer ◽  
Dirk Strauch ◽  
Reinhard Beyer ◽  
Herbert Hagendorf

2002 ◽  
Vol 58 (3) ◽  
pp. 313-338 ◽  
Author(s):  
R. Lee Lyman ◽  
Judith L. Harpole
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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