Stability of charged black holes in string theory under charged massive scalar perturbations

2013 ◽  
Vol 88 (12) ◽  
Author(s):  
Ran Li
2009 ◽  
Author(s):  
D. Georgieva ◽  
I. Stefanov ◽  
M. Todorov ◽  
S. Yazadjiev ◽  
Michail D. Todorov ◽  
...  

1992 ◽  
Vol 375 (2) ◽  
pp. 421-450 ◽  
Author(s):  
Michael D. McGuigan ◽  
Chiara R. Nappi ◽  
Scott A. Yost

2001 ◽  
Vol 36 (1) ◽  
pp. 125-128
Author(s):  
Wang Shi-Liang ◽  
Jing Ji-Liang ◽  
Wang Yong-Jiu

1996 ◽  
Vol 11 (37) ◽  
pp. 2933-2939 ◽  
Author(s):  
A. GHOSH ◽  
P. MITRA

For extremal charged black holes, the thermodynamic entropy is proportional to the mass or charges but not proportional to the area. This is demonstrated here for dyonic extremal black hole solutions of string theory. It is pointed out that these solutions have zero classical action although the area is nonzero. By combining the general form of the entropy allowed by thermodynamics with recent observations in the literature it is possible to fix the entropy almost completely.


1992 ◽  
Vol 45 (10) ◽  
pp. 3888-3888 ◽  
Author(s):  
David Garfinkle ◽  
Gary T. Horowitz ◽  
Andrew Strominger

Axioms ◽  
2020 ◽  
Vol 9 (1) ◽  
pp. 33 ◽  
Author(s):  
Grigoris Panotopoulos

We compute the quasinormal frequencies for scalar perturbations of charged black holes in five-dimensional Einstein-power-Maxwell theory. The impact on the spectrum of the electric charge of the black holes, of the angular degree, of the overtone number, and of the mass of the test scalar field is investigated in detail. The quasinormal spectra in the eikonal limit are computed as well for several different space-time dimensionalities.


1993 ◽  
Vol 47 (12) ◽  
pp. 5259-5269 ◽  
Author(s):  
S. Mignemi ◽  
N. R. Stewart

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