Higgs instability in lower-dimensional type-I string theory

1990 ◽  
Vol 41 (8) ◽  
pp. 2549-2557 ◽  
Author(s):  
L. Clavelli ◽  
P. H. Cox ◽  
B. Harms
1998 ◽  
Vol 437 (3-4) ◽  
pp. 318-324 ◽  
Author(s):  
John March-Russell
Keyword(s):  
Type I ◽  

1996 ◽  
Vol 11 (09) ◽  
pp. 689-713 ◽  
Author(s):  
A.A. TSEYTLIN

Supersymmetric extreme dyonic black holes of toroidally compactified heterotic or type-II string theory can be viewed as lower-dimensional images of solitonic strings wound around a compact dimension. We consider conformal sigma models which describe string configurations corresponding to various extreme dyonic black holes in four and five dimensions. These conformal models have regular short-distance region equivalent to a WZW theory with level proportional to magnetic charges. Arguments are presented suggesting a universal relation between the black hole entropy (area) and the statistical entropy of BPS-saturated oscillation states of solitonic string.


1997 ◽  
Vol 415 (2) ◽  
pp. 135-143 ◽  
Author(s):  
Justin R. David ◽  
Avinash Dhar ◽  
Gautam Mandal
Keyword(s):  

2001 ◽  
Vol 49 (4-6) ◽  
pp. 503-510
Author(s):  
M. Frau ◽  
L. Gallot ◽  
A. Lerda ◽  
P. Strigazzi
Keyword(s):  

1996 ◽  
Vol 387 (4) ◽  
pp. 743-749 ◽  
Author(s):  
Carlo Angelantonj ◽  
Massimo Bianchi ◽  
Gianfranco Pradisi ◽  
Augusto Sagnotti ◽  
Yassen S. Stanev
Keyword(s):  

2001 ◽  
Vol 49 (4-6) ◽  
pp. 503 ◽  
Author(s):  
M. Frau ◽  
L. Gallot ◽  
A. Lerda ◽  
P. Strigazzi
Keyword(s):  

2020 ◽  
Author(s):  
Wen-Xiang Chen

We know that string theory is purely geometric.It believes that, through the holographic principle, quantum effects can be generated by projecting onto the lower dimensional multidimensional geometry.There is a corollary here that quantum radiation cannot produce thermal effects.In this paper, in the case of superradiation, the boson boundary condition is presupposed first, which is possible to obtain higher energy than the traditional quantum effect, while the extra energy belongs to the classical domain, namely heat.


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