Brane Theory Solitons

Author(s):  
P. K. Townsend
Keyword(s):  
2011 ◽  
Vol 695 (1-4) ◽  
pp. 384-386 ◽  
Author(s):  
Jens Hoppe
Keyword(s):  

1995 ◽  
Vol 10 (36) ◽  
pp. 2775-2782 ◽  
Author(s):  
ICHIRO ODA

In this letter we consider an N-brane description of an (N+3)-dimensional black hole horizon. First of all, we start by examining in more detail a previous work where a string theory is used in describing the dynamics of the event horizon of a four-dimensional black hole. This is an attempt to understand the black hole thermodynamics by an effective two-dimensional field theory of the event horizon of a black hole. Then we consider a particle model defined on one-dimensional Euclidean line in a three-dimensional black hole as a target spacetime metric. By solving the field equations we find a “worldline instanton” which connects the past event horizon with the future one. This solution gives us the exact value of the Hawking temperature and to leading order the Bekenstein-Hawking formula of black hole entropy. We also show that this formalism is extensible to an arbitrary spacetime dimension. Finally we make a comment of many recent works of one-loop quantum correction to the black hole entropy.


Author(s):  
Dongmin Jang ◽  
Yoonbai Kim ◽  
O-Kab Kwon ◽  
D. D. Tolla
Keyword(s):  

2009 ◽  
Vol 2009 (03) ◽  
pp. 148-148 ◽  
Author(s):  
M Ali-Akbari
Keyword(s):  

2004 ◽  
Vol 584 (1-2) ◽  
pp. 171-177 ◽  
Author(s):  
A. De Castro ◽  
M.P. Garcia del Moral ◽  
I. Martin ◽  
A. Restuccia

2013 ◽  
Vol 10 (09) ◽  
pp. 1350038
Author(s):  
AUREL BEJANCU

In the present paper we obtain, in a covariant form, and in their full generality, the field equations in a relativistic general Kaluza–Klein space. This is done by using the Riemannian horizontal connection defined in [3], and some 4D horizontal tensor fields, as for instance: horizontal Ricci tensor, horizontal Einstein gravitational tensor field, horizontal electromagnetic energy–momentum tensor field, etc. Also, we present some inter-relations between STM theory and brane-world theory. This enables us to introduce in brane theory some electromagnetic potentials constructed by means of the warp function.


2010 ◽  
Vol 25 (09) ◽  
pp. 1863-1879 ◽  
Author(s):  
Y. K. GUPTA ◽  
PRATIBHA ◽  
SACHIN KUMAR

In view of renewed interest in the space–time embedded in higher-dimensional flat space which are useful in extrinsic gravity, string and brane theory, a set of six explicit solutions to Einstein's field equations for nonconformally flat accelerating and shearing perfect fluid plates is obtained using similarity transformations method by considering a five-dimensional flat metric. All the solutions thus obtained are analyzed physically. All the solutions are new in their respective category as far as authors are aware.


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