Fundamental branes and shock waves

被引:8
作者
Sfetsos, K [1 ]
机构
[1] Univ Patras, Dept Engn Sci, GR-26110 Patras, Greece
[2] Ecole Polytech, Ctr Phys Theor, F-91128 Palaiseau, France
关键词
D O I
10.1016/j.nuclphysb.2005.08.018
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We construct supersymmetric brane solutions in string and M-theory with moduli parameters that depend arbitrarily on the light-cone time. Our investigation aims in understanding time dependent phenomena in gauge theories at strong coupling within the gauge/gravity correspondence. For that reason we use, as a basic ingredient, multicenter supergravity solutions which model the Coulomb branch of the corresponding strongly coupled gauge theories. We introduce the notion of shape invariant motions and show that in a particular limit involving pulse-type motions of finite energy, the solutions represent gravitational shock waves moving on the brane background geometry. We apply the general formalism for D3-branes distributed on a disc and on a sphere as well as for NS5-branes distributed on a ring, all with time varying radii. We examine the problem of open strings attached on moving branes and suggest a mechanism which may be responsible for giving rise at a macroscopic level to gravitational shock waves. (c) 2005 Elsevier B.V. All rights reserved.
引用
收藏
页码:1 / 34
页数:34
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