The 6D superswirl

被引:28
|
作者
Parameswaran, SL
Tasinato, G
Zavala, I
机构
[1] Univ Oxford, Rudolf Peierls Ctr Theoret Phys, Oxford OX1 3NP, England
[2] Univ Cambridge, Ctr Math Sci, DAMTP, Cambridge CB3 0WA, England
[3] Perimeter Inst Theoret Phys, Waterloo, ON N2L 2YS, Canada
[4] Univ Durham, Dept Phys, IPPP, Durham DH1 3LE, England
基金
加拿大自然科学与工程研究理事会;
关键词
extra dimensions; gauged supergravity; supersymmetry; topological defects;
D O I
10.1016/j.nuclphysb.2005.12.020
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 present a novel supersymmetric solution to a nonlinear sigma model coupled to supergravity. The solution represents a static, supersymmetric, codimension-two object, which is different to the familiar cosmic strings. In particular, we consider 6D chiral gauged supergravity, whose spectrum contains a number of hypermultiplets. The scalar components of the hypermultiplet are charged under a gauge field, and supersymmetry implies that they experience a simple paraboloid-like (or 2D infinite well) potential, which is minimised when they vanish. Unlike conventional vortices, the energy density of our configuration is not localized to a string-like core. The solutions have two timelike singularities in the internal manifold, which provide the necessary boundary conditions to ensure that the scalars do not lie at the minimum of their potential. The 4D spacetime is flat, and the solution is a continuous deformation of the so-called "rugby ball" solution, which has been studied in the context of the cosmological constant problem. It represents an unexpected class of supersymmetric solutions to the 6D theory, which have gravity, gauge fluxes and hyperscalars all active in the background. (c) 2005 Elsevier B.V. All rights reserved.
引用
收藏
页码:49 / 72
页数:24
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