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Symmetries for generating string cosmologies
被引:12
作者:
Copeland, EJ
[1
]
Lidsey, JE
Wands, D
机构:
[1] Univ Sussex, Ctr Theoret Phys, Brighton BN1 9QH, E Sussex, England
[2] Univ Sussex, Ctr Astron, Brighton BN1 9QH, E Sussex, England
[3] Queen Mary & Westfield, Sch Math Sci, Astron Unit, London E1 4NS, England
[4] Univ Portsmouth, Sch Comp Sci & Math, Portsmouth PO1 2EG, Hants, England
来源:
PHYSICAL REVIEW D
|
1998年
/
58卷
/
04期
关键词:
D O I:
10.1103/PhysRevD.58.043503
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
We discuss the symmetry properties of the low-energy effective action of the type IIB superstring that may be employed to derive four-dimensional solutions. A truncated effective action, compactified on a six-torus, but including both Neveu-Schwarz-Neveu-Schwarz and Ramond-Ramond field strengths, can be expressed as a non-linear sigma model which is invariant under global SL(3,R) transformations. This group contains as a sub-group the SL(2,R) symmetry of the ten-dimensional theory and a discrete Z(2) reflection symmetry which leads to a further SL(2,R) sub-group. The symmetries are employed to analyze a general class of spatially homogeneous cosmological solutions with non-trivial Ramond-Ramond fields.
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页码:435031 / 4350311
页数:11
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