String and M theory cosmological solutions with Ramond forms
Oct, 1996
34 pages
Published in:
- Nucl.Phys.B 495 (1997) 365-399
e-Print:
- hep-th/9610238 [hep-th]
Report number:
- UPR-0723-T,
- UPR-723T,
- IASSNS-HEP-96-107,
- PUPT-1656
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Abstract:
A general framework for studying a large class of cosmological solutions of the low-energy limit of type II string theory and of M--theory, with non-trivial Ramond form fields excited, is presented. The framework is applicable to spacetimes decomposable into a set of flat, or more generally maximally symmetric, spatial subspaces, with multiple non-trivial form fields spanning one or more of the subspaces. It is shown that the corresponding low-energy equations of motion are equivalent to those describing a particle moving in a moduli space consisting of the scale factors of the subspaces together with the dilaton. The choice of which form fields are excited controls the potential term in the particle equations. Two classes of exact solutions are given, those corresponding to exciting only a single form and those with multiple forms excited which correspond to Toda theories.- 11.25.-w
- 98.80.Cq
- String theory
- M-theory
- Cosmology
- Ramond forms
- string model
- supersymmetry
- M-theory
- effective action
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