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Heating up the cold bounce
Self-dual string cosmological models provide an effective example of bouncing solutions where a phase of accelerated contraction smoothly evolves into an epoch of decelerated Friedmann--Robertson--Walker expansion dominated by the dilaton. While the transition to the expanding regime occurs at sub-P...
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| Lenguaje: | eng |
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2004
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| Acceso en línea: | https://dx.doi.org/10.1088/0264-9381/21/17/010 http://cds.cern.ch/record/741423 |