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No Open or Flat Bouncing Cosmologies in Einstein Gravity
classification
✦ hep-th
astro-ph.COgr-qc
keywords
bouncingcosmologieseinsteinflatgravityopenorderalpha-prime
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We show that bouncing open or flat Friedmann-Robertson-Walker cosmologies are inconsistent with worldsheet string theory to first approximation. Specifically, the Virasoro constraint translates to the null energy condition in spacetime at leading order in the alpha-prime expansion. Thus one must go beyond minimally-coupled Einstein gravity in order to find bounce solutions.
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Cited by 1 Pith paper
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Energy conditions of bouncing solutions in quadratic curvature gravity coupled with a scalar field
Bouncing solutions in quadratic curvature gravity with a scalar field satisfy null, weak, and dominant energy conditions but violate the strong one when using the scalar-field energy-momentum tensor, while all four co...
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