Topology from Cosmology

Physics – High Energy Physics – High Energy Physics - Theory

Scientific paper

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34 pages, added references, improved argument of observable dependence on microscopic parameters

Scientific paper

10.1088/1126-6708/2008/06/025

We show that cosmological observables can constrain the topology of the compact additional dimensions predicted by string theory. To do this, we develop a general strategy for relating cosmological observables to the microscopic parameters of the potentials and field-dependent kinetic terms of the multiple scalar fields that arise in the low-energy limit of string theory. We apply this formalism to the Large Volume Scenarios in Type IIB flux compactifications where analytical calculations are possible. Our methods generalize to other settings.

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