arXiv · 0712.1815
Topology from Cosmology
Abstract
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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Vijay Balasubramanian, Per Berglund, Raul Jimenez, Joan Simon, Licia Verde. 2008-02-25. Topology from Cosmology. https://doi.org/10.1088/1126-6708%2F2008%2F06%2F025
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