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Abstract
We study charged black hole and wormhole solutions of Type 0A/IIA string theory in two dimensions, by analysing their low energy equations of motion at leading order in α′. There is a competition between Euclidean wormholes and near extremal black holes in the thermodynamic ensemble. In a certain regime of phase space, the former can disassociate into the latter. Since such solutions are of string scale near the wormhole throat that takes an AdS2 form, there is a need for an exact worldsheet description. We discuss relevant WZW coset models which we argue will shed light on this problem. Finally, we present appropriate versions of the Type 0A/IIA matrix quantum mechanics models that are expected to describe these geometries.
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1 University of British Columbia, Department of Physics and Astronomy, Vancouver, Canada (GRID:grid.17091.3e) (ISNI:0000 0001 2288 9830)
2 International Centre for Theoretical Sciences, Tata Institute of Fundamental Research, Bengaluru, India (GRID:grid.510240.2) (ISNI:0000 0004 1761 5095)
3 Perimeter Institute for Theoretical Physics, Waterloo, Canada (GRID:grid.420198.6) (ISNI:0000 0000 8658 0851)