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arXiv · hep-th/9212027

A Time-Dependent Classical Solution of C=1 String Field Theory and Non-Perturbative Effects

Avinash Dhar·Gautam Mandal·Spenta R. Wadia
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Abstract

We describe a real-time classical solution of $c=1$ string field theory written in terms of the phase space density, $u(p,q,t)$, of the equivalent fermion theory. The solution corresponds to tunnelling of a single fermion above the filled fermi sea and leads to amplitudes that go as $\exp(- C/ \gst)$. We discuss how one can use this technique to describe non-perturbative effects in the Marinari-Parisi model. We also discuss implications of this type of solution for the two-dimensional black hole.

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Avinash Dhar, Gautam Mandal, Spenta R. Wadia. 1992-12-03. A Time-Dependent Classical Solution of C=1 String Field Theory and Non-Perturbative Effects. https://doi.org/10.1142/s0217751x93001557

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