Quantum Corrections for a Cosmological String Solution
K. Behrndt

TL;DR
This paper studies quantum effects on a cosmological string solution, showing that quantum corrections can remove classical singularities and generate a potential for scalar fields.
Contribution
It introduces a method to quantize scalar fields near singularities in string cosmology, revealing non-perturbative quantum corrections that alter the classical solution.
Findings
Singularities in scalar fields are resolved by quantum corrections.
Quantum effects generate a potential for scalar fields.
Classical solutions are modified by non-perturbative quantum effects.
Abstract
We investigate quantum corrections for a cosmological solution of the string effective action. Starting point is a classical solution containing an antisymmetric tensor field, a dilaton and a modulus field which has singularities in the scalar fields. As a first step we quantize the scalar fields near the singularity with the result that the singularities disappear and that in general non-perturbative quantum corrections form a potential in the scalar fields.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Particle physics theoretical and experimental studies
