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Euclidean thermal spinor Green's function in the spacetime of a straight cosmic string

B. Linet

gr-qcarXiv:gr-qc/9506011

Abstract

Within the framework of the quantum field theory at finite temperature on a conical space, we determine the Euclidean thermal spinor Green's function for a massless spinor field. We then calculate the thermal average of the energy-momentum tensor of a thermal bath of massless fermions. In the high-temperature limit, we find that the straight cosmic string does not perturb the thermal bath

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