Massive scalar field near a cosmic string
arXiv:gr-qc/9704077 · doi:10.1088/0264-9381/14/12/013
Abstract
The function of a massive scalar field near a cosmic string is computed and then employed to find the vacuum fluctuation of the field. The vacuum expectation value of the energy-momentum tensor is also computed using a point-splitting approach. The obtained results could be useful also for the case of self-interacting scalar fields and for the finite-temperature Rindler space theory.
15 pages, standard LaTeX, no figures. Reference [14] corrected
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Cited by in corpus (26)
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