Stochastic Quantization of Scalar Fields in Einstein and Rindler Spacetime

Simple item page
dc.creatorMenezes, G.
dc.creatorSvaiter, N. F.
dc.date2007-06-06
dc.date.accessioned2026-07-07T10:56:04Z
dc.date.available2026-07-07T10:56:04Z
dc.descriptionWe consider the stochastic quantization method for scalar fields defined in a curved manifold and also in a flat space-time with event horizon. The two-point function associated to a massive self-interacting scalar field is evaluated, up to the first order level in the coupling constant, for the case of an Einstein and also a Rindler Euclidean metric, respectively. Its value for the asymptotic limit of the Markov parameter is exhibited. The divergences therein are taken care of by employing a covariant stochastic regularization.
dc.identifierhttps://arxiv.org/abs/0706.0920
dc.identifierhttp://arxiv.org/abs/0706.0920
dc.identifierJ.Phys.A40:8545-8568,2007
dc.identifierdoi:10.1088/1751-8113/40/29/024
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/186290
dc.subjectHigh Energy Physics - Theory
dc.titleStochastic Quantization of Scalar Fields in Einstein and Rindler Spacetime
dc.typetext

Files

Collections

arXiv