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One-loop $\lambda \phi^4$ theory in Robertson-Walker spacetimes: adiabatic regularization and analytic approximation

机译:Robertson-Walker时空中的单循环$ \ lambda \ phi ^ 4 $理论:   绝热正则化和解析逼近

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摘要

The renormalization of a scalar field theory with a quartic self-coupling (a$\lambda \phi^4$ theory) via adiabatic regularization in a generalRobertson-Walker spacetime is discussed. The adiabatic counterterms arepresented in a way that is most conducive to numerical computations. Avariation of the adiabatic regularization method is presented which leads toanalytic approximations for the energy-momentum tensor of the field and thequantum contribution to the effective mass of the mean field. Conservation ofthe energy-momentum tensor for the field is discussed and it is shown that thepart of the energy-momentum tensor which depends only on the mean field is notconserved but the full renormalized energy-momentum tensor is conserved asexpected and required by the semiclassical Einstein's equation. It is alsoshown that if the analytic approximations are used then the resultingapproximate energy-momentum tensor is conserved. This allows a self-consistentbackreaction calculation to be performed using the analytic approximations. Theusefulness of the approximations is discussed.
机译:讨论了在一般Robertson-Walker时空中通过绝热正则化用四次自耦合(a $ \ lambda \ phi ^ 4 $理论)对标量场理论进行的重新归一化。绝热反项以最有助于数值计算的方式表示。提出了绝热正则化方法的变量,它导致了场能量动量张量的解析近似以及量子对平均场有效质量的贡献。讨论了该场的能量动量张量的守恒性,结果表明,仅依赖于平均场的能量动量张量的一部分不守恒,但守恒的完全归一化的能量动量张量符合半经典爱因斯坦方程的要求和要求。 。还表明,如果使用解析近似,则得到的近似能量动量张量将守恒。这允许使用解析近似来执行自洽反演计算。讨论了逼近的用处。

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