{"title":"Schrödinger evolution of a scalar field in Riemannian and pseudo Riemannian expanding metrics","authors":"Z. Haba","doi":"10.1209/0295-5075/ad64fe","DOIUrl":null,"url":null,"abstract":"\n We study the quantum field theory (QFT) of a scalar field in the Schrödinger picture in the functional formulation. We derive a formula for the evolution kernel in a flat expanding metric. We discuss a transition between Riemannian and pseudoRiemannian metrics gµν (signature inversion). We express the real time Schrödinger evolution by the Brownian motion. We discuss the Feynman integral for a scalar field in a radiation background. We show that the unitary Schrödinger evolution for positive time can go over for negative time into a dissipative evolution as a consequence of the imaginary value of √- det(gµν). The time evolution remains unitary if √- det(gµν) in the Hamiltonian is replaced by √| det(gµν)|.","PeriodicalId":503117,"journal":{"name":"Europhysics Letters","volume":" 19","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-07-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Europhysics Letters","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1209/0295-5075/ad64fe","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
We study the quantum field theory (QFT) of a scalar field in the Schrödinger picture in the functional formulation. We derive a formula for the evolution kernel in a flat expanding metric. We discuss a transition between Riemannian and pseudoRiemannian metrics gµν (signature inversion). We express the real time Schrödinger evolution by the Brownian motion. We discuss the Feynman integral for a scalar field in a radiation background. We show that the unitary Schrödinger evolution for positive time can go over for negative time into a dissipative evolution as a consequence of the imaginary value of √- det(gµν). The time evolution remains unitary if √- det(gµν) in the Hamiltonian is replaced by √| det(gµν)|.