EMP and linear Schrodinger models for a conformally Bianchi I cosmology

Simple item page
dc.creatorD'Ambroise, Jennie
dc.date2008-09-28
dc.date.accessioned2026-07-07T10:06:02Z
dc.date.available2026-07-07T10:06:02Z
dc.descriptionUsing a conformal version of the Bianchi I metric and a perfect fluid energy-momentum tensor, we show that the resulting Einstein field equations are equivalent to a generalized Ermakov-Milne-Pinney equation. Using a transformation analogous to the known correspondence between the classical EMP and a linear Schrödinger equation, we then construct the linear Schrödinger formulation for this cosmological model. Also, a note is included to show the extra term that arises when the energy-momentum tensor is taken to include a second term in addition to the scalar field.
dc.identifierhttps://arxiv.org/abs/0809.4817
dc.identifierhttp://arxiv.org/abs/0809.4817
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/170195
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleEMP and linear Schrodinger models for a conformally Bianchi I cosmology
dc.typetext

Files

Collections

arXiv