Cosmological Perturbations with Multiple Scalar Fields

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dc.creatorHwang, J.
dc.date1996-08-08
dc.date.accessioned2026-07-07T03:31:14Z
dc.date.available2026-07-07T03:31:14Z
dc.descriptionIn this brief note we present a set of equations describing the evolution of perturbed scalar fields in a cosmological spacetime with multiple scalar fields. We take into account of the simultaneously excited full metric perturbations in the context of the uniform-curvature gauge which is known to be the best choice. The equations presented in a compact form will be useful for handling the structure formation processes under the multiple episodes of inflation.
dc.description2 pages, revtex, no figures
dc.identifierhttps://arxiv.org/abs/gr-qc/9608018
dc.identifierhttp://arxiv.org/abs/gr-qc/9608018
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35790
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleCosmological Perturbations with Multiple Scalar Fields
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