Fluctuations in the Hawking Turok model

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dc.creatorCohn, J. D.
dc.date1998-04-27
dc.date1998-07-16
dc.date.accessioned2026-07-07T10:31:47Z
dc.date.available2026-07-07T10:31:47Z
dc.descriptionScalar and gravity wave subcurvature fluctuations are calculated for a background approximating the Hawking and Turok open universe model. The gravity wave cosmic microwave background contribution is finite and it appears that a normalizable scalar supercurvature mode is possible in some regions of parameter space.
dc.description10 pages, latex, uses revtex, prd and aps style files, final version to appear in Phys. Rev. D
dc.identifierhttps://arxiv.org/abs/astro-ph/9804289
dc.identifierhttp://arxiv.org/abs/astro-ph/9804289
dc.identifierPhys.Rev.D58:063507,1998
dc.identifierdoi:10.1103/PhysRevD.58.063507
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/178535
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleFluctuations in the Hawking Turok model
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