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Damping of primordial gravitational waves from generalized sources

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dc.contributor.authorDent, James B
dc.contributor.authorKrauss, Lawrence
dc.contributor.authorSabharwal, Subir
dc.contributor.authorVachaspati, Tanmay
dc.date.accessioned2015-12-13T22:30:52Z
dc.date.issued2013
dc.date.updated2015-12-11T08:57:11Z
dc.description.abstractIt has been shown that a cosmological background with an anisotropic stress tensor, appropriate for a free-streaming thermal neutrino background, can damp primordial gravitational waves after they enter the horizon, and can thus affect the cosmic microwav
dc.identifier.issn1550-7998
dc.identifier.urihttp://hdl.handle.net/1885/75037
dc.publisherAmerican Physical Society
dc.rightsAuthor/s retain copyrighten_AU
dc.sourcePhysical Review D-Particles, Fields, Gravitation and Cosmology
dc.titleDamping of primordial gravitational waves from generalized sources
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue8
local.contributor.affiliationDent, James B, University of Louisiana at Lafayette
local.contributor.affiliationKrauss, Lawrence, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationSabharwal, Subir, Arizona State University
local.contributor.affiliationVachaspati, Tanmay, Arizona State University
local.contributor.authoruidKrauss, Lawrence, u4934434
local.description.notesImported from ARIES
local.identifier.absfor020103 - Cosmology and Extragalactic Astronomy
local.identifier.ariespublicationf5625xPUB4436
local.identifier.citationvolume88
local.identifier.doi10.1103/PhysRevD.88.084008
local.identifier.scopusID2-s2.0-84885213029
local.type.statusPublished Version

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