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DOI http://dx.doi.org/10.1103/PhysRevLett.82.3952
Title Precision Detection of the Cosmic Neutrino Background
Creator/Author Lopez, R.E. ; Turner, M.S. [Department of Physics, The University of Chicago, Chicago, Illinois 60637-1433 (United States)] ; Dodelson, S. ; Turner, M.S. [NASA/Fermilab Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, Illinois 60510-0500 (United States)] ; Heckler, A. [Department of Physics, The Ohio State University, Columbus, Ohio 43210 (United States)] ; Turner, M.S. [Department of Astronomy Astrophysics, Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637-1433 (United States)]
Publication Date1999 May 01
OSTI IdentifierOSTI ID: 341405
DOE Contract NumberFG02-91ER40690
Other Number(s)Journal ID: PRLTAO; ISSN 0031-9007; TRN: TRN: 9911M0147
Resource TypeJournal Article
Resource RelationJournal Name: Physical Review Letters; Journal Volume: 82; Journal Issue: 20; Other Information: PBD: May 1999
Subject66 PHYSICS; COSMIC NEUTRINOS; COSMIC RADIATION; BACKGROUND RADIATION; COSMOLOGY; STANDARD MODEL; QUANTUM ELECTRODYNAMICS; ELECTRON-POSITRON INTERACTIONS
Description/AbstractIn the standard big bang cosmology the canonical value for the ratio of relic neutrinos to cosmic microwave background (CMB) photons is 9/11. Within the framework of the standard model of particle physics there are small corrections, in sum about 1{percent} , due to slight heating of neutrinos by electron-positron annihilations and finite-temperature QED effects. We show that this leads to changes in the predicted CMB anisotropies that will bias determination of the other cosmological parameters if not correctly taken into account. These changes might be detected by future satellite experiments. {copyright} {ital 1999} {ital The American Physical Society}
Country of PublicationUnited States
LanguageEnglish
FormatMedium: X; Size: pp. 3952-3955
System Entry Date2009 Dec 16

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