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dc.contributor.authorAbazajian, K. N.
dc.contributor.authorArnold, K.
dc.contributor.authorAustermann, J.
dc.contributor.authorBenson, B. A.
dc.contributor.authorBischoff, Colin A.
dc.contributor.authorBock, J.
dc.contributor.authorBond, J. R.
dc.contributor.authorBorrill, J.
dc.contributor.authorCalabrese, E.
dc.contributor.authorCarlstrom, J. E.
dc.contributor.authorCarvalho, C. S.
dc.contributor.authorChang, C. L.
dc.contributor.authorChiang, H. C.
dc.contributor.authorChurch, S.
dc.contributor.authorCooray, A.
dc.contributor.authorCrawford, T. M.
dc.contributor.authorDawson, K. S.
dc.contributor.authorDas, S.
dc.contributor.authorDevlin, M. J.
dc.contributor.authorDobbs, M.
dc.contributor.authorDodelson, S.
dc.contributor.authorDoré, O.
dc.contributor.authorDunkley, J.
dc.contributor.authorErrard, J.
dc.contributor.authorFraisse, A.
dc.contributor.authorGallicchio, J.
dc.contributor.authorHalverson, N. W.
dc.contributor.authorHanany, S.
dc.contributor.authorHildebrandt, S. R.
dc.contributor.authorHincks, A.
dc.contributor.authorHlozek, R.
dc.contributor.authorHolder, G.
dc.contributor.authorHolzapfel, W. L.
dc.contributor.authorHonscheid, K.
dc.contributor.authorHu, W.
dc.contributor.authorHubmayr, J.
dc.contributor.authorIrwin, K.
dc.contributor.authorJones, W. C.
dc.contributor.authorKamionkowski, M.
dc.contributor.authorKeating, B.
dc.contributor.authorKeisler, R.
dc.contributor.authorKnox, L.
dc.contributor.authorKomatsu, E.
dc.contributor.authorKovac, John M
dc.contributor.authorKuo, C.-L.
dc.contributor.authorLawrence, C.
dc.contributor.authorLee, A. T.
dc.contributor.authorLeitch, E.
dc.contributor.authorLinder, E.
dc.contributor.authorLubin, P.
dc.contributor.authorMcMahon, J.
dc.contributor.authorMiller, A.
dc.contributor.authorNewburgh, L.
dc.contributor.authorNiemack, M. D.
dc.contributor.authorNguyen, H.
dc.contributor.authorNguyen, H. T.
dc.contributor.authorPage, L.
dc.contributor.authorPryke, C.
dc.contributor.authorReichardt, C. L.
dc.contributor.authorRuhl, J. E.
dc.contributor.authorSehgal, N.
dc.contributor.authorSeljak, U.
dc.contributor.authorSievers, J.
dc.contributor.authorSilverstein, E.
dc.contributor.authorSlosar, A.
dc.contributor.authorSmith, K. M.
dc.contributor.authorSpergel, D.
dc.contributor.authorStaggs, S. T.
dc.contributor.authorStark, Antony A.
dc.contributor.authorStompor, R.
dc.contributor.authorVieregg, A. G.
dc.contributor.authorWang, G.
dc.contributor.authorWatson, S.
dc.contributor.authorWollack, E. J.
dc.contributor.authorWu, W. L. K.
dc.contributor.authorYoon, K. W.
dc.contributor.authorZahn, O.
dc.date.accessioned2014-08-05T18:40:05Z
dc.date.issued2013
dc.identifier.citationAbazajian, K. N., K. Arnold, J. Austermann, B. A. Benson, C. Bischoff, J. Bock, J. R. Bond, et al. 2013. Neutrino Physics from the Cosmic Microwave Background and Large Scale Structure. In Planning the Future of U.S. Particle Physics: The Snowmass 2013 Proceedings, ed. Norman A. Graf, Michael E. Peskin, and Jonathan L. Rosner. College Park, MD: The Division of Particles and Fields of the American Physical Society.en_US
dc.identifier.urihttp://nrs.harvard.edu/urn-3:HUL.InstRepos:12658073
dc.description.abstractThis is a report on the status and prospects of the quantification of neutrino properties through the cosmological neutrino background for the Cosmic Frontier of the Division of Particles and Fields Community Summer Study long-term planning exercise. Experiments planned and underway are prepared to study the cosmological neutrino background in detail via its influence on distance-redshift relations and the growth of structure. The program for the next decade described in this document, including upcoming spectroscopic galaxy surveys eBOSS and DESI and a new Stage-IV CMB polarization experiment CMB-S4, will achieve sigma(sum m_nu) = 16 meV and sigma(N_eff) = 0.020. Such a mass measurement will produce a high significance detection of non-zero sum m_nu, whose lower bound derived from atmospheric and solar neutrino oscillation data is about 58 meV. If neutrinos have a minimal normal mass hierarchy, this measurement will definitively rule out the inverted neutrino mass hierarchy, shedding light on one of the most puzzling aspects of the Standard Model of particle physics --- the origin of mass. This precise a measurement of N_eff will allow for high sensitivity to any light and dark degrees of freedom produced in the big bang and a precision test of the standard cosmological model prediction that N_eff = 3.046.en_US
dc.description.sponsorshipAstronomyen_US
dc.language.isoen_USen_US
dc.publisherThe Division of Particles and Fields of the American Physical Societyen_US
dc.relation.isversionofhttp://www.slac.stanford.edu/econf/C1307292/Snowmass2013Proceedings.htmlen_US
dc.relation.hasversionhttp://www.researchgate.net/profile/Edward_Wollack/publication/256926163_Neutrino_Physics_from_the_Cosmic_Microwave_Background_and_Large_Scale_Structure/file/50463524468c8a2a63.pdfen_US
dc.relation.hasversionhttp://arxiv.org/abs/1309.5383v2en_US
dash.licenseOAP
dc.titleNeutrino Physics from the Cosmic Microwave Background and Large Scale Structureen_US
dc.typeConference Paperen_US
dc.description.versionAccepted Manuscripten_US
dash.depositing.authorKovac, John M
dc.date.available2014-08-05T18:40:05Z
workflow.legacycommentsFAR 2014;en_US
dash.authorsorderedfalse
dash.contributor.affiliatedBischoff, Colin
dash.contributor.affiliatedKovac, John
dash.contributor.affiliatedStark, Antony


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