CMB and Inflation: the report from Snowmass 2001

dc.creatorChurch, S.
dc.creatorJaffe, A.
dc.creatorKnox, L.
dc.date2001-11-10
dc.date.accessioned2026-07-07T11:28:50Z
dc.date.available2026-07-07T11:28:50Z
dc.descriptionAstrophysical observations provide the best evidence of physics beyond the particle physicists' standard model. Over the past decade, the case has solidified for inflation, dark energy, dark matter and massive neutrinos. In this report we focus on inflation and dark energy as constrained by the CMB--first the evidence from current observations and then what we can expect to learn in the future. High energy physicists can contribute to the succesful realization of this future, both observationally and theoretically.
dc.description19 pages, 12 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0111203
dc.identifierhttp://arxiv.org/abs/astro-ph/0111203
dc.identifiereConfC010630:P406,2001
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196521
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleCMB and Inflation: the report from Snowmass 2001
dc.typetext

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