What Do We Really Know About Cosmic Acceleration?

dc.creatorShapiro, Charles
dc.creatorTurner, Michael S.
dc.date2005-12-23
dc.date.accessioned2026-07-07T10:43:30Z
dc.date.available2026-07-07T10:43:30Z
dc.descriptionEssentially all of our knowledge of the acceleration history of the Universe - including the acceleration itself - is predicated upon the validity of general relativity. Without recourse to this assumption, we use SNeIa to analyze the expansion history and find (i) very strong (5 sigma) evidence for a period of acceleration, (ii) strong evidence that the acceleration has not been constant, (iii) evidence for an earlier period of deceleration and (iv) only weak evidence that the Universe has not been decelerating since z~0.3.
dc.description9 pages, 8 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0512586
dc.identifierhttp://arxiv.org/abs/astro-ph/0512586
dc.identifierAstrophys.J.649:563-569,2006
dc.identifierdoi:10.1086/506470
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/182262
dc.subjectAstrophysics
dc.titleWhat Do We Really Know About Cosmic Acceleration?
dc.typetext

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