Is the Cosmological Constant Non-Zero?

dc.creatorFrampton, P. H.
dc.date1999-01-04
dc.date.accessioned2026-07-07T02:29:52Z
dc.date.available2026-07-07T02:29:52Z
dc.descriptionThere is a discussion of the temperature anisotropy of the cosmic background radiation and of how the first Doppler peak depends on the different contributions to the vacuum energy density. An analytic calculation agrees well with numerical studies and shows that the l-value of the peak depends almost entirely on the geometry of the geodesics since recombination, and not sensitively on the details of the photon-baryon accoustic waves prior to the last scattering. This, and supernovae observations, suggest the cosmological constant is not zero.
dc.description9 pages LaTeX. Talk at ORBIS-98, Lago Mar, Fort Lauderdale, Florida. December 1998
dc.identifierhttps://arxiv.org/abs/astro-ph/9901013
dc.identifierhttp://arxiv.org/abs/astro-ph/9901013
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13640
dc.subjectAstrophysics
dc.titleIs the Cosmological Constant Non-Zero?
dc.typetext

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