Quintessential Vanishing of the Cosmological Constant

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dc.creatorIzawa, K. -I.
dc.date2000-05-18
dc.date2000-12-14
dc.date.accessioned2026-07-07T03:41:31Z
dc.date.available2026-07-07T03:41:31Z
dc.descriptionWe consider an effective field theory description of gravity coupled to a scalar field with volume-preserving diffeomorphism and Weyl invariances. The smallness of the cosmological constant is achieved when the potential of the scalar is extremely flat. This implies a possible relationship between the smallness and the quintessential sector of the cosmological constant.
dc.description6 pages, latex
dc.identifierhttps://arxiv.org/abs/hep-ph/0005182
dc.identifierhttp://arxiv.org/abs/hep-ph/0005182
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/39610
dc.subjectHigh Energy Physics - Phenomenology
dc.titleQuintessential Vanishing of the Cosmological Constant
dc.typetext

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