A New Measure, Scale Invariance and See Saw Cosmology

dc.creatorGuendelman, E. I.
dc.date2001-06-11
dc.date.accessioned2026-07-07T04:11:48Z
dc.date.available2026-07-07T04:11:48Z
dc.descriptionThe cosmological constant problem and the possibility of obtaining a see saw cosmological effect, where the effective vacuum energy is highly suppressed by the existence of a large scale is investigated in the context of scale-invariant, generally covariant theory. Scale invariance is considered in the context of a gravitational theory where the action, in the first order formalism, is of the form $S = \int L_{1} Φd^4x$ + $\int L_{2}\sqrt{-g}d^4x$ where $Φ$ is a density built out of degrees of freedom independent of the metric.
dc.descriptionContribution to Pascos 2001
dc.identifierhttps://arxiv.org/abs/hep-th/0106085
dc.identifierhttp://arxiv.org/abs/hep-th/0106085
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/50730
dc.subjectHigh Energy Physics - Theory
dc.titleA New Measure, Scale Invariance and See Saw Cosmology
dc.typetext

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