Measure Fields, The Cosmological Constant and Scale Invariance

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dc.creatorGuendelman, E. I.
dc.date2000-08-15
dc.date.accessioned2026-07-07T04:10:21Z
dc.date.available2026-07-07T04:10:21Z
dc.descriptionThe consequences of considering the measure of integration in the action to be defined by degrees of freedom independent of the metric are studied. Models without the cosmological constant problem, new ways of spontaneously breaking scale symmetry which have an interesting cosmology and theories of extended objects (string, branes) without a fundamental scale appear possible.
dc.descriptionContribution to ICHEP 2000, Osaka, Japan. Latex 5 pages. To appear in the ICHEP proceedings in World Scientific format, 3 pages
dc.identifierhttps://arxiv.org/abs/hep-th/0008122
dc.identifierhttp://arxiv.org/abs/hep-th/0008122
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/50185
dc.subjectHigh Energy Physics - Theory
dc.titleMeasure Fields, The Cosmological Constant and Scale Invariance
dc.typetext

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