Decaying Gravity

dc.creatorClifton, T.
dc.creatorBarrow, John D.
dc.date2006-03-29
dc.date2006-05-18
dc.date.accessioned2026-07-07T12:29:09Z
dc.date.available2026-07-07T12:29:09Z
dc.descriptionWe consider the possibility of energy being exchanged between the scalar and matter fields in scalar-tensor theories of gravity. Such an exchange provides a new mechanism which can drive variations in the gravitational 'constant' G. We find exact solutions for the evolution of spatially flat Friedman-Roberston-Walker cosmologies in this scenario and discuss their behaviour at both early and late times. We also consider the physical consequences and observational constraints on these models.
dc.description13 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/0603116
dc.identifierhttp://arxiv.org/abs/gr-qc/0603116
dc.identifierPhys.Rev.D73:104022,2006
dc.identifierdoi:10.1103/PhysRevD.73.104022
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/215777
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleDecaying Gravity
dc.typetext

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