Solar system tests of scalar field models with an exponential potential

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dc.creatorParamos, J.
dc.creatorBertolami, O.
dc.date2007-10-30
dc.date2008-04-06
dc.date.accessioned2026-07-07T11:12:47Z
dc.date.available2026-07-07T11:12:47Z
dc.descriptionWe consider a scenario where a scalar field has dynamics ruled by an exponential potential, such as those arising from some quintessence type models, and aim at obtaining phenomenological manifestations of this entity within our Solar System. To do so, we assume a perturbative regime, derive the perturbed Schwarzschild metric, and extract the relevant post-Newtonian parameters.
dc.description5 pages
dc.identifierhttps://arxiv.org/abs/0710.5702
dc.identifierhttp://arxiv.org/abs/0710.5702
dc.identifierPhys.Rev.D77:084014,2008
dc.identifierdoi:10.1103/PhysRevD.77.084014
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191498
dc.subjectAstrophysics
dc.titleSolar system tests of scalar field models with an exponential potential
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