Semiclassical Gravity and Large Scale Structure

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dc.creatorBertoni, C.
dc.creatorCarretti, E.
dc.creatorFinelli, F.
dc.creatorMessina, A.
dc.creatorVenturi, G.
dc.date1995-05-12
dc.date1995-09-20
dc.date.accessioned2026-07-07T11:46:23Z
dc.date.available2026-07-07T11:46:23Z
dc.descriptionThe possible cosmological effects of primordial fluctuation corrections to the evolution equation of matter obtained from the Wheeler--De Witt equation are explored. In particular, both the metric and a scalar matter field are expanded around their homogeneous values and the corrections induced on the scalar field fluctuation spectrum are perturbatively estimated. Finally, results of a preliminary numerical simulation to investigate the effects on large--scale structure formation are presented.
dc.descriptionMajor changes, one figure added, several points clarified. The figure can be obtained by e-mail writing to bertoni@astbo1.bo.cnr.it
dc.identifierhttps://arxiv.org/abs/gr-qc/9505016
dc.identifierhttp://arxiv.org/abs/gr-qc/9505016
dc.identifierAstropart.Phys.5:167-174,1996
dc.identifierdoi:10.1016/0927-6505(96)00017-5
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/202205
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleSemiclassical Gravity and Large Scale Structure
dc.typetext

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