Gravitational Clustering to All Perturbative Orders

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dc.creatorAbdalla, Elcio
dc.creatorMohayaee, Roya
dc.date1998-11-08
dc.date.accessioned2026-07-07T10:51:22Z
dc.date.available2026-07-07T10:51:22Z
dc.descriptionWe derive the time evolution of the density contrast to all orders of perturbation theory, by solving the Einstein equation for scale-invariant fluctuations. These fluctuations are represented by an infinite series in inverse powers of the radial parameter. In addition to the standard growing modes, we find infinitely many more new growing modes for open and closed universes.
dc.description3 pages, revtex
dc.identifierhttps://arxiv.org/abs/astro-ph/9811119
dc.identifierhttp://arxiv.org/abs/astro-ph/9811119
dc.identifierBraz.J.Phys.31:42-44,2001
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/184799
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleGravitational Clustering to All Perturbative Orders
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