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Gravitational clustering to all perturbative orders

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dc.creator Abdalla Elcio
dc.creator Mohayaee Roya
dc.date 2001
dc.date.accessioned 2013-05-30T00:38:41Z
dc.date.available 2013-05-30T00:38:41Z
dc.date.issued 2013-05-30
dc.identifier http://www.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332001000100007
dc.identifier http://www.doaj.org/doaj?func=openurl&genre=article&issn=01039733&date=2001&volume=31&issue=1&spage=42
dc.identifier.uri http://koha.mediu.edu.my:8181/jspui/handle/123456789/3138
dc.description We 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.publisher Sociedade Brasileira de Física
dc.source Brazilian Journal of Physics
dc.title Gravitational clustering to all perturbative orders


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