Gravitational clustering to all perturbative orders

Please use this identifier to cite or link to this item: http://dspace.mediu.edu.my:8181/xmlui/handle/123456789/3138

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DC Field	Value	Language
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	-
Appears in Collections:	Physics and Astronomy

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