Uniform Expansion of the Thermonuclear Reaction Rate Formula

Please use this identifier to cite or link to this item: http://dspace.mediu.edu.my:8181/xmlui/handle/123456789/2234

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DC Field	Value	Language
dc.creator	Hussein M.S.	-
dc.creator	Pato M.P.	-
dc.date	1997	-
dc.date.accessioned	2013-05-29T22:01:10Z	-
dc.date.available	2013-05-29T22:01:10Z	-
dc.date.issued	2013-05-30	-
dc.identifier	http://www.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97331997000300005	-
dc.identifier	http://www.doaj.org/doaj?func=openurl&genre=article&issn=01039733&date=1997&volume=27&issue=3&spage=	-
dc.identifier.uri	http://koha.mediu.edu.my:8181/jspui/handle/123456789/2234	-
dc.description	The nuclear reaction rate formula used in stellar evolution calculation is carefully examined. A uniform expansion is performed up to fourth order in the relevant physical parameter. The convergence of the series is assessed and a semianalytical expression is derived, valid for all values of the expansion parameter. The formulae with electron screening and plasma dissipative collision effects are also evaluated. The agreement of the approximate analytical formulae with the exact result is excellent over a wide range of values of the parameters	-
dc.publisher	Sociedade Brasileira de Física	-
dc.source	Brazilian Journal of Physics	-
dc.title	Uniform Expansion of the Thermonuclear Reaction Rate Formula	-
Appears in Collections:	Physics and Astronomy

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