Indirect methods in nuclear astrophysics

dc.contributor.author	Bertulani, C.
dc.contributor.author	Shubhchintak
dc.contributor.author	Mukhamedzhanov, A.
dc.contributor.author	Kadyrov, Alisher
dc.contributor.author	Kruppa, A.
dc.contributor.author	Pang, D.
dc.date.accessioned	2017-01-30T10:56:54Z
dc.date.available	2017-01-30T10:56:54Z
dc.date.created	2016-05-25T19:30:16Z
dc.date.issued	2016
dc.identifier.citation	Bertulani, C. and Shubhchintak and Mukhamedzhanov, A. and Kadyrov, A. and Kruppa, A. and Pang, D. 2016. Indirect methods in nuclear astrophysics.Journal of Physics. 703: Article 012007.
dc.identifier.uri	http://hdl.handle.net/20.500.11937/6983
dc.identifier.doi	10.1088/1742-6596/703/1/012007
dc.description.abstract	We discuss recent developments in indirect methods used in nuclear astrophysics to determine the capture cross sections and subsequent rates of various stellar burning processes, when it is difficult to perform the corresponding direct measurements. We discuss in brief, the basic concepts of Asymptotic Normalization Coefficients, the Trojan Horse Method, the Coulomb Dissociation Method, (d,p), and charge-exchange reactions.
dc.rights.uri	http://creativecommons.org/licenses/by/3.0/
dc.title	Indirect methods in nuclear astrophysics
dc.type	Conference Paper
dcterms.source.volume	703
dcterms.source.issn	1742-6588
dcterms.source.title	Journal of Physics: Conference Series
dcterms.source.series	Journal of Physics: Conference Series
curtin.department	Department of Physics and Astronomy
curtin.accessStatus	Open access via publisher

Except where otherwise noted, this item's license is described as http://creativecommons.org/licenses/by/3.0/

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