The astrophysical S-factor of the reaction Be-7(P,gamma)B-8 in the direct capture model

dc.contributor.author	Krauss, H.
dc.contributor.author	Grun, K.
dc.contributor.author	Rauscher, T.
dc.contributor.author	Oberhummer, H.
dc.date.accessioned	2013-07-02T14:47:06Z
dc.date.available	2013-07-02T14:47:06Z
dc.date.issued	1993
dc.identifier.citation	Krauss , H , Grun , K , Rauscher , T & Oberhummer , H 1993 , ' The astrophysical S-factor of the reaction Be-7(P,gamma)B-8 in the direct capture model ' , Annalen der Physik , vol. 2 , no. 3 , pp. 258-266 .
dc.identifier.issn	0003-3804
dc.identifier.uri	http://hdl.handle.net/2299/11046
dc.description.abstract	The astrophysical S-factor for the reaction Be-7(p, gamma)B-8 up to an energy of 2 MeV (c.m.) and the capture cross section of Li-7(n, gamma)Li-8 up to 1 MeV (c.m.) are calculated using the Direct Capture model (DC). Both calculations are in good agreement with experimental data.	en
dc.format.extent	9
dc.format.extent	126866
dc.language.iso	eng
dc.relation.ispartof	Annalen der Physik
dc.subject	LI-7(N,GAMMA)LI-8
dc.subject	SCATTERING
dc.subject	NUCLEAR REACTIONS
dc.subject	SOLAR NEUTRINOS
dc.subject	ASTROPHYSICAL S-FACTOR
dc.subject	BE-7(P,GAMMA)B-8
dc.subject	CROSS-SECTION
dc.title	The astrophysical S-factor of the reaction Be-7(P,gamma)B-8 in the direct capture model	en
dc.contributor.institution	Centre for Astrophysics Research (CAR)
dc.description.status	Peer reviewed
rioxxterms.type	Journal Article/Review
herts.preservation.rarelyaccessed	true