Calculation of the He-3(He-3, 2p)He-4 AND H-3(H-3, 2N)He-4 astrophysical S-factor at low energies
dc.contributor.author | Winkler, S. | |
dc.contributor.author | Krauss, H. | |
dc.contributor.author | Grun, K. | |
dc.contributor.author | Rauscher, T. | |
dc.contributor.author | Oberhummer, H. | |
dc.contributor.author | Abele, H. | |
dc.contributor.author | Staudt, G. | |
dc.date.accessioned | 2013-07-31T13:03:02Z | |
dc.date.available | 2013-07-31T13:03:02Z | |
dc.date.issued | 1992-08 | |
dc.identifier.citation | Winkler , S , Krauss , H , Grun , K , Rauscher , T , Oberhummer , H , Abele , H & Staudt , G 1992 , ' Calculation of the He-3(He-3, 2p)He-4 AND H-3(H-3, 2N)He-4 astrophysical S-factor at low energies ' , Journal of Physics G: Nuclear and Particle Physics , vol. 18 , no. 8 , pp. L147-L152 . | |
dc.identifier.issn | 0954-3899 | |
dc.identifier.uri | http://hdl.handle.net/2299/11241 | |
dc.description.abstract | We have calculated the cross sections for the charge symmetric reactions He-3(He-3,2p)He-4 and He-3(He-3,2p)He-4 at sub-Coulomb energies in the potential model. Good agreement with the experimental data is obtained. The astrophysical S factors in the thermonuclear energy range are calculated. | en |
dc.format.extent | 6 | |
dc.language.iso | eng | |
dc.relation.ispartof | Journal of Physics G: Nuclear and Particle Physics | |
dc.subject | FUSION | |
dc.subject | SCATTERING | |
dc.subject | CROSS-SECTIONS | |
dc.subject | ALPHA | |
dc.title | Calculation of the He-3(He-3, 2p)He-4 AND H-3(H-3, 2N)He-4 astrophysical S-factor at low energies | en |
dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
dc.description.status | Peer reviewed | |
rioxxterms.type | Other | |
herts.preservation.rarelyaccessed | true |
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