The ^{144}Sm-αoptical potential at astrophysically relevant energies derived from ^{144}Sm(α,α)^{144}Sm elastic scattering
| dc.creator | Mohr, P. | |
| dc.creator | Rauscher, T. | |
| dc.creator | Oberhummer, H. | |
| dc.creator | Máté, Z. | |
| dc.creator | Fülöp, Zs. | |
| dc.creator | Somorjai, E. | |
| dc.creator | Jaeger, M. | |
| dc.creator | Staudt, G. | |
| dc.date | 1996-12-10 | |
| dc.date.accessioned | 2026-07-07T11:48:18Z | |
| dc.date.available | 2026-07-07T11:48:18Z | |
| dc.description | For the determination of the $^{144}Sm-α$ optical potential we measured the angular distribution of $^{144}Sm(α,α)^{144}Sm$ scattering at the energy $E_{lab} = 20 MeV$ with high accuracy. Using the known systematics of $α$-nucleus optical potentials we are able to derive the $^{144}Sm-α$ optical potential at the astrophysically relevant energy $E_{c.m.} = 9.5 MeV$ with very limited uncertainties. | |
| dc.description | 16 pages (uses revtex), 7 figures (uses psfig), accepted for publication in PRC, uuencoded tex-files and postscript-files available at ftp://is1.kph.tuwien.ac.at/pub/ohu/Sm.uu | |
| dc.identifier | https://arxiv.org/abs/nucl-ex/9612003 | |
| dc.identifier | http://arxiv.org/abs/nucl-ex/9612003 | |
| dc.identifier | Phys.Rev.C55:1523-1531,1997 | |
| dc.identifier | doi:10.1103/PhysRevC.55.1523 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/202876 | |
| dc.subject | Nuclear Experiment | |
| dc.subject | Nuclear Theory | |
| dc.title | The ^{144}Sm-αoptical potential at astrophysically relevant energies derived from ^{144}Sm(α,α)^{144}Sm elastic scattering | |
| dc.type | text |