The 144Sm-αoptical potential at astrophysically relevant energies derived from 144Sm(α,α)144Sm elastic scattering
P. Mohr, T. Rauscher, H. Oberhummer, Z. Máté, Zs. Fülöp, E. Somorjai, M. Jaeger, G. Staudt
Abstract
For the determination of the 144Sm-α optical potential we measured the angular distribution of 144Sm(α,α)144Sm scattering at the energy Elab = 20 MeV with high accuracy. Using the known systematics of α-nucleus optical potentials we are able to derive the 144Sm-α optical potential at the astrophysically relevant energy Ec.m. = 9.5 MeV with very limited uncertainties.
Create a lesson
Related papers
Differential measurement of global polarization of Λ, Ξ, and Ω hyperons in Au+Au collisions at sNN=7.7--27~GeV from the RHIC Beam Energy Scan-II
The STAR Collaboration
Regularity of core coupled high-spin structure in neutron-rich 196-202Au isotopes approaching N =126
Y. Cho, Y. H. Kim, A. Navin et al.
Global polarization of Λ, Ξ, and Ω hyperons in Au+Au collisions from the RHIC Beam Energy Scan-II
STAR Collaboration
Probing the charm-quark dead cone effect in heavy ion collisions
CMS Collaboration
Estimating cosmogenic backgrounds in nEXO at SNOLAB using Geant4 and FLUKA
R. Ross, S. Al Kharusi, T. Brunner et al.
Current Results on Light Hypernuclei in the WASA-FRS HypHI Experiment
C. Rappold, P. Achenbach, H. Alibrahim Alfaki et al.