New determination of proton spectroscopic factors and reduced widths for Be states in the MeV excitation energy region via the study of the Li(He,d)Be transfer reaction at E MeV
A. Belhout (1) S. Ouichaoui (1) · H. Beaumevieille (1) · A. Bouchemha (1) G. Bogaert (2) · S. Fortier (3) · J. Kiener (2) · A. Lefebvre-Schuhl (2) · J. M. Maison (3) · L. Rosier (3) J. Rotbard (3) · V. Tatischeff (2) · J.P. Thibaud (2) · J. Vernotte (3) ((1) Universite des Sciences et de la Technologie Houari Boumediene (USTHB), Faculte de Physique, Algeria, (2) Centre de Sciences Nucleaires et des Sciences de la Mati`ere (CSNSM), IN2P3/CNRS-Universite de Paris XI, France, (3) Institut de Physique Nucleaire, IN2P3/CNRS-Universite de Paris XI, France)
The angular distributions of Be states in the excitation energy region, E () MeV, produced in the Li(He,d)Be proton transfer reaction have been measured at the Orsay 14.8MV tandem accelerator for He ion bombarding energy, E MeV, and forward anglular range, . A high energy resolution detection system composed of a split-pole magnetic spectrometer and a ,\ position-sensitive drift chamber was used to record the energy spectra of outgoing deuterons. The measured cross section data for the direct reaction component have been separated from the compound nucleus one, then analyzed in the framework of the non local, FR-DWBA theory. New values of the and ( proton absolute and partial spectroscopic factors and related \ proton reduced widths versus the p Li channel radius have been extracted for the and isospin-mixed loosely bound states of astrophysical interest and the , unbound state of Be. They are compared to sparse earlier experimental values and to shell-model predicted ones from the literature, and are discussed. In particular, the status of the spectroscopic information on the isospin-mixed doublet is reviewed and up-dated. The application in nuclear astrophysics of the DWBA derived results is emphasised.