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Inelastic processes and form factor effects in the 162, 164Dy(3He, d) reactions at 46.5 MeV

dc.contributor.authorBroad, A. S.en_US
dc.contributor.authorLewis, D. A.en_US
dc.contributor.authorGray, W. S.en_US
dc.contributor.authorEllis, P. J.en_US
dc.contributor.authorDudek-Ellis, A.en_US
dc.date.accessioned2006-04-07T16:24:38Z
dc.date.available2006-04-07T16:24:38Z
dc.date.issued1976-11-23en_US
dc.identifier.citationBroad, A. S., Lewis, D. A., Gray, W. S., Ellis, P. J., Dudek-Ellis, A. (1976/11/23)."Inelastic processes and form factor effects in the 162, 164Dy(3He, d) reactions at 46.5 MeV." Nuclear Physics A 273(1): 69-94. <http://hdl.handle.net/2027.42/21636>en_US
dc.identifier.urihttp://www.sciencedirect.com/science/article/B6TVB-47201B3-1BS/2/27f473a3ac5fb821c6d2dfb07278d000en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/21636
dc.description.abstractThe 162, 164Dy(3He, d) reactions at E3He = 46.5 MeV are analyzed using the coupled channels Born approximation (CCBA) and improved form factors derived from a deformed Woods-Saxon potential. The latter are generated using the coupled channels procedure of Rost. The transitions considered populate the -[523], +[411], +[411], -[541] and + orbitals in 163, 165Ho. Indirect processes induced by inelastic scattering are found to have an influence on the cross sections comparable to that deduced for neutron transfer reactions on rare earth nuclei at lower energies. Considered alone, these can alter the cross sections even of strong transitions by a factor of two and of weaker ones by an order of magnitude. For the weaker transitions equally large changes can result when the improved form factors, rather than conventional spherical Woods-Saxon functions, are used in the calculations. In the examples considered these two effects tend to cancel, often, but not always, resulting in predicted cross sections similar in magnitude to the results of conventional DWBA calculations made with spherical Woods-Saxon form factors. The CCBA angular distributions are generally similar in shape to DWBA predictions, which usually give good fits to the experimental angular distributions over the 0-35[deg] range of the data. Compared with DWBA predictions which use (he same optical parameters, but spherical Woods-Saxon form factors, the CCBA with deformed Woods-Saxon form factors is in better overall agreement with the experimental cross-section magnitudes. However there are a number of cases in which the CCBA, although usually predicting larger cross sections than the DWBA, still underestimates the experimental cross sections by nearly factor of two. These cases all occur in the -[541] band or in the strongly Coriolis mixed +[411] and +[411] bands, and include the majority of transitions populating these orbitals. Since both nuclear structure and reaction mechanism effects are interwoven m the calculations, further data would be most useful in probing the origin of the discrepancy.en_US
dc.format.extent1407957 bytes
dc.format.extent3118 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherElsevieren_US
dc.titleInelastic processes and form factor effects in the 162, 164Dy(3He, d) reactions at 46.5 MeVen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbsecondlevelNuclear Engineering and Radiological Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.subject.hlbtoplevelEngineeringen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumCyclotron Laboratory, Physics Department, The University of Michigan, Ann Arbor, Michigan 48109, USAen_US
dc.contributor.affiliationumCyclotron Laboratory, Physics Department, The University of Michigan, Ann Arbor, Michigan 48109, USAen_US
dc.contributor.affiliationumCyclotron Laboratory, Physics Department, The University of Michigan, Ann Arbor, Michigan 48109, USAen_US
dc.contributor.affiliationotherSchool of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455; Nuclear Physics Laboratory, Oxford, UKen_US
dc.contributor.affiliationotherSchool of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455; Nuclear Physics Laboratory, Oxford, UKen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/21636/1/0000017.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1016/0375-9474(76)90301-8en_US
dc.identifier.sourceNuclear Physics Aen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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