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Theoretical study of halos and neutron skins through nuclear reactions and electroweak probes

Authors :
Capel, Pierre
Vanderhaeghen, Marc
Sparenberg, Jean-Marc
Vaeck, Nathalie
Sfienti, Concettina
Spichtinger, Peter
Schwenk, Achim
Colomer Martinez, Frédéric
Capel, Pierre
Vanderhaeghen, Marc
Sparenberg, Jean-Marc
Vaeck, Nathalie
Sfienti, Concettina
Spichtinger, Peter
Schwenk, Achim
Colomer Martinez, Frédéric
Publication Year :
2020

Abstract

One-nucleon halo nuclei are exotic nuclei which can be seen as a core around which orbits a loosely-bound valence nucleon. They are usually studied through reactions such as elastic scattering and breakup. The ratio method has been developed as a tool to study one-neutron halo nuclei at high energies. It consists of the ratio of angular cross sections, breakup and elastic scattering, which removes most of the sensitivity to the reaction mechanism and to the reaction model. In the simple recoil excitation and breakup (REB) model, the ratio simplifies to a form factor dependent solely on the wave function of the projectile. By measuring this observable and comparing it to the REB form factor, i.e. in the ratio method, more detailed information on the structure of the halo could be obtained. For neutron-halo nuclei at high energy, the ratio observable obtained from accurate CDCC and DEA theoretical calculations follows its REB prediction. I study the extension of this method to lower energies of the reaction which could make the measurement appropriate to facilities such as SPIRAL2 (GANIL, Caen, France) and ReA12 at FRIB (Michigan State University) and to proton halos. This is done by comparing the REB form factor to dynamical calculations of the ratio. The reactions investigated are the reaction of 11Be, the archetypical one-neutron halo nucleus, on 12C, 40Ca and 208Pb targets at 20 MeV/nucleon and of 8B, the archetypical one-proton halo nucleus, on 12C, 58Ni and 208Pb targets at44 MeV/nucleon.For these reactions, the adiabatic assumption is no longer valid due to the effect of the Coulomb interaction. This effect is mainly visible at forward angle for 11Be and is aggravated for 8B by the fact that the halo is charged. The ratio works less well than for neutron-halos at intermediate and high energies. Nevertheless, the ratio is shown to be very sensitive to the orbital angular momentum l0 in which the halo is bound and its binding energy E0, i.e. the single-particle s<br />Doctorat en Sciences de l'ingénieur et technologie<br />info:eu-repo/semantics/nonPublished

Details

Database :
OAIster
Notes :
3 full-text file(s): application/pdf | application/pdf | application/pdf, English
Publication Type :
Electronic Resource
Accession number :
edsoai.on1192460035
Document Type :
Electronic Resource