Abstract
The halo structure of Ne31 is studied using 1n-removal reactions on C and Pb targets at 230MeV/nucleon. A combined analysis of the cross sections of these nuclear and Coulomb dominated reactions that feed directly the Ne30 ground-state reveals Ne31 to have a small neutron separation energy, 0.15-0.10+0.16MeV, and spin-parity 3/2-. Consistency of the data with reaction and large-scale shell-model calculations identifies Ne31 as deformed and having a significant p-wave halo component, suggesting that halos are more frequent occurrences at the neutron drip line. © 2014 American Physical Society.
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CITATION STYLE
Nakamura, T., Kobayashi, N., Kondo, Y., Satou, Y., Tostevin, J. A., Utsuno, Y., … Yoneda, K. (2014). Deformation-driven p-wave halos at the drip line: Ne 31. Physical Review Letters, 112(14). https://doi.org/10.1103/PhysRevLett.112.142501
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