Phys.Rev. C 84, 035808 (2011)

Y.Togano, T.Gomi, T.Motobayashi, Y.Ando, N.Aoi, H.Baba, K.Demichi, Z.Elekes, N.Fukuda, Zs.Fulop, U.Futakami, H.Hasegawa, Y.Higurashi, K.Ieki, N.Imai, M.Ishihara, K.Ishikawa, N.Iwasa, H.Iwasaki, S.Kanno, Y.Kondo, T.Kubo, S.Kubono, M.Kunibu, K.Kurita, Y.U.Matsuyama, S.Michimasa, T.Minemura, M.Miura, H.Murakami, T.Nakamura, M.Notani, S.Ota, A.Saito, H.Sakurai, M.Serata, S.Shimoura, T.Sugimoto, E.Takeshita, S.Takeuchi, K.Ue, K.Yamada, Y.Yanagisawa, K.Yoneda, A.Yoshida

Resonance states in ²⁷P using Coulomb dissociation and their effect on the stellar reaction ²⁶Si(p, γ) ²⁷P

NUCLEAR REACTIONS ²⁰⁸Pb(²⁷P, p²⁶Si), E=54.2 MeV/nucleon, [secondary ²⁷P beam from ⁹Be(³⁶Ar, X), E=115 MeV primary reaction]; measured particle spectra, (²⁶Si)p-coin, cross section, Coulomb dissociation. ²⁷P; deduced levels, resonances, J, π, multipolarity, E2 resonance strengths. Comparison with shell model calculations, and with level structure of ²⁷Mg. ²⁶Si(p, γ)²⁷P; deduced reaction rates of astrophysical interest.

doi: 10.1103/PhysRevC.84.035808