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NSR database version of May 10, 2024.

Search: Author = R.B.Penney

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2009WE04      Phys.Rev. C 80, 034608 (2009); Erratum Phys.Rev. C 89, 049904 (2014)

S.P.Weppner, R.B.Penney, G.W.Diffendale, G.Vittorini

Isospin dependent global nucleon-nucleus optical model at intermediate energies

NUCLEAR REACTIONS ¹²C, ¹⁴N, ¹⁶O, ¹⁹F, ²⁷Al, ²⁸Si, ³¹P, ³²S, ³⁹K, ⁴⁰Ca, ⁴⁸Ti, ⁵¹V, ⁵²Cr, ⁵⁵Mn, ⁵⁶Fe, ⁵⁹Co(n, n), E=25-155 MeV; ^12,13C, ^16,18,20,22O, ²⁷Al, ²⁸Si, ³⁰S, ^34,40,42,44Ar, ^40,42,44,48Ca, ⁴⁵Sc, ^50,52,54Cr, ^54,56Fe, ⁵⁸Ni(p, p), E=25-155 MeV; analyzed σ, σ(θ) using isospin dependent global nucleon-nucleus optical model. ^12,13C, ¹⁶O, ²⁸Si, ⁴⁴Ar, ^40,42,44,48Ca, ^48,50Ti, ^50,52,54Cr, ^54,56Fe, ⁵⁸Ni, ⁵⁹Ni(polarized p, p), E=30-152 MeV; analyzed vector analyzing powers using isospin dependent global nucleon-nucleus optical model.

doi: 10.1103/PhysRevC.80.034608
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