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Search: Author = M.R.James

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2017MA14      Phys.Rev. C 95, 034613 (2017)

S.G.Mashnik, L.M.Kerby, K.K.Gudima, A.J.Sierk, J.S.Bull, M.R.James

Production of energetic light fragments in extensions of the CEM and LAQGSM event generators of the Monte Carlo transport code MCNP6

NUCLEAR REACTIONS ²⁷Al(p, ⁶Li), E=200 MeV; ¹⁶O(p, ¹⁴C), (p, ⁷Be), E not given; ⁹Be(p, ⁶Li), (p, ⁷Be), E=190 MeV; ¹²C(p, α), E=1.2, 1.9, 2.5 GeV; Ag(p, ⁶Li), E=480 MeV; ⁹Be(⁴⁸Ca, X), E=140 MeV/nucleon; ¹²C(¹⁴N, n), E=400 MeV/nucleon; ¹⁸¹Ta(p, t), E=400 GeV; ¹⁹⁷Au(⁴⁰Ar, X), E=137 MeV/nucleon; ²⁰Ne, ²⁰⁸Pb(²⁰Ne, X), E=800 MeV/nucleon; ¹⁹⁷Au(p, X), E=1.2, 1.9 GeV; 197Au(¹⁹⁷Au, 12C), E=400 MeV/nucleon; Ni(p, ⁷Li), E=1.2 GeV; ²⁰⁹Bi(n, t), E=317 MeV; Cu(γ, p), E=300 MeV; ⁵⁶Fe(π⁺, n), E=1.5 GeV; ¹⁹⁷Au(p, X), E=800 MeV; ²⁰⁹Bi(n, F), E=20-1000 MeV; ¹⁹⁷Au(p, ⁷Li), E=1.2 GeV; Ni(p, t), (p, ⁷Li), E=2.5 GeV; calculated double differential σ and elemental σ for A=1-28 fragment production in reactions induced by pions, gammas, nucleons, and heavy ions at incident energies of 10 MeV/nucleon to 1 TeV/nucleon. Monte-Carlo event generators cascade-exciton model (CEM), and the Los Alamos version of the quark-gluon string model (LAQGSM) in MCNP6 transport model. Comparison with experimental data.

doi: 10.1103/PhysRevC.95.034613
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