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NSR database version of April 11, 2024.

Search: Author = K.Hiroshi

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2003HO22      Nucl.Phys. A719, 9c (2003)

A.Horvath, A.Galonsky, N.Carlin, F.Deak, T.Gomi, V.Guimaraes, Y.Higurashi, K.Hiroshi, K.Ieki, Y.Iwata, A.Kiss, J.Kolata, T.Rauscher, H.Schelin, J.von Schwarzenberg, Z.Seres, S.Takeuchi, S.Typel, R.Warner, J.Weiner

Measurements of astrophysical neutron capture cross sections via the inverse reaction

NUCLEAR REACTIONS C, Al, Cu, Sn, Pb(¹⁵C, nX), E=35 MeV/nucleon; C, Al, Cu, Sn, Pb(⁹Li, nX), E=40 MeV/nucleon; measured neutron spectra, (fragment)(neutron)-coin, dissociation yields. ⁸Li, ¹⁴C(n, γ), E=low; deduced astrophysical reaction rates.

doi: 10.1016/S0375-9474(03)00951-5
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