NSR Query Results

Output year order : Descending
Format : Normal

NSR database version of April 29, 2024.

Search: Author = A.Salas

Found 3 matches.

Back to query form

2007VO08      Phys.Rev. C 76, 044602 (2007)

A.V.Voinov, S.M.Grimes, C.R.Brune, M.J.Hornish, T.N.Massey, A.Salas

Test of nuclear level density inputs for Hauser-Feshbach model calculations

NUCLEAR REACTIONS ⁵⁹Co(d, n), (d, p), (d, α), ⁵⁸Fe(³He, n), (³He, p), (³He, α)⁶¹Ni, E=7.5, 10 MeV; measured neutron, proton and α particle spectra, reaction cross sections. ⁵⁷Fe, ⁶⁰Ni, ⁶⁰Cu; deduced level densities.

doi: 10.1103/PhysRevC.76.044602
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2597.

2005PA50      Phys.Rev. C 72, 025802 (2005)

Y.Parpottas, S.M.Grimes, S.Al-Quraishi, C.R.Brune, T.N.Massey, J.E.O'Donnell, J.E.Oldendick, A.Salas, R.T.Wheeler

The ¹⁷F(p, γ)¹⁸Ne3⁺ resonance state studied with the ¹⁶O(³He, n)¹⁸Ne reaction

NUCLEAR REACTIONS ¹⁶O(³He, n), E=9.9-10.4 MeV; measured neutron spectra, σ(θ). ¹⁸Ne deduced resonance energy, width. Comparison with previous results.

doi: 10.1103/PhysRevC.72.025802
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1374.

2004PA42      Phys.Rev. C 70, 065805 (2004); Erratum Phys.Rev. C 73, 049907 (2006)

Y.Parpottas, S.M.Grimes, S.Al-Quraishi, C.R.Brune, T.N.Massey, J.E.Oldendick, A.Salas, R.T.Wheeler

Astrophysically important ²⁶Si states studied with the (³He, n) reaction and the ²⁵Al(p, γ)²⁶Si reaction rates in explosive hydrogen burning environments

NUCLEAR REACTIONS ²⁴Mg(³He, n), E=7.9, 8.11, 10.0 MeV; measured En, σ(θ). ²⁶Si deduced levels, J, π. ²⁵Al(p, γ), E=low; calculated astrophysical reaction rates.

doi: 10.1103/PhysRevC.70.065805
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1599. Data from this article have been entered in the XUNDL database. For more information, click here.