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NSR database version of April 29, 2024.

Search: Author = J.Pruet

Found 8 matches.

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2011VO12      J.Korean Phys.Soc. 59, 895s (2011)

R.Vogt, J.Randrup, J.Pruet, W.Younes

Calculation of ²³⁹Pu Fission Observables in an Event-by-Event Simulation

NUCLEAR REACTIONS ²³⁹Pu(n, f), E=0.5-5.5 MeV; calculated prompt σ(En), fragment TKE, average neutron multiplicity, correlation coefficients using FREYA event generator. Comparison to data.

doi: 10.3938/jkps.59.895
Citations: PlumX Metrics

2009VO08      Phys.Rev. C 80, 044611 (2009)

R.Vogt, J.Randrup, J.Pruet, W.Younes

Event-by-event study of prompt neutrons from ²³⁹Pu(n, f)

NUCLEAR REACTIONS ²³⁹Pu(n, f), E=0.5-5.5 MeV; analyzed prompt neutron spectra from 0.1 to 10 MeV, fragment kinetic energies and excitation energies for fragment A=80-160, and average neutron multiplicities as a function of fragment mass number using Monte Carlo model FREYA. Comparisons with experimental data and ENDF-B/VII evaluations.

doi: 10.1103/PhysRevC.80.044611
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2007HA15      Nucl.Instrum.Methods Phys.Res. B259, 895 (2007)

C.Hagmann, J.Pruet

Photon production through multi-step processes important in nuclear resonance fluorescence experiments

ATOMIC PHYSICS N, Si, Fe, Ag, W, Pb, U(γ, X-ray), E=0.5-8.0 MeV; calculated effective photon production cross sections.

doi: 10.1016/j.nimb.2007.02.105
Citations: PlumX Metrics

2006PR12      Astrophys.J. 644, 1028 (2006)

J.Pruet, R.D.Hoffman, S.E.Woosley, H.-T.Janka, R.Buras

Nucleosynthesis in early supernova winds. II. The role of neutrinos

doi: 10.1086/503891
Citations: PlumX Metrics

2005PR19      Astrophys.J. 623, 325 (2005)

J.Pruet, S.E.Woosley, R.Buras, H.-T.Janka, R.D.Hoffman

Nucleosynthesis in the hot convective bubble in core-collapse supernovae

doi: 10.1086/428281
Citations: PlumX Metrics

2005PR23      J.Appl.Phys. 97, 094908 (2005)

J.Pruet, M.-A.Descalle, J.Hall, B.Pohl, S.G.Prussin

Neutron and photon transport in seagoing cargo containers

doi: 10.1063/1.1887835
Citations: PlumX Metrics

2004PR06      Nucl.Instrum.Methods Phys.Res. B222, 403 (2004)

J.Pruet, J.Hall, M.-A.Descalle, S.Prussin

Monte Carlo models for the production of β-delayed gamma-rays following fission of special nuclear materials

NUCLEAR REACTIONS ²³⁵U, ²³⁹Pu(n, F), E=thermal; calculated β-delayed Eγ from fission product decay. Monte Carlo approach.

doi: 10.1016/j.nimb.2004.03.062
Citations: PlumX Metrics

2003PR06      Astrophys.J. 586, 1254 (2003)

J.Pruet, S.E.Woosley, R.D.Hoffman

Nucleosynthesis in gamma-ray burst accretion disks

doi: 10.1086/367957
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