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NSR database version of April 27, 2024.

Search: Author = M.Rayet

Found 11 matches.

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2006UT04      Nucl.Phys. A777, 459 (2006)

H.Utsunomiya, P.Mohr, A.Zilges, M.Rayet

Direct determination of photodisintegration cross sections and the p-process

NUCLEAR REACTIONS ¹⁸⁶W, ^185,187Re, ^190,192,198Pt, ¹⁹⁷Au, ^196,198,204Hg, ²⁰⁴Pb(γ, n), E=spectrum; analyzed reaction rate. ¹⁴⁸Gd(γ, n), (γ, α), E=0-12 MeV; calculated reaction rate integral. Hauser-Feshbach model. ¹⁸¹Ta(γ, n), E=7.5-13.5 MeV; analyzed σ. Hauser-Feshbach with quasi-particle RPA. Comparison with data.

NUCLEAR STRUCTURE ¹³⁸Ba, ¹⁴⁰Ce, ¹⁴²Nd, ¹⁴⁴Sm; analyzed B(E1).

doi: 10.1016/j.nuclphysa.2004.06.025
Citations: PlumX Metrics

2003GO24      Nucl.Phys. A718, 596c (2003)

S.Goriely, J.Jose, M.Hernanz, M.Rayet, M.Arnould

P-process nucleosynthesis during He-detonation in sub-Chandrasekhar CO white dwarfs

doi: 10.1016/S0375-9474(03)00879-0
Citations: PlumX Metrics

2001MA04      Nucl.Phys. A679, 337 (2001)

A.Mamdouh, J.M.Pearson, M.Rayet, F.Tondeur

Fission Barriers of Neutron-Rich and Superheavy Nuclei Calculated with the ETFSI Method

NUCLEAR STRUCTURE Z=84-120; A=214-318; calculated fission barrier heights. Extended Thomas-Fermi plus Strutinsky integral method.

doi: 10.1016/S0375-9474(00)00358-4
Citations: PlumX Metrics

2001RA22      Nucl.Phys. A688, 74c (2001)

M.Rayet, V.Costa, M.Arnould

News from the p-Process: Is the s-process a troublemaker ?

NUCLEAR REACTIONS ²²Ne(α, n), E=low; analyzed, surveyed reaction rates; deduced importance on production of neutron-poor p-nuclei. Network calculations, supernovae.

doi: 10.1016/S0375-9474(01)00672-8
Citations: PlumX Metrics

1999AN35      Nucl.Phys. A656, 3 (1999)

C.Angulo, M.Arnould, M.Rayet, P.Descouvemont, D.Baye, C.Leclercq-Willain, A.Coc, S.Barhoumi, P.Aguer, C.Rolfs, R.Kunz, J.W.Hammer, A.Mayer, T.Paradellis, S.Kossionides, C.Chronidou, K.Spyrou, S.Degl'Innocenti, G.Fiorentini, B.Ricci, S.Zavatarelli, C.Providencia, H.Wolters, J.Soares, C.Grama, J.Rahighi, A.Shotter, M.Lamehi-Rachti

A Compilation of Charged-Particle Induced Thermonuclear Reaction Rates

COMPILATION ¹H(p, e⁺ν), ²H, ^6,7Li, ^7,9Be, ^10,11B, ^12,13C, ^13,14,15N, ^16,17,18O, ¹⁹F, ^20,21,22Ne, ^22,23Na, ^24,25,26Mg, ^26,27Al, ²⁸Si(p, γ), ²H(d, γ), (d, p), ^2,3H(d, n), ^2,3H, ³He, ⁷Li, ⁷Be, ¹²C, ^14,15N, ^16,18O, ^20,22Ne(α, γ), ³He(³He, 2p), ^6,7Li, ⁹Be, ^10,11B, ^14,15N, ^17,18O, ¹⁹F, ²⁰Ne, ²³Na, ²⁴Mg, ²⁷Al(p, α), ⁷Li, ⁹Be, ¹³C, ¹⁴N, ^17,18O, ^21,22Ne, ²³Na, ^25,26Mg, ²⁷Al(α, n), ⁹Be, ¹¹B, ¹³C, ^14,15N, ¹⁹F, ²³Na(p, n), ⁹Be(p, d), E < 10 MeV; compiled, analyzed σ, S-factors; calculated astrophysical reaction rates vs T₉. Analytical approximations.

doi: 10.1016/S0375-9474(99)00030-5
Citations: PlumX Metrics

1999PE22      Acta Phys.Hung.N.S. 10, 159 (1999)

J.M.Pearson, F.Tondeur, A.Mamdouh, M.Rayet

Nuclear Masses and Fission Barriers via the ETFSI Method

NUCLEAR STRUCTURE Z=92; calculated fission barriers for N ≈ 140-190. ETFSI method, Skyrme force.

1998MA86      Nucl.Phys. A644, 389 (1998); Erratum Nucl.Phys. A648, 282 (1999)

A.Mamdouh, J.M.Pearson, M.Rayet, F.Tondeur

Large-Scale Fission-Barrier Calculations with the ETFSI Method

NUCLEAR STRUCTURE Z=80-100; calculated fission barrier heights. Extended Thomas-Fermi plus Strutinsky Integral method. Astrophysical implications discussed.

doi: 10.1016/S0375-9474(98)00576-4
Citations: PlumX Metrics

1998SO07      Astron.Astrophys. 333, 1112 (1998)

E.Somorjai, Zs.Fulop, A.Z.Kiss, C.E.Rolfs, H.P.Trautvetter, U.Greife, M.Junker, S.Goriely, M.Arnould, M.Rayet, T.Rauscher, H.Oberhummer

Experimental Cross Section of ¹⁴⁴Sm(α, γ)¹⁴⁸Gd and Implications for the p-Process

NUCLEAR REACTIONS ¹⁴⁴Sm(α, γ), E=10.5-13.4 MeV; measured σ; deduced astrophysical S-factors, stellar production ratio. Activation method.

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA0416.

1997SO19      Nucl.Phys. A621, 293c (1997)

E.Somorjai, Zs.Fulop, A.Z.Kiss, C.Rolfs, H.-P.Trautvetter, U.Greife, M.Junker, M.Arnould, M.Rayet, H.Oberhummer

Experimental Cross Section of ¹⁴⁴Sm(α, γ)¹⁴⁸Gd

NUCLEAR REACTIONS, ICPND ¹⁴⁴Sm(α, γ), E=10.5-13.4 MeV; measured residual nucleus α-decay; deduced production σ. Activation method, solid state nuclear track detectors. Statistical model calculations.

doi: 10.1016/S0375-9474(97)00258-3
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA0416.

1990AR10      Ann.Phys.(Paris) 15, 783 (1990)

M.Arnould, M.Rayet

Nuclear Reactions in Astrophysics

COMPILATION A ≤ 300; compiled, reviewed astrophysical reaction data.

1981RA18      Nucl.Phys. A367, 381 (1981)

M.Rayet

Skyrme Parametrization of an Effective Lambda-Nucleon Interaction

NUCLEAR STRUCTURE ⁵He, ¹³C, ¹⁶O; calculated binding energies of hyper-nuclei. Effective lambda-nucleon interaction, Hartree-Fock formalism.

doi: 10.1016/0375-9474(81)90655-2
Citations: PlumX Metrics