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NSR database version of May 24, 2024.

Search: Author = M.Arnould

Found 18 matches.

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2020AR05      Prog.Part.Nucl.Phys. 112, 103766 (2020)

M.Arnould, S.Goriely

Astronuclear Physics: A tale of the atomic nuclei in the skies

doi: 10.1016/j.ppnp.2020.103766
Citations: PlumX Metrics


2013XU14      Nucl.Phys. A918, 61 (2013)

Y.Xu, K.Takahashi, S.Goriely, M.Arnould, M.Ohta, H.Utsunomiya

NACRE II: an update of the NACRE compilation of charged-particle-induced thermonuclear reaction rates for nuclei with mass number A ≤ 16

COMPILATION 2,3H, 3He, 6,7Li, 7,9Be, 10,11B, 12,13C, 13,14,15N(p, X), (α, X), E≈0.1 keV-1 MeV;2,3H, 3He(d, X), E≈0.1 keV-1 MeV;3He(3He, 2p), E≈0.1 keV-1 MeV; compiled, evaluated Q-value, σ, S-factor, reaction rates using DWBA, potential models; deduced model parameters.

doi: 10.1016/j.nuclphysa.2013.09.007
Citations: PlumX Metrics


2007AR34      Phys.Rep. 450, 97 (2007)

M.Arnould, S.Goriely, K.Takahashi

The r-process of stellar nucleosynthesis: Astrophysics and nuclear physics achievements and mysteries

NUCLEAR STRUCTURE Z=31-83; calculated r-process isotopic abundances.

doi: 10.1016/j.physrep.2007.06.002
Citations: PlumX Metrics


2006AR29      Nucl.Phys. A777, 157 (2006)

M.Arnould, S.Goriely

Microscopic nuclear models for astrophysics: The Brussels BRUSLIB nuclear library and beyond

NUCLEAR REACTIONS 84,86Sr, 90Zr, 93Nb, 92,94,95Mo, 96,98Ru(p, γ), E=1-6 MeV; 37Cl, 42Ca, 56Fe, 58,62,64Ni, 70Ge, 106Cd, 144Sm(α, γ), E=3-20 MeV; 181Ta(γ, n), E=7.5-13.5 MeV; calculated σ. 144Sm(α, γ), E=9-13.5 MeV; calculated astrophysical S-factor. 186W, 190,192,198Pt, 198Au, 196,198,204Hg, 204Pb(γ, n), E not given; calculated reaction rates. MOST model with Hauser-Feshbach, global optical potential and quasi-particle RPA, different reaction mechanisms discussed. Comparison with data. Detailed description of BRUSLIB given.

doi: 10.1016/j.nuclphysa.2005.02.116
Citations: PlumX Metrics


2004UT01      Nucl.Phys. A738, 136 (2004)

H.Utsunomiya, K.Y.Hara, S.Goko, H.Akimune, T.Yamagata, M.Ohta, H.Ohgaki, H.Toyokawa, T.Hayakawa, T.Shizuma, P.Mohr, Y.-W.Lui, H.Ohkuma, H.Yonehara, K.Soutome, M.Arnould

Photonuclear reaction studies at synchrotron radiation facilities in Japan

doi: 10.1016/j.nuclphysa.2004.04.022
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetM0664.


2003AR14      Phys.Rep. 384, 1 (2003)

M.Arnould, S.Goriely

The p-process of stellar nucleosynthesis: astrophysics and nuclear physics status

doi: 10.1016/S0370-1573(03)00242-4
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


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


1999AR06      Rep.Prog.Phys. 62, 395 (1999)

M.Arnould, K.Takahashi

Nuclear Astrophysics

doi: 10.1088/0034-4885/62/3/003
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.


1996DE07      Nucl.Phys. A597, 231 (1996)

F.de Oliveira, A.Coc, P.Aguer, C.Angulo, G.Bogaert, J.Kiener, A.Lefebvre, V.Tatischeff, J.-P.Thibaud, S.Fortier, J.M.Maison, L.Rosier, G.Rotbard, J.Vernotte, M.Arnould, A.Jorissen, N.Mowlavi

Determination of α-Widths in 19F Relevant to Fluorine Nucleosynthesis

NUCLEAR REACTIONS 15N(7Li, t), (7Li, 7Li), E=28 MeV; measured σ(θ); deduced astrophysical reaction rate. 19F levels deduced α-width, spectroscopic factors. Finite-range DWBA analysis, Hauser-Feshbach contribution, α-transfer reactions, cluster model. Enriched gas target.

doi: 10.1016/0375-9474(95)00455-6
Citations: PlumX Metrics


1995TA18      Nucl.Phys. A588, 333c (1995)

T.Tachibana, M.Arnould

Beta-Decay Properties of Exotic Nuclei and the Astrophysical r-Process

NUCLEAR STRUCTURE A=80-200; calculated relative r-process abundances; deduced neutron rich nuclei β-decay T1/2 evaluation discrepancies. Three different β-decay models.

doi: 10.1016/0375-9474(95)00158-W
Citations: PlumX Metrics


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

M.Arnould, M.Rayet

Nuclear Reactions in Astrophysics

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


1990IL01      Nucl.Phys. A512, 509 (1990)

Ch.Iliadis, Th.Schange, C.Rolfs, U.Schroder, E.Somorjai, H.P.Trautvetter, K.Wolke, P.M.Endt, S.W.Kikstra, A.E.Champagne, M.Arnould, G.Paulus

Low-Energy Resonances in 25Mg(p, γ)26Al, 26Mg(p, γ)27Al and 27Al(p, γ)28Si

NUCLEAR REACTIONS 25,26Mg, 27Al(p, γ), E < 340 keV; measured γ-spectra, γ-branchings. 26,27Al, 28Si deduced resonances, J, π, Γ, γ-branching ratios.

doi: 10.1016/0375-9474(90)90084-Y
Citations: PlumX Metrics


1990SE09      Nucl.Phys. A514, 471 (1990)

S.Seuthe, C.Rolfs, U.Schroder, W.H.Schulte, E.Somorjai, H.P.Trautvetter, F.B.Waanders, R.W.Kavanagh, H.Ravn, M.Arnould, G.Paulus

Resonances in the 22Na(p, γ)23Mg Reaction

NUCLEAR REACTIONS, ICPND 22Na(p, γ), E=0.17-1.29 MeV; measured γ-spectra; deduced stellar reaction rates. 23Mg deduced resonances, resonance strengths.

doi: 10.1016/0375-9474(90)90153-D
Citations: PlumX Metrics


1976AR14      Nucl.Phys. A274, 295 (1976)

M.Arnould, W.M.Howard

Diffuse Surface Nuclear and Coulomb Potential Energies for Heavy-Ion Reactions

NUCLEAR REACTIONS 13C, 16O, 58,60Ni, 208Pb(16O, X), 12,13C(28Si, X), 13C(32S, X), 208Pb(12C, X), (11B, X), (20Ne, X); calculated nuclear, Coulomb potential energies. Modified liquid-drop model.

doi: 10.1016/0375-9474(76)90242-6
Citations: PlumX Metrics


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