NSR Query Results
Output year order : Descending NSR database version of April 26, 2024. Search: Author = M.Arnould Found 18 matches. 2020AR05 Prog.Part.Nucl.Phys. 112, 103766 (2020) Astronuclear Physics: A tale of the atomic nuclei in the skies
doi: 10.1016/j.ppnp.2020.103766
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
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
2006AR29 Nucl.Phys. A777, 157 (2006) 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
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
2003AR14 Phys.Rep. 384, 1 (2003) The p-process of stellar nucleosynthesis: astrophysics and nuclear physics status
doi: 10.1016/S0370-1573(03)00242-4
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
2001RA22 Nucl.Phys. A688, 74c (2001) 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
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
1999AR06 Rep.Prog.Phys. 62, 395 (1999) Nuclear Astrophysics
doi: 10.1088/0034-4885/62/3/003
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
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
1995TA18 Nucl.Phys. A588, 333c (1995) 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
1990AR10 Ann.Phys.(Paris) 15, 783 (1990) 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
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
1976AR14 Nucl.Phys. A274, 295 (1976) 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
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