NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = C.Arlandini Found 17 matches. 2004KA26 Phys.Rev. C 69, 055802 (2004) F.Kappeler, C.Arlandini, M.Heil, F.Voss, K.Wisshak, R.Reifarth, O.Straniero, R.Gallino, S.Masera, C.Travaglio Stellar neutron capture on 180Tam. II. Defining the s-process contribution to nature's rarest isotope NUCLEAR REACTIONS 180mTa(n, γ), E=low; analyzed capture σ; deduced s-process contribution to solar abundance.
doi: 10.1103/PhysRevC.69.055802
2004RA29 Phys.Rev. C 70, 065803 (2004) U.Ratzel, C.Arlandini, F.Kappeler, A.Couture, M.Wiescher, R.Reifarth, R.Gallino, A.Mengoni, C.Travaglio Nucleosynthesis at the termination point of the s process NUCLEAR REACTIONS 208Pb, 209Bi(n, γ), E=spectrum; measured σ. Astrophysical implications discussed. Activation technique.
doi: 10.1103/PhysRevC.70.065803
2004WI07 Phys.Rev. C 69, 055801 (2004) K.Wisshak, F.Voss, C.Arlandini, F.Kappeler, M.Heil, R.Reifarth, M.Krticka, F.Becvar Stellar neutron capture on 180Tam. I. Cross section measurement between 10 keV and 100 keV NUCLEAR REACTIONS 180m,181Ta, 197Au(n, γ), E=10-100 keV; measured Eγ, capture σ. 180mTa(n, γ), E < 700 keV; deduced Maxwellian averaged σ.
doi: 10.1103/PhysRevC.69.055801
2003RE39 Astrophys.J. 582, 1251 (2003) R.Reifarth, C.Arlandini, M.Heil, F.Kappeler, P.V.Sedyshev, A.Mengoni, M.Herman, T.Rauscher, R.Gallino, C.Travaglio Stellar Neutron Capture on Promethium: Implications for the s-Process Neutron Density NUCLEAR REACTIONS 147Pm(n, γ), E=25 keV; measured reaction products, Eγ, Iγ; deduced Maxwellian-averaged σ and its uncertainties. NUCLEAR REACTIONS 147,148,149Pm(n, γ), E=5-100 keV; calculated Maxwellian-averaged σ. COMPILATION 146,147,148Nd, 147,148,149Pm, 147,148,149,150Sm(n, γ), E=10, 25, 30 keV; compiled Maxwellian-averaged σ and its uncertainties.
doi: 10.1086/344718
2002BE18 Phys.Rev. C65, 035801 (2002) D.Belic, C.Arlandini, J.Besserer, J.de Boer, J.J.Carroll, J.Enders, T.Hartmann, F.Kappeler, H.Kaiser, U.Kneissl, E.Kolbe, K.Langanke, M.Loewe, H.J.Maier, H.Maser, P.Mohr, P.von Neumann-Cosel, A.Nord, H.H.Pitz, A.Richter, M.Schumann, F.-K.Thielemann, S.Volz, A.Zilges Photo-Induced Depopulation of the 180Tam Isomer via Low-Lying Intermediate States: Structure and astrophysical implications NUCLEAR REACTIONS 180mTa(γ, γ'), E=0.8-3.1 MeV bremsstrahlung; measured delayed Eγ, Iγ, X-ray spectra; deduced activation yields. 180Ta deduced intermediate states energies, transition strengths. Astrophysical implications discussed. Comparisons with previous results, model predictions. RADIOACTIVITY 180Ta(EC), (β-); measured T1/2.
doi: 10.1103/PhysRevC.65.035801
2001AR14 Nucl.Phys. A688, 487c (2001) C.Arlandini, M.Heil, R.Reifarth, F.Kappeler, P.V.Sedyshev Stellar Neutron Capture Rate of 147Pm for Constraining the s-Process Neutron Density NUCLEAR REACTIONS 147Pm(n, γ), E<106 KeV; measured Eγ, σ at average energy corresponding to s-process conditions.
doi: 10.1016/S0375-9474(01)00764-3
2001BE33 Phys.Rev. C64, 015801 (2001) J.Best, H.Stoll, C.Arlandini, S.Jaag, F.Kappeler, K.Wisshak, A.Mengoni, G.Reffo, T.Rauscher s-Process Branchings at 151Sm, 154Eu, and 163Dy NUCLEAR REACTIONS 151,153Eu, 152,154Sm, 164,170Er(n, γ), E=spectrum; measured σ. 151,152,153,154,155Eu(n, γ), E=1-2000 keV; calculated σ. Activation technique, comparisons with previous measurements. Astrophysical implications discussed.
doi: 10.1103/PhysRevC.64.015801
2001GO28 Nucl.Phys. A688, 225c (2001) J.Gorres, C.Arlandini, U.Giesen, M.Heil, F.Kappeler, H.Leiste, E.Stech, M.Wiescher Topics in Stellar He Burning NUCLEAR REACTIONS 14N(α, γ), E=low; measured σ, resonance energy and strength, reaction rates. Comparison with earlier data, network calculations.
doi: 10.1016/S0375-9474(01)00703-5
2001VO13 Nucl.Phys. A688, 237c (2001) P.von Neumann-Cosel, C.Arlandini, D.Belic, J.Besserer, J.de Boer, J.J.Carroll, J.Enders, T.Hartmann, F.Kappeler, H.Kaiser, U.Kneissl, M.Loewe, H.J.Maier, H.Maser, P.Mohr, A.Nord, H.H.Pitz, A.Richter, M.Schumann, S.Volz, A.Zilges Photoactivation of 180mTa and s-Process Nucleosynthesis of Nature's Rarest Naturally Occuring Isotope NUCLEAR REACTIONS 180Ta(γ, γ'), E=0.8-3.1 MeV; measured Eγ, σ; deduced 180Ta effective half-life under s-process conditions.
doi: 10.1016/S0375-9474(01)00706-0
2001WI13 Nucl.Phys. A688, 533c (2001) K.Wisshak, F.Voss, C.Arlandini, M.Heil, F.Kappeler, R.Reifarth, M.Krticka, F.Becvar Stellar Neutron Capture Cross Section of the Rarest Stable Isotope 180mTa NUCLEAR REACTIONS 180Ta(n, γ), E=10-100 keV; measured Eγ. Production of 180Ta in stellar environments discussed.
doi: 10.1016/S0375-9474(01)00779-5
2001WI22 Phys.Rev.Lett. 87, 251102 (2001) K.Wisshak, F.Voss, C.Arlandini, F.Becvar, O.Straniero, R.Gallino, M.Heil, F.Kappeler, M.Krticka, S.Masera, R.Reifarth, C.Travaglio Neutron Capture on 180Tam: Clue for an s-process origin of nature's rarest isotope NUCLEAR REACTIONS 180mTa(n, γ), E=10-100 keV; measured capture σ; deduced astrophysical average capture σ.
doi: 10.1103/PhysRevLett.87.251102
2000GO43 Phys.Rev. C62, 055801 (2000) J.Gorres, C.Arlandini, U.Giesen, M.Heil, F.Kappeler, H.Leiste, E.Stech, M.Wiescher Low-Energy Resonances in 14N(α, γ)18F and Their Astrophysical Implications NUCLEAR REACTIONS 14N(α, γ), E=550-1300 keV; measured Eγ, Iγ(t), resonance yields; deduced astrophysical reaction rates. 18F deduced resonance energies, strengths. Implications for isotopic abundances discussed.
doi: 10.1103/PhysRevC.62.055801
2000WI08 Phys.Rev. C61, 065801 (2000) K.Wisshak, F.Voss, C.Arlandini, F.Kappeler, L.Kazakov Stellar Neutron Capture Cross Sections of the Yb Isotopes NUCLEAR REACTIONS 170,171,172,173,174,176Yb(n, γ), (n, X), E=3-225 keV; measured total, capture σ, isomer ratios; deduced Maxwellian averaged σ. Implications for stellar nucleosynthesis discussed.
doi: 10.1103/PhysRevC.61.065801
1999AR31 Astrophys.J. 525, 886 (1999) C.Arlandini, F.Kappeler, K.Wisshak, R.Gallino, M.Lugaro, M.Busso, O.Straniero Neutron Capture in Low-Mass Asymptotic Giant Branch Stars: Cross Sections and Abundance Signatures COMPILATION 140,141,142Ce, 141,142Pr, 142,143,144Nd(n, γ); compiled experimental nuclear reaction σ data; deduced sensitive test for models of s-process nucleosynthesis.
doi: 10.1086/307938
1999BE65 Phys.Rev.Lett. 83, 5242 (1999) D.Belic, C.Arlandini, J.Besserer, J.de Boer, J.J.Carroll, J.Enders, T.Hartmann, F.Kappeler, H.Kaiser, U.Kneissl, M.Loewe, H.J.Maier, H.Maser, P.Mohr, P.von Neumann-Cosel, A.Nord, H.H.Pitz, A.Richter, M.Schumann, S.Volz, A.Zilges Photoactivation of 180Tam and Its Implications for the Nucleosynthesis of Nature's Rarest Naturally Occurring Isotope NUCLEAR REACTIONS Ta, 180mTa(γ, γ'), E=0.8-3.1 MeV bremsstrahlung; measured ground-state production yield. Implications for s-process nucleosynthesis discussed. Enriched and natural targets.
doi: 10.1103/PhysRevLett.83.5242
1999VO02 Phys.Rev. C59, 1154 (1999) F.Voss, K.Wisshak, C.Arlandini, F.Kappeler, L.Kazakov, T.Rauscher Stellar Neutron Capture Cross Sections of Pr and Dy Isotopes NUCLEAR REACTIONS 141Pr, 160,161,162,163,164Dy(n, γ), E=3-225 keV; measured total, capture σ; deduced Maxwellian averaged neutron capture σ at stellar energies. Astrophysical implications discussed.
doi: 10.1103/PhysRevC.59.1154
1997GA19 Nucl.Phys. A621, 423c (1997) R.Gallino, C.Arlandini, M.Lugaro, M.Busso, O.Straniero The New s-Process in Low Mass TP-AGB Stars
doi: 10.1016/S0375-9474(97)00284-4
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