NSR Query Results
Output year order : Descending NSR database version of April 26, 2024. Search: Author = S.Jaag Found 10 matches. 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
1999DO03 Phys.Rev. C59, 492 (1999) C.Doll, H.G.Borner, S.Jaag, F.Kappeler, W.Andrejtscheff Lifetime Measurement in 176Lu and Its Astrophysical Consequences NUCLEAR REACTIONS 175Lu(n, γ), E=reactor; measured Doppler-broadened Eγ, Iγ. 176Lu level deduced T1/2. Gamma-ray induced Doppler broadening technique. Astrophysical implications discussed.
doi: 10.1103/PhysRevC.59.492
1997JA08 Nucl.Phys. A621, 247c (1997) The Stellar (n, γ) Cross Section of the Unstable 135Cs NUCLEAR REACTIONS 135Cs(n, γ), E=thermal; measured Eγ, Iγ; deduced σ. Quasi-stellar neutron spectrum.
doi: 10.1016/S0375-9474(97)00247-9
1997JA09 Nucl.Phys. A621, 251c (1997) The Stellar (n, γ) Cross Sections of the Stable Iridium Isotopes NUCLEAR REACTIONS 191,193Ir(n, γ), E ≈ 30 keV; measured Eγ, Iγ; deduced capture σ. Quasi-stellar neutron spectrum.
doi: 10.1016/S0375-9474(97)00248-0
1996JA07 Phys.Rev. C53, 2474 (1996) Moxon-Rae Setup for the Measurement of Stellar (n, γ) Rates and the Example of 87Rb NUCLEAR REACTIONS 87Rb(n, γ), E=10-100 keV; measured σ(E); deduced Maxwellian averaged σ(E).
doi: 10.1103/PhysRevC.53.2474
1996JA28 Astrophys.J. 464, 874 (1996) The Stellar (n, γ) Cross Section of the Unstable Isotope 163Ho and the Origin of 164Er NUCLEAR REACTIONS 163Ho(n, γ), E=25, 30 keV; measured reaction products, Eγ, Iγ; deduced Maxwellian-averaged σ and its uncertainties.
doi: 10.1086/177375
1995JA07 Phys.Rev. C51, 3465 (1995) Stellar (n, γ) Cross Section of the Unstable Isotope 155Eu NUCLEAR REACTIONS 155Eu(n, γ), E=quasistellar spectrum; measured Eγ, Iγ; deduced stellar σ(n, γ), relevance to s-process branchings at A=151, 152 and 154 with respect to helium shell burning temperature in low mass stars.
doi: 10.1103/PhysRevC.51.3465
1995SC02 Phys.Rev. C51, 379 (1995) H.Schatz, S.Jaag, G.Linker, R.Steininger, F.Kappeler, P.E.Koehler, S.M.Graff, M.Wiescher Stellar Cross Sections for 33S(n, α)30Si, 36Cl(n, p)36S, and 36Cl(n, α)33P and the Origin of 36S NUCLEAR REACTIONS 33S(n, α), 36Cl(n, p), (n, α), E=10-260 keV; measured < σ(E) >; deduced stellar reaction rate for 33S(n, α), nucleosynthesis of 36S. Ionization chamber.
doi: 10.1103/PhysRevC.51.379
1992XI01 Phys.Rev. C45, 2487 (1992) Y.Xia, Th.W.Gerstenhofer, S.Jaag, F.Kappeler, K.Wisshak Neutron Cross Sections of 122Te, 123Te, and 124Te between 1 and 60 keV NUCLEAR REACTIONS 93Nb, 122,123,124Te(n, γ), E=1-60 keV; measured capture σ relative to gold standard. 122,123,124Te(n, X), E=10-100 keV; measured total σ.
doi: 10.1103/PhysRevC.45.2487
1991KA10 Astrophys.J. 366, 605 (1991) F.Kappeler, S.Jaag, Z.Y.Bao, G.Reffo The s-Process Branchings at 185W and 186Re NUCLEAR REACTIONS 185,187Re(n, γ), E=25 keV; measured capture σ; deduced 185W, 186Re s-process branchings.
doi: 10.1086/169596
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