NSR Query Results
Output year order : Descending NSR database version of May 3, 2024. Search: Author = T.S.Suzuki Found 6 matches. 2003TO17 Nucl.Phys. A718, 401c (2003) A.Tomyo, Y.Nagai, T.S.Suzuki, T.Kikuchi, T.Shima, T.Kii, M.Igashira Measurement of the p(n, γ)d reaction cross section between En = 100 and 350 keV NUCLEAR REACTIONS 1H(n, γ), E=100-350 keV; measured Eγ, Iγ, σ. Comparison with previous results, model predictions.
doi: 10.1016/S0375-9474(03)00814-5
1999OH04 Nucl.Instrum.Methods Phys.Res. A425, 302 (1999) T.Ohsaki, Y.Nagai, M.Igashira, T.Shima, T.S.Suzuki, T.Kikuchi, T.Kobayashi, T.Takaoka, M.Kinoshita, Y.Nobuhara An NaI(Tl) Spectrometer System for keV Neutron Radiative-Capture Reactions NUCLEAR REACTIONS 12C(n, γ), E ≈ 42 keV; measured capture σ(E).
doi: 10.1016/S0168-9002(98)01364-3
1998KI09 Phys.Rev. C57, 2724 (1998) T.Kikuchi, Y.Nagai, T.S.Suzuki, T.Shima, T.Kii, M.Igashira, A.Mengoni, T.Otsuka Nonresonant Direct p- and d-Wave Neutron Capture by 12C NUCLEAR REACTIONS 12C(n, γ), E=550 keV; measured Eγ, Iγ; deduced partial capture σ. 13C level deduced spectroscopic factor. Direct radiative capture calculations.
doi: 10.1103/PhysRevC.57.2724
1997NA22 Phys.Rev. C56, 3173 (1997) Y.Nagai, T.S.Suzuki, T.Kikuchi, T.Shima, T.Kii, H.Sato, M.Igashira Measurement of the 1H(n, γ)2H Reaction Cross Section at a Comparable M1/E1 Strength NUCLEAR REACTIONS 1H(n, γ), E=550 keV; measured Eγ, Iγ, σ; deduced transition M1, E1 components, meson exchange currents role.
doi: 10.1103/PhysRevC.56.3173
1996NA27 Hyperfine Interactions 103, 43 (1996) Y.Nagai, T.Shima, T.S.Suzuki, H.Sato, T.Kikuchi, T.Kii, M.Igashira, T.Ohsaki Fast Neutron Capture Reactions in Nuclear Astrophysics NUCLEAR REACTIONS 1H, 12C, 16O(n, γ), E=10-300 keV; measured Eγ, Iγ, capture σ at some neutron energies. Implications for primordial and stellar nucleosynthesis.
doi: 10.1007/BF02317341
1995SU10 Astrophys.J. 439, L59 (1995) T.S.Suzuki, Y.Nagai, T.Shima, T.Kikuchi, H.Sato, T.Kii, M.Igashira First Measurement of a p(n, γ)d Reaction Cross Section between 10 and 80 keV NUCLEAR REACTIONS 1H(n, γ), E=10-80 keV; measured Eγ, Iγ; deduced σ(E), primordial light elements abundances implications.
doi: 10.1086/187744
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