NSR Query Results
Output year order : Descending NSR database version of April 26, 2024. Search: Author = A.Tomyo Found 10 matches. 2005NA15 Phys.Rev. C 71, 055803 (2005) Y.Nagai, M.Igashira, T.Takaoka, T.Kikuchi, T.Shima, A.Tomyo, A.Mengoni, T.Otsuka 7Li(n, γ)8Li reaction and the S17 factor at Ec.m. > 500 keV NUCLEAR REACTIONS 7Li(n, γ), E ≈ 10-80 keV; measured Eγ, Iγ, σ; deduced interaction potential features. 7Be(p, γ), E ≈ 0.1-3 MeV; calculated astrophysical S-factor.
doi: 10.1103/PhysRevC.71.055803
2005NA31 Nucl.Phys. A758, 537c (2005) Y.Nagai, A.Tomyo, Y.Temma, M.Segawa, T.Shima, H.Makii, M.Igashira, T.Ohsaki Measurement of the keV neutron capture cross section of 62Ni NUCLEAR REACTIONS 62Ni(n, γ), E=5, 5-90 MeV; measured Eγ, Iγ, capture σ; deduced Maxwellian averaged σ.
doi: 10.1016/j.nuclphysa.2005.05.097
2005SE23 J.Phys.Soc.Jpn. 74, 2981 (2005) M.Segawa, A.Tomyo, Y.Nagai, Y.Temma, T.Masaki, T.Shima, J.Nishiyama, T.Ohsaki, M.Igashira New Approach for Measuring the (n, γ) Cross Section of a Nucleus by a Few keV Neutron NUCLEAR REACTIONS 197Au(n, γ), E=spectrum; measured Eγ, Iγ; deduced neutron flux. 7Li(p, n), E not given; deduced neutron spectrum. 62Ni(n, γ), E ≈ 5.5-20 keV; measured σ; deduced Maxwellian-averaged σ.
doi: 10.1143/JPSJ.74.2981
2005TO14 Astrophys.J. 623, L153 (2005) A.Tomyo, Y.Temma, M.Segawa, Y.Nagai, H.Makii, T.Shima, T.Ohsaki, M.Igashira 62Ni(n, γ)63Ni reaction and overproduction of Ni isotopes NUCLEAR REACTIONS 62Ni(ν, γ), E=5.5-90 keV; measured Eγ, capture σ; deduced Maxwellian-averaged σ.
doi: 10.1086/430129
2003MA47 Nucl.Phys. A718, 475c (2003) H.Makii, E.Sano, K.Mishima, Y.Nagai, T.Shima, M.Segawa, N.Maehara, A.Tomyo, M.Igashira Preparation for the 12C(α, γ)16O experiment using pulsed α beam
doi: 10.1016/S0375-9474(03)00861-3
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
2003TO18 Nucl.Phys. A718, 527c (2003) A.Tomyo, Y.Nagai, Y.Nobuhara, T.Shima, H.Makii, K.Mishima, M.Igashira Neutron capture cross section measurement of 20, 22Ne for stellar nucleosynthesis NUCLEAR REACTIONS 20,22Ne(n, γ), E=15-60 keV; measured Eγ, Iγ, σ; deduced Maxwellian averaged capture σ. Astrophysical implications discussed.
doi: 10.1016/S0375-9474(03)00833-9
2003TO19 Nucl.Phys. A718, 530c (2003) A.Tomyo, Y.Nagai, T.Shima, H.Makii, K.Mishima, M.Segawa, M.Igashira 84Kr(n, γ)85Kr reaction cross section measured by an NaI(Tl) spectrometer between 10 and 80 keV NUCLEAR REACTIONS 84Kr(n, γ), E=10-80 keV; measured Eγ, Iγ; deduced Maxwellian averaged capture σ. Astrophysical implications discussed.
doi: 10.1016/S0375-9474(03)00834-0
1999NA15 Nucl.Instrum.Methods Phys.Res. A423, 404 (1999) S.Naito, A.Tomyo, T.Shima, T.Kii, T.Baba, T.Takahashi, Y.Nagai KENS keV Neutron Flux for Nuclear Astrophysics NUCLEAR REACTIONS 7Li(p, n), E not given; measured neutron spectra; deduced detector efficiency. Ta(p, nX), E=500 MeV; measured neutron spectra, flux. Spallation neutron source characteristics.
doi: 10.1016/S0168-9002(98)01307-2
1998NA15 Nucl.Instrum.Methods Phys.Res. A402, 408 (1998) Y.Nagai, T.Kobayashi, T.Kikuchi, F.Okazaki, K.Takaoka, S.Naito, A.Tomyo, T.Shima, M.Igashira, S.Ishikawa Nuclear and Nuclear Astrophysical Interest in D(n, γ)3H Reaction NUCLEAR REACTIONS 2H(n, γ), E=10-80 keV; measured σ. Astrophysical implications.
doi: 10.1016/S0168-9002(97)00881-4
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