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NSR database version of April 11, 2024.

Search: Author = R.Fujimoto

Found 9 matches.

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2011WA32      J.Korean Phys.Soc. 59, 1040s (2011)

Y.Watanabe, K.Kosako, S.Kunieda, S.Chiba, R.Fujimoto, H.Harada, M.Kawai, F.Maekawa, T.Murata, H.Nakashima, K.Niita, N.Shigyo, S.Shimakawa, N.Yamano, T.Fukahori

Status of JENDL High Energy File

COMPILATION Z=1-95(n, X), (p, X), E=0-3 GeV; compiled, evaluated σ, dσ.

doi: 10.3938/jkps.59.1040
Citations: PlumX Metrics

2005OT01      Acta Phys.Pol. B36, 1213 (2005)

T.Otsuka, T.Suzuki, R.Fujimoto, D.Abe, H.Grawe, Y.Akaishi

Evolution of shell and collective structures in exotic nuclei

NUCLEAR STRUCTURE 40,42,44,46,48Ca, 68,70,72,74,76,78Ni; calculated proton single-particle energies. Z=40-50; calculated neutron single-particle energies for N=51 isotones.

2005OT03      Phys.Rev.Lett. 95, 232502 (2005)

T.Otsuka, T.Suzuki, R.Fujimoto, H.Grawe, Y.Akaishi

Evolution of Nuclear Shells due to the Tensor Force

NUCLEAR STRUCTURE Ca, Ni; Z=40-50; calculated neutron and proton effective single-particle energies; deduced role of tensor force in shell evolution.

doi: 10.1103/PhysRevLett.95.232502
Citations: PlumX Metrics

2003SU04      Phys.Rev. C 67, 044302 (2003)

T.Suzuki, R.Fujimoto, T.Otsuka

Gamow-Teller transitions and magnetic properties of nuclei and shell evolution

NUCLEAR STRUCTURE 10,11,12,13B, 11,12Be, 12,13,14,15C, 15O; calculated level energies. 6,8He, 9,11Li, 7Be, 12,13,14B, 9,10,11,12,14,15C, 13N, 14,15O; calculated Gamow-Teller transition strengths. 7,8,9,11Li, 8,9,10,11,12,13,14,15B, 9,11Be, 9,11,13,15C, 12,13,14,15N, 13,15O; calculated μ. Shell model, enhanced spin-flip proton-neutron interaction, comparison with data.

doi: 10.1103/PhysRevC.67.044302
Citations: PlumX Metrics

2003SU28      Nucl.Phys. A722, 538c (2003)

T.Suzuki, R.Fujimoto, T.Otsuka

New aspects of spin degrees of freedom in nuclei

NUCLEAR STRUCTURE 12C, 12N, 11B, 11Be; calculated Gamow-Teller transition strengths. Comparison with data.

NUCLEAR MOMENTS 7,8,9,11Li, 8,9,10,11,12,13,14,15B, 9,11Be, 9,11,13,15C, 12,13,14,15N, 13,15O; calculated μ. Comparison with data.

doi: 10.1016/S0375-9474(03)01423-4
Citations: PlumX Metrics

2002FU22      Prog.Theor.Phys.(Kyoto), Suppl. 146, 551 (2002)

R.Fujimoto, T.Otsuka, T.Suzuki, Y.Utsuno

Spectra of Neutrons Emitted from Excited/Ground States of 24, 25O

NUCLEAR STRUCTURE 24,25O; calculated level configurations, neutron emission probabilities.

doi: 10.1143/PTPS.146.551
Citations: PlumX Metrics

2002OT01      Eur.Phys.J. A 13, 69 (2002)

T.Otsuka, Y.Utsuno, R.Fujimoto, B.A.Brown, M.Honma, T.Mizusaki

Frontiers and Challenges of the Nuclear Shell Model

NUCLEAR STRUCTURE Z=8-20; calculated levels, shell features far from stability. Monte Carlo shell model.

doi: 10.1007/s10050-002-8721-5
Citations: PlumX Metrics

2002OT03      Eur.Phys.J. A 15, 151 (2002)

T.Otsuka, Y.Utsuno, R.Fujimoto, B.A.Brown, M.Honma, T.Mizusaki

Frontiers and challenges of nuclear shell model

doi: 10.1140/epja/i2001-10244-6
Citations: PlumX Metrics

2001OT04      Phys.Rev.Lett. 87, 082502 (2001)

T.Otsuka, R.Fujimoto, Y.Utsuno, B.A.Brown, M.Honma, T.Mizusaki

Magic Numbers in Exotic Nuclei and Spin-Isospin Properties of the NN Interaction

NUCLEAR STRUCTURE 24O, 30Si; calculated effective single-particle energy levels. 9He, 11Be, 13C; calculated levels, J, π. 24O, 26Ne, 28Mg, 30Si, 32S, 34Ar, 36Ca; calculated effective shell gap. Shell-model magic numbers in exotic nuclides, role of spin-isospin contribution discussed.

doi: 10.1103/PhysRevLett.87.082502
Citations: PlumX Metrics

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