| Relativistic equation of state of nuclear matter for supernova and neutron star H Shen, H Toki, K Oyamatsu, K Sumiyoshi Nuclear Physics A 637 (3), 435-450, 1998 | 1129 | 1998 |
| Relativistic equation of state of nuclear matter for supernova explosion H Shen, H Toki, K Oyamatsu, K Sumiyoshi Progress of Theoretical Physics 100 (5), 1013-1031, 1998 | 584 | 1998 |
| Nuclear shapes in the inner crust of a neutron star K Oyamatsu Nuclear Physics A 561 (3), 431-452, 1993 | 357 | 1993 |
| Relativistic equation of state for core-collapse supernova simulations H Shen, H Toki, K Oyamatsu, K Sumiyoshi The Astrophysical Journal Supplement Series 197 (2), 20, 2011 | 230 | 2011 |
| Symmetry energy at subnuclear densities and nuclei in neutron star crusts K Oyamatsu, K Iida Physical Review C—Nuclear Physics 75 (1), 015801, 2007 | 220 | 2007 |
| Quantum molecular dynamics approach to the nuclear matter below the saturation density T Maruyama, K Niita, K Oyamatsu, T Maruyama, S Chiba, A Iwamoto Physical Review C 57 (2), 655, 1998 | 168 | 1998 |
| Probing the equation of state of nuclear matter via neutron star asteroseismology H Sotani, K Nakazato, K Iida, K Oyamatsu Physical review letters 108 (20), 201101, 2012 | 127 | 2012 |
| Saturation of nuclear matter and radii of unstable nuclei K Oyamatsu, K Iida Progress of theoretical physics 109 (4), 631-650, 2003 | 113 | 2003 |
| Can the equation of state of asymmetric nuclear matter be studied using unstable nuclei? K Oyamatsu, I Tanihata, Y Sugahara, K Sumiyoshi, H Toki Nuclear Physics A 634 (1-2), 3-14, 1998 | 110 | 1998 |
| Effect of superfluidity on neutron star oscillations H Sotani, K Nakazato, K Iida, K Oyamatsu Monthly Notices of the Royal Astronomical Society: Letters 428 (1), L21-L25, 2012 | 87 | 2012 |
| Formula for proton–nucleus reaction cross section at intermediate energies and its application K Iida, A Kohama, K Oyamatsu Journal of the Physical Society of Japan 76 (4), 044201, 2007 | 83 | 2007 |
| Further study of the nuclear shape in high-density matter K Oyamatsu, M Hashimoto, M Yamada Progress of Theoretical Physics 72 (2), 373-375, 1984 | 83 | 1984 |
| Neutron star profiles in the relativistic Brueckner-Hartree-Fock theory K Sumiyoshi, K Oyamatsu, H Toki Nuclear Physics A 595 (3), 327-345, 1995 | 69 | 1995 |
| Shell energies of non-spherical nuclei in the inner crust of a neutron star K Oyamatsu, M Yamada Nuclear Physics A 578 (1-2), 181-203, 1994 | 68 | 1994 |
| Possible constraints on the density dependence of the nuclear symmetry energy from quasi-periodic oscillations in soft gamma repeaters H Sotani, K Nakazato, K Iida, K Oyamatsu Monthly Notices of the Royal Astronomical Society 434 (3), 2060-2068, 2013 | 67 | 2013 |
| Gyroid phase in nuclear pasta K Nakazato, K Oyamatsu, S Yamada Physical review letters 103 (13), 132501, 2009 | 67 | 2009 |
| Variational calculation for the equation of state of nuclear matter at finite temperatures H Kanzawa, K Oyamatsu, K Sumiyoshi, M Takano Nuclear Physics A 791 (1-2), 232-250, 2007 | 62 | 2007 |
| New method for calculating aggregate fission product decay heat with full use of macroscopic-measurement data K Oyamatsu, H Takeuchi, M Sagisaka, J Katakura Journal of nuclear science and technology 38 (7), 477-487, 2001 | 51 | 2001 |
| Possible origin of the gamma-ray discrepancy in the summation calculations of fission product decay heat T Yoshida, T Tachibana, F Storrer, K Oyamatsu, J Katakura Journal of nuclear science and technology 36 (2), 135-142, 1999 | 51 | 1999 |
| Possible identifications of newly observed magnetar quasi-periodic oscillations as crustal shear modes H Sotani, K Iida, K Oyamatsu New Astronomy 43, 80-86, 2016 | 48 | 2016 |
Kei IidaKochi UniversityBestätigte E-Mail-Adresse bei kochi-u.ac.jp
