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Iwata, Yoshihiro; Sekiya, Hiroyuki*; Ito, Chikara
no journal, ,
no abstracts in English
Utsuno, Yutaka; Shimizu, Noritaka*; Homma, Michio*; Mizusaki, Takahiro*; Otsuka, Takaharu*
no journal, ,
no abstracts in English
Nishio, Katsuhisa; Andreyev, A. N.*; Elseviers, J.*; Huyse, M.*; Van Duppen, P.*; Antalic, S.*; Barzakh, A.*; Bree, N.*; Cocolios, T. E.*; Comas, V. F.*; et al.
no journal, ,
no abstracts in English
Iimura, Hideki; Oba, Masaki; Koizumi, Mitsuo; Miyabe, Masabumi; Wakaida, Ikuo
no journal, ,
no abstracts in English
Asai, Masato; Tsukada, Kazuaki; Sato, Nozomi; Sato, Tetsuya; Toyoshima, Atsushi; Miyashita, Sunao; Oe, Kazuhiro; Kaneya, Yusuke*; Ishii, Tetsuro; Nagame, Yuichiro; et al.
no journal, ,
- spectroscopy of Db, the element 105, was performed for the first time, and the first experimental information on the proton configuration of the ground state of Db was obtained. Non observation of and X rays following its decay indicates that the decay of Db directly populates the 7/2[514] ground state or the 1/2[521] isomeric state in the daughter nucleus Lr, and does not populate the 9/2[624] excited state. This result indicates that the proton configuration of the ground state of Db should not be the theoretically predicted 9/2[624], but the 7/2[514] or 1/2[521].
Okamoto, Minoru; Maruyama, Toshiki; Yabana, Kazuhiro*; Tatsumi, Toshitaka*
no journal, ,
We have numerically performed three dimensional calculation of inhomogeneous low-density nuclear matter in beta-equilibrium without any assumption on the geometry, and explored the structures and its properties. We have observed two type of nuclear pasta with different crystalline structures. One is a face-centered cubic lattice and another is a body-centered cubic lattice. So far, it has been regarded that there appears only a body-centered cubic. But in our self-consistent calculation with non-uniformity of electrons, ground-state matter has lattice structure of not only a body-centered cubic but also a face-centered cubic. We also calculated the shear modulus of neutron star crust matter using three-dimensional data we obtained. Because of the Coulomb screening, shear modulus have lower value than previous one.
Maruyama, Toshiki; Yasutake, Nobutoshi*; Tatsumi, Toshitaka*
no journal, ,
no abstracts in English
Ichikawa, Yudai; Imai, Kenichi
no journal, ,
no abstracts in English
Hayakawa, Takehito; Horikawa, Ken*; Mochizuki, Takayasu*; Miyamoto, Shuji*; Amano, So*; Izawa, Yasukazu*; Imasaki, Kazuo*; Chiba, Satoshi*
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no abstracts in English
Angell, C.; Hammond, S. L.*; Karwowski, H. J.*; Kelley, J. H.*; Krtika, M.*; Kwan, E.*; Makinaga, A.*; Rusev, G.*
no journal, ,
Hayakawa, Takehito
no journal, ,
no abstracts in English