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Oral presentation

In beam $$gamma$$-ray measurement of the neutron-rich nucleus $$^{246}$$Pu

Makii, Hiroyuki; Ishii, Tetsuro; Asai, Masato; Tsukada, Kazuaki; Toyoshima, Atsushi; Matsuda, Makoto; Makishima, Akiyasu*; Kaneko, Junichi*; Tome, Hayato; Ichikawa, Shinichi; et al.

no journal, , 

no abstracts in English

Oral presentation

Production of Sg isotopes in the fusion reaction $$^{30}$$Si + $$^{238}$$U

Nishio, Katsuhisa; Mitsuoka, Shinichi; Ikezoe, Hiroshi; Hofmann, S.*; He${ss}$berger, F. P.*; Ackermann, D.*; Antalic, S.*; Comas, V. F.*; Gan, Z.*; Heinz, S.*; et al.

no journal, , 

Seaborgium isotopes were produced in the fusion reaction $$^{30}$$Si + $$^{238}$$U as evaporation residues (ERs), and the cross sections were determined. The experiment was carried out at GSI in Darmstadt, Germany. At the center-of-mass energy of E$$_{c.m.}$$= 144 MeV, three $$alpha$$ decay chains starting from $$^{263}$$Sg were observed, and the corresponding ER cross section was determined to be 67 pb. At the sub-barrier energy of E$$_{c.m.}$$= 133 MeV, three spontaneous fission events of a new isotope $$^{264}$$Sg were detected. The cross section was 10 pb. The half-life of $$^{264}$$Sg was determined to be 120 ms. The ER cross sections were compared with a statistical model calculation. In the fusion process, the coupled channel calculation taking into account the prolate deformation of $$^{238}$$U was adopted to determine the capture cross section. The calculated capture cross section agrees well with the fission cross section of $$^{30}$$Si + $$^{238}$$U obtained at the JAEA tandem accelerator. The measured cross section of $$^{264}$$Sg at the sub-barrier energy is factor 10$$^{4}$$ larger than the calculation based on the one-dimensional model in the fusion process, showing the fusion enhancement caused by the deformation of $$^{238}$$U. However, disagreement with the calculation suggests the presence of quasi-fission channel. At the above barrier energy of E$$_{c.m.}$$ = 144 MeV, the measured cross section is well reproduced by the calculation. This means that the interaction of $$^{30}$$Si at the equotorial side of $$^{238}$$U has advantage on the fusion process.

Oral presentation

$$alpha$$-$$gamma$$ spectroscopy of $$^{255}$$No

Asai, Masato; Tsukada, Kazuaki; Haba, Hiromitsu*; Toyoshima, Atsushi; Ishii, Tetsuro; Nagame, Yuichiro; Nishinaka, Ichiro; Ichikawa, Takatoshi*; Kojima, Yasuaki*; Sueki, Keisuke*

no journal, , 

$$gamma$$ rays following the $$alpha$$ decay of $$^{255}$$No have been measured by means of $$alpha$$-$$gamma$$ coincidence spectroscopy to establish neutron single-particle states in odd-mass superheavy nuclei. Seven $$gamma$$ transitions were observed, and excitation energies of the daughter nucleus $$^{251}$$Fm were determined. Spin-parities and neutron single-particle configurations of the excited states in $$^{251}$$Fm as well as the ground state of $$^{255}$$No were identified, and energy spacings and order of neutron single-particle states in N=151 isotones were established. It was found that the N=152 deformed neutron shell gap is larger in Fm and No nuclei than in lighter nuclei of Cf, Cm and Pu, which provides important information to clarify the shell structure of superheavy nuclei.

Oral presentation

Direct measurement of the $$^{8}$$Li(d,t)(d,p)(d,$$alpha$$) reaction cross sections

Hashimoto, Takashi; Ishiyama, Hironobu*; Hirayama, Yoshikazu*; Watanabe, Yutaka*; Imai, Nobuaki*; Miyatake, Hiroari; Jeong, S.-C.*; Yoshikawa, Nobuharu*; Tanaka, Masahiko*; Nomura, Toru*; et al.

no journal, , 

no abstracts in English

Oral presentation

Proposal of nuclear cosmic chronometer of neutrino process in supernova explosions

Hayakawa, Takehito; Shizuma, Toshiyuki; Kajino, Toshitaka*; Ogawa, Kengo*; Nakada, Hitoshi*

no journal, , 

no abstracts in English

Oral presentation

Systematic calculation of unstable nuclei in the N=28 region studied with shell model

Utsuno, Yutaka; Otsuka, Takaharu*; Homma, Michio*; Mizusaki, Takahiro*

no journal, , 

no abstracts in English

Oral presentation

Fusion barrier distribution in $$^{70}$$Zn+$$^{208}$$Pb,$$^{209}$$Bi reactions

Mitsuoka, Shinichi; Ikezoe, Hiroshi; Nishio, Katsuhisa; Jeong, S.-C.*; Watanabe, Yutaka*

no journal, , 

no abstracts in English

Oral presentation

Quark-hyperon mixed phase in compact stars

Maruyama, Toshiki; Tatsumi, Toshitaka*; Schulze, H.-J.*; Chiba, Satoshi

no journal, , 

no abstracts in English

Oral presentation

Highly polarized neutron beam produced by a quadrupole magnet and its application to fundamental physics

Yamada, Satoru; Oku, Takayuki; Mishima, Kenji*; Sato, Hiromi*; Hirota, Katsuya*; Morishima, Takahiro*; Ono, Masashi*; Shinohara, Takenao; Suzuki, Junichi; Shimizu, Hirohiko*

no journal, , 

no abstracts in English

Oral presentation

Neutron induced reaction and Re/Os cosmochronometer, 3

Segawa, Mariko; Nagai, Yasuki*; Masaki, Tomohiro*; Shima, Tatsushi*; Makii, Hiroyuki; Mishima, Kenji*; Ueda, Hitoshi*; Temma, Yasuyuki*; Igashira, Masayuki*; Osaki, Toshiro*; et al.

no journal, , 

no abstracts in English

Oral presentation

Charge-state breeding of neutron-rich medium-heavy nuclides using KEK charge breeder

Oyaizu, Mitsuhiro*; Ishiyama, Hironobu*; Imai, Nobuaki*; Kawakami, Hirokane*; Tanaka, Masahiko*; Jeong, S.-C.*; Hirayama, Yoshikazu*; Fuchi, Yoshihide*; Miyatake, Hiroari; Watanabe, Yutaka*; et al.

no journal, , 

Experimental results on the charge breeding efficiencies for medium-hevy elements, such as indium, barium, Zenon, etc, including radioactive isotopes were reported.

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