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HfAlayed, B.*; Page, R. D.*; Joss, D. T.*; Uusitalo, J.*; Qi, C.*; Briscoe, A. D.*; AlAqeel, M. A. M.*; Andel, B.*; Antalic, S.*; Auranen, K.*; et al.
Physical Review C, 110(3), p.034303_1 - 034303_9, 2024/09
Times Cited Count:2 Percentile:44.78(Physics, Nuclear)
Hg,
Hg,
Hg and
HgWrzosek-Lipska, K.*; Rezynkina, K.*; Bree, N.*; Zieli
ska, M.*; Gaffney, L. P.*; Petts, A.*; Andreyev, A. N.; Bastin, B.*; Bender, M.*; Blazhev, A.*; et al.
European Physical Journal A, 55(8), p.130_1 - 130_23, 2019/08
Times Cited Count:19 Percentile:78.85(Physics, Nuclear)
s isomeric state in
IrGillespie, S. A.*; Andreyev, A. N.; Al Monthery, M.*; Barton, C. J.*; Antalic, S.*; Auranen, K.*; Badran, H.*; Cox, D.*; Cubiss, J. G.*; O'Donnell, D.*; et al.
Physical Review C, 99(6), p.064310_1 - 064310_6, 2019/06
Times Cited Count:6 Percentile:43.22(Physics, Nuclear)
HgM
ller-Gatermann, C.*; Dewald, A.*; Fransen, C.*; Auranen, K.*; Badran, H.*; Beckers, M.*; Blazhev, A.*; Braunroth, T.*; Cullen, D. M.*; Fruet, G.*; et al.
Physical Review C, 99(5), p.054325_1 - 054325_7, 2019/05
Times Cited Count:12 Percentile:66.95(Physics, Nuclear)no abstracts in English
Es and
BkKonki, J.*; Khuyagbaatar, J.*; Uusitalo, J.*; Greenlees, P. T.*; Auranen, K.*; Badran, H.*; Block, M.*; Briselet, R.*; Cox, D. M.*; Dasgupta, M.*; et al.
Physics Letters B, 764, p.265 - 270, 2017/01
Times Cited Count:25 Percentile:83.83(Astronomy & Astrophysics)Gaffney, L. P.*; Robinson, A. P.*; Jenkins, D. G.*; Andreyev, A. N.; Bender, M.*; Blazhev, A.*; Bree, N.*; Bruyneel, B.*; Butler, P.*; Cocolios, T. E.*; et al.
Physical Review C, 91(6), p.064313_1 - 064313_11, 2015/06
Times Cited Count:11 Percentile:56.09(Physics, Nuclear)
-ray spectroscopy of a superheavy element; The
RfRubert, J.*; Dorvaux, O.*; Gall, B. J. P.*; Greenlees, P. T.*; Asfari, Z.*; Piot, J.*; Andersson, L. L.*; Asai, Masato; Cox, D. M.*; Dechery, F.*; et al.
Journal of Physics; Conference Series, 420, p.012010_1 - 012010_10, 2013/03
Times Cited Count:0 Percentile:0.00(Physics, Nuclear)The first prompt in-beam
-ray spectroscopy of a superheavy element,
Rf, has been performed successfully. A development of an intense isotopically enriched
Ti beam using the MIVOC method enabled us to perform this experiment. A rotational band up to a spin of 20
has been discovered in
Rf, and its moment of inertia has been extracted. These data suggest that there is no evidence of a significant deformed shell gap at
= 104.
=104 nucleus
RfGreenlees, P. T.*; Rubert, J.*; Piot, J.*; Gall, B. J. P.*; Andersson, L. L.*; Asai, Masato; Asfari, Z.*; Cox, D. M.*; Dechery, F.*; Dorvaux, O.*; et al.
Physical Review Letters, 109(1), p.012501_1 - 012501_5, 2012/07
Times Cited Count:66 Percentile:88.59(Physics, Multidisciplinary)Rotational band structure of the
=104 nucleus
Rf has been observed for the first time using an in-beam
-ray spectroscopic technique. This nucleus is the heaviest among the nuclei whose rotational band structure has ever been observed. Thus, the present result provides valuable information on the single-particle shell structure and pairing interaction in the heaviest extreme of nuclei. The deduced moment of inertia indicates that there is no deformed shell gap at
=104, which is predicted in a number of current self-consistent mean-field models.