Speaker
Description
The rapid spherical to prolate shape transition at N = 60 in the mid-shell region around Z = 40 has been evidenced from diverse experiments [1-5], and the shape evolution for more neutron-rich nuclei has been of interest because of the emergence of the triaxial degree of freedom. Theoretical predictions suggested further phase transitions such as a shape transition to oblate spheroid [6-8], a transition to triaxial ground shapes [6, 9] and doubly magic behavior at N = 70 [10]. Experimental information for the low-lying states of even-odd nuclei can be the key since they exhibit the properties of orbitals of the un-paired nucleon near the Fermi surface and the orbital configuration is sensitive to the nuclear shape.
The shape and shell evolution for molybdenum nuclei (Mo, Z = 42) with N ≥ 60 have been studied in various experiments [11-16] but the detailed shell structure near the Fermi surface is still unresolved. The excited states of 109Mo were studied through the spontaneous fissions of 248Cm and 252Cf [11, 12], but the recent discovery of an isomeric transition in 109Mo has revealed that previous studies on 109Mo were limited to the excited states above the ground state [16, 17].
In the present study, the low-lying states in 109Mo are investigated from the γ-rays detected following the β decay of 109Nb. The data was collected as part of the EURICA project in RIKEN [18]. Two new isomeric γ-rays are identified together with the known isomeric γ-ray [16, 17]. Their transition multipolarities have been scrutinized considering internal conversion coefficients and recommended upper limits [19]. New excited states including a new first excited state below the isomeric state are assigned. The results of mean-field calculations [20] and intrinsic gyromagnetic moment calculations [21] are considered to assign associated neutron orbitals for the low-lying states. The analysis results for the most likely quasi-particle configurations of the low-lying states including ground band and isomeric band will be presented.
[1] H. Wollnik et al., Nucl. Phys. A 291, 2, p. 355, (1977)
[2] R. E. Azuma et al., Phys. Lett. B 86, 1, p. 5, (1979)
[3] M. A. C. Hotchkis et al., Nucl. Phys. A 530, 1, p. 111, (1991)
[4] K. Heyde and J. L. Wood, Rev. Mod. Phys. 83, 1467 (2011)
[5] J.-M. Régis et al. Phys. Rev. C 95, 054319 (2017)
[6] J. Skalski, S. Mizutori and W. Nazarewicz, Nucl. Phys. A 617, 3, p. 282, (1997)
[7] F. R. Xu, P. M. Walker, and R. Wyss, Phys. Rev. C 65, 021303(R) (2002)
[8] R. Rodriguez-Guzman, P. Sarriguren, and L. M. Robledo, Phys. Rev. C 82, 044318 (2010)
[9] P. Möller et al. Phys. Rev. Lett. 97, 162502 (2006)
[10] M. Bender et al. Phys. Rev. C 80, 064302 (2009)
[11] J. K. Hwang et al., Phys. Rev. C 56, 1344, (1997)
[12] W. Urban et al., Phys. Rev. C 73, 037302, (2006)
[13] C. Goodin et al., Phys. Rev. C 80, 014318, (2009)
[14] J. Marcellino et al., Phys. Rev. C 96, 034319, (2017)
[15] J. Ha et al., Phys. Rev. C 101, 044311, (2020)
[16] W. Urban et al., Phys. Rev. C 102, 024318, (2020)
[17] D. Kameda et al., Phys. Rev. C 86, 054319, (2012)
[18] P. A. Söderström et al., JPS Conf. Proc. 1, 013046 (2014),
[19] P. M. Endt, At. Data Nucl. Data Tables, 26, 1, p. 47, (1981)
[20] F. R. Xu et al. Phys. Lett. B 435, p. 257, (1998)
[21] P. M. Walker et al. Nucl. Phys. A 568, p. 397 (1994)
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Are you a student or postdoc? | yes |