Briselet, R, Theisen, Ch, Sulignano, B, Airiau, M, Auranen, K, Cox, DM, Dechery, F, Drouart, A, Favier, Z, Gall, B et al (show 33 more authors)
(2020)
In-beam γ-ray and electron spectroscopy of <SUP>249,251</SUP>Md.
PHYSICAL REVIEW C, 102 (1).
014307-.
Text
2001.10235v1.pdf - Submitted version Download (1MB) | Preview |
Abstract
The odd-$Z$ $^{251}$Md nucleus was studied using combined $\gamma$-ray and conversion-electron in-beam spectroscopy. Besides the previously observed rotational band based on the $[521]1/2^-$ configuration, another rotational structure has been identified using $\gamma$-$\gamma$ coincidences. The use of electron spectroscopy allowed the rotational bands to be observed over a larger rotational frequency range. Using the transition intensities that depend on the gyromagnetic factor, a $[514]7/2^-$ single-particle configuration has been inferred for this band, i.e., the ground-state band. A physical background that dominates the electron spectrum with an intensity of $\simeq$ 60% was well reproduced by simulating a set of unresolved excited bands. Moreover, a detailed analysis of the intensity profile as a function of the angular momentum provided a method for deriving the orbital gyromagnetic factor, namely $g_K = 0.69^{+0.19}_{-0.16}$ for the ground-state band. The odd-$Z$ $^{249}$Md was studied using $\gamma$-ray in-beam spectroscopy. Evidence for octupole correlations resulting from the mixing of the $\Delta l = \Delta j = 3$ $[521]3/2^-$ and $[633]7/2^+$ Nilsson orbitals were found in both $^{249,251}$Md. A surprising similarity of the $^{251}$Md ground-state band transition energies with those of the excited band of $^{255}$Lr has been discussed in terms of identical bands. Skyrme-Hartree-Fock-Bogoliubov calculations were performed to investigate the origin of the similarities between these bands.
Item Type: | Article |
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Uncontrolled Keywords: | nucl-ex, nucl-ex, nucl-th |
Depositing User: | Symplectic Admin |
Date Deposited: | 31 Jan 2020 14:41 |
Last Modified: | 09 Oct 2023 02:26 |
DOI: | 10.1103/PhysRevC.102.014307 |
Related URLs: | |
URI: | https://livrepository.liverpool.ac.uk/id/eprint/3072818 |