γ emission from neutron-unbound states in 133Sn

17 Apr 2019, 14:15
15m
LIT, JINR

LIT, JINR

Oral Nuclear Physics Nuclear Physics

Speaker

Ms Monika Piersa (Faculty of Physics University of Warsaw)

Description

The study of 133Sn provides excellent conditions to investigate single-particle transitions relevant in the neutron-rich 132Sn region due to the simplicity of its nuclear structure. After many experimental activities employing one-neutron transfer reactions [1–4], traditional β-decay studies are an attractive technique to refine our knowledge on 133Sn. Since the positions of neutron single-particle states in 133Sn were established and confirmed in many measurements [1–5], our focus moves to single-hole states expected at higher excitation energies. Because of the low neutron-separation energy of 133Sn, Sn=2.4 MeV [6], all of them are supposed to be neutron-unbound. β-decay studies are therefore a natural choice to investigate their nature since there is a large energy window for their population in the β decay of 133In (Q_β =13.4(2) MeV [6]). Our experiment was performed at the ISOLDE Decay Station, where excited states in 133Sn were investigated via the β decay of 133In. Isomer-selective ionization using the ISOLDE RILIS enabled the β decays of 133gIn (Iπ =9/2+) and 133mIn (Iπ=1/2−) to be studied independently for the first time. Thanks to the large spin difference of those two β-decaying states, it is possible to investigate separately the lower- and higher-spin states in the daughter 133Sn and thus to probe independently different single-particle and single-hole levels. We identified new γ transitions following the 133In→133Sn decay. Single-hole states in 133Sn were found at energies exceeding S_n up to 3.7 MeV [7]. Due to centrifugal barrier hindering the neutron from leaving the nucleus, the contribution of electromagnetic decay of those unbound states was found to be significant. [1] K. L. Jones et al., Nature (London) 465, 454 (2010). [2] K. L. Jones et al., Phys. Rev. C 84, 034601 (2011). [3] J. M. Allmond et al., Phys. Rev. Lett. 112, 172701 (2014). [4] V. Vaquero et al., Phys. Rev. Lett. 118, 202502 (2017). [5] P. Hoff et al., Phys. Rev. Lett. 77, 1020 (1996). [6] M. Wang et al., Chin. Phys. C 41, 030003 (2017). [7] M. Piersa et al., Phys. Rev. C 99, 024304 (2019).

Primary author

Ms Monika Piersa (Faculty of Physics University of Warsaw)

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