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First observation of unbound $^{11}$O, the mirror of the halo nucleus $^{11}$Li

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arxiv 1812.08880 v2 pith:JQHNZIBP submitted 2018-12-20 nucl-ex nucl-th

classification nucl-exnucl-th
keywords nucleusstatesbroadfirsthalomirrorpeakpotential
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

The structure of the extremely proton-rich nucleus $^{11}_{~8}$O$_3$, the mirror of the two-neutron halo nucleus $^{11}_{~3}$Li$_8$, has been studied experimentally for the first time. Following two-neutron knockout reactions with a $^{13}$O beam, the $^{11}$O decay products were detected after two-proton emission and used to construct an invariant-mass spectrum. A broad peak of width $\sim$3\,MeV was observed. Within the Gamow coupled-channel approach, it was concluded that this peak is a multiplet with contributions from the four-lowest $^{11}$O resonant states: $J^{\pi}$=3/2$^-_1$, 3/2$^-_2$, 5/2$^+_1$, and 5/2$^+_2$. The widths and configurations of these states show strong, non-monotonic dependencies on the depth of the $p$-$^9$C potential. This unusual behavior is due to the presence of a broad threshold resonant state in $^{10}$N, which is an analog of the virtual state in $^{10}$Li in the presence of the Coulomb potential. After optimizing the model to the data, only a moderate isospin asymmetry between ground states of $^{11}$O and $^{11}$Li was found.

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  1. Lattice simulation of nucleon distribution and shell closure in the proton-rich nucleus $^{22}$Si

    nucl-th 2024-11 conditional novelty 7.0 of 10

    Lattice chiral EFT simulations predict that 22Si is bound against two-proton emission and that its protons and neutrons fill the Z=14 and N=8 shells.

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