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We perform three-body model calculations for a $sd$-shell hypernucleus $^{19}_{Lambda}$F ($^{17}_{Lambda}{rm O}+p+n$) and its core nucleus $^{18}$F ($^{16}{rm O}+p+n$), employing a density-dependent contact interaction between the valence proton and neutron. We find that the $B(E2)$ value from the first excited state (with spin and parity of $I^pi=3^+$) to the ground state ($I^pi=1^+$) is slightly decreased by the addition of a $Lambda$ particle, which exhibits the so called shrinkage effect of $Lambda$ particle. We also show that the excitation energy of the $3^+$ state is reduced in $^{19}_{Lambda}$F compared to $^{18}$F, as is observed in a $p$-shell nucleus $^{6}$Li. We discuss the mechanism of this reduction of the excitation energy, pointing out that it is caused by a different mechanism from that in $^{7}_{Lambda}$Li.
We study the effect of a $Lambda$ hyperon immersed in the doubly magic nuclei, $^{16}$O, $^{40}$Ca, $^{48}$Ca, and $^{208}$Pb, as well as the neutron magic nucleus $^{90}$Zr. For a $Lambda$ in the $1s$ and $1p$ states in $^{17}_{Lambda}$O, $^{41}_{La
The impurity effect of hyperon on atomic nuclei has received a renewed interest in nuclear physics since the first experimental observation of appreciable reduction of $E2$ transition strength in low-lying states of hypernucleus $^{7}_Lambda$Li. Many
Fission of atomic nuclei often produces mass asymmetric fragments. However, the origin of this asymmetry was believed to be different in actinides and in the sub-lead region [A. Andreyev {it et al.}, Phys. Rev. Lett. {bf 105}, 252502 (2010)]. It has
Coherent one-particle one-hole (1p1h) excitations have given us effective insights into general nuclear excitations. However, the two-particle two-hole (2p2h) excitation beyond 1p1h is now recognized as critical for the proper description of experime
The structure of neutron stars is determined by the equation of state of the matter inside the star, which relies on the knowledge of nuclear interactions. While radii of neutron stars mostly depend on the equation of state of neutron matter at nucle