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Ab initio study in the island of inversion within the two-major-shell valence space

X. C. Cao, C. F. Jiao

TL;DR

The study addresses the island of inversion around $N=20$ in light nuclei by deriving ab initio multishell valence-space Hamiltonians that span the $sd$, $sdf_{7/2}p_{3/2}$, and $sdfp$ shells. These Hamiltonians are obtained with the valence-space IMSRG (VS-IMSRG) from chiral NN and 3N forces and are used in a quantum-number projected generator coordinate method (PGCM) to sample deformed configurations. Expanding the valence space from $sd$ to $sdf_{7/2}p_{3/2}$ and finally to $sdfp$ substantially improves the description of quadrupole collectivity; the calculated $2^+_1$ energies are lowered and $B(E2;0^+_1\rightarrow2^+_1)$ values increase, indicating intruder-driven deformation. Neutron occupancies show cross-shell mp-mh excitations into the $fp$ shell, with roughly $1.5$ to $2$ neutrons promoted in the Mg isotopes near $N=20$, consistent with intruder configurations, while $^{34}$Si remains largely $sd$-shell dominated. The VS-IMSRG+PGCM framework provides a scalable, parameter-free ab initio approach to describe deformation and collectivity across multiple major shells, offering a path toward reliable predictions for heavier open-shell nuclei.

Abstract

We present an \textit{ab initio} study of nuclear structure in the island of inversion around neutron number $N=20$, using multishell effective Hamiltonians derived from the valence-space in-medium similarity renormalization group approach combined with the quantum-number projected generator coordinate method. By progressively expanding the valence space from the \textit{sd} shell to the intermediate $sdf_{7/2}p_{3/2}$ space and, for the first time, to the full \textit{sdfp} shell, we investigate low-lying spectra, $E2$ transition strengths, deformation properties, and neutron occupancies in even-even Ne, Mg, and Si isotopes around $N=20$. Our results show that enlarging the valence space significantly improves the description of quadrupole collectivity, yielding better agreement with experimental data for key observables such as the lowered $2^+$ energies and the enhanced $B(E2;0^+_1\rightarrow2_1^+)$ values. The analysis reveals the critical role of cross-shell multi-particle multi-hole excitations in breaking the $N=20$ shell closure and establishing intruder-dominated ground states. It also demonstrates the ability of the VS-IMSRG+PGCM framework to capture both dynamical (short range) and static (long range) correlations across multiple major-oscillator shells.

Ab initio study in the island of inversion within the two-major-shell valence space

TL;DR

The study addresses the island of inversion around in light nuclei by deriving ab initio multishell valence-space Hamiltonians that span the , , and shells. These Hamiltonians are obtained with the valence-space IMSRG (VS-IMSRG) from chiral NN and 3N forces and are used in a quantum-number projected generator coordinate method (PGCM) to sample deformed configurations. Expanding the valence space from to and finally to substantially improves the description of quadrupole collectivity; the calculated energies are lowered and values increase, indicating intruder-driven deformation. Neutron occupancies show cross-shell mp-mh excitations into the shell, with roughly to neutrons promoted in the Mg isotopes near , consistent with intruder configurations, while Si remains largely -shell dominated. The VS-IMSRG+PGCM framework provides a scalable, parameter-free ab initio approach to describe deformation and collectivity across multiple major shells, offering a path toward reliable predictions for heavier open-shell nuclei.

Abstract

We present an \textit{ab initio} study of nuclear structure in the island of inversion around neutron number , using multishell effective Hamiltonians derived from the valence-space in-medium similarity renormalization group approach combined with the quantum-number projected generator coordinate method. By progressively expanding the valence space from the \textit{sd} shell to the intermediate space and, for the first time, to the full \textit{sdfp} shell, we investigate low-lying spectra, transition strengths, deformation properties, and neutron occupancies in even-even Ne, Mg, and Si isotopes around . Our results show that enlarging the valence space significantly improves the description of quadrupole collectivity, yielding better agreement with experimental data for key observables such as the lowered energies and the enhanced values. The analysis reveals the critical role of cross-shell multi-particle multi-hole excitations in breaking the shell closure and establishing intruder-dominated ground states. It also demonstrates the ability of the VS-IMSRG+PGCM framework to capture both dynamical (short range) and static (long range) correlations across multiple major-oscillator shells.

Paper Structure

This paper contains 4 sections, 8 equations, 5 figures, 1 table.

Figures (5)

  • Figure 1: Calculated low-lying spectra of $^{32}$Mg obtained within the $sd$, $sdf_{7/2}p_{3/2}$, and $sdfp$ valence spaces, compared with experimental data. The arrows indicate the $B(E2)$ transition strengths from $0^{+}_{1}$ to $2^{+}_{1}$ in units of $e^2fm^4$. The experimental data are taken from the atomic mass evaluation (AME 2020) Wang_2021 and the National Nuclear Data Center (NNDC) NNDC.
  • Figure 2: (a) Projected potential energy of $^{32}$Mg with particle-number projection and angular-momentum projection onto $J=0$ against axial deformation $\beta_2$, calculated in the $sd$, $sdf_{7/2}p_{3/2}$, and $sdfp$ spaces. For clarity, the spherical configuration energy has been set to zero. (b) The distributions of the collective wavefunction of the $0^{+}_{1}$ state in 3 different model spaces. (c) Same as panel (b) but for $2^{+}_{1}$ states.
  • Figure 3: Neutron occupancies calculated within the $sd$, $sdf_{7/2}p_{3/2}$, and $sdfp$ spaces. Note that "0d" denotes the occupation of the neutron $0d_{5/2}$ and $0d_{3/2}$ orbitals.
  • Figure 4: Calculated low-lying spectra of $^{30}$Ne, $^{30-34}$Mg, and $^{34}$Si within $sdfp$ model space, compared with experimental data. The arrows indicate the $B(E2;0^+_1\rightarrow2^+_1)$ values in units of $e^2fm^4$. The experimental data are taken from the AME 2020 Wang_2021 and NNDC NNDC. The calculations are done with $e_{max}=12$ and $E_{3\mathrm{max}}=16$.
  • Figure 5: Neutron occupancies calculated within the full $sdfp$ space for the ground states of $^{30-34}$Mg and the adjacent $N=20$ isotones $^{30}$Ne, $^{34}$Si. Note that "0d" denotes the occupation of the neutron $0d_{5/2}$ and $0d_{3/2}$ orbitals.