logo

Investigation of the level spectra of nuclei in the northeast region of doubly magic 40Ca with intruder orbit g9/2

NUCLEAR PHYSICS AND INTERDISCIPLINARY RESEARCH

Investigation of the level spectra of nuclei in the northeast region of doubly magic 40Ca with intruder orbit g9/2

Jin-Zhong Han
Shuai Xu
Amir Jalili
Han-Kui Wang
Nuclear Science and TechniquesVol.34, No.6Article number 85Published in print Jun 2023Available online 21 Jun 2023
52100

This study utilizes large-scale shell model calculations with the extended pairing and multipole-multipole force model (EPQQM) to investigate low-lying states in the nuclei of 42Ca, 42Sc, and 42-44Ti. The model space in this study includes the fp shell as well as the intruder g9/2 orbit, which accurately reproduces the positive parity levels observed in the aforementioned nuclei and predicts high-energy states with negative parity coupled with the intruder g9/2. The study further predicts two different configurations in 43Ti at around 6 MeV, specifically πf7/22νg9/2 and πf7/2g9/2vf7/2, both of which involve the intruder orbit g9/2. The levels coupled with the intruder g9/2 in 44Ti are predicted to lie between 7 and 11 MeV. The inclusion of the intruder orbit g9/2 is crucial for the exploration of high-energy states in the northeast region of the doubly magic nucleus 40Ca.

Shell modelDoubly magicLevel structure
1

Introduction

The study of nuclei in the northeast of the doubly magic nucleus 40Ca is a topic of great interest in both experimental and theoretical nuclear structure research. In pioneering experimental research, the lifetimes of higher-lying positive parity levels have been determined with limited precision [1-3]. Subsequently, negative parity states have been investigated, ultimately determining the 4- [4]. The negative parity level 3- was first confirmed by a preliminary lifetime analysis in a conference proceeding in 2011 [5]. More recently, the lifetimes of excited states have been determined in 44Ti with high accuracy, using the recoil distance Doppler-shift method [6, 7]. Some of the recent advancements in both experimental and theoretical research regarding 2p decay, including technical innovations for measuring nucleon-nucleon correlations as well as developments in the models used to connect the structural aspects of nuclei with their corresponding decay properties, are presented in Ref. [8]. In the IMS experiments, charge resolution provides crucial information for the particle identification of ion pairs [9]. These newly proposed models were used to predict the cross-sections of ERIs produced in projectile fragmentation reactions of 140 MeV/u 78,86Kr/58,64Ni/40,48Ca + 9Be [10].

The half-life of β-decay and β-delayed neutron emission (βn) are crucial parameters in the advancement of basic science and industrial applications, including nuclear physics and nuclear energy, according to theoretical considerations [11]. The excited states of Ti isotopes have been studied microscopically within a single j-shell formalism [12]. A comparative study has been performed in pf shell nuclei using the cranked Nilsson-Strutinsky model and the spherical shell model [13]. Over the decades, various models have been developed to study the spectroscopic properties of nuclei such as the large-scale spherical shell model calculations, which have demonstrated excellent agreement with observed data. One such model is the SDPFMU interaction [14], which is based on existing interactions and uses valence shells sd and pf. For instance, it is based on the USD interaction [15] and GXPF1 [16] for the sd and pf shells, respectively. The monopole interactions are based on the SDPF-M model [17], and the monopole- and quadrupole-pairing matrix elements are replaced with KB3 [18]. Another model, the EPQQM (expanded pairing, quadrupole-quadrupole, and multipole force with monopole corrections) model, has been found to work efficiently in various mass regions, such as the proton-rich pf shell [19], the pf5/2g9/2 shell [20], the neutron-rich fpg shell [21], and the sd-pf shell [22]. This model has been particularly successful in explaining both the low-lying levels and the high core excitations in the heavy, neutron-rich region near A = 130 [23-25], in addition to confirming the persistence of the N = 82 shell closure and effectively describing the ground state inversion in 129Cd driven by monopole interaction between protons and neutrons [26, 27].

The intruder orbit g9/2 is crucial between the df and pf shells. Intruder states refer to those states that lie outside the traditional or expected valence configurations. These states can have a significant impact on the structure of a nucleus. For example, they can lead to ground state or low-lying excited-state inversions, where the ordering of the energy levels is different from the traditional shell model predictions. Intruder states can also affect various properties of nuclei, including their energy levels and ratios. These states are particularly significant in comprehending the evolution of nuclear structure as the number of neutrons or protons changes. In the present study, the EPQQM model, which includes the intruder g9/2 orbit in the model space, is used to investigate the energy levels of nuclei in the northeast of 40Ca. The inclusion of the intruder orbit allows for a more complete description of the positive-parity levels and the high-energy states of negative-parity levels in these nuclei.

In this model, the predicted energy levels are rigorously compared with experimental data to validate and refine its accuracy. This study highlights the importance of considering intruder states in the analysis of nuclear structure and the need for experimental measurements in validating model predictions. Intruder states can also be related to the phenomenon of shape coexistence, which is the existence of different shapes in the ground state of a nucleus, due to the mixing of different configurations [28, 29]. This phenomenon is observed in various nuclei, and the inclusion of intruder states in the model space allows for a more complete description of the observed shape coexistence. Therefore, the inclusion of intruder states in nuclear models is vital for gaining a deeper understanding of the evolution of nuclear shape, the phenomenon of shape coexistence, and the potential emergence of new magic numbers.

In this work, the EPQQM model in the model space of the pf shell, including the intruder g9/2 orbit, is applied to investigate the energy levels of nuclei in the northeast of 40Ca. The positive parity levels and intruder states in 42Ca, 42Sc, and 42Ti are efficiently described by the EPQQM interaction. The nuclei 43Ti and 44Ti are also examined by comparing them with experimental data [30], serving as an additional means to further test the two-body strengths in nuclear models. The calculations for the nuclei 43Ti and 44Ti are performed using the shell-model code NUSHELLX@MSU [31]. The SDPFUM interaction is utilized to explore the cross-shell excitation originating from the d5/2 orbit under Z = 20 (N = 20). Additionally, the GXPF1A interaction [16] is employed for comparison purposes to study the energy levels within the pf shell.

2

Theoretical Framework

The results obtained from the study of nuclei in the northeast region of the doubly magic nucleus 40Ca have significant implications for nuclear physics research. In particular, the inclusion of intruder states, such as the g9/2 orbit, have been demonstrated to be critical for a comprehensive understanding of nuclear structure. This study provides additional support for the utilization of the EPQQM model in describing the energy levels of nuclei, particularly focusing on the northeast region of 40Ca.

Theoretical models are essential in nuclear physics as they provide valuable insights into the properties of nuclei that are difficult to measure directly through experiments. The SDPFMU and EPQQM models, in particular, have shown promising results in various mass regions, including the sd-pf, proton-rich pf shell, and heavy neutron-rich region near A=130. These models can accurately predict the properties of nuclei, such as their energy levels and ratios, as well as describe shape coexistence and ground state inversions. They have helped recognize the importance of intruder states in the evolution of nuclear structure.

Although theoretical models are powerful tools, their predictions must be validated through experimental measurements to ensure their full verification. The results of this this study can guide future experimental investigations in the northeast region of 40Ca, such as the determination of the lifetimes of higher-lying positive parity levels with greater precision. The combination of experimental and theoretical approaches is crucial for advancing our understanding of nuclear structure and the fundamental properties of matter.

2.1
Hamiltonian

In the proton-neutron (pn) representation, the present Hamiltonian is composed of the pairing-plus-multipole force and the monopole corrections: H=Hsp+HP0+HP2+HQQ+HOO+HHH+Hmc=α,iεaicα,icα,i12J=0,2iigJ,iiMPJM,iiPJM,ii12iiχ2,iib4M:Q2M,iiQ2M,ii:12iiχ3,iib6M:O3M,iiO3M,ii:12iiχ4,iib8M:H4M,iiH4M,ii:+ac,iikmc(ia,ic)JMAJM(ia,ic)AJM(ia,ic). (1) This effective interaction (1) includes the single-particle Hamiltonian (Hsp), the J=0 and J=2 pairing (P0P0 and P2P2), the quadrupole-quadrupole (QQ), the octupole-octupole (OO), the hexadecapole-hexadecapole (HH) terms, and the monopole corrections (Hmc). In the pn representation, PJM,ii and AJM(ia,ic) are the pair operators, while Q2M,ii, O3M,ii, and H4M,ii are the quadrupole, octupole, and hexadecapole operators, in which i (i’) are indices for protons (neutrons). The parameters gJ,ii’, χ2,ii’, χ3,ii’, χ4,ii’, and kmc(ia,i’c) are the corresponding force strengths, and b is the harmonic-oscillator range parameter. The two-body force strengths suited for the present model space are listed in Table 1.

Table 1
Two-body force strengths (in MeV) used in the present calculation
ii’ g0,ii’ g2,ii’ χ2,ii’ χ3,ii’ χ4,ii’
pp 0.450 0.470 -0.107 0.075 0.0010
nn 0.422 0.449 0 0.075 0.00010
pn 0 0 0.256 0 0.0009
Show more
2.2
Model space

In addition to the Hamiltonian, the choice of model spaces with single particle energies are crucial for shell model calculations. In this work, the model space for protons (neutrons) consists of all the pf shell orbits (1f7/2, 1f5/2, 2p1/2, 2p3/2) with frozen core 40Ca. Further, an intruder state, the 1g9/2 orbit is added to study high energy levels. The low-lying levels in 41Ca (41Sc) are selected as neutron (proton) single particle states in this model space to obtain single particle energies. Marking εf7/2π as the single particle energy (SPE) of the ground state 7/2- in 41Sc, π denoting proton (ν neutron), we obtain SPE as the difference in binding energies (BE) of 41Sc and 40Ca, εf7/2π=BE(41Sc)BE(40Ca)=1.089 MeV. (2) The other proton SPE in 41Sc can be obtained by adding this value ϵf7/2π=1.089 MeV to the excited energies. Thus, all SPEs are obtained as follows (MeV): εf7/2π=1.089 , εf7/2ν=8.387 ,εp3/2π=0.627 , εp3/2ν=6.444 ,εf5/2π=1.499 , εf5/2ν=5.811 ,εp1/2π=2.376 , εp1/2ν=4.773 ,εg9/2π=3.425 , εg9/2ν=3.936 . (3) For these neutron SPEs, the excited energies are taken as 0, 1.943, 2.576, 3.614 and 4.451 MeV from 7/2-, 3/2-, 5/2-, 3/2- and 9/2+ levels in 41Ca. For proton SPEs, they are 0, 1.716, 2.588, 3.465, and 4.514 MeV from 7/2-, 3/2-, 5/2-, 1/2-, and 9/2+ levels in 41Sc.

2.3
Monopole corrections

In the present Hamiltonian, the monopole corrections can be investigated as follows: Mc=kmc(ia,ic)JMAJM(ia,ic)AJM(ia,ic). (4) Here AJM(ia,ic) and AJM represent the pair operators, and kmc is the monopole force strength. Monopole correction terms should consider corresponding data. Note that the maximum multiplet is J = 8 coupled by the configuration 1f7/2 1g9/2. The datum 8- at 6.408 MeV in 42Ca is selected to determine the force strength of monopole correction between neutron orbits 1f7/2 and 1g9/2. There is no datum 8- in 42Ti; therefore, the force strength between proton orbits 1f7/2 and 1g9/2 refers to the value in 42Ca. Mc1kmc(νf7/2,νg9/2)=1.10 MeV,Mc2kmc(πf7/2,πg9/2)=1.10 MeV. (5) Owing to missing three-body contributions in the Hamiltonians derived from realistic two-body potentials [32, 33], monopole corrections become necessary for two-body interactions [34]. The extended pairing plus multipole-multipole force (EPQQM model) is advantageous in employing monopole correction (Mc) terms [35]. Monopole-driven shell evolutions are discussed with different effects of tensor forces in Ref. [36]. Monopole interactions are critical in shifting the spherical-shell model to account for the nonconventional shell evolution observed in neutron-rich nuclei. Experimental studies have shown that the monopole interaction between the neutron orbits h11/2 and d3/2 provides an effective description of ground-state inversions observed in isotopes ranging from 130In(129Cd) to 128In(127Cd) [37]. The energy gap of the neutron N = 82 can be modified by using a monopole term between h11/2 and f7/2. Experimental confirmation has validated the inverse low-lying levels of 129Cd predicted by the monopole effect between g9/2 and h11/2. Monopole corrections have recently helped in constructing a new Hamiltonian above 132Sn with core excitations and an intruder orbit i13/2.

3

Results and discussions

In this part, structure analysis is carried out for 42Ti, 42Ca, 42Sc, and 43,44Ti with EPQQM, GXPF1A and SDPFMU effective interactions. This work includes intruder states involving the g9/2 orbit, with no restriction on the pf shell and g9/2 orbit. The GXPF1A effective interaction has proven to be highly effective in the pf shell and its results serve as a valuable benchmark for comparison. The SDPFMU interaction is applied to study the proton (neutron) core excitations across the Z=20(N=20) energy gap, and one proton (neutron) core excitation is allowed across the Z=20 (N=20) shell gap from d5/2 in sd shell.

3.1
42Ca

The g9/2 orbit plays a crucial role in the energy spectrum of 42Ca. Being an intruder orbit, it lies outside the traditional valence shell configuration of 40Ca, which is composed of the pf shell. By including the g9/2 orbit in the model space, additional degrees of freedom for nucleons are introduced, leading to new configurations and the possibility of new quantum numbers.

42Ca, as a stable nucleus, exhibits a rich spectrum of excited states up to 11 MeV and spins up to J = 12. Only positive parity levels can be coupled with two valence nucleons in the pf shell, with the highest spin J = 6, resulting from the configuration coupling. However, negative parity levels arise from two distinct sources: cross-shell excitations or coupling with the intruder orbit g9/2. In this study, we employ the EPQQM interaction to discuss levels coupled by the intruder orbit g9/2 and the SDPFMU interaction to explore cross-shell excitations.

The determination of pairing and multipole force strengths in the neutron model space is facilitated by studying the low-lying states of 42Ca. Figure 1 depicts a comparison between the experimental data for 42Ca and shell model calculations. The ground state and excited levels 2+, 4+, and 6+ exhibit the same main configuration νf7/22 as suggested by the EPQQM, GXPF1A, and SDPFMU interactions. The second 2+ and 4+ levels predominantly feature the configuration νf7/2p3/2.

Fig. 1
The experimental energy levels in 42Ca [30], and the theoretical levels calculated by interactions EPQQM, GXPF1A, and SDPFMU
pic

Regarding negative parity levels, the 8- configuration νf7/2g9/2 closely corresponds to the observed 8- state at 6.408 MeV. This configuration successfully reproduces the (3-), (5-), and 6- states. The 7- state at 6.703 MeV is in proximity to the datum at 6.718 MeV, although its parity information remains unconfirmed. The levels 1-, 2-, and 4- are well-predicted in this study. However, the GXPF1A interaction fails to reproduce the negative parity levels in 42Ca due to the absence of cross-shell and intruder orbits in the model space. In contrast, the SDPFMU interaction, which considers the cross-shell proton (neutron) d5/2 orbit under Z=20 (N=20), successfully predicts negative levels around 6 MeV with the primary configuration ν d-15/2f37/2.

The low-lying states of 42Ca can be used to determine the pairing and multipole force strengths in the neutron model space. As shown in Fig. 1, the experimental data in 42Ca are listed and compared with shell model calculations. The ground state and excited levels 2+, 4+, and 6+ are consistently described by the same main configuration νf7/22 according to three different interactions: EPQQM, GXPF1A, and SDPFMU. There are also small differences in the mixed minor configurations. In the EPQQM model, the ground state 0+ has approximately 82% of νf7/22 6.3 % of νp3/22, and 8.3% of νf5/22. The configurations νp1/22 and νg9/22 occupy only about 2% respectively. In GXPF1A model, the ground state 0+ has 97 % of νf7/22, and only 1.6 % of νp3/22. In SDPFMU model, the ground state 0+ has 92 % of νf7/22, and no other configuration more than 1.52%.

In EPQQM, the first 2+ state has 79.8 % of νf7/22 and 10.4% of νf7/2p3/2, while it has 96.8% of νf7/22 and 2.8 % of νf7/2p3/2 by GXPF1A model. The second 2+ level has 73.7% of configuration νf7/2p3/2 and 16.8% of νf7/22 in this work, while it has 92.7% of νf7/2p3/2 in GXPF1A model. The difference increases in the minor configuration of this level, between EPQQM and GXPF1A models. The second 4+ has 97.1% of νf7/2p3/2 in EPQQM, while it has 93.2% of νf7/2p3/2 in GXPF1A. The difference decreases in the second 4+.

For negative parity level states, the 8- coupled by νf7/2g9/2 is very close to the datum 8- at 6.408 MeV. This configuration has 8 members from the 1- to 8- level, effectively reproducing the data of (3-), (5-), and 6- states. The 7- state at 6.703 MeV is close to the datum 6.718 MeV, which includes unconfirmed parity information. This study successfully predicts the levels 1-, 2-, and 4-. The 8- level at 6.468MeV has 100 % of νf7/2g9/2, because only this configuration can produce the J = 8 state. In addition to the main configuration νf7/2g9/2, the 7- state has a minor configuration of νf5/2g9/2, only 0.5%. The 6- (5-)state has a minor configuration of νp3/2g9/2, 2.9 (3.93) %. The levels 4- and 3- also have a little part of νp3/2g9/2. The levels 2- and 1- are only reproduced by configuration νf7/2g9/2 in the present model space. For the other two interactions, the GXPF1A is not able to reproduce the negative parity levels in 42Ca owing to the lack of cross-shell and intrusive orbits in the model space. While considering the cross-shell proton (neutron) d5/2 orbit under Z=20 (N=20), the SDPFMU provides negative levels at approximately 6 MeV with the main configuration νd5/21f7/23.

3.2
42Ti

The ground state of 42Ti, which is the mirror nucleus of 42Ca, is unstable with a half-life of 211.7 ms (19), as determined from analysis of beta decay and correlated implantations. Levels of 42Ti excit up around 7 MeV with the highest spin = 6+. The low-lying states in 42Ti are used to determine the strengths of pairing and multipole forces in the proton model space. In the even-even nucleus of 42Ti, the EPQQM model suggests that the main configuration of the 0+, 2+, 4+, and 6+ levels is πf7/22 (Fig. 2). In this work, the ground state 0+ has 81 % of πf7/22, 8.8 % of πf5/22, and 6 % of πp3/22. In GXPF1A model, the ground state has 97 % of πf7/22 and 1.6 % of πp3/22. In SDPFMU model, the ground state has 73.4 % of πf7/22 and 16.3 % of πp1/22. These three models have the same main configuration and only some difference in minor configurations. In the second 2+ and 4+ levels, these three interactions show a small difference in configurations. The EPQQM has 78.7 % (94.4 %) configuration πf7/2p3/2 in the second 2+ (4+) levels, while in GXPF1A is 92.7 % (93.2 %) The SDPFMU has 53 % (65 %) of πf7/2p3/2 in the second 2+ (4+) levels respectively.

Fig. 2
The calculations and experimental energy levels in 42Ti[30].
pic

In this study, the negative parity levels ranging from 1- to 8- coupled by the configuration πf7/2g9/2 are found to be good predictions, which appear at approximately 6 MeV. There is still no experimental data of negative parity levels in this energy range. The high-spin level 8- at 6.602 MeV is only coupled by the configuration πf7/2g9/2. The level 7- at 6.651 MeV has 99.7% of πf7/2g9/2 and 0.3% of πf5/2g9/2. The level 6- at 5.593 MeV has 96.0% of πf7/2g9/2 and 4.0% of πp3/2g9/2. The level 5- (4-) at 5.789(6.567) MeV has 97.1(95.6)% of πf7/2g9/2 and 2.6(3.5)% of πp3/2g9/2. The levels 1-, 2-, and 3- are also coupled by configuration πf7/2g9/2 completely. Another type of negative parity levels are coupled by neutron cross-shell excitations from the sd shell under N=20. The 1- and 3- levels, obtained from the SDPFMU interaction, exhibit a dominant configuration of πf7/22νd15/2f7/2.

When comparing the experimental data of 42Ca and 42Ti, some differences are observed in the low-lying energy levels. For example, the first 2+, 4+, and 6+ levels of 42Ti are slightly higher than those of 42Ca, while the GXPF1A interaction predicts the same energy values. The EPQQM interaction, by incorporating different force strengths for protons and neutrons, effectively captures the distinction between 42Ca and 42Ti. As shown in Table 1, the pairing force strength of g0,pp (g2,pp) is 0.450 (0.470), while g0,nn (g2,nn) is 0.422 (0.449). This small discrepancy in force strengths can accurately reproduce the energy difference between 42Ca and 42Ti as observed in experiments.

3.3
42Sc

As an odd-odd nucleus, 42Sc offers a unique opportunity to investigate the correlations between proton and neutron states. The excited states in 42Sc extend up to energies of 13 MeV, with the highest observed spin being J = 15. However, at present, the parity information for these states remains unknown. Theoretical calculations suggest that the configurations of low-lying states in 42Sc are formed by coupling the proton and neutron single particle states appearing in 41Sc and 41Ca (Fig. 3). Shell-model calculations predict that the main configuration of the ground state in 42Sc is πf7/2νf7/2 that couples eight states from 0+ to 7+. Here, the 0+ state is taken as the ground state in 42Sc and it matches the experimental data well. The interactions of GXPF1A (Th. 2) and SDPFMU (Th. 3) provide the 7+ state as the lowest state. The 7+ level at 0.616 MeV from the level systematics and shell model expectations is a long half-life isomer with an average of 61.7(4)s, which is significantly longer than the ground state 0+ at 680.79(28) ms [30].

Fig. 3
The calculations and experimental energy levels in 42Sc [30].
pic

In EPQQM model, the ground state 0+ has 91.4% of configuration πf7/2νf7/2 and 7.7% of configuration πp3/2νp3/2. The first excited state 1+ at 0.361MeV has 94.0% of configuration πf7/2νf7/2 and 4.6% of configuration πp3/2νp3/2. The level 7+ at 0.965 MeV is near to the datum 0.616 MeV, which is completely coupled by configuration πf7/2νf7/2. The level 5+ at 1.570 MeV is close to the datum 1.510 MeV, which has 77.3% of configuration πf7/2νf7/2, 12.6% of configuration πp3/2νf7/2, and 9.9% of configuration πf7/2νp3/2. The level 6+ is predicted at 1.763 MeV with a main configuration of πf7/2νf7/2. Theoretical calculations based on the three different interactions efficiently fit the experimental data of the observed 1+, 3+, and 5+ states.

As for negative parity levels coupled by the intruder orbit g9/2, they lie above 5 MeV with a main configuration πf7/2νg9/2. There is no datum observed in this energy extent. The level 1- at 5.269MeV is completely coupled by the configuration πf7/2νg9/2. The level 2- at 5.488MeV has 99.6 % of configuration πf7/2νg9/2. The level 8- at 5.569MeV is completely coupled by the configuration πf7/2νg9/2. The SDPFMU interaction provides negative parity levels as neutron core excitations around 5 MeV, with the main configuration πf7/2νd5/21f7/22.

3.4
43Ti

In this study, the energy levels in 43Ti are examined as an additional test of the current model (Fig. 4). Owing to the presence of an odd number of valence nucleons, the pf shell model space only couples negative parity levels. The positive parity levels can be coupled through intruder orbit g9/2 or cross-shell excitations. The ground state 7/2- is well reproduced by all three different models with a main configuration of πf7/22νf7/2, while some difference exists in percentages and minor configurations. In EPQQM, the ground state has 76.9% of configuration πf7/22νf7/2, 6.1% of configuration πf5/22νf7/2, and 5.0% of configuration πp3/22νf7/2. In GXPF1A, the ground state has 86.8% of configuration πf7/22νf7/2, 2.3% of configuration πf5/22νp1/2, and 1.8% of configuration πf7/2p3/2νf7/2. In SDPFMU, the ground state has 79.2% of configuration πf7/22νf7/2, 4.7% of configuration πp1/22νf1/2, and 3.8% of configuration πf7/2p3/2νf7/2.

Fig. 4
Calculations and experimental energy levels in 43Ti [30].
pic

The state 3/2- has mixed configurations as follows: 27.9% (30.4%) of πf7/22νf7/2, 28.0% (23.9%) of πf7/22νp3/2, and 20.7% (24.1%) πf7/2p3/2νf7/2 by EPQQM (GXPF1A) model. The SDPFMU model has some difference in this state’s configurations, which has a major part of 50.1% πf7/2f5/2νf7/2, and a minor part of 24.6% of πf7/22νf7/2. In EPQQM, the level 11/2- at 1.842 MeV is very close to the datum 1.858 MeV, with a difference factor 0.991. Its state has 70.7% of configuration πf7/22νf7/2 and 16.7% of configuration πf7/2p3/2νf7/2. The levels 15/2-, and 19/2- also have a main configuration πf7/22νf7/2.

The positive parity states around 6 MeV are coupled by two main configurations πf7/2g9/2νf7/2 and πf7/22νg9/2. The level 11/2+ at 5.708 MeV has 95.1% of πf7/2g9/2νf7/2. The level 13/2+ at 5.990 MeV has 91.4% of πf7/2g9/2νf7/2. The levels 15/2+, 17/2+, and 19/2+ have about 95 % of πf7/2g9/2νf7/2. Except the level 9/2+, the states from 1/2+ to 21/2+ around 6 MeV are all coupled by this configuration. The level 9/2+ at 4.923 MeV belongs to configuration πf7/22νg9/2. The interaction SDPFMU produces positive parity states near 2 MeV, which are coupled by neutron core excitations of configuration πf7/22νd5/21f7/22.

3.5
44Ti

As a self-conjugated nucleus, 44Ti is a benchmark for shell model calculations in the northeast of the doubly magic nucleus 40Ca. With two protons and two neutrons as valence nucleons, the nucleus 44Ti has more complicated and high energy states. The excited states in 44Ti reach up to 16 MeV, and the highest spin is 15 with negative parity information. For the positive parity levels shown in Fig. 5, the 0+, 2+, 4+, 6+, and 12+ levels have a main configuration πf7/22νf7/22 according to the three different interactions, while some difference is found in percentages and minor configurations.

Fig. 5
The calculations and experimental energy levels in 44Ti[30].
pic

In the EPQQM model, the ground state 0+ of 42Ca is composed of 56.7% πf7/22νf7/22 configuration. On the other hand, in the GXPF1A and SDPFMU models, the ground state 0+ consists of 70.4% and 78.5% πf7/22νf7/22 configurations, respectively.

Similarly, for the 2+ state, the EPQQM model predicts a 50.0% πf7/22νf7/22 configuration, while the GXPF1A and SDPFMU models assign 64.1% and 79.1% πf7/22νf7/22 configurations, respectively.

In the case of the 4+ state, the EPQQM model predicts a 54.8% πf7/22νf7/22 configuration, whereas the GXPF1A and SDPFMU models assign 56.7% and 74.6% πf7/22νf7/22 configurations, respectively.

Overall, the configurations in the GXPF1A and SDPFMU models tend to be more concentrated in the states of 42Ca compared to the EPQQM model, indicating a stronger dominance of the πf7/22νf7/22 configuration in these models.

In this study, the calculated energy levels from 0+ to 6+ are found to be in good agreement with the experimental data, indicating a successful reproduction of these states by the model used. Furthermore, when considering the high spin levels 8+, 10+, and 12+, the EPQQM model yields better results compared to the GXPF1A and SDPFMU models.

With even-valence nucleons, only positive parity levels can be coupled in the model space of the pf shell. The negative parity levels are from cross-shell excitations or are coupled by the intruder orbit g9/2. As neutron core excitations, the SDPFMU interactions provide negative parity states from 1- to 12- in the energy range from 4 to 9 MeV. Their main configuration is πf7/22νd5/21f7/23, while the 5- to 9- states fit the corresponding experimental data well.

For the negative parity states coupled by the intruder orbit g9/2, the EPQQM model reproduces very well the data (1-), (8-), (10-), (11-), and (12-), which has a main configuration πf7/22νf7/2g9/2. This good fit, coupled with intruder orbit g9/2 in nuclei 42Sc, 42Ti, and 43Ti confirms our predictions. The level 1- at 6.309 MeV has 77.5 % of configuration πf7/22νf7/2g9/2, which is very close to datum 1- at 6.220 MeV. The level 8- at 7.012 MeV has 79.5 % of configuration πf7/22νf7/2g9/2, with a difference factor 1.013 to the datum (8-) at 6.924 MeV. The level 10- at 8.968 MeV has a difference factor 1.012 by comparing with datum (10-) at 8.861 MeV. The level 11- at 9.815 MeV has 86.8 % of configuration πf7/22νf7/2g9/2, with a difference factor 1.009 to its corresponding datum (11-) at 9.723 MeV. The level 12- at 10.455 MeV has 86.8 % of configuration πf7/22νf7/2g9/2, with a difference factor 0.9992 to its corresponding datum (12-) at 10.463 MeV. The shell model with EPQQM interaction works very accurately even at about 10 MeV.

4

Summary

In this work, we have developed a new interaction with the pf shell and the intruder orbit g9/2, and studied the energy levels of nuclei 42Ca, 42Sc, and 42-44Ti near the doubly magic nucleus 40Ca. The main conclusions of the present study are as follows:

(1) For 42Ca, 42Sc, and 42Ti, the low-lying levels in positive parity have been well-reproduced, and negative parity levels have been predicted to be coupled by the intruder orbit g9/2. In 42Ca (42Ti), the negative parity members of νf7/2g9/2 (πf7/2g9/2) are predicted around 6 MeV, while in 42Sc, the negative parity levels coupled by the configuration πf7/2νg9/2 are predicted to be above 5 MeV.

(2) In the case of 43Ti, the theoretical calculations successfully reproduce the negative parity levels. Additionally, the positive parity configurations, specifically πf7/2g9/2νf7/2, which are coupled by the intruder orbit g9/2, are predicted to appear at approximately 6 MeV

(3) In the case of 44Ti, all three different interactions used in the study successfully reproduce the energy levels of the first 2+, 4+, and 6+ states. Specifically, the EPQQM interaction shows excellent agreement with the experimental data for the (1-), (8-), (10-), (11-), and (12-) states, which have a dominant configuration of πf7/22νf7/2g9/2. This successful reproduction of the data further confirms the accuracy of the predictions made for the levels of 42Sc, 42Ti, and 43Ti, which are coupled by the intruder orbit g9/2.

(4) It is necessary to consider the intruder orbit g9/2 when studying the high energy states in nuclei near the doubly magic nucleus 40Ca. The present work provides a new, useful interaction for further experimental and theoretical research in this region, such as, band mixing in this region.

References
1. W. R. Dixon, R. S. Storey, and J. J. Simpson,

Lifetimes of 44Ti levels

. Nucl. Phys. A 202, 579 (1973). doi: 10.1016/0375-9474(73)90644-1
Baidu ScholarGoogle Scholar
2. J. J. Simpson, W. R. Dixon, and R. S. Storey,

Evidence for rotational bands in 44Ti

. Phys. Rev. Lett. 31, 946 (1973). doi: 10.1103/PhysRevLett.31.946
Baidu ScholarGoogle Scholar
3. W. R. Dixon, R. S. Storey, and J. J. Simpson,

Levels of 44Ti from the 40Ca(α, γ) 44Ti reaction

. Phys. Rev. C 15, 1896 (1977). doi: 10.1103/PhysRevC.15.1896
Baidu ScholarGoogle Scholar
4. J.W. Olness, J. J. Kolata, E.K. Warburton,

High-spin states in 44Ti and 44Sc*

. Phys. Rev. C 10, 1663 (1974). doi: 10.1103/PhysRevC.10.1663
Baidu ScholarGoogle Scholar
5. C. Michelagnoli, C.A. Ur, E. Farnea et al.,

Lifetime measurement in the N = Z nucleus 44Ti*

. Acta Phys. Pol. B 42, 825 (2011). doi: 10.5506/APhysPolB.42.825
Baidu ScholarGoogle Scholar
6. K. Arnswald, T. Braunroth, M. Seidlitz et al.,

Enhanced collectivity along the N = Z line: Lifetime measurements in 44Ti, 48Cr, and 52Fe

. Phys. Lett. B 772, 599-606 (2017). doi: 10.1016/j.physletb.2017.07.032
Baidu ScholarGoogle Scholar
7. K. Arnswald, P. Reiter, A. Blazhev et al.,

Lifetime measurements in 44Ti

. Phys. Rev. C 102, 054302 (2020). doi: 10.1103/PhysRevC.102.054302
Baidu ScholarGoogle Scholar
8. L. Zhou, S. M. Wang, D. Q. Fang et al.,

Recent progress in two-proton radioactivity

. Nucl. Sci. Tech. 33, 105 (2022). doi: 10.1007/s41365-022-01091-1
Baidu ScholarGoogle Scholar
9. X. Zhou, M. Wang, Y. H. Zhang et al.,

Charge resolution in the isochronous mass spectrometry and the mass of 51Co

. Nucl. Sci. Tech. 32, 37 (2021). doi: 10.1007/s41365-021-00876-0
Baidu ScholarGoogle Scholar
10. X. B. Wei, H. L. Wei, Y. T. Wang et al.,

Multiple-models predictions for drip line nuclides in projectile fragmentation of 40,48Ca, 58,64Ni, and 78,86Kr at 140 MeV/u

. Nucl. Sci. Tech. 33, 155 (2022). doi: 10.1007/s41365-022-01137-4
Baidu ScholarGoogle Scholar
11. Y. F. Gao, B. S. Cai, C. X. Yuan et al.,

Investigation of β- decay half-life and delayed neutron emission with uncertainty analysis

. Nucl. Sci. Tech. 34, 9 (2023). doi: 10.1007/s41365-022-01153-4
Baidu ScholarGoogle Scholar
12. A. A. Raduta, L. Zamick, E. Moya de Guerra et al.,

Description of single and double analog states in the f7/2 shell: The Ti isotopes

. Phys. Rev. C 68, 044317 (2003). doi: 10.1103/PhysRevC.68.044317
Baidu ScholarGoogle Scholar
13. A. Juodagalvis, I. Ragnarsson, and S. Aberg,

Cranked Nilsson-Strutinsky vs the spherical shell model:A comparative study of pf-shell nuclei

. Phys. Rev. C 73, 044327 (2006). doi: 10.1103/PhysRevC.73.044327
Baidu ScholarGoogle Scholar
14. Y. Utsuno, T. Otsuka, B. Alex Brown et al.,

Shape transitions in exotic Si and S isotopes and tensor-force-driven Jahn-Teller effect

. Phys. Rev. C 86, 051301(R) (2012). doi: 10.1103/PhysRevC.86.051301
Baidu ScholarGoogle Scholar
15. B. A. Brown, B. H. Wildenthal,

Status of the nuclear shell model

. Annu. Rev. Nucl. Part. Sci. 38, 29 (1988). doi: 10.1146/annurev.ns.38.120188.000333
Baidu ScholarGoogle Scholar
16. M. Honma, T. Otsuka, B.A. Brown et al.,

Shell-model description of neutron-rich pf-shell nuclei with a new effective interaction GXPF1

. Eur. Phys. J. A 25, 499 (2005). doi: 10.1140/epjad/i2005-06-032-2
Baidu ScholarGoogle Scholar
17. Y. Utsuno, T. Otsuka, T. Mizusaki et al.,

Varying shell gap and deformation in N;20 unstable nuclei studied by the Monte Carlo shell model

. Phys. Rev. C 60, 054315 (1999). doi: 10.1103/PhysRevC.60.054315
Baidu ScholarGoogle Scholar
18. A. Poves, A. Zuker,

Theoretical spectroscopy and the fp shell

. Phys. Rep. 70, 235 (1981). doi: 10.1016/0370-1573(81)90153-8
Baidu ScholarGoogle Scholar
19. M. Hasegawa, K. Kaneko, and S. Tazaki,

Improvement of the extended P + QQ interaction by modifying the monopole field

. Nucl. Phys. A 688, 765 (2001). doi: 10.1016/S0375-9474(00)00602-3
Baidu ScholarGoogle Scholar
20. K. Kaneko, M. Hasegawa, T. Mizusaki,

Quadrupole and octupole softness in the N = Z nucleus 64Ge

. Phys. Rev. C 66, 051306(R) (2002). doi: 10.1103/PhysRevC.66.051306
Baidu ScholarGoogle Scholar
21. K. Kaneko, Y. Sun, M. Hasegawa et al.,

Shell model study of single-particle and collective structure in neutron-rich Cr isotopes

. Phys. Rev. C 78, 064312 (2008). doi: 10.1103/PhysRevC.78.064312
Baidu ScholarGoogle Scholar
22. K. Kaneko, Y. Sun, T. Mizusaki et al.,

Shell-model study for neutron-rich sd-shell nuclei

. Phys. Rev. C 83, 014320 (2011). doi: 10.1103/PhysRevC.83.014320
Baidu ScholarGoogle Scholar
23. H. K. Wang, S. K. Ghorui, Z. Q. Chen et al.,

Analysis of low-lying states, neutron-core excitations, and electromagnetic transitions in tellurium isotopes 130-134Te

. Phys. Rev. C 102, 054316 (2020). doi: 10.1103/PhysRevC.102.054316
Baidu ScholarGoogle Scholar
24. H. K. Wang, S. K. Ghorui, K. Kaneko et al.,

Large-scale shell-model study for excitations across the neutron N = 82 shell gap in 131-133Sb

. Phys. Rev. C 96, 054313 (2017). doi: 10.1103/PhysRevC.96.054313
Baidu ScholarGoogle Scholar
25. H. K. Wang, Y. Sun, H. Jin et al.,

Structure analysis for hole-nuclei close to 132Sn by a large-scale shell-model calculation

. Phys. Rev. C 88, 054310 (2013). doi: 10.1103/PhysRevC.88.054310
Baidu ScholarGoogle Scholar
26. H. K. Wang, K. Kaneko, and Y. Sun,

Isomerism and persistence of the N = 82 shell closure in the neutron-rich 132Sn region

. Phys. Rev. C 89, 064311 (2014). doi: 10.1103/PhysRevC.89.064311
Baidu ScholarGoogle Scholar
27. H. K. Wang, K. Kaneko, Y. Sun et al.,

Monopole effects, isomeric states, and cross-shell excitations in the A = 129 hole nuclei near 132Sn

. Phys. Rev. C 95, 011304 (2017). doi: 10.1103/PhysRevC.103.024317
Baidu ScholarGoogle Scholar
28. A. J. Majarshin, Y. A. Luo, F. Pan et al.,

Nuclear structure and band mixing in 194Pt

. Phys. Rev. C 103, 024317 (2021). doi: 10.1103/PhysRevC.103.024317
Baidu ScholarGoogle Scholar
29. A. J. Majarshin, Y. A. Luo, F. Pan et al.,

Structure of rotational bands in 109Rh

. Phys. Rev. C 104, 014321 (2021). doi: 10.1103/PhysRevC.104.014321
Baidu ScholarGoogle Scholar
30. http://www.nndc.bnl.gov/ensdf/.
31. B. A. Brown, W. D. M. Rae,

The Shell-Model Code NuShellX@MSU

. Nucl. Data Sheets 120, 115 (2014). doi: 10.1016/j.nds.2014.07.022
Baidu ScholarGoogle Scholar
32. Y. Z. Ma, L. Coraggio, L. D. Augelis et al.,

Contribution of chiral three-body forces to the monopole component of the effective shell-model Hamiltonian

. Phys. Rev. C 100, 034324 (2019). doi: 10.1103/PhysRevC.100.034324
Baidu ScholarGoogle Scholar
33. S. R. Stroberg, H. Hergert, S. K. Bogner et al.,

Nonempirical interactions for the nuclear shell model: An update

. Annu. Rev. Nucl. Part. Sci. 69, 307 (2017). doi: 10.1146/annurev-nucl-101917-021120
Baidu ScholarGoogle Scholar
34. A. P. Zuker,

Three-body monopole corrections to realistic interactions

. Phys. Rev. Lett. 90, 042502 (2003). doi: 10.1103/PhysRevLett.90.042502
Baidu ScholarGoogle Scholar
35. H. K. Wang, Z. H. Li, Y. B. Wang et al.,

High-spin levels, β-decay and monopole effects in A = 128 hole nuclei near 132Sn

. Phys. Lett. B. 833, 137337 (2022). doi: 10.1016/j.physletb.2022.137337
Baidu ScholarGoogle Scholar
36. R. F. Takaharu Otsuka, Toshio Suzuki, H. Grawe et al.,

Evolution of nuclear shells due to the tensor force

. Phys. Rev. Lett. 95, 232502 (2005). doi: 10.1103/PhysRevLett.95.232502
Baidu ScholarGoogle Scholar
37. H. K. Wang, Z.Q. Chen, H. Jin et al.,

Ground state inversions in hole nuclei near 132Sn driven by the monopole interaction

. Phys. Rev. C 104, 014301 (2021). doi: 10.1103/PhysRevC.104.014301
Baidu ScholarGoogle Scholar
Footnote

The authors declare that they have no competing interests.