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.
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.
Hamiltonian
In the proton-neutron (pn) representation, the present Hamiltonian is composed of the pairing-plus-multipole force and the monopole corrections:
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 |
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
Monopole corrections
In the present Hamiltonian, the monopole corrections can be investigated as follows:
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.
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
-202306/1001-8042-34-06-005/alternativeImage/1001-8042-34-06-005-F001.jpg)
Regarding negative parity levels, the 8- configuration
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
In EPQQM, the first 2+ state has 79.8 % of
For negative parity level states, the 8- coupled by
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 Jπ = 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
-202306/1001-8042-34-06-005/alternativeImage/1001-8042-34-06-005-F002.jpg)
In this study, the negative parity levels ranging from 1- to 8- coupled by the configuration
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.
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
-202306/1001-8042-34-06-005/alternativeImage/1001-8042-34-06-005-F003.jpg)
In EPQQM model, the ground state 0+ has 91.4% of configuration
As for negative parity levels coupled by the intruder orbit g9/2, they lie above 5 MeV with a main configuration
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
-202306/1001-8042-34-06-005/alternativeImage/1001-8042-34-06-005-F004.jpg)
The state 3/2- has mixed configurations as follows: 27.9% (30.4%) of
The positive parity states around 6 MeV are coupled by two main configurations
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
-202306/1001-8042-34-06-005/alternativeImage/1001-8042-34-06-005-F005.jpg)
In the EPQQM model, the ground state 0+ of 42Ca is composed of 56.7%
Similarly, for the 2+ state, the EPQQM model predicts a 50.0%
In the case of the 4+ state, the EPQQM model predicts a 54.8%
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
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
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
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
(2) In the case of 43Ti, the theoretical calculations successfully reproduce the negative parity levels. Additionally, the positive parity configurations, specifically
(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
(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.
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