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Shape polarization and coexistence of high-K three-quasiparticle states in odd-mass N=106 isotones

NUCLEAR PHYSICS AND INTERDISCIPLINARY RESEARCH

Shape polarization and coexistence of high-K three-quasiparticle states in odd-mass N=106 isotones

Run-Yan Dong
Chang-Feng Jiao
Nuclear Science and TechniquesVol.37, No.5Article number 78Published in print May 2026Available online 09 Feb 2026
9600

Three-quasiparticle K-isomeric states in odd-mass N=106 isotones within the A~180 mass region were systematically investigated using configuration-constrained potential energy surface calculations. The calculations successfully reproduced the excitation energies and deformations of the known high-K isomers in nuclei from 175Tm to 181Re. For the nuclei closer to the Z=82 shell closure (183Ir, 185Au, and 187Tl), predictions of the configurations of the observed and yet-to-be-observed isomers are provided. The results reveal strong shape polarization, where the three-quasiparticle states are driven to larger deformations compared to the often shape-soft or spherical ground states. A particularly rich spectrum of shape coexistence is predicted in 187Tl, where several high-K three-quasiparticle configurations with distinct prolate, oblate, and triaxial shapes are found to coexist at similar excitation energies. Notably, the oblate-deformed =29/2+ configuration at Ex = 1839 keV was proposed to be responsible for a long-lived isomer. This study provides a comprehensive picture of shape evolution and coexistence in high-K multi-quasiparticle states, offering valuable insights for future experimental studies.

Shape polarizationShape coexistenceHigh-K isomeric stateConfiguration-constrained potential energy surface
1

Introduction

Neutron-deficient isotones around N=106 mid-shell are characterized by the existence of an abundance of low-lying high-seniority isomeric states. In this region, the orbitals with large Ω, namely the projection of individual angular momentum onto the intrinsic symmetric axis, approach the neutron Fermi surface at moderate quadrupole deformations. This facilitates the formation of broken-pair states with high K values (where ) near the yrast line. According to the selection rules for electromagnetic transitions, the transitions of multipolarity λ would be significantly hindered if ΔK > λ. The so-called K-hindrance can lead to relatively long half-lives (on the order of nanoseconds or longer) [1-3], leading to the formation of “K isomers”. One of the most well-known examples of high-K isomers is found in 178Hf, in which two 2-quasiparticle (qp) = 8- isomers and a long-lived four-quasiparticle = 16+ isomer with a half-life of 31 years have been observed [4, 5]. Since the occurrence of K isomers is a combined effect of the unpaired nucleons occupying high-Ω states and the nuclear deformation, the study of K isomeric states is pivotal for understanding the interplay between the shell structure of “individual” nucleons and the collective behavior of a strongly correlated nucleus [1].

Another common feature associated with the A~180 mass region is the shape of the transition. In this region, the ground-state (g.s.) shape can change from a well-deformed prolate ellipsoid with for 176Yb to a very soft spheroid for 188Pb [6, 7]. Moreover, the soft shape gives rise to a novel shape coexistence phenomenon, characterized by the emergence of low-lying states with different intrinsic shapes in one atomic nucleus. In general, it originates from the combining effect of approaching the Z=82 spherical shell closures and the deformed shell gaps around the neutron mid-shell at N = 104-106 due to quadrupole-quadrupole correlations. It has drawn considerable interest [8-11]. The most well-known example is the differently shaped 0+ triplet observed in 186Pb, which corresponds to the coexistence of the prolate, oblate, and spherical configurations [12, 13]. Coexisting 0+ states in even-even Pt, Hg, Pb, and Po isotopes around the neutron midshell have been extensively studied [9, 14-22].

In addition to the shape change resulting from collective correlations, such as quadrupole-quadrupole interactions, unpaired nucleons are found to strongly polarize the nuclear shape [23]. Because K isomeric states are coupled by high-Ω unpaired nucleons, shape polarization may yield considerable differences in shape between the high-K states and ground states, leading to novel structures that involve both K isomerism and shape isomerism. For example, the two-quasineutron isomeric states which are systematically observed in the even-even N=106 isotones between 174Er and 188Pb (see [24, 25] and references therein). Previous theoretical investigations have shown that the ground states (g.s.) are oblate deformed with for 186Hg and spherical for 188Pb, whereas the K=8- isomeric states are polarized to prolate deformed with . The K=8- isomers with shapes different from those of the g.s. have been confirmed by measuring the rotational bands built on them [26, 27]. Furthermore, it was found that for shape-soft nuclei, the shape changes, particularly in the triaxial deformations, can be important for understanding the observed behaviors of isomeric states, such as decay properties [6].

While the shape evolution and coexistence of high-K states in even-even nuclei around the neutron mid-shell and A~180 have been extensively studied, the structural properties, such as the shape changing effects of 3-qp high-K states in their odd-proton neighbors, have not been systematically investigated. In odd-A nuclei, although the unpaired nucleon introduces additional complexity, it serves as a sensitive probe of the underlying shell structure. The shape polarization effect induced by the single nucleon can be either parallel to or opposed to that of the high-K 2-qp configuration, thereby amplifying or diminishing the shape difference between the 3-qp states and the g.s.. Recently, the 3-qp high-K isomers, originated from the coupling between the odd proton and the aforementioned = 8- configuration in even-mass cores, have been observed in odd-mass N = 106 isotones from 175Tm to 187Tl (except the 183Ir) [28-34]. In addition, a substantial amount of experimental data also suggest that the low-lying 1-qp states of neutron-deficient odd-mass Au and Tl isotopes exhibit shape coexistence [8-10, 35, 36]. The extent to which the observed 3-qp isomers can be considered to involve shape isomerism, in addition to K isomerism, remains unclear. Thus, it has greatly stimulated our interest in pursuing theoretical studies on shape polarization and coexistence in the 3-qp high-K states within this mass region.

In this study, we investigate the 3-qp K-isomeric states of odd-A nuclei in the N = 106 isotonic chain using the configuration-constrained potential energy surface (PES) method [37]. This method includes the axially asymmetric γ-degree of freedom. Furthermore, in this method, we do not introduce an adjustable parameter for the pairing strength, and the deformation is determined self-consistently by minimizing the corresponding PES. At prolate deformations, we mainly focus on the study of the high-K 3-qp configurations composed of the coupling of the unpaired proton and the = 8- 2-qp configuration that are observed systematically in even-even N=106 nuclei. We predicted the possible configurations of the isomers in 185Au and 187Tl, with particular attention to the shape-polarization effect of multi-qp excitations. Furthermore, we explored the high-K states with distinct shapes (oblate, prolate, and triaxial) that coexist at comparable excitation energies in 187Tl, and analyzed the impact of different quasiparticle configurations on shape evolution in detail.

2

The model

We employed the configuration-constrained PES approach [37], based on the macroscopic-microscopic model. The macroscopic energy contribution was computed using the standard liquid-drop model [38] with parameters taken from Ref. [39]. The microscopic correction includes the Strutinsky shell correction [40] and the pairing correction. The single-particle levels required for the microscopic energy calculations were obtained from a non-axially deformed Woods-Saxon potential [41] using the “universal” parameter set [42]. The so-called universal parameter set (listed in Table 1) was optimized by simultaneously fitting the single-particle energies in 208Pb, particularly those corrected for nucleon-nucleus interactions beyond the independent particle model, as well as the high-spin yrast spectra of 212Rn and 204Pb [42]. These parameters have been further tested for light nuclei [41], and for heavier nuclei with [43], showing satisfactory performance in describing not only the single (quasi)particle level sequences but also the nuclear equilibrium deformations. Because these parameters were optimized for the lead region, they were validated as the best-fit Woods-Saxon potential parameters for this mass region.

Table 1
The universal parameters of the Woods-Saxon potential
Particles V0 κ a rn λn
Neutron 49.6 0.86 0.70 1.347 35.0 1.31
Proton 49.6 0.86 0.70 1.275 36.0 1.30
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To avoid the collapse of pairing correlations in multi-quasiparticle states, we used the Lipkin-Nogami (LN) version of the Bardeen-Cooper-Schrieffer (BCS) method [44] as an approximate particle-number projection scheme, incorporating monopole pairing. The pairing strength G was initially determined using the average-gap method [45, 46]. Although it is often further adjusted to reproduce the odd-even mass difference using a five-point formula, we note that irregularities may arise near magic numbers (e.g., Au and Tl isotopes) [45]. This is partly due to the limitations of the BCS approach and the artifacts from the LN correction. It is also because the odd-even mass difference equations used to extract experimental pairing gaps are derived under the assumption that there are no non-smooth contributions to the masses apart from pairing effects, while this assumption is often not fulfilled at magic numbers [45]. Therefore, following the recommendation of Ref. [45], closed-shell nuclei were excluded from the pairing-strength calibration. For consistency, we adopted a standard pairing strength across all isotopes under investigation.

In the PES calculations, a deformation mesh in was used, with the hexadecapole deformation β4 variation at each mesh point. For broken-pair configurations, the microscopic energy incorporates contributions from unpaired nucleons occupying specific single-particle orbitals (see Ref. [37] for more details). These orbitals were continuously tracked and adiabatically blocked throughout the (β2, γ) deformation plane. For axially deformed nuclei, single-particle orbitals can be specified by their individual spin projection, Ω. However, for axially asymmetric shapes, Ω is no longer conserved. In addition, several single-particle orbits with approximately the same spin projection |Ω| may become energetically close at given (β2, γ) deformations. To reliably track orbits, we computed and compared not only the average spin projection |Ω| but also the expectation values of the Nilsson numbers , , and between two adjacent deformation mesh points. We verified that, although the Nilsson numbers N, nz, Λ, and |Ω| are not strictly conserved, their expectation values exhibit slow variation, allowing for a reliable configuration assignment. Therefore, each configuration was identified by computing the average Nilsson quantum numbers of the blocked orbitals. The total energy of a multi-qp state with unpaired nucleons can be decomposed into the deformation energy and configuration energy, where the latter originates from qp excitations due to pair breaking and excitations of particles that define the specific configuration.

Quasiparticle excitations, particularly in deformation-soft nuclei, can induce significant shape polarization, resulting in an equilibrium deformation of the multi-qp state that differs from that of the ground state. The configuration-constrained PES method effectively accounts for this polarization caused by the unpaired nucleon and offers a self-consistent description of both the deformation and excitation energy of multi-qp states [6, 47]. The excitation energy was computed as the energy difference between the PES minimum of the excited configuration and that of the ground-state configuration, enabling a direct comparison with the experimental values.

3

Calculations and discussions

3.1
Systematics of 3-qp states involved

For nuclei in the A~180 region, an abundance of high-K isomeric states has been discovered [48]. Among them, the two-quasineutron isomeric states exist systematically in even-even N = 106 isotones, which have been investigated using configuration-constrained PES calculations in Ref. [6]. The calculated excitation energies agree well with the experimental data, and strong shape polarizations were found when approaching the Z=82 shell closure. For odd-mass N = 106 isotones in this mass region, most of the observed 3-qp K isomers consistently involve a two-quasineutron configuration coupled to = 8- states that are identified in the aforementioned even-even nuclei. For example, in nuclei such as 175Tm [28, 49], 177Lu [29, 50], 179Ta [30, 51, 52], and 181Re [31, 53], 3-qp K isomers have been assigned as the two-quasineutron = 8- configuration coupled to the energetically lowest one-quasiproton configuration. Furthermore, in 181Re, 179Ta, and 177Lu, the meta-stable =9/2- states are found, assigned to the π9/2- [514] configuration, leading to the presence of 3-qp states associated with the coupling of a = 8- two-quasineutron configuration with π9/2- [514] [29-31]. In 175Tm, a K isomer that may involve the coupling of the two-quasineutron = 8- configuration with the π 7/2- [523] has been found [28]. The half-lives of these isomers range from a few microseconds to several days. The extent to which these high-K states are associated with shape polarization and shape isomerism remains an open question.

We performed configuration-constrained PES calculations on the 1-quasiproton and 3-qp states in N = 106 odd-mass isotones. Table 2 presents the calculated deformations and energies of the g.s., possible high-Ω 1-quasiproton, and low-lying high-K 3-qp states, compared with the available experimental data. Our calculations reproduce the experimentally assigned spin-parity of the g.s. of these nuclei, except for 177Lu, in which the calculated lowest 1-quasiproton configuration is the π9/2-[514] rather than the experimentally assigned π7/2+[404] [54]. However, the calculated π7/2+[404] configuration lies only 259 keV above the π9/2-[514] state. Given the strong dependence of the 1-qp state energies on the ordering and spacing of the single-particle levels, the deviation in their relative positions falls within an acceptable range.

Table 2
Calculated deformations and excitation energies Ecal for odd-A nuclei in the N = 106 isotopic chain
Nuclei Configuration Eexp (keV) Ecal (keV) β2 β4 γ
175Tm 0 0 0.279 -0.042 0.04
439 28 0.276 -0.041 0.08
1004.8 1176 0.281 -0.042 0.06
1517.7 1343 0.279 -0.043 0.06
177Lu 0 259 0.257 -0.043 -0.05
150.4 0 0.270 -0.055 0.06
970.2 1487 0.261 -0.043 0.06
1324.4 1197 0.273 -0.054 0.05
179Ta 0 0 0.248 -0.049 0.04
30.7 16 0.245 -0.047 0.00
1252.6 1313 0.241 -0.049 -0.09
1328 1260 0.254 -0.048 0.17
1317 1279 0.254 -0.046 0.13
181Re 0 0 0.219 -0.045 -0.18
262.9 201 0.216 -0.040 -0.63
1656.4 1657 0.230 -0.043 -0.36
1880.6 1864 0.229 -0.037 -0.48
183Ir 0 0.224 -0.030 0.02
645.3 492 0.222 -0.023 -2.10
1552 0.233 -0.030 0.03
2011 0.245 -0.025 0.05
185Au 0 0.151 -0.025 23.53
24 169 0.183 -0.001 -59.08
523 0.235 -0.029 11.70
8.9 269 0.198 -0.022 -24.84
1967 0.230 -0.033 1.04
1981 0.246 -0.031 1.14
187Tl 0 0 0.024 0.001 -2.27
952 888 0.214 -0.014 18.32
2312 0.225 -0.016 -12.13
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The experimental energies Eexp can be found in Refs. [33, 48] and references therein

One may ask the sensitivity of these calculated results to the pairing strengths or Woods-Saxon parameters. Note that previous work has shown that the adjustment of pairing strength mainly influences the quasiparticle energy gaps and only slightly affects the deformations [37], while the ordering of single-particle levels at a certain deformation is primarily determined by the choice of Woods-Saxon potential parameters. To examine the robustness of this result, we tested several known parameter sets, including those of Blomquist and Wahlborn [55], the parameters of Chepurnov [56], the parameters given by Rost [57], and the “new” parameters [58]. We found that the deviation in the relative positions of the π9/2-[514] and π7/2+[404] configurations of 177Lu was preserved with different parameter sets. To accurately reproduce the ordering of the low-lying 1-qp states of 177Lu, an improvement in the Woods-Saxon potential is needed.

Experimentally, the spin and parity of the g.s. of 183Ir [59] and 185Au [60-62] have been assigned to be the 5/2- states built on the π1/2-[541] configuration, while a strong mixing between the π1/2-[541] and π3/2-[532] configurations attributed to the Coriolis interactions has been proposed for the 5/2- g.s. of 185Au [63]. Our calculations show that the π1/2-[541] configuration has the lowest energy, whereas the π3/2-[532] state is approximately 500 keV higher. The present PES calculations show that these two low-lying 1-quasiproton states both have considerable triaxial deformations, which would reinforce substantial configuration mixing. However, the configuration mixing calculations are beyond the scope of the present study.

The present configuration-constrained PES calculations also reasonably reproduce the high-Ω 1-qp isomeric states observed in odd-mass N=106 isotones, except for the aforementioned deviation in 177Lu. Notably, the configuration-constrained PES calculations show that the =9/2- isomer of 185Au and the =11/2- state of 187Tl have moderate triaxial deformations with which are remarkably polarized when compared with their ground states. This indicates the appearance of single-proton-induced shape polarization in shape-soft odd-proton nuclei when approaching the Z=82 closed shell.

Now, we turn to the investigation of energetically low-lying 3-qp states in odd-mass N=106 isotones. We mainly focus on the 3-qp states that consist of the two-quasineutron configuration coupled to different 1-quasiproton configurations, since the =8- isomeric states are systematically identified as the configuration in even-even N=106 isotones. As shown in Table 2, the calculated energies of these 3-qp states in 175Tm, 179Ta, and 181Re agree well with the experimental data. For 177Lu, the calculated configuration is overpredicted, while the state is slightly underestimated. This can be attributed to the deviation of the π7/2+[404] and π9/2-[514] orbitals found in the calculations of the 1-quasiproton states.

Furthermore, the configuration-constrained PES calculations predict the candidate configurations of the 3-qp isomeric states in odd-A N=106 isotones when moving towards the Z=82 shell closure. To date, no experimental evidence has been reported for three-quasiparticle high-K isomers in 183Ir. We proposed two possible high-K 3-qp states that are composed of two-quasineutron coupled with the proton configurations of π1/2-[541] and 9/2-[514], respectively. For 185Au, a new isomer at an excitation energy of 1504.2(4) keV with a half-life of 630(80) ns was identified in γ-γ coincidence analysis [34]. The possible spins of this isomer are constrained to a range from 13/2 to 21/2 in comparison with the predictions from the Weisskopf estimates [34]. Our calculations suggest two possible 3-qp high-K configurations that are consistent with the systematics of 3-qp configurations in lighter odd-mass N=106 isotones. They both lie at excitation energies of approximately 1900 keV, which is slightly overpredicted. However, Ref. [34] argued that the g.s. configuration of 185Au is more likely π3/2-[532], and the calculated energy differences of these two 3-qp states with respect to the 3/2-[532] configuration are 1444 and 1458 keV, respectively, which is in great agreement with the observation. For nucleus 187Tl, two isomers with microsecond lifetimes (T1/2 = 1.11 μs and 0.69 μs) have been reported [32]. Spin-parities = 27/2+, 31/2- are tentatively assigned to the isomer at 2584 keV with a lifetime T1/2 = 0.69 μs based on the deduced total conversion coefficient [33]. Our calculation presents a = 27/2+, configuration with an excitation energy of 2312 keV, which is in agreement with the prolate high-K configuration suggested in Ref. [32]. This implies that the T1/2 = 0.69 μs isomer observed in 187Tl involves the two-quasineutron configuration, which is consistent with the systematics of the 3-qp isomers observed in lighter odd-mass N=106 isotones. However, further experimental data are required to unambiguously assign the spin-parity and configuration of these observed isomers. We will discuss the other T1/2 = 1.1 μs isomer later in Sect. 3.2.

In addition, intrinsic shape evolution is crucial for understanding the behavior of isomeric states, such as their decay properties. In a previous study [6], strong shape polarization was shown in even-even nuclei with A~180 and N=106, especially in nuclei close to the Z = 82 shell closure. For systematic comparison, we plot the variation of β2 and γ deformations of the high-K 3-qp states and the g.s. along with the proton number Z in Fig. 1. When approaching the shell closure of Z = 82, the β2 value of the g.s. gradually decreases, indicating that the g.s. shape evolves towards a spheroid, whereas the 3-qp states are polarized to have distinct prolate shapes. The g.s. of 185Au, for example, has a remarkably γ-soft shape with a very shallow PES minimum at . Considering that the g.s. of 185Au can be interpreted as the coupling of a low-Ω π 1h9/2 proton with the 184Pt core, the PES of the g.s. of 185Au exhibits similar γ softness compared to 184Pt. This γ-soft nature of 184Pt is mainly because the prolate-to-oblate shape transition going through a transitional γ-soft shape occurs in Pt isotopes around N=110, which has been suggested by the self-consistent HFB calculation using the Gogny-D1S interaction and the interacting boson model [64], as well as the five-dimensional collective Hamiltonian (5DCH) based on covariant density-functional theory [65]. In contrast, the predicted two 3-qp high-K states of 185Au both have an approximately prolate shape with and about a 60% increase in β2 deformation. The nucleus 187Tl has a spherical g.s. with a proton that singly occupies the π3s1/2 orbital, while the calculated state is predicted to have a moderately axially-asymmetric shape with β2≈0.23 and , exhibiting the greatest difference in quadrupole deformation between the 3-qp state and the g.s.. In fact, the calculated high-K 3-qp configurations of 187Tl present an ensemble of multiple nuclear shapes, which will be analyzed in detail in Sect. 3.2.

Fig. 1
Calculated β2 and γ deformations for the g.s. and 3-qp states of odd-A nuclei in the N=106 isotonic chain. For Z=69-79, the 3-qp states correspond to the coupling of the 2-qp =8- configuration with the g.s. configurations of odd-A nuclei, which are π1/2+[411], π7/2+[404], π7/2+[404], π5/2+[402], π1/2-[541], and π1/2-[541], respectively. For Z=81, the 3-qp state is . These 3-qp states correspond to observed high-K isomers
pic
3.2
Shape coexistence in high-K 3-qp states of 187Tl

The shape-coexisting configurations in this mass region are mainly attributed to the large spherical and deformed shell gaps that simultaneously appear near the proton shell closure at Z=82 and the neutron mid-shell at . Moreover, the unpaired nucleon that occupies different single-particle orbitals polarizes the shape of the odd-A nucleus in different ways, leading to a more profound shape coexistence phenomenon. An abundance of experimental data has demonstrated that different-shaped configurations in these odd-A nuclei are observed not only in the low-lying 1-qp states but also in the higher-seniority isomeric states [9].

For 187Tl, previous studies [66-69] have proposed the coexistence of different nuclear shapes based on an analysis of the observed low-lying collective structures. As the proton-hole neighbor of 188Pb, the I=1/2+ g.s. of 187Tl can be interpreted as the coupling of the π3s1/2 hole with the spherical state of 188Pb core. The observed =9/2- and =13/2+ isomeric states can be understood as filling the π9/2-[505] and π13/2+[606] intruder orbitals that are lowered along with the increase in oblate deformation, respectively [70, 71], while the rotational band built on the =11/2- state is suggested to be the prolate deformed π 11/2-[505] configuration [32, 33]. The calculated deformations and excitation energies for the 1-quasiproton states are listed in Table 3. The configuration-constrained PES calculations reproduce the measured excitation energies well and clearly show the coexisting shapes of these 1-qp states. Note that the π 11/2-[505] configuration has been predicted to have a considerable axial-asymmetric shape of , which breaks down the K- and shape-hindrance and would explain why it decays rapidly to the oblate =9/2- isomeric state [32].

Table 3
Calculated deformations and excitation energies Ecal for the g.s., the low-lying high-Ω 1-qp, and high-K 3-qp states of 187Tl
Configuration Eexp (keV) Ecal (keV) β2 β4 γ
0 0 0.024 0.001 -2.27
335 147 0.164 -0.005 -59.62
952 888 0.214 -0.014 18.32
1061 1202 0.184 0.007 -59.95
1216 0.267 -0.012 -17.49
742 0.168 -0.019 -59.89
1839 0.192 -0.018 -59.46
2312 0.225 -0.016 -12.13
2518 0.147 0.001 -63.46
2543 0.154 0.000 -59.83
2562 0.224 -0.016 12.10
2630 0.203 0.003 -38.51
2835 0.209 -0.007 -20.82
2933 0.180 -0.004 -29.17
2939 0.181 -0.007 -28.83
2962 0.214 -0.014 -15.55
2983 0.235 0.004 -58.26
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The experimental data can be found in Refs. [32, 33] and references therein

In addition to the high-Ω proton orbitals mentioned above, other deformation-driving high-j high-Ω orbitals, including the high-Ω members of the proton π h9/2 shell and the high-Ω members of the neutron νh9/2, νi13/2, and νf7/2 shells, would appear close to the proton and neutron Fermi surfaces at both the oblate and prolate sides, respectively. The couplings of these high-Ω orbitals would form energetically low-lying high-K 3-qp configurations that are polarized into different shapes. We summarize the calculated deformations and excitation energies of possible high-K 3-qp configurations in Table 3. Coexisting different types of intrinsic shapes are obtained for a variety of high-K 3-qp configurations from the configuration-constrained PES calculations. Figure 2 depicts the typical PES’s corresponding to the 3-qp configurations with spherical, γ-soft prolate, oblate, and axially asymmetric shapes, respectively.

Fig. 2
(Color online) Calculated 187Tl potential energy surfaces (PES’s) of (a) the near-spherical g.s., (b) the prolate =27/2+, state, (c) the oblate = 29/2+, state, (d) the triaxial = 25/2+, state. The energy difference between the neighboring contours was 100 keV. The black dots denote the minima of PES’s
pic

Among them, the lowest prolate high-K 3-qp state given by the configuration-constrained PES is the =27/2+, configuration. The calculated PES for this configuration is shown in panel (b) of Fig. 2. As discussed in Sect. 3.1, this configuration is most likely to be assigned to the observed isomeric state with excitation energy Ex = 2584.6 keV and a lifetime T1/2 = 0.69 μs. Experimentally, it was found that the 2584.6-keV isomer decays to the = 25+ member of the rotational band, which is assigned to the low-Ω π1/2+[660] configuration [32, 33]. To understand this transition, we also compute the deformation and excitation energy of the low-Ω π1/2+[660] state (see Table 2). The calculated energy of the π1/2+[660] state was 1216 keV, which was compatible with the estimation of the bandhead energy of the observed rotational band. Note that both the π1/2+[660] and configurations have very soft axially asymmetric deformations of . The γ-soft shape breaks down the K-conservation and allows the decay from the =27/2+ state to the = 25+ state built on the π1/2+[660] configuration. The configuration-constrained PES calculations predict another =27/2+ configuration that consists of with a smaller β2≈0.18 and a larger . However, the large axially asymmetric deformation violates K-conservation, and hence may prohibit the formation of the K isomeric state.

Another interesting 3-qp state that we predict is the =29/2+, configuration. As shown in panel (c) of Fig. 2, its calculated PES shows a minimum that appears at an oblate deformation of β2≈0.19 and . The combination of the high K value, axially symmetric shape, and calculated low energy of Ex=1839 keV supports the existence of a long-lived K isomer. Therefore, we suggest that this =29/2+ configuration could be assigned to the observed isomeric state with a lifetime T1/2=1.1 μs, although the position and spin-parity of this isomer cannot be firmly determined because the γ rays linking this isomer to low-lying states are still missing [32, 33]. More recently, it was found that this isomer decays to the low-lying 13/2+ isomer at 1061 keV [33]. This implies that the T1/2=1.1 μs isomeric state may be oblate deformed and be composed of the same π13/2+[606] configuration, which is compatible with the predicted =29/2+, state. Thus, we propose that two long-lived 3-qp high-K isomeric states with different shapes coexist with intermediate excitation energies in 187Tl. Further measurements of observables, such as gyromagnetic ratios or electromagnetic transition properties of rotational bands built on these two long-lived states, would help us unambiguously determine the shapes and intrinsic structures of these observed isomers.

Other low-lying 3-qp high-K states are predicted by the configuration-constrained PES calculations. Among them, the = 25/2-, configuration is of particular interest because of its very low energy and high spin value. Because it is calculated to be even energetically lower than the observed lowest =13/2+ state, the calculated = 25/2- state can be expected to form a “spin trap” [1]. As Dracoulis et al. [72] have pointed out, a very low energy could result in long-lived states that would preferentially β decay and thus be missed. Therefore, it provides a challenge for both experimental and theoretical studies and, in effect, a test of the reliability of the models.

4

Summary

We present a systematic theoretical study of shape polarization and coexistence in high-K 3-qp states of odd-mass N=106 isotones (175Tm, 177Lu, 179Ta, 181Re, 183Ir, 185Au, 187Tl) using the configuration-constrained PES method.

The investigation focuses on 3-qp states formed by coupling a single proton to the systematic two-quasineutron =8- isomeric configuration known in the even-even N=106 cores. The calculations demonstrate excellent agreement with the experimental data for the well-established isomers in lighter isotones (Z=69-75), validating the theoretical approach. As the proton number increases towards the Z=82 shell closure, the ground states become progressively softer and less deformed, whereas the high-K 3-qp states exhibit significant shape polarization, maintaining well-defined prolate deformations. This leads to a substantial shape difference between the isomers and the ground states in nuclei such as 185Au and 187Tl.

Furthermore, we analyze in detail the intrinsic shapes of the 3-qp states in 187Tl. The configuration-constrained PES calculations identify a multitude of low-lying high-K configurations with distinctly different shapes (including prolate, oblate, and triaxial) coexisting within a narrow energy range. Two specific long-lived isomers observed in 187Tl are assigned to configurations with different shapes: the T1/2=0.69 μs isomer is associated with a prolate-deformed =27/2+ state, while the T1/2=1.1 μs isomer is proposed to be an oblate-deformed =29/2+ state characterized by a high K value, an axial shape, and a low excitation energy of 1839 keV, which favors a long lifetime. The study also predicts a very low-lying =25/2- 3-qp state in 187Tl, which could act as a “spin trap” and presents a challenge for future experimental detection.

In summary, this study presents a systematic description of high-K isomers in the N=106 isotonic chain. The calculated excitation energies and deformations are in reasonable agreement with the available experimental data, highlighting the crucial role of unpaired nucleons in driving shape polarization and revealing the possible coexistence of distinct shapes in neutron-deficient odd-mass nuclei near the Z=82 shell closure. We hope that the present results will provide useful guidance for future spectroscopic investigations in this mass region.

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Footnote

The authors declare that they have no competing interests.