Abstract
Three-quasiparticle K-isomeric states in odd-mass N=106 isotones within the A~180 mass region are systematically investigated using configuration-constrained potential energy surface calculations. The calculations successfully reproduce the excitation energies and deformations of known high-K isomers in the nuclei from 175Tm to 181Re. For the nuclei closer to the Z=82 shell closure (183Ir, 185Au, and 187Tl), predictions for the configurations of 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 Kπ=29/2+ configuration at E_x = 1839 keV is 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 research.
Full Text
Preamble
Shape polarization and coexistence of high- three-quasiparticle states in odd-mass = 106 isotones Runyan Dong and Changfeng Jiao 1, 2, 1 School of Physics and Astronomy, Sun Yat-sen University, Zhuhai 519082, China Guangdong Provincial Key Laboratory of Quantum Metrology and Sensing, Sun Yat-sen University, Zhuhai 519082, China Three-quasiparticle -isomeric states in odd-mass = 106 isotones within the mass region are systematically investigated using configuration-constrained potential energy surface calculations. The calcula- tions successfully reproduce the excitation energies and deformations of known high- isomers in the nuclei Tm to Re. For the nuclei closer to the shell closure ( Au, and Tl), predic- tions for the configurations of 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 where several high- three-quasiparticle configurations with distinct prolate, oblate, and triaxial shapes are found to coexist at similar excitation energies. Notably, the oblate-deformed configuration at = 1839 keV is proposed to be responsible for a long-lived isomer. This study provides a comprehensive picture of shape evolution and coexistence in high- multi-quasiparticle states, offering valuable insights for future experimental research.
Keywords
Shape polarization, shape coexistence, high- isomeric state, configuration-constrained potential energy surface.
INTRODUCTION
Neutron-deficient isotones around N = 106 mid-shell are 2
characterized by the existence of an abundance of low-lying,
high seniority isomeric states. In this region, the orbitals with 4
large , namely the projection of individual angular momen- tum onto the intrinsic symmetric axis, approach the neutron Fermi surface at moderate quadrupole deformations. It facil- itates the formation of broken-pair states with high values
(where K = �
) near the yrast line. According to the se- lection rules for electromagnetic transitions, the transitions of
multipolarity λ would be significantly hindered if ∆ K > λ . 11
The so-called -hindrance can lead to relatively long half- lives (on the order of nanoseconds or longer) [ ], leading to the formation of “ isomers”. One of the most well-known examples of high- isomers is found in , in which two
2-quasiparticle (qp) K π = 8 − isomers and a long-lived four- 16
quasiparticle K π = 16 + isomer with a half-life of 31 years 17
are observed [ ]. Since the occurrence of isomers is a combined effect of the unpaired nucleons occupied high- states and the nuclear deformation, the study of isomeric states is therefore pivotal for understanding the interplay be- tween the shell structure of “individual” nucleons and the col- lective behavior of a strongly correlated nucleus [ Another common feature associated with the mass region is the shape transition. In this region, the ground- state (g.s.) shape can change from a well-deformed prolate ellipsoid with Yb to a very soft spheroid ]. Moreover, the soft shape gives rise to the novel shape coexistence phenomenon, which is characterized by the emergence of low-lying states with different intrin- sic shapes in one atomic nucleus. In general, it originates Supported by the National Natural Science Foundation of China (No.12275369)
from the combining effect of approaching the Z = 82 spher- 32
ical shell closures and the deformed shell gaps around the
neutron mid-shell at N = 104 − 106 due to quadrupole- 34
quadrupole correlations. It has drawn considerable interest The most well-known example is the differently shaped triplet observed in Pb, which corresponds to the coexistence of the prolate, oblate, and spherical configu- rations [ ]. Coexisting states in even-even Pt, Hg, Pb, and Po isotopes around the neutron midshell have been extensively studied [ In addition to the shape change resulting from collective correlations such as quadrupole-quadrupole interactions, un- paired nucleons are found to strongly polarize the nuclear shape [ ]. Since isomeric states are coupled by high- unpaired nucleons, shape polarization possibly yields con- siderable differences in shape between high- states and ground states, leading to novel structures that involve both isomerism and shape isomerism. For example, the two-
quasineutron K π = 8 − ( ν { 7 / 2 − [514] ⊗ 9 / 2 + [624] } ) iso- 50
meric states which are systematically observed in the even-
even N =106 isotones between 174 Er and 188 Pb (see [ 24 , 25 ] 52
and references therein). Previous theoretical investigation has shown that the the g.s. are oblate deformed with
for 186 Hg and spherical for 188 Pb, whereas the K = 8 − iso- 55
meric states are polarized to prolate deformed with
0 . 25 . The K = 8 − isomers with shapes different from those 57
of the g.s. have later been confirmed by measuring rotational bands built on them [ ]. Furthermore, it is 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 proper- ties [ While the shape evolution and coexistence of high- states in even-even nuclei around neutron mid-shell and have been extensively studied, the structural properties such as the shape changing effects of 3-qp high- states in their odd-proton neighbors are lacking systematic investigations.
In odd- nuclei, although the unpaired nucleon introduces additional complexity, it also 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 op- posed to that of the high- 2-qp configuration, thereby am-
plifying or diminishing the shape difference between the 3- 74
qp states and the g.s.. Recently, the 3-qp high- isomers, originated from the coupling between the odd proton and the
aforementioned K π = 8 − configuration in even-mass cores, 77
have been observed in odd-mass N = 106 isotones from 78
175 Tm to
Tl (except the Ir) [ 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 [ ]. The ex- tent to which the observed 3-qp isomers can be considered to involve shape isomerism, in addition to isomerism, re- mains unclear. It thus has greatly stimulated our interest in pursuing theoretical studies on shape polarization and coex- istence in the 3-qp high- states within this mass region.
In this work, we investigate the 3-qp -isomeric states
of odd- A nuclei in the N = 106 isotonic chain using 89
the configuration-constrained potential energy surface (PES) method [ This method includes the axially asymmetric -degree of freedom. Furthermore, in this method, we do not introduce an adjustable parameter of the pairing strength,
and the deformation is determined self-consistently by mini- 94
mizing the corresponding PES. At prolate deformations, we mainly focus on the study of the high- 3-qp configurations composed of the coupling of the unpaired proton and the
K π = 8 − 2-qp configuration that are observed systematically 98
in even-even N = 106 nuclei. We predicted the possible con- 99
figurations of the isomers in Au and Tl, with particular attention to the shape-polarization effect from multi-qp exci- tations. Furthermore, we explored the high- states with dis- tinct shapes (oblate, prolate, and triaxial) that coexist at com- parable excitation energies in Tl, and analyzed the impact of different quasiparticle configurations on shape evolution in detail.
THE MODEL employ configuration-constrained proach [ ], based on the macroscopic–microscopic model.
The macroscopic energy contribution was computed using the standard liquid-drop model [ ] with parameters taken from Ref. [ The microscopic correction includes the Strutinsky shell correction [ ] and the pairing correction.
The single-particle levels required for the microscopic energy calculations were obtained from a non-axial deformed
Woods-Saxon potential [ 41 ] using the “universal” parameter 116
set [ 42 ]. The so-called universal parameter set (listed 117
in Table ) was optimized by simultaneously fitting the single-particle energies in Pb, particularly those corrected for nucleon-nucleus interactions beyond the independent particle model, as well as the high-spin yrast spectra of
212 Rn and
]. These parameters have been further tested for light nuclei [ ], and for heavier nuclei with ], showing satisfactory performance in describing not only the single (quasi)particle level sequences but also the nuclear equilibrium deformations.
Since these parameters were optimized for the lead region, they have been validated as the best-fit Woods-Saxon potential parameters for this mass region.
To avoid the collapse of pairing correlations in multi- quasiparticle states, we used the Lipkin-Nogami (LN) ver- an approximate particle-number projection scheme, incorpo-
rating monopole pairing. The pairing strength G was initially 134
determined via the average-gap method [ ]. Although it is often further adjusted to reproduce the odd-even mass difference using a five-point formula, we note that irregu- larities may arise near magic numbers (e.g., Au and Tl iso- approach and the artefacts from the LN correction. It is also because the odd-even mass difference equations used to ex- tract experimental pairing gaps are derived under the assump- tion that there are no non-smooth contributions to the masses apart from pairing effects, while this assumption is often not fulfilled at magic numbers [ Therefore, following the rec- ommendation of Ref. [ ], closed-shell nuclei were excluded from the pairing strength calibration. For consistency, we adopted the standard pairing strength across all isotopes un- In the PES calculations, a deformation mesh in used, with the hexadecapole deformation variation at each mesh point. For broken-pair configurations, the microscopic energy incorporates contributions from unpaired nucleons oc- cupying specific single-particle orbitals (see Ref. [ ] for de- tails).
These orbitals are continuously tracked and adiabati- cally blocked throughout the deformation plane. For axially deformed nuclei, single-particle orbitals can be spec- ified by their individual spin projection . For axially asym- metric shapes, however, is no longer conserved. In ad- dition, several single-particle orbits with approximately the same spin projection may become energetically close at given deformations. To reliably track orbits, we com- puted and compared not only the average spin projection but also the expectation values of the Nilsson numbers , and between two adjacent deformation mesh points.
We have verified that, although the Nilsson numbers , and are not strictly conserved, their expectation val- ues exhibit slow variation, allowing for a reliable configura- tion assignment.
Therefore, each configuration is 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 the configuration energy, where the latter origi-
nates 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 177
an equilibrium deformation for 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 descrip- tion of both the deformation and excitation energy of multi- qp states [ ]. The excitation energy is computed as the
energy difference between the PES minimum of the excited 184
configuration and that of the ground-state configuration, en- abling direct comparison with experimental values.
CALCULATIONS AND DISCUSSIONS Systematics of 3-qp states involved [624] [514] For nuclei in the region, an abundance of high- isomeric states has been discovered [ ]. Among them, the
two-quasineutron K π = 8 − ( ν { 7 / 2 − [514] ⊗ 9 / 2 + [624] } ) 192
isomeric states exist systematically in even-even N = 106 193
isotones, which have been investigated by means of the configuration-constrained PES calculation in Ref. [ ]. The calculated excitation energies agree well with the experi- mental data, and strong shape polarizations have been found
when approaching the Z = 82 shell closure. For odd-mass 198
N = 106 isotones in this mass region, most of the observed 199
isomers consistently involve a two-quasineutron con-
figuration coupled to K π = 8 − states that are identified in 201
the aforementioned even-even nuclei. For example, in nuclei such as ], 3-qp isomers have been assigned as
the two-quasineutron K π = 8 − configuration coupled to the 205
energetically lowest one-quasiproton configuration. Further-
more, in 181 Re, 179 Ta, and 177 Lu, the meta-stable K π = 207
states are found, assigned to the [514] config- uration, leading to the presence of 3-qp states associated with
the coupling of a K π = 8 − two-quasineutron configuration 210
[514] ]. In Tm, a isomer which may
involve coupling of the two-quasineutron K π = 8 − config- 212
uration with the [523] has been found [ ]. The half- lives of these isomers range from a few microseconds to sev- eral days. To what extent these high- states are associated with shape polarization and shape isomerism is still an open question.
We have performed the configuration-constrained PES cal-
culations on the 1-quasiproton and 3-qp states in N = 106 219
odd-mass isotones. Table presents the calculated defor- mations and energies of the g.s., the possible high- quasiproton and low-lying high- 3-qp states, compared with the available experimental data. Our calculations repro- duce the experimentally assigned spin-parity of the g.s. of these nuclei, except for Lu, in which the calculated low- est 1-quasiproton configuration is the [514] rather than the experimentally assigned [404] ]. However, the calculated [404] configuration lies only 259 keV above [514] state. Given the strong dependence of 1-qp state energies on the ordering and spacing of single-particle levels, the deviation in their relative positions falls within an acceptable range.
One may ask the sensitivity of these calculated results to the pairing strengths or the Woods–Saxon parameters. Note that previous work has shown that adjustment of pairing strength mainly influences the quasiparticle energy gaps and only slightly affects the deformations [ ], while the ordering of single-particle levels at a certain deformation is primarily determined by the choice of the Woods–Saxon potential pa- rameters. To examine the robustness of this result, we there- fore have tested with several known parameter sets, includ- ing those of Blomquist and Wahlborn [ ], the parameters of Chepurnov [ ], the parameters given by Rost [ ], and the “new” parameters [ ]. We found that the deviation in the relative positions of the [514] [404] config- urations of Lu is preserved with different parameter sets.
To accurately reproduce the ordering of the low-lying 1-qp states of Lu, an improvement of the Woods-Saxon poten- tial is needed.
Experimentally, the spin and parity of the g.s. of ] have been assigned to be the states built on the [541] configuration, while a strong mix- ing between the [541] [532] configurations attributed to the Coriolis interactions has been proposed for g.s. of ]. Our calculations show that [541] configuration has the lowest energy, while [532] state is about 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, configuration mixing calculations are beyond the scope of the present work.
The present configuration-constrained PES calculations also reasonably reproduce the high- 1-qp isomeric states ob-
served in odd-mass N = 106 isotones except for the afore- 265
mentioned deviation in Lu. Notably, the configuration-
constrained PES calculations show that the K π = 9 / 2 − iso- 267
mer of 185 Au and the K π = 11 / 2 − state of 187 Tl have mod- 268
erate triaxial deformations with which are remark- ably polarized when compared with their g.s.. It indicates the appearance of single-proton-induced shape polarization in
shape-soft odd-proton nuclei when approaching the Z = 82 272
closed shell. Now we turn to the investigation of energetically low-
lying 3-qp states in odd-mass N = 106 isotones. We 275
mainly focus on the 3-qp states that consist of the two- quasineutron [514] [624] configuration cou- pled to different 1-quasiproton configurations, since the
K π = 8 − isomeric states are systematically identified as 279
[514] [624] configuration in even-even
N = 106 isotones. As seen in Table 2 [TABLE:2] , the calculated en- 281
ergies of these 3-qp states in Ta, and Re agree well with the experimental data. For Lu, the calculated
K π = 23 / 2 − π 7 / 2 + [404] ⊗ ν { 9 / 2 + [624] ⊗ 7 / 2 − [514] } 284
configuration is overpredicted, while the K π = 25 / 2 + 285
and excitation energies for odd- nuclei in the = 106 isotopic chain. The experimental energies can be found in Refs. [ ] and references therein.
183 Ir
[541] [514] [541] [624] [514] [514] [624] [514]
185 Au
[541] [411] [532] [505] [541] [624] [514] [532] [624] [514]
187 Tl
[400] [514] [624] [514] state is slightly underestimated. This can be attributed to the deviation of the [404] [514] orbitals that we found in the cal- culations of the 1-quasiproton states.
Furthermore, the configuration-constrained PES calcula- tions predict the candidate configurations of the 3-qp isomeric
states in the odd- A N = 106 isotones when moving towards 292
the Z = 82 shell closure. To date, no experimental evidence 293
has been reported on three-quasiparticle high- isomers in 183 Ir. We proposed two possible high- 3-qp states that are [505] [505] [624] [514]
β 2 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 K π = 8 −
configuration [514] [624] with the g.s. configurations of odd- nuclei, which are [411] [404] [404] [402] [541] , and [541] , respectively. For , the 3-qp state is [505] [624] [514] These 3-qp states correspond to observed high- isomers. [514] , respectively. For Au, a new isomer at an exci- tation energy of 1504.2(4) keV with a half-life of 630(80) ns possible spins of this isomer are constrained to a range from 13/2 to 21/2 in comparison with predictions from the Weis- skopf estimates [ ]. Our calculations suggest two possible 3- qp high- configurations that are consistent with systematics
of 3-qp configurations in lighter odd-mass N = 106 isotones. 305
They both lie at excitation energies of about 1900 keV, which is a bit overpredicted. However, Ref. [ ] argued that the g.s. configuration of Au is more likely [532] , and the calculated energy differences of these two 3-qp states with re- spect to the [532] configuration are 1444 and 1458 keV, respectively, which is in great agreement with the observa- tion. For nucleus Tl, two isomers with microsecond life-
times ( T 1 / 2 = 1 . 11 µ s and 0.69 µ s) have been reported [ 32 ]. 313
Spin-parities J π = 27 / 2 + , 31 / 2 − are tentatively assigned 314
to the isomer lies at 2584 keV with lifetime T 1 / 2 = 0 . 69 315
s based on the deduced total conversion coefficient [
Our calculation presents a K π = 27 / 2 + , π 11 / 2 − [505] ⊗ 317
[624] [514] configuration with an excitation energy of 2312 keV, which is in accord with the prolate high- configuration suggested in Ref. [ ]. This implies that
the T 1 / 2 = 0 . 69 µ s isomer observed in 187 Tl involves the 321
two-quasineutron [624] [514] configuration, which is consistent with the systematics of 3-qp isomers ob-
served in lighter odd-mass N = 106 isotones. However, fur- 324
ther experimental data are required to unambiguously assign the spin-parity and configuration of these observed isomers.
We would discuss the other T 1 / 2 = 1 . 1 µ s isomer later in 327
Sect. III B In addition, intrinsic shape evolution is crucial for un- derstanding the observed behavior of isomeric states, such as their decay properties. In the previous study [ ], strong shape polarization has been shown in even-even nuclei with
A ∼ 180 and N = 106 , especially in nuclei close to the 333
Z = 82 shell closure. For systematic comparison, we plot 334
the variation of deformations of the high- qp states and the g.s. along with the proton number
When approaching the shell closure of Z = 82 , 337
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. g.s. of Au, for example, has a remarkably -soft shape
with a very shallow PES minimum at γ ≈ 24 ◦ . Consid- 342
ering that the g.s. of Au can be interpreted as the cou- pling of a low- proton with the Pt core, the PES of the g.s. of Au exhibits similar softness com- pared to Pt. This -soft nature of Pt is mainly because the prolate-to-oblate shape transition going through a transi-
tional γ -soft shape occurs in Pt isotopes around N = 110 , 348
which has been suggested by the self-consistent HFB calcu- lation using Gogny-D1S interaction and the interacting bo- son model [ ], as well as the five-dimensional collective
Hamiltonian (5DCH) based on covariant density-functional 352
theory [ In contrast, the predicted two 3-qp high- states of Au both have an approximately prolate shape and about a increase in deforma- tion.
The nucleus Tl has a spherical g.s. with a proton that singly occupies the orbital, while the calculated
K π = 27 / 2 + π 11 / 2 − [505] ⊗ ν { 9 / 2 + [624] ⊗ 7 / 2 − [514] } 358
state is predicted to have a moderately axially-asymmetric shape with , exhibiting the great- est difference in quadrupole deformation between the 3-qp state and the g.s.. In fact, the calculated high- 3-qp con- figurations of Tl present an ensemble of multiple nuclear shapes, which would be analyzed in detail in Sect.
III B Shape coexistence in high- 3-qp states of 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 N ≈ 106 . Moreover, 369
the unpaired nucleon that occupies different single-particle orbitals would polarize the shape of the odd- nucleus in dif- ferent ways, leading to more profound shape coexistence phe- nomenon. An abundance of experimental data has demon-
strated that differently-shaped configurations in these odd- nuclei are observed not only in the low-lying 1-qp states but
also in the higher-seniority isomeric states [ 9 ]. 376
Tl, previous studies [ ] have proposed the co- existence of different nuclear shapes by the analysis of ob- served low-lying collective structures.
As the proton-hole
neighbor of 188 Pb, the I = 1 / 2 + g.s. of 187 Tl can be in- 380
terpreted as the coupling of the hole with the spher-
ical 0 + 1 state of 188 Pb core. The observed K π = 9 / 2 − and 382
K π = 13 / 2 + isomeric states can be understood as filling 383
[505] [606] intruder orbitals that are lowered along with the increase in oblate deformation, re- spectively [ ], while the rotational band built on the
I π = 11 / 2 − state is suggested to be the prolate deformed 387
[505] configuration [ ]. The calculated defor- mations and excitation energies for these 1-quasiproton states are listed in Table . The configuration-constrained PES cal- culations well reproduce the measured excitation energies, and clearly show the coexisting shapes for these 1-qp states.
Note that the [505] configuration has been predicted to have a considerable axial-asymmetric shape of which breaks down the - and shape-hindrance and would
explain why it decays fast to the oblate K π = 9 / 2 − isomeric 396
state [ In addition to the high- proton orbitals mentioned above, other deformation-driving high- high- orbitals, including the high- members of the proton shell, the high- members of neutron , and shells, would appear close to the proton and neutron Fermi surfaces at both oblate and prolate sides, respectively. The couplings of these high- orbitals would form energetically low-lying high- 3-qp configurations that are polarized to different shapes. We summarize the calculated deformations and excitation ener- gies of possible high- 3-qp configurations in Table . Co- existing different types of intrinsic shape are obtained for a variety of high- 3-qp configurations from the configuration- constrained PES calculations. Fig. depicts the typical PES’s corresponding to the 3-qp configurations with spherical, soft prolate, oblate, and axially asymmetric shapes, respec- tively.
Among them, the lowest prolate high- 3-qp state given
by the configuration-constrained PES is the K π = 27 / 2 + , 415
[505] [624] [514] configuration. The calculated PES of this configuration is shown in the panel (b) of the Fig. . As we discussed in Sect.
III A , this con- figuration is most likely to be assigned to the observed iso-
meric state with excitation energy E x = 2584 . 6 keV and life- 420
time T 1 / 2 = 0 . 69 µ s. Experimentally, it is found that the 421
2584.6-keV isomer decays to the I π = 25 + member of the 422
rotational band, which is assigned to the low- [660] configuration [ ]. To understand this transition, we also compute the deformation and excitation energy of the low- [660] state (see them in Table ). The calculated energy of the [660] state is 1216 keV, which is com- patible with the estimation of the bandhead energy of the ob- served rotational band. Note that both the [660] [505] [624] [514] configurations have very soft axially asymmetric deformations of -soft shape breaks down the -conservation and allows
the decay from the K π = 27 / 2 + state to the I π = 25 + state 433
built on the 2 + [660] configuration. The CCPES calcu-
lations predict another K π = 27 / 2 + configuration that con- 435
sists of [505] [505] [633] with a smaller and a larger . However, the large axially asymmetric deformation violates the -conservation, and hence may prohibit the formation of the isomeric state. potential energy surfaces (PES’s) of (a) the near-spherical g.s., (b) the prolate [505] [624] [514] state, (c) the oblate [606] [624] [633] state, (d) the triaxial [505] [633] [503] state.
The energy difference between neighboring contours is 100 keV. The black dots denote the minima of PES’s.
Another interesting 3-qp state that we predict is the K π = 440
[606] [624] [633] config- uration. As seen in the panel (c) of Fig. , its calculated PES
shows a minimum that appears at oblate deformation of β 2 ≈ 443
. The combination of high value, axially
symmetric shape, and its calculated low energy of E x = 1839 445
keV, supports the existence of a long-lived isomer. There-
fore, we suggest that this K π = 29 / 2 + configuration could 447
be assigned to the observed isomeric state with a lifetime
T 1 / 2 = 1 . 1 µ s, although the position and spin-parity of this 449
isomer cannot be firmly determined because the rays link- ing this isomer to low-lying states are still missing [ More recently, it has been found that this isomer decays to the low-lying isomer that lies at 1061 keV [ ]. This
implies that the T 1 / 2 = 1 . 1 µ s isomeric state may be oblate 454
deformed and be composed of the same [606] config-
uration, which is compatible with the predicted K π = 29 / 2 + , 456
[606] [624] [633] state. We thus propose that two long-lived 3-qp high- isomeric states with
and excitation energies for the g.s., the low-lying high- 1-qp, and high- 3-qp states of Tl. The experimental data can be found in Refs. [ ] and references therein. different shapes coexist with intermediate excitation energies Tl. Further measurement of observables, such as gy- romagnetic ratios or electromagnetic transition properties of rotational bands built on these two long-lived states, would help us to unambiguously pin down the shapes and intrinsic structures of these observed isomers.
Other low-lying 3-qp high- states are predicted by the configuration-constrained PES calculations.
Among them, [505] [624] [633] configuration is of particular interest because of its very low energy and high spin value. Since it is calculated to be even
energetically lower than the observed lowest I π = 13 / 2 + 470
state, the calculated state can be expected to form a “spin trap” [ ]. As Dracoulis et al ] have pointed out, a very low energy could result in long-lived states that would preferentially decay and thus be missed. It there- fore provides a challenge for both experimental and theoreti- cal studies and, in effect, a test of the reliability of the models.
SUMMARY
We present a systematic theoretical study of shape polar- ization and coexistence in high- 3-qp states of odd-mass
N = 106 isotones ( 175 Tm, 177 Lu, 179 Ta, 181 Re, 183 Ir, 185 Au, 480
187 Tl) using the configuration-constrained PES method.
The investigation focuses on 3-qp states formed by cou- pling a single proton to the systematic two-quasineutron
K π = 8 − isomeric configuration known in the even-even 484
N = 106 cores. The calculations demonstrate excellent 485
agreement with the experimental data for the well-established
isomers in lighter isotones ( Z = 69 − 75 ), validating the theo- 487
retical approach. As the proton number increases towards the
Z = 82 shell closure, the ground states become progressively 489
softer and less deformed, while the high- 3-qp states ex-
hibit significant shape polarization, maintaining well-defined 491
prolate deformations. This leads to a substantial shape differ- ence between the isomers and the ground states in nuclei like
185 Au and
Furthermore, we analyze in detail the intrinsic shapes of 3-qp states in Tl. The configuration-constrained PES cal- culations identify a multitude of low-lying high- config- urations with distinctly different shapes (including prolate oblate , and triaxial ) coexisting within a narrow energy range.
Two specific long-lived isomers observed in Tl are as-
signed to configurations with different shapes: the T 1 / 2 = 501
0 . 69 µ s isomer is associated with a prolate-deformed K π = 502
27 / 2 + state, while the T 1 / 2 = 1 . 1 µ s isomer is proposed to 503
be an oblate-deformed K π = 29 / 2 + state characterized by 504
a high 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 K π = 25 / 2 − 3-qp state in 187 Tl, 507
which could act as a “spin trap” and presents a challenge for future experimental detection.
In summay, this work presents a systematic description of
high- K isomers in the N = 106 isotonic chain. The calcu- 511
lated excitation energies and deformations are in reasonable agreement with available experimental data, highlighting the crucial role of unpaired nucleons in driving shape polariza- tion and revealing the possible coexistence of distinct shapes P. Walker and G. Dracoulis, Energy traps in atomic nuclei, Na- , 35 (1999).
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