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symmetry S S Review Review of Shape Phase Transition Studies for Bose-Fermi Systems: The Effect of the Odd-Particle on the Bosonic Core M. Böyükata 1,* , C. E. Alonso 2,3 , J. M. Arias 2,3 , L. Fortunato 4,5 and A. Vitturi 4,5 Citation: Böyükata, M.; Alonso, C.E.; Arias, J.M.; Fortunato, L.; Vitturi, A. Review of Shape Phase Transition Studies for Bose-Fermi Systems: The Effect of the Odd-Particle on the Bosonic Core. Symmetry 2021,13, 215. https://doi.org/10.3390/ sym13020215 Academic Editor: Francesco Pederiva Received: 23 December 2020 Accepted: 22 January 2021 Published: 28 January 2021 Publisher’s Note: MDPI stays neutral with regard to jurisdictional claims in published maps and institutional affiliations. Copyright: © 2021 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (https:// creativecommons.org/licenses/by/ 4.0/). 1Physics Department, Faculty of Science and Arts, University of Kırıkkale, 71450 Kırıkkale, Turkey 2Departamento de Física Atómica, Molecular y Nuclear, Facultad de Física, Universidad de Sevilla, Apartado 1065, 41080 Sevilla, Spain; [email protected] (C.E.A.); [email protected] (J.M.A.) 3Instituto Carlos I de Física Teórica y Computacional, Universidad de Granada, Fuentenueva s/n, 18071 Granada, Spain 4Dipartimento di Fisica e Astronomia “G. Galilei”, Università di Padova, I-35131 Padova, Italy; [email protected] (L.F.); [email protected] (A.V.) 5INFN-Sezione di Padova, Via Marzolo 8, 35131 Padova, Italy *Correspondence: [email protected] Abstract: The quantum phase transition studies we have done during the last few years for odd-even systems are reviewed. The focus is on the quantum shape phase transition in Bose-Fermi systems. They are studied within the Interacting Boson-Fermion Model (IBFM). The geometry is included in this model by using the intrinsic frame formalism based on the concept of coherent states. First, the critical point symmetries E(5/4) and E(5/12) are summarized. E(5/4) describes the case of a single j= 3 / 2 particle coupled to a bosonic core that undergoes a transition from spherical to γ -unstable. E(5/12) is an extension of E(5/4) that describes the multij case ( j= 1 / 2,3 / 2,5 / 2) along the same transitional path. Both, E(5/4) and E(5/12), are formulated in a geometrical context using the Bohr Hamiltonian. Similar situations can be studied within the IBFM considering the transitional path from U BF (5) to O BF (6). Such studies are also presented. No critical points have been proposed for other paths in odd-even systems as, for instance, the transition from spherical to axially deformed shapes. However, the study of such shape phase transition can be done easily within the IBFM considering the path from U BF (5) (spherical) to SU BF (3) (axial deformed). Thus, in a second part, this study is presented for the multij case. Energy levels and potential energy surfaces obtained within the intrinsic frame formalism of the IBFM Hamiltonian are discussed. Finally, our recent works within the IBFM for a singlej fermion coupled to a bosonic core that performs different shape phase transitional paths are reviewed. All significant paths in the model space are studied: from spherical to γ -unstable shape, from spherical to axially deformed (prolate and oblate) shapes, and from prolate to oblate shape passing through the γ -unstable shape. The aim of these applications is to understand the effect of the coupled fermion on the core when moving along a given transitional path and how the coupled fermion modifies the bosonic core around the critical points. Keywords: nuclear structure models and methods; collective models; models based on group theory PACS: 21.60.-n; 21.60.Ev; 21.60.Fw 1. Introduction An interesting aspect of modern nuclear physics is the study of the quantum shape phase transition in atomic nuclei. Phase transitions are usually discussed and well defined for macroscopic systems. However, in the last few years, precursors of phase transitions have been observed in mesoscopic systems and then one talks about quantum phase transitions. Classical phase transitions are usually classified into two classes, called firstorder and continuous phase transitions depending on the behavior of the order parameter at the critical point. At this point, the order parameter changes typically from zero to a Symmetry 2021,13, 215. https://doi.org/10.3390/sym13020215 https://www.mdpi.com/journal/symmetry
Symmetry 2021,13, 215 2 of 26 finite value. When this variation is discontinuous at the critical point it is said that the transition is first order. On the contrary, when the variation of the order parameter is smooth at the critical point, the transition is said to be continuous. The same ideas can be translated to quantum phase transitions. It is clear that the concept of critical point is intimately linked to the subject of phase transitions. In this context, about twenty years ago, Iachello introduced the concept of the critical point symmetry [ 1 ] in relation to quantum systems as atomic nuclei. Iachello worked out two critical point symmetries within the geometrical model using the Bohr Hamiltonian [ 2 ]. One of them, called E(5), describes the critical point in the shape transition from spherical to deformed γ -unstable shapes [ 1 ] and is appropriate for continuous shape phase transitions. The other symmetry proposed by Iachello, called X(5), describes the critical point in the transition from spherical to axially deformed shapes [3] and is a benchmark for first order phase transitions. Although the Interacting Boson Model (IBM) [ 4 ] is formulated from the beginning in a second quantization formalism, one can obtain a geometric image of the model using the idea of coherent state and intrinsic state formalism. In this way, one finds geometrical shapes, as in the Bohr model, linked to the different dynamical symmetries of the model. Thus, the U(5) limit corresponds to spherical shapes, the SU(3) ( SU(3) ) limit produces prolate (oblate) axially symmetric shapes, and the O(6) limit generates deformed γ -unstable shapes. Therefore, one can look for the equivalent to E(5) or X(5) symmetries in the IBM. In this case, the critical points are called e( 5 ) and x( 5 ) and correspond to the transitional paths from U(5) to O(6) and from U(5) to SU(3), respectively. Many experimental and theoretical studies have been performed for quantum phase transitions especially for even-even nuclei within the IBM [4], as reported in different review papers [5–9]. Relatively less attention has been devoted to the parallel topic of quantum phase transitions in Bose-Fermi systems. In addition to the above mentioned critical point symmetries for even-even systems, Iachello, also within the Bohr Hamiltonian, proposed to extend the concept of critical point symmetry to Bose-Fermi systems for using it in odd-even nuclei. Iachello worked out the case of an odd j= 3 / 2 particle coupled to a bosonic core that undergoes a transition from spherical to γ -unstable shapes [ 10 ]. Soon after, an extension to multij case, called E(5/12), including j= 1 / 2,3 / 2, and 5 / 2 also within the Bohr Hamiltonian was proposed [ 11 ]. No other critical point symmetries have been proposed for odd-even systems. As in the case of even-even nuclei, the Interacting Boson-Fermion Model (IBFM) [ 12 ] can be used to study similar transitional situations as those described in the Bohr model and through any of the relevant transitional paths. Special relevance have the paths from spherical to deformed γ -unstable and from spherical to axially deformed shapes [ 11 , 13 , 14 ]. Although the E(5/4) and E(5/12), in the geometric model, and the corresponding critical point in the IBFM (spherical to deformed γ -unstable) are different, the results obtained within the IBFM and those from E(5/12) show a remarkable agreement for the energy levels spectrum and electromagnetic transitions. The transition from spherical to axially deformed shape in Bose-Fermi systems has also been considered in the framework of the IBFM, where the odd fermion occupies the set of j= 1 / 2,3 / 2,5 / 2 orbitals [ 15 ]. The energy levels and the electromagnetic transitions of the odd-even system have been calculated within the IBFM Hamiltonian and also the intrinsic frame formalism was employed to describe this quantum phase transition. During the last decade, we have developed a systematic investigation of the quantum shape phase transition in Bose-Fermi systems for the case of a singlej fermion coupled to a bosonic core [ 16 – 20 ], making use of the intrinsic frame formalism to associate a given shape to the solution of a IBFM Hamiltonian. Transitions from spherical to γ –unstable shape [ 16 ], from spherical to prolate shape [ 18 ], from spherical to oblate shape [ 19 ] have been studied up to now, with the aim of understanding the effect of the coupled fermion on the core when moving to the transition paths and around the critical points. More recently, we have closed the circle, by investigating the phase transition from prolate to oblate shape passing through the γ -unstable shape in odd-even systems [ 20 ]. The different paths are marked in Figure 1.
Symmetry 2021,13, 215 3 of 26 U(5) SU(3) SU(3) χ χ=− − χ=0 χ=+ − x=1, 7 2 7 2 O(6) path 1 path 2 path 3 path 4 x=0 x x=1, x=1, Figure 1. Schematic representation of the Interacting Boson Model (IBM) model space with two control parameters: one radial (x) and one angular (χ) (see boson hamiltonian (1)). We would like to mention that other relevant contributions to the topic of shape phase transitions in odd-even nuclei have been presented in the last 15 years in Refs. [10,21–36]. In this review paper, we present a summary of the most important results we have obtained within the IBFM for shape phase transitions in odd-even nuclei, namely the critical point symmetries for the specific E(5/4) [ 13 ] and E(5/12) [ 11 , 14 ] cases; the U BF (5)-SU BF (3) transition in odd nuclei for multij orbits, j= 1 / 2,3 / 2,5 / 2 [ 15 ]; the results of our recent works related to the case of a singlej fermion coupled to the bosonic core that performs different transitions mentioned in previous paragraph [ 16 , 18 – 20 ]. The paper is organized as follows. The IBFM model with its Hamiltonian and the intrinsic frame formalism for Bose-Fermi systems are revised in Section 2. In Section 3, the E(5/4) and E(5/12) critical point symmetries and some results for equivalent situations in IBFM are discussed. In Section 4, the IBFM U BF (5) to SU BF (3) phase transition in odd nuclei for multij orbits is briefly outlined and results are presented for energy levels and energy surfaces. The results of the phase transitions in Bose-Fermi systems investigated within the intrinsic frame formalism of the IBFM for the case of a singlej fermion coupled to a bosonic core are reviewed in Section 5. General conclusions are drawn in the final section. 2. Methods: The IBFM Hamiltonian and the Intrinsic Frame Formalism The IBM model [ 4 ] is designed to describe collective properties of medium and heavy mass even-even nuclei. The model has three basic approximations: (i) only valence particles are taken into account, (ii) these fermions are coupled to angular momentum L= 0 and L= 2, and (iii) those coupled fermions are treated as bosons ( s− bosons with L= 0 and d− bosons with L= 2). With these approximations, many studies have been done for even-even nuclei. The boson hamiltonian in terms of s−and d−bosons can be written as, HB= (1−x)ˆ nd−x αNB ˆ Q(χ) B·ˆ Q(χ) B, (1) where NBis the number of bosons, αis a parameter, ˆ ndis the d−boson number operator, ˆ nd=∑ µ d† µdµ, (2)
Symmetry 2021,13, 215 4 of 26 and ˆ Q(χ) Bis the boson quadrupole operator given by ˆ Q(χ) B= (s†×˜ d+d†×˜ s)(2)+χ(d†×˜ d)(2). (3) The control parameters of the model are x , and χ . In Figure 1, the IBM model space is schematically plotted. There are four dynamical symmetries in the model: U(5), SU(3), SU(3) , and O(6). Shapes can be obtained in the model by using the intrinsic state formalism based on a coherent state (Refs. [37–39]) |Φgs(β,γ)i=1 √NB![b† gs(β,γ)]NB|0i, (4) where NB is the number of bosons for a particular nucleus, | 0 i is the boson vacuum, and b† gs(β,γ)is the ground state boson condensate creation operator given by b† gs(β,γ) = 1 p1+β2s†+βcos γd† 0+β √2sin γ(d† 2+d† −2). (5) β and γ are shape variables that are related to the quadrupole deformation parameters of the geometric collective model of Bohr-Mottelson [ 2 ]. The ground state energy surface is established by calculating the expectation value of the given bosonic HB Hamiltonian (1) in the intrinsic state (4) Egs(β,γ) = hΦgs(β,γ)|HB|Φgs(β,γ)i. (6) Mathematically, β and γ are variational parameters in the intrinsic formalism of IBM model in the classical limit [ 37 – 39 ] that can be determined by minimizing the energy surface (6). This connection has been done and the correspondence with the IBM dynamical symmetries is: U(5) corresponds to x= 0 and then β= 0, spherical shape, SU(3) ( SU(3) ) corresponds to x= 1 and χ=−√7/ 2 ( χ= +√7/ 2) and produces β=√2 and γ= 0 ( γ= 60 ◦ ), axially deformed prolate (oblate) shape, and, finally, O(6) corresponds to x= 1 and χ=0, and gives a deformed γ-unstable shape. See Figure 1. The IBFM model [ 12 ] is the extension of the IBM model [ 4 ] for the description of the properties of a system of NB bosons plus one fermion, the typical application being represented by an odd-even nuclei. The general model Hamiltonian for the coupling of an single fermion to the bosonic core is written as follows: H=HB+HF+VBF, (7) where HBis the pure bosonic Hamiltonian Equation (1), HFis the fermion Hamiltonian HF=∑ j εja† j·˜ aj, (8) where εj are the single-particle energies for the orbits j allowed for the fermion, and the third term in (7), V BF , couples the bosonic and fermionic parts. Usually, a quadrupolequadrupole boson-fermion interaction is assumed: ˆ VBF =−2x αNB ˆ Q(χ) B·ˆ qF, (9) where Q(χ) B is the boson quadrupole operator given in Equation (3) and ˆ qF is the fermion quadrupole operator ˆ qF=∑ j tj(a† jט aj)(2), (10)
Symmetry 2021,13, 215 5 of 26 where j indicates the single particle orbitals. In the case of a singlej shell, the coefficients tj can be set to one without loss of generality. Notice that, in the case of j= 1 / 2, this operator cannot be defined. The intrinsic frame formalism for odd-even systems [ 40 – 42 ] leads itself to the description of the shapes involved in a quantum phase transition. A potential energy surface, depending on the shape variables, can be associated to a given model Hamiltonian, such as (7), in this formalism. To consider the intrinsic frame states of the mixed boson-fermion system, the single-fermion states have to be coupled to the bosonic intrinsic ground-state |Φgs(β , γ)i given by Equation (4). To obtain the lowest states of the odd-even nucleus, we first construct the coupled states as follows |ΨjK(β,γ)i=|Φgs(β,γ)i⊗|jKi, (11) and then diagonalize the total boson-fermion Hamiltonian in this basis, thus obtaining a set of energy eigenvalues En ( β , γ ), that are functions of the variational parameters, where n is an index that counts the solutions of the odd-even system. In the following, we will use this formalism to study different transitional situations in IBFM, starting with path 1 in Figure 1and the comparison with the proposed critical point symmetries. 3. The E(5/4) and E(5/12) Critical Points of the Boson-Fermion System The concept of critical point symmetries in boson-fermion systems was fist proposed by Iachello [ 10 ]. He studied the case of an odd particle moving in a single j= 3 / 2 shell coupled to an E(5) bosonic core, and called the corresponding symmetry E(5/4). The analytic solution of the E(5/4) model was first obtained from the Bohr Hamiltonian. Later on, the IBFM Hamiltonian was used to study the corresponding phase transition, called e(5/4), along the U(5)-O(6) line [ 13 ] for the even-even part, and the results are in good agreement with those of Bohr Hamiltonian for E(5/4) model. A more complex case of the critical point symmetry so-called as E(5/12) model [ 11 , 14 ] has been described for the case of multij orbitals, again starting from the Bohr Hamiltonian. In addition, in this case, comparable results are obtained within the IBFM model, called e(5/12). In this richer case, the fermion that can occupy a set of single-particle states with angular momenta j = 1 / 2, 3 / 2, 5 / 2 and is coupled to a bosonic core undergoing the transition (path 1) from spherical to deformed γ-unstable situation. These two cases are discussed below. 3.1. The E(5/4) Critical Point of the Boson-Fermion System For the bosonic part of both mentioned E(5/4) and E(5/12) critical point symmetries, the bosonic Hamiltonian used is (7) with α= 1 (the selection of other α value displaces the critical point in x but all the characteristics remain the same). Since the transition in the bosonic core is from spherical to deformed γ -unstable shapes (path 1 in Figure 1), the value of χ= 0 is fixed along the path. Thus, there is a single control parameter, x , that changes in the interval [ 0,1 ] . For x= 0, the system is in the U(5) dynamical symmetry (spherical), and, for x= 1, the system is in the O(6) dynamical symmetry (deformed γ -unstable). All along the path, the system is γ -independent. Notice that the quadrupole operator does not show for this path the term with the coupling of two d bosons, since χ= 0 for this leg of the Casten triangle. The critical point occurs at xc=NB/(5NB−8) . This result is obtained analytically by using the intrinsic frame formalism [13]. The Hamiltonian (7) within the IBFM model [ 12 ], where a single fermion is coupled to the even-even bosonic core, can be used to discuss the energy spectra evolution in odd nuclei and the corresponding behavior around the critical point. The bosonic part for this case is γ -independent, consequently, the Hamiltonian is only a function of β . The pure
Symmetry 2021,13, 215 6 of 26 fermion part (8) in Equation (7) is just a constant for a single fermion: HF=constant . The fermion quadrupole operator for this single-jcase (j=3/2) is qF= (a† 3/2 ט a3/2)(2), and the coupling term for the boson-fermion interaction is given by Equation (9) with α=1. The intrinsic frame states of the mixed boson-fermion system can be built by coupling the j= 3 / 2 orbital with the ground state |Φgs(β , γ)i of the boson condensate given in Equation (4) obtaining |Φgs(β , γ)i⊗|jKi , Equation (11). The fermionic part, as mentioned above, is just a constant because of the singlej , and so only the ˆ VBF coupling term has to be diagonalized in this basis. The doubly degenerate eigenvalues E±(β)are given by E±(x,β) = ±2xβ 1+β2. (12) Here, the coupled fermion does not destroy or alter the γ -instability of the system and the energy surfaces obtained for the different intrinsic states of the odd system are still γ -independent [ 42 ]. This special case of supersymmetry is known from the work of Bayman and Silverberg [43]. The corresponding evolution of the spectrum is displayed as a function of the control parameter x given in Hamiltonian (1) in Figure 2. The levels in the even-even system (left side) are compared with those in the odd-even system (right panel). The number of bosons is NB= 7 for both cases and the odd particle is assumed to be in the j= 3 / 2 orbital. The critical point is xc=NB/(5NB−8) = 7 / 27 ≈ 0.26 for seven bosons as marked in Figure 2. The level evolution of the odd-even system exhibits quite a similar behavior to that of the even-even system. In the odd system, the group Spin BF (5) replaces the group O B (5) of the bosonic case and leads to a richer pattern for the fermionic case. In particular, the multiplet ( 3 / 2,1 / 2 ) plays the role of the τ= 1 multiplet of the even-even case, and leads to a larger set of degenerate angular momenta, namely j= 1 / 2,5 / 2 and 7 / 2. This is a clear signature for the occurrence of this symmetry: there should be a relatively well isolated multiplet with these quantum numbers, in order to speak of an underlying Spin BF (5) symmetry. The energy ratios of the odd-even case are also slightly different from that of even-even case. In the x= 0 limit, the ground-band with maximum σ values for both systems are obtained ( σ = NB for even-even nuclei and σ1=NB+ 1 / 2 for odd-even nuclei). The energy ratio E (5/2,1/2) /E (3/2,1/2) of ground band is 2.4 and close to the ratio R 4/2 =2.5 of O B (6) symmetry. To better evidence the peculiarity of the j= 3 / 2 case, we compare in Figure 3the evolution of the spectrum in the singlej cases, j= 3 / 2 and j= 5 / 2, as a function of the control parameter x . As seen in this figure, the spectrum of the j= 5 / 2 case (right panel) is more complex because of the degeneracies are broken, even though it exhibits a qualitatively similar behavior with respect to that of the j= 3 / 2 case, displayed in the left panel. To summarize this subsection, we reviewed the results obtained within the IBFM model for the coupling of a j= 3 / 2 particle to a bosonic core that undergoes a transition from spherical to γ -unstable shapes. The energy levels of the odd-even system display qualitatively similar behaviors with respect to levels of the even-even system. A more detailed investigation can be found in Ref. [ 13 ], including a comparison of these results with the E(5/4) model [10] based on the Bohr Hamiltonian.
Symmetry 2021,13, 215 7 of 26 Figure 2. (Taken from Ref. [ 13 ]) The energy levels (normalized to the energy of the first excited state) are plotted as a function of the parameter x for the even-even system ( left ) and the odd-even system ( right ). In parenthesis, the value of (τ) in the even-even system and the values of (τ1 , τ2) in the odd-even system. Figure 3. (Taken from Ref. [ 13 ]) The energy levels for the odd system are displayed as a function of the parameter x for the odd particle taken in the j= 3 / 2 orbital ( left panel ) and in the j= 5 / 2 orbital (right panel). The number of bosons is NB=7 for both cases.
Symmetry 2021,13, 215 8 of 26 3.2. The E(5/12) Critical Point of the Boson-Fermion System The E(5/12) critical point within the collective Bohr hamiltonian for the multij case [ 11 , 14 ] is an extension of the E(5/4) critical point [ 10 , 13 ]. In this subsection, we review the corresponding results for the equivalent critical point within the IBFM model, called e(5/12), for the coupling of a single fermion moving in the j= 1 / 2,3 / 2,5 / 2 single-particle orbits to the bosonic core undergoing a transition from spherical to γ -unstable shape (path 1 in Figure 1). It is worth mentioning that the Bohr Hamiltonian in this multij case has two extra parameters as given explicitly in (Ref. [11], Equation (1)). The bosonic term in the general IBFM Hamiltonian (7), parametrized as in Equation (1) , can be recasted into a combination of Casimir operators as follows [11,14]; HB= (1−x)C1[UB(5)] −x 2αNB{C2[OB(6)] −C2[OB(5)]}, (13) where C1 [U B (5)] is the linear Casimir operator of the U B (5) algebra, and C2 [O B (6)] and C2 [O B (5)] are the quadratic Casimir operators of the O B (6) and O B (5) algebras. For the following results, we used α= 1. This bosonic Hamiltonian can produce a phase transition from spherical to γ -unstable case along the U(5)–O(6) line by sweeping the control parameter xfrom 0 to 1, and the critical point occurs at xc=NB/(5NB−8)[11,13,14]. The remaining pure fermionic term and the boson-fermion interaction term, that are needed in the general Hamiltonian (7), have been parametrized as follows, in Refs. [ 11 , 14 ], HF+VBF =k0 2NB C2[OF(5)] + k 2NB{C2[OBF(5)] −C2[OB(5)] −C2[OF(5)]}, (14) where C2 [O F (5)] and C2 [O BF (5)] are the quadratic Casimir operators of the O F (5) and O BF (5) algebras, respectively. k and k0 are the new parameters of the multij E(5/12) model, that were fixed to k=− 1 / 4 and k0= 5 / 2 in Ref. [ 11 ]. For the IBFM comparison to the geometric E(5/12), the same values for k=−1/4 and k0=5/2 have been used. The general Hamiltonian (7) can be thus rewritten in terms of Casimir operators as H= (1−x)C1[UB(5)] −x 2NB{C2[OB(6)] −C2[OB(5)]} +k 2NB{C2[OBF(5)] −C2[OB(5)] −C2[OF(5)]}+k0 2NB C2[OF(5)]. (15) This Hamiltonian is designed to mimic the corresponding Hamiltonian in the geometrical E(5/12) model [11]. The energy spectrum of the odd-even system corresponding to the results of the IBFM calculation with the Hamiltonian (15) at the critical point, given in the lower panel of Figure 4 is compared with the corresponding energy spectrum of the odd-even system obtained within the E(5/12) model (upper panel). The critical point xc is roughly 0.26 for the choice of NB= 7 bosons. As seen in this figure, the energy spectrum obtained in both approaches are structurally analogous with each other, even though small differences remain in the energies and transition rates. The above IBFM Hamiltonian (15) has been specifically designed to match the E(5/12) Hamiltonian. An alternative way for checking the results of the E(5/12) model is to apply the Hamiltonian (1) used in the previous subsection for the U(5)-O(6) transition in eveneven system and to select the critical point under these conditions. For the odd-even system, the odd fermion, allowed to span the set of j= 1 / 2,3 / 2,5 / 2 orbitals, is coupled to the bosonic core using the standard form of quadrupole-quadrupole boson-fermion interaction. In this case, the single-particle energies in Equation (8) are taken as ε1/2 = 0,
Symmetry 2021,13, 215 9 of 26 and ε3/2 = ε5/2 = ( 1 −x) + 4 x/NB . For the boson-fermion part, the usual form Equation (9) is used with the fermion quadrupole operator given in this situation as [14] ˆ qF=t(2) F"−r4 5(a† 1/2 ט a3/2 +h.c.)(2)−r6 5(a† 1/2 ט a5/2 +h.c.)(2)#. (16) With these choices, the total Hamiltonian (7) can be recast in a way that is formally equivalent to that given in Equation (13) for the boson part, namely HBF = (1−x)C1[UBF(5)] −x 2NB{C2[OBF(6)] −C2[OBF(5)]}. (17) Figure 4. (Taken from Ref. [ 14 ]) Energy levels (normalized to the energy of the first excited state) in the odd system within E(5/12) critical point (upper panel) and within the Interacting Boson-Fermion Model (IBFM) Hamiltonian (15) at the critical point (lower panel). The value of the critical point xc≈0.26 for the number of bosons is NB=7. The evolution of the spectrum as a function of the control parameter x is shown in Figure 5. The boson number used is NB= 7, and the critical point is xc=NB/(5NB−8)≈0.26 as marked by a line. Energies are normalized to the energy difference between the first excited state (which is always a 3 / 2 − 5 / 2 doublet) and the JBF = 1 / 2 ground state. Each state is characterized by the (τ1 , τ2) quantum numbers, and the set [N1 , N2](σ1 , σ2 , σ3) , different for each band, is given for each state on the right side of the figure.
Symmetry 2021,13, 215 16 of 26 of generality since a singlej shell case is considered. Notice that, in the case of j= 1 / 2, this operator cannot be defined. The pure fermion part of the general IBFM Hamiltonian, given in Equation (7), is just a constant for the singlej shell case. Thus, the IBFM Hamiltonian used is H=HB+VBF = (1−x)ˆ nd−x 4NB ˆ Qχ B·ˆ Qχ B−x 2NB ˆ Qχ B·ˆ qF. (23) Consequently, there are two control parameters in the Hamiltonian: x and χ . Changing appropriately these control parameters, one can explore the full IBM model space (see Figure 1) to which the fermion is coupled in IBFM. Each dynamical symmetry of the model corresponds to specific values of xand χ. The intrinsic formalism discussed in Section 2is used for the present applications. For the single angular momentum j= 9 / 2 cases, the possible magnetic components are K=− 9 / 2, ..., 9 / 2 and there are ten different states in total. However, these states can be restricted to five due to the symmetry involving the K↔ −Kcomponents. 5.1. Quantum Phase Transition in Bose-Fermi Systems for a Single-j Orbit: From Spherical to γ-Unstable Shapes In this subsection, we discuss the effect of the coupling of a single fermion with j= 9 / 2 to a bosonic core with NB= 5 bosons that performs a transition from spherical to γ -unstable shape. Spherical and γ -unstable shapes are obtained by taking all along the path χ= 0 in the boson quadrupole operator and selecting x= 0 and x= 1, respectively, in the Hamiltonian (23). The critical point is found at xc=NB/( 2 NB− 2 ) for this secondorder shape phase transition and its value is 0.625 for NB= 5 bosons. Please note that, in preceding Section 3, the critical point in the even-even system for the transitional path from spherical to γ− unstable shapes was xc=NB/( 5 NB− 8 ) , but that was the case with α= 1 in the Hamiltonian. In this section, as in Section 4, we are using α= 4 in the Hamiltonian so as to have the critical point around the middle of the xinterval. In the right side of Figure 10, the bosonic energy surface is plotted in the β - γ plane at the critical point ( x= 0.625 for NB= 5 bosons). As seen from Figure 10c, the even-even core is γ -unstable and has a spherical minimum. The single fermion with j= 9 / 2 is coupled to this core using the boson-fermion interaction in Equation (23). Then, the five fermionic energy surfaces are plotted as a function of β for γ= 0 ◦ in Figure 10d including also the bosonic one as reference, plotted as a red color line. The positive and negative β values indicate prolate and oblate shapes, respectively. As it is clearly seen in this figure, the even-even energy surface is very flat, and this is a clue that indicates that it is the critical point of a continuous phase transition. However, the odd-even system prefers prolate shapes for K= 1 / 2, 3 / 2, 5 / 2, while it prefers to be oblate for K= 7 / 2, 9 / 2. The left side of Figure 10 includes the bosonic energy surface of a purely γ -unstable core in the β - γ plane, and the energy surfaces as a function of β are obtained by coupling a j= 9 / 2 particle to this bosonic core (again shown as a reference marked by red in Figure 10b). It is seen from this panel that the even-even energy surface has two degenerate minima with the same deformation value βmin =± 0.78 in both prolate and oblate sides. This suggests γ -independence. The behavior of the odd-even energy surfaces are similar to the ones in Figure 10d. The states with K= 1 / 2, 3 / 2, 5 / 2 have prolate minima, and the other K -states have oblate minima, for roughly the same ±βmin of the bosonic core. In Figure 11, the evolution of the bosonic and fermionic energy surfaces as a function of β deformation for γ= 0 ◦ is given for a set of x values along the transitional region. When the core is inside the spherical region ( β minimum in zero), the preference of K=1/2, 3/2, 5/2 states is for the prolate side shapes, and the preference of others K -states is for oblate shapes with quite small values of deformation. When the core jumps into deformed γ -unstable at the critical point and moves to more β− deformed γ -unstable shapes, the behavior of all K -states remains similar, but the modulus of their β values at the energy minimum increases, showing the differences more appreciably.
Symmetry 2021,13, 215 17 of 26 Figure 10. (Color online) (Taken from Ref. [ 16 ]) Potential energy surfaces in the case of five bosons. ( a ) Bosonic energy surface for the γ -unstable shape. ( b ) Bosonic (red) and five fermionic energy surfaces as a function of β for γ= 0 ◦ . ( c ) Bosonic energy surfaces as a function of β and γ at the critical point xc= 0.625. ( d ) Five fermionic energy surfaces as a function of β for γ= 0 ◦ ; the bosonic one is also plotted, red line, for reference. Figure 11. (Color online) (Taken from Ref. [ 17 ]) Evolution of the energy surfaces as a function of β (keeping γ= 0 ◦ ) for the bosonic core (red, upper left panel) and for the different K states in the odd-even system. The control parameter xis changed in the Hamiltonian (23), where χ=0.
Symmetry 2021,13, 215 18 of 26 5.2. Quantum Phase Transition in Bose-Fermi Systems for a Single-j Orbit: From Spherical to Prolate Shapes In this part, we discuss the effect of the coupling of a single j= 9 / 2 fermion to a bosonic core with NB= 5 that performs a transition from spherical to prolate shapes, in particular, at and around the critical point. To obtain pure prolate shape, one has to choose χ=−√7/ 2 and x= 1 in the Hamiltonian (23). In this situation, the phase transition occurs at the critical point xcr = 16 NB/( 34 NB− 27 ) along the transition spherical-prolate shapes, as discussed in Section 4. For NB= 5, the value of the critical point is xcr = 0.56, and the transition in the even-even system is known to be first-order [3]. To study the effect of the coupled fermion on the core around the U(5)-SU(3) critical point, the control parameter values are taken as x= 0.5, xcr = 0.56, x= 0.6 in the Hamiltonian (23). Their ground state energy surface is obtained by calculating the expectation value of this Hamiltonian in the intrinsic state. The bosonic energy surfaces as a function of β and γ are plotted around the critical point as seen Figure 12. Later, the single fermion with j= 9 / 2 is coupled to the core using the boson-fermion interaction VBF in Equation (23). The behavior of the fermionic energy surfaces as a function of β (for γ= 0 ◦ ) is illustrated around the critical point in the right side of each panel in Figure 12, where the bosonic core is marked with red color as a reference. As seen in the middle panel, the bosonic surface has two minima at xcr = 0.56. The even-even core is spherical before this point (in the first panel) and then it jumps to prolate (in the last panel). The intrinsic states of the odd-even system have a tendency to show prolate or oblate shapes, while the bosonic core is located at critical point or in its close surroundings. Figure 12. (Color online) (Taken from Ref. [ 18 ]) Bosonic energy surfaces in the β - γ plane for NB= 5 bosons at x= 0.5 in ( a ), at the critical point xcr = 0.56 in ( b ), at x= 0.6 in ( c ). Fermionic energy surfaces for different K -states as a function of β (γ=0◦) are also given, including also the bosonic one as a reference (red line). The evolution of the equilibrium deformation parameter for the bosonic core and five fermionic states is illustrated in Figure 13 along the transition from spherical to prolate shape (left panel). Fermionic states with smaller K= 1 / 2, 3 / 2, 5 / 2 always favor the prolate shapes, while states with K= 7 / 2, 9 / 2 are oblate up to x7/2 ≃ 0.6 and x9/2 ≃ 0.69. Later, these states with larger K suddenly jump to prolate shapes. It is clearly seen that both states, K= 7 / 2, 9 / 2, show first order transitions at certain specific values of the control parameter. In the prolate region, the core drives all K states into the prolate side and they have roughly the same βmin ≃ 1.28. The case of U(5) to O(6) transition discussed in the previous subsection is also given in the right panel of Figure 13 for the comparison. Here, the tendency of the states with smaller K ’s is always to be prolate, while states with higher K’s always tend to oblate shapes.
Symmetry 2021,13, 215 19 of 26 Figure 13. (Color online) (Taken from Ref. [ 18 ]) Evolution of the equilibrium deformation parameter for the bosonic core (red) and for the different K -states in the odd-even system as a function of the control parameter x along the spherical to deformed region: the transition from U(5) to SU(3) is shown in the left panel , while the transition from U(5) to O(6) is shown in the right panel , discussed in Section 5.1. Positive and negative values of βmin indicate prolate and oblate shapes, respectively. 5.3. Quantum Phase Transition in Bose-Fermi System for a Single-j Orbit: From Spherical to Oblate Shapes The effect of the coupling of a fermion moving in a single j= 9 / 2 shell to a bosonic core with NB= 5 that performs the transition from spherical to oblate shapes is discussed. The aim is to see how the coupled fermion modifies the shape of the coupled odd system and how each of the odd states behaves along the given transition path (path 3 in Figure 1). We show the case of j = 9/2, but the overall results for the effect of the coupled fermion are also presented for a set of different values of j ranging from 3 / 2 to 13 / 2 along the same transitional region. This case is similar to the preceding case, and we discuss it for the sake of completeness. The spherical shape is obtained for the control parameter x= 0 in the Hamiltonian (23) , while x= 1 and χ= +√7/ 2 produce a pure well deformed oblate shape. The critical point is found at xcr = 16 NB/( 34 NB− 27 ) in between spherical and oblate shapes, which correspond to the value xcr = 0.56 in the case of five bosons. This value is exactly the same value of the critical point that occurs in between spherical and prolate shapes. The bosonic energy surfaces are plotted as a function of the deformation parameters ( β , γ ) for NB= 5 around the critical point as shown in upper panels of Figure 14. As seen in the middle panel (b), the bosonic surface has two degenerate minima (one spherical and one oblate) at the critical point value xcr = 0.56. Before this point, the even-even system is spherical and after it jumps to oblate shape. Comparing Figures 12 and 14, one sees that the two bosonic cases are completely symmetric with respect of the sign change in chi, as expected. As seen in the lower panels of Figure 14, the fermionic intrinsic states prefer either prolate or oblate shapes depending on their K value; hence, their behavior around the critical point is quite different from that illustrated in Figure 12. The evolution of the equilibrium deformation parameter for the fermionic states and the bosonic case along the transitional path from spherical to oblate shape is illustrated in Figure 15. As seen in fourth panel (d) of Figure 15 for the case of j= 9 / 2, the states with K= 7 / 2,9 / 2 always favor oblate shapes, while states with the lower K= 1 / 2, 3 / 2, 5 / 2 are prolate up to their specific critical x values. After these values, they suddenly jump from prolate to oblate shapes. They present two degenerate minima for these values and as a result the components with lower K ’s show first-order phase transitions. On the contrary, in the case of phase transitions along the U(5) → SU(3) path, as illustrated in the first panel of Figure 13, the states that show first order characteristics are those with higher K= 7 / 2, 9 / 2. As seen in the panels of Figure 15 for the different singlej from 3 / 2 to 13 / 2, the lower K states always prefer to be prolate up to their specific critical point, then they
Symmetry 2021,13, 215 20 of 26 jump to oblate shape at these specific x values, while the higher K states always prefer oblate shapes along the full transitional path. In the well deformed oblate region, close to x= 1, once again we see that the oblate core drives all states to the oblate shape, with approximately the same βmin ≃ −1.28. Figure 14. (Color online) (Taken from Ref. [ 19 ]) Similar to Figure 12. Bosonic energy surfaces in the β - γ plane for different x values around the critical point appeared in between spherical to oblate shapes. In the lower panels, the energy surfaces as a function of β(γ=0◦) for the five Kstates of j=9/2, with the even-even core shown in red for reference. Figure 15. (Color online) (Taken from Ref. [ 19 ]) Similar to Figure 13. Evolution of the equilibrium deformation parameter in the odd-even system as a function of the control parameter x along the transition path from spherical to oblate shapes. Each panel represents a different single-jcase. The bosonic case is shown in red color.
Symmetry 2021,13, 215 21 of 26 5.4. Quantum Phase Transition in Bose-Fermi System for a Single-j Orbit: From Prolate to Oblate Shapes Recently, we investigated [ 20 ] the case of a singlej= 9 / 2 fermion coupled to a bosonic core with NB= 5 that performs a transition from prolate to oblate shapes. We focused on the effect of the coupled fermion on the whole system along the transitional path from prolate to oblate shapes, passing through the γ -unstable shape. For this transition, one can move in between the SU(3) → O(6) →SU(3) symmetries (path 4 in Figure 1) in the deformed region by taking a fixed value of x= 1 and changing the χ parameter from χ=−√7/2, through χ=0 to χ= +√7/2 in the Hamiltonian (23). The deformed prolate, γ -unstable, and oblate shapes of the even-even core with NB= 5 bosons are produced for different χ values as in the previous subsections of the Section 5. Their ground state energy surface for each shape is obtained by calculating the expectation value of the corresponding Hamiltonian (23) in the intrinsic state given in Equation (4). These energy surfaces in the β and γ plane are presented for deformed prolate shape in Figure 8left panel. In this case, the bosonic energy surface has the minimum at γ= 0. The projection of this energy surface on the γ= 0 plane is the dashed line. In the same plot, the energy surfaces of the odd-even system are displayed. All of them follow the behavior of the core with approximately the same deformation. The case for the deformed oblate shape is similar to the prolate case but the deformations are for negative β (or alternatively for γ= 60 ◦ ). Thus, one could conclude that all the magnetic substates of the coupled single-fermion with j= 9 / 2 would be driven by the shape of the bosonic core. However, for the γ -unstable case, Figure 10 (panel a) presents the bosonic energy surface in the (β , γ) plane. This figure also include, in panel b, the odd-even energy surfaces of a single fermion with angular momentum j= 9 / 2 coupled to it using the boson-fermion interaction given in Equation (23). Now, we will show that, in the surroundings of the O(6) point, the odd-fermion system follows some unexpected and unique paths. The energy surfaces as a function of β and γ are calculated for the obtained odd-even states. The notation with n= 1,..., 5 is used instead of K , for the five magnetic substates of j= 9 / 2 because K is not a good quantum number along this transition (it is still a good quantum number at the extreme points where axial symmetry is recovered). These calculated odd-even energy surfaces in ( β , γ ) are shown in Figure 16 for each n state for different χ values. The three rows in the figure refer to three χ values selected around the critical region for each n -state. The energy minimum is denoted by a blue dot in each panel also including the values βmin , γmin , and Emin . In the middle panels of n= 2 and n=4 states, there are two blue circles since prolate and oblate minima are degenerate for slightly different β -deformations separated by a small barrier with the Ebar marked with blue squares. For the complete analysis of the absolute minimum evolution for each n -state, polar plots in the (β , γ) plane are presented in Figure 17. Each panel corresponds to a different n -state and the β and γ values provide the absolute minima of the energy surface for different χ -values. It is clearly seen that the five components of the j= 9 / 2 orbital seem to show quite interesting and unexpected behavior. Two odd-states ( n= 1,4) move slowly from the prolate ( γ= 0) to the oblate ( γ= 60 ◦ ) shape by venturing into the triaxial region, showing γ -softness around their slow shape-changing region. The other three odd-states ( n= 2,3,5) show sudden jumps (critical point) at some χcrit from prolate side to oblate side without passing through triaxial structures what generates shape coexistence, although one of them ( n= 3) is fairly close to γ -instability. Of course, care has been used here to ensure that the jump is not a numerical artifact due to scales changing too slowly or too rapidly.
Symmetry 2021,13, 215 22 of 26 Figure 16. (Color online) (Taken from Ref. [ 20 ]) The contour plots of the odd-even energy surfaces as a function of β and γ for each n -state for different χ values. The absolute minima are marked with a blue dot, and the values of the energy barriers’ heights are marked with blue squares.
Symmetry 2021,13, 215 23 of 26 Figure 17. (Color online) (Taken from Ref. [ 20 ]) The values of (β , γ) at the energy minima for different χ values between −√7/2 and +√7/2 for the five n-states. The absolute minima of the energy surface are indicated by full dots. 6. Summary and Conclusions In this contribution, our works on quantum phase transition for Bose-Fermi systems within the intrinsic frame formalism associated with the IBFM model have been reviewed. The main aim of these studies is to understand the effect of the coupled fermion on the core when moving along a given transitional path and how the coupled fermion modifies the characteristics of the bosonic core around the critical points. First, we presented some IBFM results trying to mimic the situation described by the E(5/4) critical point symmetry, for the case of a single j= 3 / 2, and its extended version, the E(5/12) critical point symmetry, for multij orbits ( j= 1 / 2,3 / 2,5 / 2). A possible example of the E(5/4) is 133 Ba built on the single particle level d 3/2 . The multij situation of E(5/12) can occur in odd-neutron Pt isotopes with the active orbits 3 p1/2 , 3 p3/2 , 2 f5/2 and in odd-proton Ir isotopes with active orbits 2 d5/2 , 2 d3/2 , 3 s1/2 around the A≃ 190 mass region and also in odd-neutron Ba isotopes with relevant orbits 2 d5/2 , 2 d3/2 , 3 s1/2 around the A≃ 130 mass region. Later, we recapitulated the IBFM results for the U BF (5) to SU BF (3) transition in odd nuclei for the same multij orbits. These results include the energy levels along the transition from spherical to the axially deformed shape and also the energy surfaces for the even-even and odd-even cases. According to these results, the main effect of the coupled fermion is to produce a systematic shift of the critical point location in the odd-even system with respect to the one characterizing the even-even core. Finally, in Section 5, we reviewed our systematic studies for the case of a singlej fermion coupled to a bosonic core that performs different transitions: from spherical to γ -unstable shape, from spherical to axially deformed (prolate and oblate) shapes, and from prolate to oblate shape passing through the γ -unstable shape. As a specific test case, we took into account a singlej fermion with angular momentum j= 9 / 2 coupled to a bosonic core with small number of bosons ( NB= 5). When the bosonic system exhibits a second-order phase transition moving from spherical and γ -unstable shapes, the fermionic
Symmetry 2021,13, 215 24 of 26 states with lower K= 1 / 2, 3 / 2, 5 / 2 values show oblate shapes, while the K= 7 / 2, 9 / 2 states prefer prolate ones. However, when the even-even system performs the transition from spherical to prolate shape for the bosonic core, the fermionic states with smaller K ’s always favor prolate shapes, and the states with K= 7 / 2,9 / 2 are oblate up to a certain point beyond the critical point for the bosonic system, but then these states also jump to the prolate side, showing first-order phase transitions. When the bosonic core moves from spherical shape to oblate shape, states with the lower K= 1 / 2, 3 / 2, 5 / 2 show first-order phase transitions, jumping to oblate at some value of the control parameter x beyond the bosonic critical point. States with higher K= 7 / 2, 9 / 2 always favor oblate shapes. For this transitional path, we also presented the results for different singlej values from 3 / 2 to 13 / 2 to show that their behavior is similar, and we can thus take just one (say the j= 9 / 2) as a representative for any of them. Finally, the results of our last work on the prolate to oblate phase transition in Bose-Fermi systems show quite interesting and unexpected behavior. Two states in the odd-even system move slowly from the prolate to the oblate shape by venturing into the triaxial region, also showing a γ -softness behavior in the middle, while the other three states show sudden jumps from prolate to oblate shapes. Evidence of quantum phase transitions in odd systems were reported in recent works [27–34]. The experimental evidence for transition from spherical to the γ -unstable shapes in odd-mass 127−137 Ba and 101−109 Rh, and 123−135 Xe nuclei was presented in Refs. [ 27 , 28 , 32 ] and analyzed by calculating their nuclear properties, such as B(E2) values and two-neutron separation energies, within the IBFM model for the U BF (5)–O BF (6) transition along the isotopic chain. The signatures of the quantum shape phase transition in odd-mass 129−137 Ba, 129−137 La, 127−135 Xe, and 127−135 Cs nuclei in the A ≈ 130 mass region were studied by taking into account their bosonic cores 128−136 Ba for 129−137 Ba, 129−137 La, and 126−134 Xe [ 30 , 31 ]. These cores empirically exhibit a transition from nearly spherical to γ -soft shape. The calculations of the low-energy states and the electromagnetic transition rates of given γ -soft odd-mass nuclei provide a reasonable agreement with the experimental data along the isotopic chain [ 30 , 31 ]. A microscopic description of the quantum shape phase transition was performed for the the axially-deformed odd-mass 147−155 Sm and 147−155 Eu nuclei [ 29 ] by taking into consideration their common bosonic cores 148−154 Eu that show the transition from spherical to axially-deformed shape. Another description along the same transition path was carried out for odd-mass 149−155 Eu isotopes and their even-even neighbors, 148−154 Sm and 150−156 Gd nuclei [ 33 ]. In this study, the energy surfaces were presented for even-even nuclei, later the energy spectra of odd-mass 149−155 Eu isotopes were analyzed and their two-neutron separation energies, isotope shifts, quadrupole moments, and E2 reduced transition matrix elements were calculated along the isotopic chain and the results show good agreement with experimental data [ 33 ]. The prolate to oblate shape phase transition was studied in neutron-rich odd-mass 185−193 Os, 185−195 Ir, and 185−199 Pt nuclei in the A ≈ 190 mass region to see the effect of the odd particle [ 34 ]. Their even-even neighboring nuclei 186−200 Pt and 186−194 Os were also taken into account and their energy surfaces were plotted as a function deformation parameters ( β , γ ) exhibiting good examples for the transition from prolate to oblate shape and also including γ -soft shape. Spectroscopic properties of given odd-mass Os, Ir, and Pt nuclei were calculated within the effective IBFM Hamiltonian based on the nuclear energy density functional theory [ 45 ]. More recently, a description of the quantum shape phase transition has been simultaneously performed in the even-even 94−102 Zr and the odd-even 95−103 Zr nuclei [ 46 ]. Their spectroscopic properties, related to the quantum shape phase transitions, are calculated within the IBFM model, and the results are in good agreement with the experimental data. Author Contributions: M.B., C.E.A., J.M.A., L.F. and A.V. contributed equally to this review article. All authors have read and agreed to the published version of the manuscript. Funding: This work was supported by the Scientific and Technical Research Council of Turkey (TÜB˙ ITAK), under the project number 119T127. M.B. thanks to Scientific Research Projects Coordination Unit of Kırıkkale University for the supports of travel expenses to join scientific meetings held at Padova University in 2018 and 2019, under project numbers 2016/001-351 and 2019/040. This
Symmetry 2021,13, 215 25 of 26 work has been also partially supported by the Consejería de Economía, Conocimiento, Empresas y Universidad de la Junta de Andalucía (Spain) under Group FQM-160, by the Spanish Ministerio de Ciencia e Innovación, ref. FIS2017-88410-P and PID2019-104002GB-C22, and by the European Commission, ref. H2020-INFRAIA-2014-2015 (ENSAR 2). Institutional Review Board Statement: Not applicable. Informed Consent Statement: Not applicable. Data Availability Statement: Data related to this work are available on request from the authors. Conflicts of Interest: The authors declare no conflict of interest. References 1. Iachello, F. Dynamic Symmetries at the critical point. Phys. Rev. Lett. 2000,85, 3580–3583. [CrossRef] 2. Bohr, A.; Mottelson, B. Nuclear Structure; Benjamin: Reading, MA, USA, 1975; Volume 2. 3. Iachello, F. Analytic description of critical point nuclei in a spherical-axially deformed shape phase transition. Phys. Rev. Lett. 2001,87, 052502. 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