pith. sign in

arxiv: 2604.11918 · v1 · submitted 2026-04-13 · ⚛️ nucl-th

Parameter-free deformation variables of the proxy-SU(3) symmetry in even-even atomic nuclei with Z=28-82, N=28-126

Pith reviewed 2026-05-10 15:34 UTC · model grok-4.3

classification ⚛️ nucl-th
keywords proxy-SU(3)deformation variablesbeta and gammaeven-even nucleihighest-weight irrepnuclear shapesshell modelPauli principle
0
0 comments X

The pith

Proxy-SU(3) symmetry predicts nuclear deformation variables beta and gamma parameter-free for even-even nuclei with Z=28-82 and N=28-126.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The paper demonstrates that the proxy-SU(3) approximation restores SU(3) symmetry in the shell model beyond the sd shell and uses it to calculate the collective shape parameters beta and gamma for even-even nuclei. Selection of the highest-weight irreducible representation of SU(3), dictated by the Pauli principle and the short-range attractive nucleon-nucleon force, supplies the predictions without any adjustable parameters. Complete tables of these representations and the resulting beta and gamma values are supplied for the entire range from nickel to lead isotopes, with a few examples showing how the assignments illuminate specific trends in different parts of the nuclear chart. A sympathetic reader would care because the approach covers a large fraction of the chart of stable and near-stable nuclei using only group-theoretical rules.

Core claim

The proxy-SU(3) approximation predicts the collective deformation variables beta and gamma of even-even atomic nuclei in a parameter-free way, based on the most symmetric irreducible representation of SU(3) allowed by the Pauli principle and the short-range nature of the nucleon-nucleon interaction, which in group theoretical language is the highest weight irrep. In the few cases in which the hw irrep turns out to be completely symmetric and able to accommodate only the ground state band, the next hw irrep becomes indispensable. Complete tables of the hw and nhw irreps are given for all nuclei from Z=28, N=28 to Z=82, N=126, along with the corresponding parameter-free predictions for beta, 2

What carries the argument

The highest-weight (hw) irreducible representation of SU(3) under the proxy-SU(3) mapping, which selects the most symmetric allowed state to fix the ground-state deformation variables beta and gamma.

If this is right

  • The tabulated hw and nhw irreps directly yield beta and gamma values that can be compared to measured deformations throughout the given nuclear range.
  • When the hw irrep is fully symmetric, switching to the nhw irrep supplies the additional states needed for collective bands.
  • The assignments provide a group-theoretical explanation for the onset and variation of deformation in different mass regions.
  • The same parameter-free procedure applies uniformly from the lightest to the heaviest nuclei in the stated window.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • If the predictions hold, the dominant contribution to ground-state nuclear shapes in this range arises from symmetry selection rules rather than from details of the residual interaction.
  • The tables could be used as a starting point for calculations that later add configuration mixing to refine energies or transition rates.
  • Similar proxy mappings might be constructed for nuclei outside the stated Z and N limits provided the underlying harmonic-oscillator shell structure remains valid.

Load-bearing premise

The proxy-SU(3) mapping together with automatic choice of the highest-weight or next-highest-weight irrep is enough to fix ground-state beta and gamma accurately across the full range without corrections from the complete shell-model Hamiltonian or configuration mixing.

What would settle it

A precise experimental measurement of beta for any even-even nucleus in the Z=28-82, N=28-126 range that differs substantially from the tabulated prediction based on its hw or nhw irrep.

Figures

Figures reproduced from arXiv: 2604.11918 by Andriana Martinou, Dennis Bonatsos, D. Petrellis, N. Minkov, P. Vasileiou, S. K. Peroulis, T. J. Mertzimekis, V. K. B. Kota.

Figure 1
Figure 1. Figure 1: FIG. 1. (a) The parameter-free predictions for the collective [PITH_FULL_IMAGE:figures/full_fig_p032_1.png] view at source ↗
Figure 2
Figure 2. Figure 2: FIG. 2. (a) The parameter-free predictions for the collective [PITH_FULL_IMAGE:figures/full_fig_p033_2.png] view at source ↗
Figure 3
Figure 3. Figure 3: FIG. 3. (a) The parameter-free predictions for the collective [PITH_FULL_IMAGE:figures/full_fig_p034_3.png] view at source ↗
read the original abstract

The proxy-SU(3) approximation to the shell model, which restores the SU(3) symmetry of the 3-dimensional harmonic oscillator beyond the sd shell, predicts the collective deformation variables beta and gamma of even-even atomic nuclei in a parameter-free way, based on the most symmetric irreducible representation (irrep) of SU(3) allowed by the Pauli principle and the short-range nature of the nucleon-nucleon interaction, which in group theoretical language is the highest weight (hw) irrep. In the few cases in which the hw irrep turns out to be completely symmetric, thus being able to accommodate only the ground state band, the next hw (nhw) irrep becomes indispensable. In the present article complete tables of the hw and nhw irreps are given for all atomic nuclei ranging from Z=28, N=28 to Z=82, N=126, along with the corresponding parameter-free predictions for the deformation variables beta and gamma. A few examples using the tabulated results for providing microscopic insight for specific effects in various regions of the nuclear chart are also given.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

2 major / 2 minor

Summary. The manuscript tabulates the highest-weight (hw) and next-highest-weight (nhw) SU(3) irreducible representations for all even-even nuclei with 28 ≤ Z ≤ 82 and 28 ≤ N ≤ 126 within the proxy-SU(3) approximation to the shell model. These irreps are selected by the Pauli principle and the short-range character of the nucleon-nucleon interaction; the corresponding (λ, μ) labels are then converted to parameter-free predictions for the collective deformation variables β and γ. A small number of illustrative examples are given to show how the tabulated values can furnish microscopic insight into specific nuclear phenomena.

Significance. If the central mapping holds, the work supplies a fully parameter-free, symmetry-based route to nuclear deformations over a wide swath of the chart, together with exhaustive tables that can be used directly by the community. The explicit construction from group labels and the absence of fitted parameters constitute a clear methodological strength, especially for regions where large-scale shell-model diagonalizations remain prohibitive.

major comments (2)
  1. [§4] §4 (examples): the claim that the hw/nhw irrep furnishes the ground-state β and γ rests on the assumption that configuration mixing and non-SU(3) terms in the realistic Hamiltonian do not shift the ground state away from this irrep. No quantitative comparison of the predicted β, γ values to experimental data or to full shell-model results is presented for any of the illustrated cases, leaving the size of the approximation error untested.
  2. [Tables 1–10] Tables 1–10 (hw/nhw tabulations): the conversion from (λ, μ) to β and γ is performed with a fixed, parameter-free formula, but the manuscript does not state the explicit expression used (or its reference) nor provide uncertainty estimates arising from the proxy-orbital mapping itself. This omission makes it impossible to judge how sensitive the tabulated deformations are to the details of the proxy construction.
minor comments (2)
  1. The notation for the deformation variables (β, γ) is introduced without a brief reminder of the standard Bohr-Mottelson definitions; a single sentence would improve readability for readers outside nuclear structure.
  2. A few table entries list the same (λ, μ) for both hw and nhw; a footnote clarifying when this occurs (completely symmetric irreps) would prevent confusion.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for the positive assessment of the significance of our work and for the constructive comments. We respond point by point to the major comments below, indicating where revisions will be incorporated.

read point-by-point responses
  1. Referee: [§4] §4 (examples): the claim that the hw/nhw irrep furnishes the ground-state β and γ rests on the assumption that configuration mixing and non-SU(3) terms in the realistic Hamiltonian do not shift the ground state away from this irrep. No quantitative comparison of the predicted β, γ values to experimental data or to full shell-model results is presented for any of the illustrated cases, leaving the size of the approximation error untested.

    Authors: We acknowledge that the manuscript presents no quantitative comparisons of the predicted β and γ values to experimental data or full shell-model results in §4. The examples are intended to illustrate how the tabulated hw/nhw irreps can furnish microscopic insight into specific nuclear phenomena, rather than to serve as a systematic validation of the approximation. The underlying assumption—that the hw (or nhw) irrep dominates the ground state—is inherent to the proxy-SU(3) framework, which selects the most symmetric allowed irrep on the basis of the Pauli principle and the short-range character of the nucleon-nucleon interaction. We agree that an explicit discussion of the possible effects of configuration mixing and non-SU(3) terms would strengthen the presentation. In the revised manuscript we will expand the introductory paragraph of §4 to state these assumptions clearly and to note that the size of the approximation error is left for future quantitative studies, while emphasizing that the current work focuses on delivering the complete, parameter-free tabulation. revision: partial

  2. Referee: [Tables 1–10] Tables 1–10 (hw/nhw tabulations): the conversion from (λ, μ) to β and γ is performed with a fixed, parameter-free formula, but the manuscript does not state the explicit expression used (or its reference) nor provide uncertainty estimates arising from the proxy-orbital mapping itself. This omission makes it impossible to judge how sensitive the tabulated deformations are to the details of the proxy construction.

    Authors: We thank the referee for identifying this omission. The conversion from the SU(3) labels (λ, μ) to the deformation parameters β and γ employs the standard, parameter-free relations derived from the quadratic Casimir operator of SU(3) and the mapping to the collective quadrupole deformation (as introduced in the original proxy-SU(3) papers). We will add the explicit expressions together with the appropriate references in the revised manuscript, most naturally in the paragraph preceding the tables. With regard to uncertainty estimates, the proxy-orbital mapping is fixed by construction to restore the SU(3) symmetry of the harmonic oscillator as accurately as possible within each major shell; the scheme is therefore parameter-free by design. We will nevertheless insert a concise discussion of the robustness of the proxy construction, referencing earlier works that examined its accuracy, so that readers can assess the sensitivity of the tabulated values to the details of the mapping. revision: yes

Circularity Check

0 steps flagged

No circularity: beta/gamma predictions follow directly from hw/nhw irrep selection via fixed SU(3) mapping

full rationale

The derivation selects the highest-weight (or next-highest-weight) SU(3) irrep for each nucleus using the Pauli principle plus the short-range NN interaction rule, then converts the resulting (lambda, mu) labels to beta and gamma through the standard, parameter-free SU(3) deformation formulas. No step fits parameters to data or renames a fitted quantity as a prediction; the output is not equivalent to the input by construction. Self-citations to prior proxy-SU(3) papers exist but are not load-bearing for the central mapping, which remains independent and externally falsifiable against measured deformations.

Axiom & Free-Parameter Ledger

0 free parameters · 2 axioms · 0 invented entities

The central claim rests on the proxy-SU(3) approximation itself and on the rule that selects the highest-weight irrep on the basis of the Pauli principle and the short-range attractive character of the nucleon-nucleon force; both are domain assumptions rather than derived results.

axioms (2)
  • domain assumption Proxy-SU(3) restores an effective SU(3) symmetry of the 3D harmonic oscillator beyond the sd shell
    Invoked in the first sentence of the abstract as the foundation of the method.
  • domain assumption The Pauli principle together with the short-range attractive nucleon-nucleon interaction selects the highest-weight irrep
    Explicitly stated as the basis for choosing the irrep that determines beta and gamma.

pith-pipeline@v0.9.0 · 5549 in / 1584 out tokens · 39313 ms · 2026-05-10T15:34:05.725751+00:00 · methodology

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Reference graph

Works this paper leans on

183 extracted references · 183 canonical work pages

  1. [1]

    On the Consequences of the Symmetry of the Nuclear Hamiltonian on the Spectroscopy of Nuclei

    Wigner, E. On the Consequences of the Symmetry of the Nuclear Hamiltonian on the Spectroscopy of Nuclei. Phys. Rev.1937,51, 106

  2. [2]

    Nobel Foundation.Nobel Lectures, Physics 1963-1970; Elsevier: Amsterdam, The Netherlands, 1972

  3. [3]

    Mayer, M. G. On Closed Shells in Nuclei.Phys. Rev. 1948,74, 235

  4. [4]

    Mayer, M. G. On Closed Shells in Nuclei. II.Phys. Rev. 1949,75, 1969

  5. [5]

    Haxel, O.; Jensen, J. H. D.; Suess, H. E. On the ”Magic Numbers” in Nuclear Structure.Phys. Rev.1949,75, 1766

  6. [6]

    G.; Jensen, J

    Mayer, M. G.; Jensen, J. H. D.Elementary Theory of Nuclear Shell Structure; Wiley: New York, 1955

  7. [7]

    Heyde, K. L. G.The Nuclear Shell Model; Springer: Berlin, 1990

  8. [8]

    Talmi, I.Simple Models of Complex Nuclei: The Shell Model and the Interacting Boson Model; Harwood: Chur, 1993

  9. [9]

    G.Classical Groups for Physicists; Wi- ley: New York, NY, USA, 1974

    Wybourne, B. G.Classical Groups for Physicists; Wi- ley: New York, NY, USA, 1974

  10. [10]

    F.The Harmonic Oscil- lator in Modern Physics; Harwood: Amsterdam, 1996

    Moshinsky, M.; Smirnov, Yu. F.The Harmonic Oscil- lator in Modern Physics; Harwood: Amsterdam, 1996

  11. [11]

    Iachello, F.Lie Algebras and Applications; Springer: Berlin, 2006

  12. [12]

    Exact boson mappings for nuclear neutron (proton) shell-model algebras having SU(3) subalgebras.Ann

    Bonatsos, D.; Klein, A. Exact boson mappings for nuclear neutron (proton) shell-model algebras having SU(3) subalgebras.Ann. Phys. (NY)1986,169, 61

  13. [13]

    Elliott, J. P. Collective motion in the nuclear shell model. I. Classification schemes for states of mixed con- figurations.Proc. Roy. Soc. A Ser. A1958,245, 128

  14. [14]

    Elliott, J. P. Collective motion in the nuclear shell model II. The introduction of intrinsic wave-functions.Proc. Roy. Soc. A Ser. A1958,245, 562

  15. [15]

    P.; Harvey, M

    Elliott, J. P.; Harvey, M. Collective motion in the nu- clear shell model III. The calculation of spectra.Proc. Roy. Soc. A Ser. A1963,272, 557

  16. [16]

    P.; Wilsdon, C

    Elliott , J. P.; Wilsdon, C. E. Collective motion in the nuclear shell model IV. Odd-mass nuclei in the sd shell. Proc. Roy. Soc. A Ser. A1968,302, 509

  17. [17]

    The nuclear SU 3 model.Adv

    Harvey, M. The nuclear SU 3 model.Adv. Nucl. Phys. 1968,1, 67; M. Baranger, M., Vogt, E., Eds.; Plenum: New York

  18. [18]

    The coupling of nuclear surface oscillations to the motion of individual nucleons

    Bohr, A. The coupling of nuclear surface oscillations to the motion of individual nucleons. Dan. Mat. Fys. Medd.1952, 26, no. 14

  19. [19]

    Bohr, A.; Mottelson, B. R. Collective and individual- particle aspects of nuclear structure.Dan. Mat. Fys. Medd.1953,27, no. 16

  20. [20]

    R.Nuclear Structure Vol

    Bohr, A.; Mottelson, B. R.Nuclear Structure Vol. I: Single-Particle Motion; World Scientific: Singapore, 1998

  21. [21]

    R.Nuclear Structure Vol

    Bohr, A.; Mottelson, B. R.Nuclear Structure Vol. II: Nuclear Deformations; World Scientific: Singapore, 1998

  22. [22]

    Kota, V. K. B.SU(3) symmetry in atomic nuclei; Springer Nature: Singapore, 2020

  23. [23]

    Pseudo LS coupling and pseudo SU3 coupling schemes.Phys

    Arima, A.; Harvey, M.; Shimizu, K. Pseudo LS coupling and pseudo SU3 coupling schemes.Phys. Lett. B1969, 30, 517

  24. [24]

    T.; Adler, A

    Hecht, K. T.; Adler, A. Generalized seniority for fa- voredJ̸= 0 pairs in mixed configurations.Nucl. Phys. A1969,137, 129

  25. [25]

    D.; Draayer, J

    Ratna Raju, R. D.; Draayer, J. P.; Hecht, K. T. Search 24 for a coupling scheme in heavy deformed nuclei: The pseudo SU(3) model.Nucl. Phys. A1973,202, 433

  26. [26]

    P.; Weeks, K

    Draayer, J. P.; Weeks, K. J.; Hecht, K. T. Strength of theQ π ·Q ν interaction and the strong-coupled pseudo- SU(3) limit.Nucl. Phys. A1982,381, 1

  27. [27]

    P.; Weeks, K

    Draayer, J. P.; Weeks, K. J. Shell-Model Description of the Low-Energy Structure of Strongly Deformed Nuclei. Phys. Rev. Lett.1983,51, 1422

  28. [28]

    P.; Weeks, K

    Draayer, J. P.; Weeks, K. J. Towards a shell model de- scription of the low-energy structure of deformed nuclei I. Even-even systems.Ann. Phys. (NY)1984,156, 41

  29. [29]

    P.; Moszkowski, S

    Bahri, C.; Draayer, J. P.; Moszkowski, S. A. Pseudospin symmetry in nuclear physics.Phys. Rev. Lett.1992,68, 2133

  30. [30]

    Ginocchio, J. N. Pseudospin as a Relativistic Symmetry. Phys. Rev. Lett.1997,78, 436

  31. [31]

    P.; Retamosa, J.; Poves, A.; Caurier, E

    Zuker, A. P.; Retamosa, J.; Poves, A.; Caurier, E. Spherical shell model description of rotational motion. Phys. Rev. C1995,52, R1741(R)

  32. [32]

    P.; Poves, A.; Nowacki, F.; Lenzi, S

    Zuker, A. P.; Poves, A.; Nowacki, F.; Lenzi, S. M. Nilsson-SU3 self-consistency in heavy N=Z nuclei.Phys. Rev. C2015,92, 024320

  33. [33]

    E.; Minkov, N.; Martinou, A.; Cakirli, R

    Bonatsos, D.; Assimakis, I. E.; Minkov, N.; Martinou, A.; Cakirli, R. B.; Casten, R. F.; Blaum, K. Proxy- SU(3) symmetry in heavy deformed nuclei.Phys. Rev. C2017,95, 064325

  34. [34]

    E.; Minkov, N.; Martinou, A.; Sarantopoulou, S.; Cakirli, R

    Bonatsos, D.; Assimakis, I. E.; Minkov, N.; Martinou, A.; Sarantopoulou, S.; Cakirli, R. B.; Casten, R. F.; Blaum, K. Analytic predictions for nuclear shapes, pro- late dominance, and the prolate-oblate shape transi- tion in the proxy-SU(3) model.Phys. Rev. C2017,95, 064326

  35. [35]

    K.; Mertz- imekis, T

    Bonatsos, D.; Martinou, A.; Peroulis, S. K.; Mertz- imekis, T. J.; Minkov, N. The Proxy-SU(3) Symmetry in Atomic Nuclei.Symmetry2023,15, 169

  36. [36]

    D.; Draayer, J

    Dytrych, T.; Sviratcheva, K. D.; Draayer, J. P.; Bahri, C.; Vary, J. P. Ab initio symplectic no-core shell model. J. Phys. G: Nucl. Part. Phys.2008,35, 123101

  37. [37]

    D.; Draayer, J

    Launey, K. D.; Draayer, J. P.; Dytrych, T.; Sun, G.-H.; Dong, S.-H. Approximate symmetries in atomic nuclei from a large-scale shell-model perspective.Int. J. Mod. Phys. E2015,24, 1530005

  38. [38]

    D.; Dytrych, T.; Draayer, J

    Launey, K. D.; Dytrych, T.; Draayer, J. P. Symmetry- guided large-scale shell-model theory.Prog. Part. Nucl. Phys.2016,89, 101

  39. [39]

    D.; Dytrych, T.; Sargsyan, G

    Launey, K. D.; Dytrych, T.; Sargsyan, G. H.; Baker, R. B.; Draayer, J. P. Emergent symplectic symmetry in atomic nuclei: Ab initio symmetry-adapted no-core shell model.Eur. Phys. J. Special Topics2020,229, 2429

  40. [40]

    D.; Mercenne, A.; Dytrych, T

    Launey, K. D.; Mercenne, A.; Dytrych, T. Nuclear Dynamics and Reactions in the Ab Initio Symmetry- Adapted Framework.Annu. Rev. Nucl. Part. Sci.2021, 71, 253

  41. [41]

    Rosensteel, G.; Rowe, D. J. Nuclear Sp(3,R) Model. Phys. Rev. Lett.1977,38, 10

  42. [42]

    J.; On the algebraic formula- tion of collective models III

    Rosensteel, G.; Rowe, D. J.; On the algebraic formula- tion of collective models III. The symplectic shell model of collective motion.Ann. Phys. (NY)1980,126, 343

  43. [43]

    Rowe, D. J. Microscopic theory of the nuclear collective model.Rep. Prog. Phys.1985,48, 1419

  44. [44]

    P.; Barrett, B

    Navr´ atil, P.; Vary, J. P.; Barrett, B. R. Properties of 12C in the Ab Initio Nuclear Shell Model.Phys. Rev. Lett.2000,84, 5728

  45. [45]

    P.; Barrett, B

    Navr´ atil, P.; Vary, J. P.; Barrett, B. R. Large-basis ab initio no-core shell model and its application to 12C. Phys. Rev. C2000,62, 054311

  46. [46]

    Diagonaliza- tion of Hamiltonians for Many-Body Systems by Auxil- iary Field Quantum Monte Carlo Technique.Phys

    Honma, M.; Mizusaki, T.; Otsuka, T. Diagonaliza- tion of Hamiltonians for Many-Body Systems by Auxil- iary Field Quantum Monte Carlo Technique.Phys. Rev. Lett.1995,75, 1284

  47. [47]

    Nuclear Shell Model by the Quantum Monte Carlo Diagonalization Method.Phys

    Honma, M.; Mizusaki, T.; Otsuka, T. Nuclear Shell Model by the Quantum Monte Carlo Diagonalization Method.Phys. Rev. Lett.1996,77, 3315

  48. [48]

    Quantum Monte Carlo diagonalization with angular momentum projec- tion.Phys

    Mizusaki, T.; Honma, M.; Otsuka, T. Quantum Monte Carlo diagonalization with angular momentum projec- tion.Phys. Rev. C1996,53, 2786

  49. [49]

    Struc- ture of the N=Z=28 Closed Shell Studied by Monte Carlo Shell Model Calculation.Phys

    Otsuka, T.; Michio Honma, M.; Mizusaki, T. Struc- ture of the N=Z=28 Closed Shell Studied by Monte Carlo Shell Model Calculation.Phys. Rev. Lett.1998, 81, 1588

  50. [50]

    Monte Carlo shell model for atomic nuclei

    Otsuka, T.; Honma, M.; Mizusaki, T.; Shimizu, N.; Ut- suno, Y. Monte Carlo shell model for atomic nuclei. Prog. Part. Nucl. Phys.2001,47, 319

  51. [51]

    Transition from Spherical to Deformed Shapes of Nu- clei in the Monte Carlo Shell Model.Phys

    Shimizu, N.; Otsuka, T.; Mizusaki, T.; Honma, M. Transition from Spherical to Deformed Shapes of Nu- clei in the Monte Carlo Shell Model.Phys. Rev. Lett. 2001,86, 1171

  52. [52]

    Emerging concepts in nuclear structure based on the shell model.Physics2022,4, 258

    Otsuka, T. Emerging concepts in nuclear structure based on the shell model.Physics2022,4, 258

  53. [53]

    Prevailing triaxial shapes in atomic nuclei and a quantum theory of rotation of composite objects

    Otsuka, T.; Tsunoda, Y.; Shimizu, N.; Utsuno, Y.; Abe, T.; Ueno, H. Prevailing triaxial shapes in atomic nuclei and a quantum theory of rotation of composite objects. Eur. Phys. J. A2025,61, 126

  54. [54]

    Collective Nuclear States as Rep- resentations of a SU(6) GroupPhys

    Arima, A.; Iachello, F. Collective Nuclear States as Rep- resentations of a SU(6) GroupPhys. Rev. Lett.1975, 35, 1069

  55. [55]

    Interacting boson model of col- lective states I

    Arima, A.;Iachello, F. Interacting boson model of col- lective states I. The vibrational limit.Ann. Phys. (NY) 1976,99, 253

  56. [56]

    Interacting boson model of col- lective nuclear states II

    Arima, A.; Iachello, F. Interacting boson model of col- lective nuclear states II. The rotational limit.Ann. Phys. (NY)1978,111, 201

  57. [57]

    Interacting boson model of col- lective nuclear states IV

    Arima, A.; Iachello, F. Interacting boson model of col- lective nuclear states IV. The O(6) limit.Ann. Phys. (NY)1979,123, 468

  58. [58]

    Press: Cambridge, 1987

    Iachello, F.; Arima, A.The Interacting Boson Model; Cambridge U. Press: Cambridge, 1987

  59. [59]

    F.; Warner, D.D

    Casten, R. F.; Warner, D.D. The interacting boson ap- proximation.Rev. Mod. Phys.1988,60, 389

  60. [60]

    Press: Cambridge, 1991

    Iachello, F.; Van Isacker, P.The Interacting Boson- Fermion Model; Cambridge U. Press: Cambridge, 1991

  61. [61]

    F., ed.,Algebraic Approaches to Nuclear Structure: Interacting Boson and Fermion Models; Har- wood: Chur, 1993

    Casten, R. F., ed.,Algebraic Approaches to Nuclear Structure: Interacting Boson and Fermion Models; Har- wood: Chur, 1993

  62. [62]

    Frank, A.; Van Isacker, P.Symmetry Methods in Molecules and Nuclei; S y G Editores: Mexico, D.F., 2005

  63. [63]

    The program package PHINT for IBA cal- culations

    Scholten, O. The program package PHINT for IBA cal- culations. InComputational Nuclear Physics 1: Nuclear structure; Langanke, K.; Maruhn, J. A.; Koonin, S. E., Eds.; Springer: Berlin, 1991; p. 88

  64. [64]

    User’s Manual of the Pro- gram NPBOS.Japan Atomic Energy Research Institute, JAERI-M 85-094

    Otsuka, T.; Yoshida, N. User’s Manual of the Pro- gram NPBOS.Japan Atomic Energy Research Institute, JAERI-M 85-094

  65. [65]

    Casperson, R. J. IBAR: Interacting boson model calcu- lations for large system sizes.Comput. Phys. Commun. 2012,183, 1029. 25

  66. [66]

    Interacting bo- son model of collective nuclear states III

    Scholten, O.; Iachello, F.; Arima, A. Interacting bo- son model of collective nuclear states III. The transition from SU(5) to SU(3).Ann. Phys. (NY)1978;115, 325

  67. [67]

    H.; Gilmore, R.; Deans, S

    Feng, D. H.; Gilmore, R.; Deans, S. R. Phase transitions and the geometric properties of the interacting boson model.Phys. Rev. C1981,23, 1254

  68. [68]

    V.; Casten, R

    Iachello, F.; Zamfir, N. V.; Casten, R. F. Phase Coexis- tence in Transitional Nuclei and the Interacting-Boson Model.Phys. Rev. Lett.1998,81, 1191

  69. [69]

    F.; von Brentano, P.; Werner, V

    Jolie, J.; Casten, R. F.; von Brentano, P.; Werner, V. Quantum Phase Transition forγ-Soft Nuclei.Phys. Rev. Lett.2001,87, 162501

  70. [70]

    F.; Heinze, S.; Linne- mann, A.; Werner, V

    Jolie, J.; Cejnar, P.; Casten, R. F.; Heinze, S.; Linne- mann, A.; Werner, V. Triple Point of Nuclear Deforma- tions.Phys. Rev. Lett.2002,89, 182502

  71. [71]

    A triple point in nuclei.Nature2002,420, 614

    Warner, D. A triple point in nuclei.Nature2002,420, 614

  72. [72]

    K.; Mertz- imekis, T

    Bonatsos, D.; Martinou, A.; Peroulis, S. K.; Mertz- imekis, T. J.; Minkov, N. Prolate-oblate shape tran- sitions and O(6) symmetry in even–even nuclei: a the- oretical overviewPhys. Scr.2024,99, 062003

  73. [73]

    Dynamic Symmetries at the Critical Point

    Iachello, F. Dynamic Symmetries at the Critical Point. Phys. Rev. Lett.2000,85, 3580

  74. [74]

    Analytic Description of Critical Point Nu- clei in a Spherical-Axially Deformed Shape Phase Tran- sition.Phys

    Iachello, F. Analytic Description of Critical Point Nu- clei in a Spherical-Axially Deformed Shape Phase Tran- sition.Phys. Rev. Lett.2001,87, 052502

  75. [75]

    Casten, R. F. Shape phase transitions and critical-point phenomena in atomic nuclei.Nature Phys.2006,2, 811

  76. [76]

    F.; McCutchan, E

    Casten, R. F.; McCutchan, E. A. Quantum phase tran- sitions and structural evolution in nuclei.J. Phys. G: Nucl. Part. Phys.2007,34, R285

  77. [77]

    Casten, R. F. Quantum phase transitions and structural evolution in nuclei.Prog. Part. Nucl. Phys.2009,62, 183

  78. [78]

    Quantum phase transitions in the interacting boson model.Prog

    Cejnar, P.; Jolie, J. Quantum phase transitions in the interacting boson model.Prog. Part. Nucl. Phys.2009, 62, 210

  79. [79]

    Cejnar, P.; Jolie, J.; Casten, R. F. Quantum phase tran- sitions in the shapes of atomic nuclei.Rev. Mod. Phys. 2010,82, 2155

  80. [80]

    Nilsson, S. G. Binding states of individual nucleons in strongly deformed nuclei.Dan. Mat. Fys. Medd.1955, 29, no. 16

Showing first 80 references.