Open problems at the N=Z line P. Van Isacker, GANIL, France S3 opportunity for N=Z What’s so interesting about N=Z? Some selected topics SPIRAL2 week, Caen, November 2016 Nuclear regions covered by S3 What’s so interesting about N=Z? Superallowed 0+ -> 0+ β decay and precision tests of the standard model (unitarity CKM matrix). Charge symmetry and charge independence of the nuclear interaction (isospin symmetry). Extra binding energy due to enhanced correlation effects (e.g., Wigner energy). Neutron-proton pairing. D.D. Warner, M.A. Bentley & PVI, Nature Physics 2 (2006) 311 Superallowed 0+ -> 0+ β decay Conservation of vector current (CVC) hypothesis: 2π 3! 7 ln 2 / me5c 4 ft1/2 = = constant 2 2 GV M F Requires corrections: 2π 3! 7 ln 2 / me5c 4 Ft1/2 ≡ ft1/2 (1+ δR" ) (1+ δNS − δC ) = = constant 2 V 2GV (1+ Δ R ) Experiment gives t1/2, Q values & branching ratio. (Nuclear structure) theory gives δNS and δC. J.C. Hardy & I.S. Towner, Phys. Rev. C 91 (2015) 025501 Example: 74Rb Superallowed 0+ -> 0+ β decay SUPERALLOWED 0+ → 0+ NUCLEAR β DECAYS: A CRITICAL SURVEY WITH . . . 3090 74 PHYSICAL REVIEW Rb 3070 34 ft (s) Calculated Ar FIG. 4. Experimental function of the charge on Z. The bands represent th Ft/[(1 + δR′ )(1 − δC + δN distinguish those β em nuclei have isospin Tz = from those with Tz = 0 (l 22 Mg 38 Km 3050 34 Cl 42 10 C 14 46 V O 26 Al 3030 0 54 Sc 10 50 Mn Co m 20 30 40 Z of daughter J.C. Hardy & I.S. Towner, Phys. Rev. C 71 (2005) 055501 values. The method, which is illustrated in Fig. 4, is based on the validity of the CVC hypothesis that the corrected These new experiments can follow diff to improve the precision on the nine super J. C. HARDY AND I. S. TOWNER Error budget Frac. Uncertainty (%) have b the ex 0.04 have t is an of a th approa compl 0.02 A=2 precisi Of the unc the sta ` resolu V Exp R R C NS Never accept 2 FIG. 8. Uncertainty budget for |VJ.C. | as& obtained from ud Hardy I.S. Towner, Phys. Rev. Csuperal91 (2015) 025501 sum is + + lowed 0 → 0 β decay. The contributions are separated into four |Vud |. 51Fe 51Mn Experiment Shell Model 6 fp-shell Model Energy (MeV) Experiment Isospin symmetry 25 21 CED 17 2J 3 13 9 0 5 100 0 -100 CED (keV) The J=2 (0?) anomaly in 0f7/2 M.A. Bentley et al., Phys. Rev. C 92 (2015) 024310 Status of the anomaly Bentley, Lenzi et al.: a comprehensive analysis of mirror energy differences for A=42-54. Evidence for an nucleon-nucleon isovector term with a strong J dependence. The isospin symmetry breaking is not consistent with that found in the bare nn interaction and its J dependence differs from Coulomb. The anomaly is not understood. This calls for similar studies for higher A. Wigner binding energy Binding energy from Wigner supermultiplet theory: 2 ( N − Z ) + 6δpairing ( N, Z ) + 8 N − Z + 8δN,Z π np with δpairing(N,Z)=0, 1, 2 for even-even, odd-mass, odd-odd, and πnp=1 for odd-odd. Empirical expression for Wigner binding energy: BW ( N, Z ) = −W ( A) N − Z − d ( A) δ N,Z π np So, what’s the problem? E. Wigner, Phys. Rev. 51 (1937) 106 Pairing Pairing refers to the interaction between particles in ‘time-reversed orbits’. In nuclei: nucleons with orbital angular momenta coupled to L=0. Pairing is essential to understand the properties of nuclei. Analogous to the superconducting metallic state (BCS theory). Pairing with neutrons and protons For neutrons and protons two pairs and hence two pairing interactions are possible: 1S 0 3S 1 isovector or spin singlet (S=0,T=1) isoscalar or spin triplet (S=1,T=0) Nucleon-nucleon interaction ç Nucleon-nucleon interaction ç Nucleon-nucleon interaction ç Neutron-proton correlations The question is not whether T=0 interactions between nucleons exist or whether they are important. They do and they are. The question is whether T=0 correlations exist, similar to BCS-type ones for T=1. Test from two-nucleon transfer reactions. Related (but different) question: Are aligned T=0 neutron-proton pairs dominantly important? Test from magnetic & electric moments of N=Z nuclei. T=1 pair vibrations in Pb A. Bohr & B.R. Mottelson, Volume 2, page 646 T=0 pair vibrations in Ca-Sc-Ti-V? �� ������ �� �� �� �� �� �� �� �� �� �� � �� �+ �+ �+ �+ �σ/� | �+ 〉≈| �� ��〉 �+ �+ �σ | �+ 〉≈| �� ��〉 �+ �+ σ �+ | �+ 〉=| � 〉 Spin-aligned coupling scheme B. Cederwall et al., Nature 469 (2011) 68 Moments of isomers in 94Ag Quadrupole moment of 21+ isomer: 81949367824 2 3 Q ( b∞ 21) = (eν + eπ ) ( ho ) ≈ 0.44 b 3489855625 Quadrupole moment of 7+ isomer: 30930277300923364 2 3 Q ( b [16 ] 7) = (eν + eπ ) ( ho ) ≈ 0.64 b 627253477610841 ∴ Measurement of quadrupole moments tests spin-aligned scheme. Conclusions Superallowed 0+ -> 0+ β decay: mirror transitions constrain the nuclear-structure corrections. The J=2 (0?) anomaly remains unresolved and calls for experiments at higher A. A BCS-like phase for T=0 pairing? Test from deuteron transfer. Dominance of T=0 aligned pairs? Test from magnetic and quadrupole moments. T=1 pair vibrations rm produces a spectrum s. any) collective correlations for T = 0 pairing. In fact, this small lowering of the energy of the T = 0 state with respect to the single-particle excitation, can be accounted for by a residual np diagonal56 interaction, ∼ 20MeV/A, rather than any collective effect. Pair vibrations on E x (MeV) 60 Pb isotopes 4.5 Zn T=1 Isoscalar 58 Cu Phonon T=0 60Zn T=0 3.0 58Zn 58 1.5 (1,0,0) 212 Aon spectrum for addition b. The excitation energies Pb isotopes derived from 60 Cu -1 T=1 Ni Ni T=1 (0,0,1) (0,1,0) 56 0 (0,1,1) 58 Cu T=1 60Cu T=2 (1,0,1) T=2 (0,2,0) T=1 208 210 Ni hω + hω 0 1 hω0 60Ni T=2 (0,0,2) Isovector Phonon 2hω 1 hω 1 T=0 0 1 T 2 A.O. Macchiavelli et al., arXiv:nucl-th/9912041 Pair vibrations & rotations Pairing hamiltonian for several shells. For two shells and identical nucleons: Ĥ ( Δε, g) = Δε ( n̂+ − n̂− ) − gV̂J=0,T =1 Phase transition occurs as a function of g/Δε: For g<gcrit: pair vibrations (ex: Pb isotopes) For g>gcrit: pair rotations (ex: Sn isotopes) Two different coupling schemes: $ U 1 ×U 1 +( ) −( ) & SU + ( 2 ) × SU − ( 2 ) ⊃ & SU ( 2 ) % ' )⊃ U 1 () ) ( Pair vibrations and rotations Pair correlations result in a constructive interference of reaction amplitudes giving a enhanced two-nucleon transfer. σ ( Αgs→ Α+2gs)/σsp Superfluids ∼ (Δ/G)2 ∼ Ω2 Vibrations ~ (n +1 ) ∼ Ω Single Particle Ao Closed shell Closed shell A.O. Macchiavelli T=1 pair vibrations in Ca T=1 pair vibrations in Ca-Sc-Ti-V? �� ������ �� �� �� �� �� �� �� �� �� �� � �� �+ �σ/� | �+ 〉≈| �� ��〉 �+ �σ �+ σ �+ | �+ 〉=| � 〉 | �+ 〉≈| �� ��〉 T=0 pair vibrations in Ca-Sc-Ti-V? �� ������ �� �� �� �� �� �� �� �� �� �� � �� �+ �+ �+ �+ �σ/� | �+ 〉≈| �� ��〉 �+ �+ �σ | �+ 〉≈| �� ��〉 �+ �+ σ �+ | �+ 〉=| � 〉 T=0 aligned pairs in Ca-Sc-Ti-V? �� ������ �� �� �� �� �� �� �� �� �� �� � �� �+ �+ �+ �+ ��σ/�� | �+ 〉≈| �� ��〉 �+ �σ | �+ 〉≈| �� ��〉 �+ �+ σ �+ | �+ 〉=| � 〉 A new coupling scheme? Our results reveal evidence for a spin-aligned, isoscalar neutron–proton coupling scheme. [T]his coupling scheme replaces normal superfluidity (characterized by seniority coupling) in the ground and low-lying excited states of the heaviest N=Z nuclei. B. Cederwall et al., Nature 469 (2011) 68 Spectrum of 94Ag Expt SM ! 21 18!! 21! 19 Energy #MeV$ 16! 17! 5 14!! 15 12!! 13 7! 0 2! ! 10! 11 4!! 6! 5! 9! 8! 3! 1! 7 B3 ! 18 21!! 19! 16 17! b3 !2" 18!! 21! 19! 16 17! b3 !3"! 18 21!! 19! 16 17! 14!! 15 1! 4!! 3 ! 12! 13 14!! 15 1! 4!! 3 ! 12! 13 6!! 5 ! 11! 10 6!! 5 ! 11! 10 6!! 5 ! 11! 10 9!! 8 7! 9! 8! 9!! 8 7! 14!! 15 1! 94 47 Ag 47 7! 4!! 3 ! 12! 13 B-pair analysis of 1.0 0.5 0.0 94Ag 0 13 10 24 19 28 24 30 22 27 19 20 14 14 8 0 1 0 2 1 2 2 3 2 3 2 2 2 2 1 !J1 B3 ; J" 2 9 2 4 1 4 1 2 1 2 1 0 0 1 1 94 47Ag47 0 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 J Magnetic dipole moments For any state in a single-j shell " 0.52 to 0.55 1 f ( 7/2 ) $ 1 g (α J ) = ( gν + gπ ) ≈ # 2 $% 0.51 to 0.54 (1g9/2 ) The same result is obtained with b-IBM mapped from a single-j shell model. ∴ Magnetic dipole moments test approximation (A) but are insensitive to (B) and (C). In 46V: µ (3+ ) = 1.64(3) µ N In 50Mn: µ ( 5+ ) = 2.76(1) µ N 1 1 F.C. Charlwood et al., Phys. Lett. B 690 (2010) 346 Q moment of 21+ isomer in 94Ag Shell model in pf5/2g9/2 space (M=21 -> dim=2): + Q 21 ( 1 ) = 0.44 b Shell model in 1g9/2 (J=21 -> dim=1): 196 2 Q ( 211+ ) = e + e ( ν π ) ( ho ) ≈ 0.42 b 9 Expression in terms of b bosons: 81949367824 2 Q ( b 21) = (eν + eπ ) ( ho ) ≈ 0.44 b 3489855625 3 ∞ ∴ Measurement of Q(21+) tests (A). Calculation confirms (B+C). A. Poves, private communication LSSM Q moment of 7+ isomer in 94Ag Shell model in pf5/2g9/2 space (M=7 -> dim=37327): + Q 7 ( 1 ) = 0.62 b Shell model in 1g9/2 (J=7 -> dim=84): Q ( 71+ ) = 6.60 (eν + eπ ) ( ho )2 ≈ 0.60 b Expression in terms of b bosons: 30930277300923364 2 Q ( b [16 ] 7) = (eν + eπ ) ( ho ) ≈ 0.64 b 627253477610841 3 ∴ Measurement of Q(7+) tests (A). Calculation confirms (B+C). A. Poves, private communication LSSM
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