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E0 transitions: where we have been, where we are going,
where we would like to go
John L. Wood
School of Physics
Georgia Institute of Technology
E0: transition operator and matrix element--a model independent description
E0 transition strengths are a measure of theoff-diagonal matrix elements of themean-square charge radius operator.
Mixing of configurations with different mean-square charge radii producesE0 transition strength.
Ω values: http://bricc.anu.edu.au
τ: partial lifetime for E0 decay branch
J. Kantele et al. Z. Phys. A289 157 1979and seeJLW et al. Nucl. Phys. A651 323 1999
Comments on model-motivated research
• Research should be pursued to falsify models, not to promote them
• When a model fails, we have learned something—recall that failure of the Standard Model of particles and fields is being sought, avidly
• Models provide powerful schemes for organizing data
Wave functions must overlap for a transition to occur
Figure from JLW et al.,Nucl. Phys. A651 323 1999
solid line—schematic potential
dashed line—schematic wave function
In the earlier literature there are some serious misconceptions onthis point
E0 transition between states with very different deformations and mean-square charge radii
6.6 x 10-7
B(E1) W.u.
B(E2) W.u.
ρ2(E0) x 103
238 U
J. Kantele et al., Phys. Rev. Lett. 51, 91 (1983)
Figure from JLW et al.,Nucl. Phys. A651 323 1999
The E0 strength from the238U “fission” isomer isthe weakest known
T. Kibédi and R.H. Spear, ADNDT 89 77 2005
E0 transitions in the light Ni isotopes:the 02 01 strength in 58Ni is very small indicating near-pure neutron
configurations are involved (en = 0)
6.3 x 10-3
8030
1 < < 27
784266
> 0.43
T. Kibédi and R.H. Spear, ADNDT 89 77 2005
Figure from JLW et al.,Nucl. Phys. A651 323 1999
π2p-2h from 2-, 4-proton transfer RX
ρ2(E0) 103
E0 transitions associated with shape coexistence in 114-120Sn
.
0+
2+
0+
0+
2+
4+
1953
2240
2614
1:93
1300
2610
2156
0
4+
2530
2+
0+
0+
2+
0+ 0+ 0+
2+
0+
2+
4+
0+
4+
2+
0+
0+
2+
2113
1757
2027
1294
0
2489
2043
1758
2056
1230
0
2644
2097
1875
2160
1171
0
4.38 3.76 2.47
0.8718 >0.48
8719
1:100 1:75 1:37
J. Kantele et al., ZP A289, 157 (1979) T. Kibedi and R.H. Spear, ADNDT 89, 277 (2005)
114Sn 116Sn 118Sn 120Sn
ρ2(E0) 103
>36
Mixing of close lying configurations with different mean-square charge radii produces E0 strength
E2 transitions associated with shape coexistence in 114-120Sn
.
0+
2+
0+
0+
2+
4+
1953
2240
2614
1300
153
2156
0
4+
2530
2+
0+
0+
2+
0+ 0+ 0+
2+
0+
2+
4+
0+
4+
2+
0+
0+
2+
2113
1757
2027
1294
0
2489
2043
1758
2056
1230
0
2644
2097
1875
2160
1171
0
228
13030
12.44 12.15 11.42
445
397 5620
183 193 12.617
114Sn 116Sn 118Sn 120Sn
B(E2) W.u. Data from ENSDF
150
100
50
0
0 400 800 1200 1600
B(E
2)
(W.u
.)
E (keV)
Systematics of B(E2; 0+2 2+
1) vs. E (0+2 – 2+
1)
0+2 2+
1
2+1
0+1
0+2
strong
weak
B(E2; 02+ 21
+) vs. E(02+) – E(21
+): coexistence and mixing yields B(E2; 02
+21
+) ~ α2 β2 (ΔQ)2
Recall:B02 = 5 x B20
Deformed bands in 112-120Sn built on the first excited 0+ states
Figure from Rowe & Wood B(E2)’s in W.u. [100 = rel. value]
The nature of the shape coexisting state in 116Sn revealed by (3He,n) transfer reaction spectroscopy
Spectrum taken from H.W.Fielding et al., NP A281, 389 (1977)
Excited 0+ states at closed shells: intruder states in the Pb and Sn isotopes
neutron numbermid shell mid shell
green—yrast statesred—non-yrast states
Coexistence in even-Pb isotopes: multiple parabolas and spherical (seniority) structure
Figure: Heyde & Wood Heavy arrows indicate E0+M1+E2 transitions188Pb: G.D. Dracoulis et al., PR C67 R 051301 2003
Coexistence in the odd-Pb isotopes:Data for E0 transitions are from:J.C. Griffin et al., NP A530 (1991) 401—195Pb (UNISOR / LISOL);J. Vanhorenbeeck et al., NP A531 (1991) 63—197Pb (LISOL);K. Van de Vel et al., PR C65, 064301 (2002)—189,191Pb (KUL @ JYFL)
spin sequence in 195,197Pbimplies oblate deformation
Heavy downward vertical arrows indicate E0+M1+E2 transitions
Diagonal arrows indicateα-decay strength (from Po)
Shape coexistence in the even-Hg isotopes: NOTE characteristic parabolic energy trend
80Hgmid-shell
Figure from J. Elseviers et al.PR C84 034307 2011
Conversion electron spectroscopy:uniquely sensitive to E0 transitions, identifies shape coexistence
E0 E0 +
M1
+ E
2
E0 +
M1
+ E
2
E0 +
…
M.O. Kortelahti et al.,PR C43 484 1991 UNISOR
E0 transitions: αK > αK(M1)
M.O. Kortelahti et al., PR C43 484 1991
190Hg
21+-01
+ 41+-21
+ 61+-41
+
0+ 0+ decays are pure E0: no γ’s (190Hg)
M.O. Kortelahti et al. PR C43 484 1991 1279 keV pure E0evidence
The ground states of 178-186Pt and 177-187Ptare intruder states
Figure from: JLW et al.,Phys. Repts. 215, 101 (1992)
mid shellN = 104 See P.M. Davidson et al.,
NP A657 219 1999 (ANU)
Coexistence in the odd-Pt isotopesChapter 2. Background 19
Figur e 2.4: Systemat ics of yrast states in A = 168− 194 Pt isotopes as a funct ion of
the neutron number N . The even-A isotopes (open symbols) are plot ted with respect
to the 0+ ground state. Posit ive-signature states of odd-A isotopes (filled symbols) are
plot ted taking the 13/ 2+ state as a reference. Vert ical dashed lines highlight N = 95, 97
of 173,175Pt , respect ively. Around the neutron mid shell (N = 104) the excitat ion
energies of these yrast states have a pronounced staggering between the odd-A and
even-A nuclei. When moving away from the neut ron mid shell, the mot ion of the odd
neut ron is seen to become weakly coupled to the core deformat ion. This is seen from
the similarity of the excitat ion energy between even and odd-A Pt isotopes at N 97
and N ≥ 109. Data are taken from [Pii75, Jan88, Bes76, Nyb90, Bur67, De Voigt90,
Bag09, Dra86, Dra90, Dra91, Ced98, Jos05, GH09].
P. Peura, Ph.D. thesis, JYFL 2014mid shellN = 104
Coexistence in the even-Pt isotopes:mixing and E0 transition strength
From: J. von Schwarzenberg,PhD thesis, Ga Tech 1991
E (sph.gs) = 0
E (gs) = 0
ρ2(E0)
V = 50, 100, 400 keV
Coexistence in the even-Pt isotopes:coexistence of K = 0 and K = 2 bands in 184Pt
Y. Xu et al. PRL 68 3853 1992 UNISOR
E2 / M1 from low-temperaturenuclear orientation on-line
Coexistence in the even-Pt isotopes:K = 0 and K = 2 bands
Y. Xu et al. PRL 68 3853 1992 UNISOR
★
★
★
★
M1 + E2
Pure E0’s in an odd-mass nucleus
J. von Schwarzenberg et al., PR C45 R896 1992 UNISOR
185Au 185Pt
Isotope shifts: Pt, Au, Hg, Tl, Pb, Bi, Po, At
From: Barzakh INPC 2013
International Nuclear Physics Conference INPC2013: 2-7 June 2013, Firenze, Italy
Shape coexistence and charge radii in thallium, gold and astatine
isotopes studied by in-source laser spectroscopy at RILIS-ISOLDE
A. Barzakh
Petersburg Nuclear Physics Institute (PNPI), NRC Kurchatov Institute, 188300 Gatchina, Russia
On behalf of York-KU Leuven-Gatchina-Mainz-Bratislava-Liverpool-ISOLDE collaboration
Contact email: [email protected]
The competition between spherical and deformed nuclear shapes at low energy gives rise to
shape coexistence in the region of the neutron-deficient lead isotopes with Z~82 and N~104 [1]. In
order to determine to which extent the ground and/or isomeric states of those and neighboring nu-
clides are affected by this phenomenon, a campaign of investigation of changes in the mean-square
charge radii and electromagnetic moments is on-going at ISOLDE. By combining the high sensitiv-
ity of the in-source laser spectroscopy technique, ISOLDE mass separation and Windmill alpha-
decay spectroscopy setup [2], it has been possible to study long isotopic chains of lead [3] and po-
lonium [4], down to N=100 and N=107 respectively, and, recently, thallium isotopic chain down to
N=98.
In this contribution, we present the the preliminary results of the charge radii,
electromagnetic moments and spins measurements in thallium, gold and astatine isotopes. In the
gold and astatine cases, next to Faraday cup and Windmill measurements, also the Multi-Reflection
Time-of-Flight (MR-ToF) mass separation technique [5] involving the ISOLTRAP collaboration
was used.
100 105 110 115 120 125 130 135
-2.5
-2.0
-1.5
-1.0
-0.5
0.0
0.5
1.0
1.5
2.0
2.5
3.0
177Au
179Tl
182Pb
197At
85At
78Pt
191Po
82Pb
N=133,
octu
po
le d
efo
rma
tio
n
N=104,
sh
ap
e c
oe
xis
ten
ce
84Po
83Bi
81Tl
80Hg
d<
r2>
N, N
0
Neutron number
79Au
N=126,
sh
ell
eff
ect
Figure 1: Charge radii for Pt-At isotopes. For the sake of clarity the data for different elements are
shifted relative to each other by a vertical off-set. Tl data for the light isotopes are from ISOLDE [5]
and Gatchina. Preliminary data for gold and astatine chains are from [6].
[1] K. Heyde and J. Wood. Rev. Mod. Phys., 83, 1467 (2011);
[2] A.N. Andreyev et al., Phys. Rev. Lett., 105, 252502,(2010);
[3] H. De Witte et al., Phys. Rev. Lett., 98, 112502 (2007);
[4] T.E. Cocolios et al., Phys. Rev. Lett., 106, 052503 (2011);
[5] R.N. Wolf et al., Nucl. Instr. and Meth. A 686, 82-90 (2012).
(fm
2)
Odd-mass Au systematics showingthe h9/2 intruder state
Figure from: M.O. Kortelahti et al., JP G14 1361 (1988)
E0 transitions between “single”and “double” intruder states in 185Au
9/2- state @ 9 keV: “double” intruder state:πh9/2 (1p) × 184Pt [π(2p-6h)] = π(3p-6h)
9/2- state @ 322 keV: “single” intruder state:πh9/2 (1p) × 184Pt [π(4h)] = π(1p-4h)
C.D. Papanicolopulos PhDthesis Ga Tech 1987 andZP A330 371 1988 UNISOR
Z = 79 427 keVmult αK
E1 0.010E2 0.027M1 0.11
expt. 0.33
E0 transitions between “spherical” states and “core” intruder states in 185Au
11/2- state @ 220 keV: “spherical” state:πh11/2 (1h) × 186Hg [π(2h)] = π(3h)
11/2- state @ 712 keV: “core” intruder state:πh11/2 (1h) × 186Hg [π(2p-4h)] = π(2p-5h)
C.D. PapanicolopulosPhD thesis Ga Tech 1987ZP A330 371 1988UNISOR
Z = 79 492 keVmult αK
E1 0.007E2 0.020M1 0.073
expt. 0.21
E0 transitions between “single”and “double” intruder states in 187Au
D. Rupnik et al. PR C51 R2867 1995 UNISOR
E2
E0 transitions between “single”and “double” intruder states in 187Au
D. Rupnik et al. PR C51 R2867 1995 UNISOR
WHEN STUDYING THE QUANTUM MECHANICAL MANY-BODY PROBEM, ALWAYS BE MINDFUL OF:
• "We are to admit no more causes of natural things than such as are both true and sufficient to explain their appearances.
Therefore, to the same natural effects we must, so far as
possible, assign the same causes.”--Isaac Newton
(From William of Ockham [near Guildford, UK], ca. 1320)
• “Everything should be made as simple as possible,
but not simpler.”-- Albert Einstein
Systematics of 02+ states in Zr isotopes, 50 ≤ N ≤ 62:
electric monopole transition strengths
0+ 0+ 0+ 0+ 0+ 0+
0+
0+
21+
0+
0+
0+
0+
0+
0+
3.5
8.0
7.6
11.2
90 92 94 96 98 100 102
0
1
2
E(MeV)
108
ρ2(E0)103
02+ is first excited state
in only 15 known nuclei:3 are here
large ρ2(E0)103 indicatescoexistence and strongmixing
Data are taken from T. Kibédi and R.H. Spear, ADNDT 89, 77 (2005)
11.5
Systematic of 21+ states in Zr isotopes, 50 ≤ N ≤ 62:
electric quadrupole transition strengths
0+ 0+ 0+ 0+ 0+ 0+
02+
0+
2+
2+ 2+
2+
2+
2+2+
5.4
6.4
2.3
>0.04
75 105
4.9
B(E2) W.u.
largest known change in 21
+ propertieson mass surface
90 92 94 96 98 100 102
0
1
2
E(MeV)
Ground-state properties are a direct signature of shell and deformation structures
R&W Fig. 1.41
R&W Fig. 1.42
Differences in mean-square charge radii (isotope shifts)determined by:
optical hyperfine spectroscopy using lasers
Two-neutron separation energies deduced from nuclear masses determined by:
direct mass measurements
21+ state properties are a strong signature of
shell and deformed structures
R&W Fig. 1.39
R&W Fig. 1.40
Energies of 21+ states determined by:
gamma-ray spectroscopy following β decayproblem—β-decaying parent is further from stability and yield will be (much)
lower than nucleus of interest
gamma-ray spectroscopy following Coulomb excitation
Reduced E2 transition rates, B(E2) from 21+ states
determined by:lifetime measurements using fast β-γ timing following β decay
problem--see above
gamma-ray yields following Coulomb excitation
Excited 0+ states at closed shells--mixing and repulsion of pair configurations in 90Zr
p1/22
0+
g9/22
0+
+0 0
1761
+0N=50: g9/2 seniority structure
j = ½ orbitals can only contributeto v = 0 states, at low energy
90Zr E(21+) is high: suggests a closed
subshell, BUT is due to depressionof the ground-state energy
Figure from Heyde & Wood
Shape coexistence at and near closed subshells: the nuclei 96Sr and 98Zr
Figure from K. Heyde and J.L. Wood, Rev. Mod. Phys. 83, 1467 (2011)
E0 transitions: ρ2(E0)103 values
are shown
96Sr5898Zr58
G. Lhersonneau et al., PR C49, 1379 (1994)
C.Y. Wu et al.,PR C70, 064312
(2004)
G. Lhersonneau et al., PR C49, 1379 (1994)
C.Y. Wu et al.,PR C70, 064312 (2004)
ρ2(E0)103 = 21031
in 96Sr is largest known for A > 56
21076
61
11
Deformation in Zr isotopes, 50 ≤ N ≤ 62
0+ 0+ 0+ 0+ 0+ 0+
0+
0+
0+
0+
0+
0+
0+
0+
90 92 94 96 98 100 102
0
1
2
E(MeV)
2+
4+
deformedbands
0+
2+
4+
2+
4+
2+
4+
94Zr—A. Chakraborty et al.PRL 110 022504 2013
A deformed structure can intrude to become a ground state:
appears to produce a “collective phase change”
Proton particle-hole excitations across the Z = 64 gap may be the source of the coexisting shapes.
There is no a priori way to determine the nature of the unmixed configurations or the strength of the mixing.
En
erg
y
N90 92 9484 86 88
2+
0+
“p(2h)”
“p(2p-4h)”
2+
0+
2+
0+
normal
collectivity
suppressed
collectivity
N=90
2+
0+
2+
0+
mixedunmixed
E0
2+
2+
Less-deformed 2h and more-deformed 2p-4h structures coexist at low energy at N=90.
Strong mixing obscures the energy differences that are indicative of different shapes.
Strong E0 transitions are a key signature of the mixing of coexisting structures.
As observed, the K=2 bands will also mix strongly, resulting in E0 transitions.
24
Nuclei are manifestations of coexisting structuresthat may invert by addition of a few nucleons, and may mix.
52 54 56 58 60 62
N=58
Proton pair excitations with respect to the Z = 40 subshell
π(2p-2h)
π(0p-0h)
Ground state properties, S2n and δ<r2>, in the regions of N = 60, 90 are very similar
Figure from Heyde & WoodFigure from S. Naimi et al. Phys. Rev. Lett. 105 032502 (2010)
Shape coexistence in the N = 90 isotones:revealed by E0 transition strengths
Strong mixing of coexisting shapes produces strong electric monopole (E0) transitions and identical bands.
E0 strength is a function of mixing.
0 2 4 6 8
I(I+1)
En
erg
y
2
1
0
E(MeV)
Sm9062
152Gd
9064154
Dy9066
156
0+
2+
4+
6+
8+
10+
0+
4+
2+
6+
0+
2+
4+
6+
8+
10+
0+
2+
4+
6+
8+
10+
0+
2+
4+
6+
8+
10+
0+
2+
4+
6+
8+
10+
0+
2+
4+
6+
8+
10+
8917
749
8814
696
239
0.74
515
0+
2+
4+
1:9
r2•103
707
4214
7520
6310
6815
ρ2 ·103 = α2β2 ∆ r2 2·103 Z2
R40
≈ 356α2β2,
R0 = 1.2A1/3 fm
∆ r2 = 0.39fm2
ρ2 ·103 = α2β2 ∆ r2 2·103 Z2
R40
R0 = 1.2A1/3 fm
1
Thursday, 9 July 2009
Note: mixing produces “identical bands”
Data from Heyde and Wood (2011)
Mixing of coexisting structures in 152Sm
0.75690.70710.64330.57700.5334J
0.65360.70710.76560.81670.8458J
86420J
0+ 0
2+ 159
4+ 454
6+ 840
8+ 1290
0+ 296
2+ 378
4+ 563
6+ 840
8+ 1199
unmixed mixedV = 310 keV
4+
6+
8+
0+ 0
2+ 136
389
726
1127
8+ 1754
6+ 1346
0+ 687
2+ 793
4+ 1019
experimen
t
2+
0+
4+
6+
8+
685
810
1023
1311
1666
4+
6+
8+
366
706
1125
2+
0+ 0
122
(from Eu)
51570.8
69677.3
881484.4
87.0
85.2
exptcalc
148Ce 154Sm
Mixing of coexisting structures in 154Gd
0.53270.56860.61760.67020.7071J
0.84630.82260.78650.74220.7071J
86420J
0+ 0
2+ 159
4+ 454
6+ 840
8+ 1290
0+ 0
2+ 89
4+ 288
6+ 585
8+ 965
unmixed mixedV = 340 keV
4+
6+
8+
0+ 0
2+ 122
361
690
1091
8+ 1844
6+ 1416
0+ 680
2+ 806
4+ 1061
experimen
t
2+
0+
4+
6+
8+
681
815
1048
1366
1756
4+
6+
8+
371
718
1144
2+
0+ 0
123
(from Eu)
891791.0
74990.1
70785.9
79.6
74.0
exptcalc
148Ce 156Gd
152Sm: B(E2) values
Grodzins’ rule for quadrupole strength
Rotor matrix elements
e.g.,
*Grodzins +8%
Multi-Coulex of 152Sm 02+(685 keV):
strongest response is to head of K=2+ band at 1769 keV(in-band response attenuated by 99.7% decay out @ 811 level)
The strongest response is from the band head of the
K=2+ structure at 1769 keV.
1084122
126
356
288
446
100
200
300
400
288
212
356
414
446
2+ 122
4+ 366
6+ 707
8+ 1125
10+ 1609
12+ 2149
14+ 2736
0+ 0
2+ 811
4+ 1023
6+ 1311
8+ 1666
10+ 2058
12+ 2526
0+ 685
2+ 1293
4+ 1613
6+ 2004
0+ 1083
2+ 1944
0+ 1755
2+ 1086
4+ 1371
6+ 1728
8+ 2140
10+ 2662
9+ 2376
3+ 1234
7+ 1946
5+ 1559
2+ 1769
4+ 2052
6+ 2417
3+ 1907
7+ 2623
5+ 2237
563
1084
414
200 600 1000 1400 E (keV)
Co
un
ts/c
ha
nn
el W.D. Kulp et al., Phys. Rev. C77 061301 2008152Sm
Gammasphere + CHICO@ 88” (Berkeley)
Multi-Coulex:152Sm beam + 208Pb target
1084
1084
563gate
Shape coexistence in the N = 90 isotones:coexisting K = 2 bands revealed by E0 transitions
Kulp, Wood, Garrett, Zganjar and others
E (MeV)
3+, K = 2 3+, K = 2: 631 keV transition in 158Er has no observable γ-ray strength, only ce’s[ 3K2 – I(I+1) = 0 ] are observed --accidental cancellation of E2; M1 is very weak.
152Sm: W.D. Kulp et al., Phys. Rev. C77 061301 2008
cf. 184Pt
Multistep Coulomb excitation of 74,76Kr using radioactive beams of Kr on a 208Pb target
76Kr
74Kr 74Kr 76Kr
E. Clément et al.,PR C75 054313 2007
Quadrupole shape invariants constructed from E2 matrix elements for 74,76Kr
for the ground state
E. Clément et al.,PR C75 054313 2007
CONCLUSIONS: E0 TRANSITIONS
1). They give a unique perspective on shape coexistencein nuclei
2). They probe the proton and neutron configurations thatoccur in nuclei
3). They probe K quantum numbers through their ΔK = 0selection rule
We need more data for:T1/2(0+) [and T1/2(2+), T1/2(4+), T1/2(3+)] conversion electron intensitiesE2 / M1 mixing ratios—to extract E2 + M1 + E0
Electric monopole transition strengths: critical test of phase transition models
P. von Brentano et al., PRL 93, 152502 (2004)
Shape coexistence in the Hg and Cd isotopes
midshell midshellneutron number
E(M
eV)
--02+
-- intruder 0+,2+,4+,6+Z=48Z=80
Shape coexistence in the Cd isotopes
Fielding NP A281 389 1977
108Pd(3He,n)110Cd
110Pd(3He,n)112Cd
Pd targets π(4h)
The spectroscopy of mixing in the Cd isotopes:ρ2 (E0) values in 114Cd
0
1
2
E(MeV)114Cd
ρ2(E0)103
ΔK=0τ(n,n’γ ) fs: >500
>800
0.655
1.8313
192
438
891
2
0+
2+ 558
0
1284
4+0+ 1306
0+ 1135
2+
1364
4+ 17320+
2+
2+
other
2+
1210
3+
4+
1864
19322+ 184
2
4+ 2152
3+ 2205
12020
<130<120
STRONG
Conv. Elec. ILL BILL/GAMSMheemeed NP A412 113 1984
Lifetimes n,n’γ Doppler U. KentuckyBandyopadhyay PR C76 054308 2007
Shape%coexistence%in%the%N%=%90%isotones:%%revealed%by%E0%transi6on%strengths%
Strong mixing of coexisting shapes produces strong electric monopole (E0) transitions and identical bands.
E0 strength is a function of mixing.
0 2 4 6 8
I(I+1)
En
erg
y
2
1
0
E(MeV)
Sm9062
152Gd
9064
154Dy
9066
156
0+
2+
4+
6+
8+
10+
0+
4+
2+
6+
0+
2+
4+
6+
8+
10+
0+
2+
4+
6+
8+
10+
0+
2+
4+
6+
8+
10+
0+
2+
4+
6+
8+
10+
0+
2+
4+
6+
8+
10+
8917
749
8814
696
239
0.74
515
0+
2+
4+
1:9
r2•103
707
4214
7520
6310
6815
ρ2 ·103 = α2β2 ∆ r2 2·103 Z2
R40
≈ 356α2β2,
R0 = 1.2A1/ 3 fm
∆ r2 = 0.39fm2
ρ2 ·103 = α2β2 ∆ r2 2·103 Z2
R40
R0 = 1.2A1/3 fm
1
Thursday, 9 July 2009
Note:%mixing%produces%“iden6cal%bands”%
Data%from%Heyde%and%Wood%(2011)%
Based on a figure in WoodNP A651 323 1999
E0 transition strengths in 114Cd support the existence of good K quantum numbers
STRONG Δ K=2 E0 Δ K=2 MIXING
0
1
2
E(MeV)114Cd
ρ2(E0)103
ΔK=2τ(n,n’γ ) fs: >500>450
Bke: 0.00003640
0+
2+ 558
0
1284
4+0+ 1306
0+ 1135
2+
1364
4+ 17320+
2+
2+
other
255
2+
1210
3+
4+
1864
19322+ 184
2
4+ 2152
3+ 2205
2020
<0.1 nil
nil
<1.5 nil
nil
<300
WEAK
Spectroscopy of mixing in the Cd isotopes:ρ2 (E0)103 values in 114Cd
0
1
2
E(MeV)114Cdρ2(E0)103
0.655
1.8313
192
438
891
2
0+
2+ 558
0
1284
4+0+ 1306
0+ 1135
2+
1364
4+ 1732
2+
1210
3+
4+
1864
19322+ 184
2
4+ 2152
3+ 2205
12020
<130<120
Conv. Elec. ILL BILL/GAMS Mheemeed NP A412 113 1984
Lifetimesn,n’γ Doppler U. Kentucky Bandyopadhyay PR C76 054308 2007Coulex yield multiple ions Fahlander NP A485 327 1988p-e(t) (d,pe) Julin ZP A296 315 1980Coulex yield 16-O Julin thesis Univ. Jyvaskyla 1979
255
NOTE:despite the proximity of these two 2+ states, the ρ2 (E0) value is not large
ρJ J2 (E0) 103 ~ 400 αJ
2 βJ2
ρ2(E0)103 max ~ 100 (obs.)
Δ<r2 > ~ 0.45 fm2 [2nd est.]
β0 / α0 ~ 0.23
Spectroscopy of mixing in the Cd isotopes:116Cd (p,t) 114Cd and ρ2 (E0) 103
Fortune PR C35 2318 1987
VJ=0 330 keV
β0 / α0 0.28
ρ0 02 (E0) 103 = 19 = 482 [Δ<r2 >]2 103 [0.28 x 0.96]2
[1.2 x 1141/3]4
ρJ J2 (E0) 103 ~ 300 αJ
2 βJ2
Δ<r2 > ~ 0.4 fm2 [first estimate]
. 02+
01+ 01
+
114Cd 116Cd(p,t)
σpt(02+)
σpt(01+)
0def+
0sph+
Ed
Es
02+
01+
1135
0
~
~
114Cd(expt)
ρ0 02 (E0) ~ [Δ<r2 >]2 α0
2 β02
Δ<r2 > = <r2 >def - <r2 >sph [unknown] E0
Wood et al.NP A651 323 1999
α02 + β0
2 = 1
98Sr6038
100Zr6040
102Mo6042
104Ru6044
Systematics of low-lying collective states in N=60 isotones
0+ 0 0+ 0 0+ 0 0+ 0
2+ 144
4+ 434
6+ 867
8+ 1432
0+ 215
2+ 871
2+ 212
4+ 564
6+ 1063
8+ 1687
0+ 829
2+ 878
4+ 1415
6+ 1856
0+ 331
2+ 1196
2+ 297
4+ 744
6+ 1328
8+ 2019
0+ 1334
2+ 1250
0+ 698
3+ 1246
4+ 1398
2+ 848
6+ 2009
2+ 358
4+ 889
6+ 1556
0+ 1335
2+ 1515
0+ 988
3+ 1242
4+ 1502
2+ 893
5+ 1872
4+ 2081
6+ 2196
8+ 2320
96
127
57515 82
101
67
10819 74
89 7030
12050
60
81 25
36
23
B(E2) W.u.
2(E0)•103
Spectroscopy of mixing in the Cd isotopes:ρ2 (E0)103 values in 114Cd
0
1
2
E(MeV)114Cdρ2(E0)103
0.655
1.8313
192
438
891
2
0+
2+ 558
0
1284
4+0+ 1306
0+ 1135
2+
1364
4+ 1732
2+
1210
3+
4+
1864
19322+ 184
2
4+ 2152
3+ 2205
12020
<130<120
255
αJ2 βJ
2
0102 0.95 0.052123 0.88 0.124142 0.67 0.332224 0.50 0.502223 0.93 0.07mixing is 2-state
αJ2 βJ
2
0102 0.99 0.012123 0.97 0.024142 0.94 0.052224 0.87 0.042223 0.87 0.09
Garrett, Green, Wood PR C78 044307 2008To fit B(E2)’s
IBM2-MIXmixing is multi-state
expt
th
Excited 0+ decays in the Cd isotopes
TRIUM F EEC Update on Research Proposal Update of Proposed Research for Experiment # :1288
7.9
40
1680
27.0
0.051
80
30.2 31.1 33.5
0.730
27.40.0
127
0 0
2 658
2 1476 01473
0 1731
0 0
2 618
012242 1313
0 1433
0 0
2 558
2 12100 1306
01135
0 0
2 513
212130 1283
01380
110Cd 112Cd 114Cd 116Cd
<
(8) (3) (19) (12)
<< (12)
99(14)(14)
(16)
26(4)(17)
(6)9(22)
3.0(8) 104
Figure 2: Port ion of the level schemes for 110,112,114,116Cd showing the decays from the low-lying 0+
states. The observed transit ions between levels are indicated by arrows with widths proport ional to
the B(E2) values and are labeled with the absolute B(E2) values or limits, with the uncertaint ies
in parentheses.
The result of our studies with the 8π spectrometer have been extremely successful. Very recent ly,
we have published our first results from the 110In decay to 110Cd from S984 [9]. Combining level
lifet imes from the (n, n γ) react ion, and the branching rat ios or limits from the β-decay data, we
could, for the first t ime, extract B(E2) values or limits for every possible decay from the previously-
purported mult i-phonon states. What we found was remarkable – aside from the 0+ int ruder band
head and 6+ state in the ground state band, there was a lack of enhancement in any of the tran-
sitions between the intruder configuration and the non-intruder states. Comparison with theoret ical
calculat ions indicated that this scenario could only occur if the mixing were weak [9].
The reject ion of the strong-mixing scenario in 110Cd immediately raised the quest ion of the
explanat ion of the decay of the excited 0+ states. In the previous vibrat ional picture, the 0+3 level
was a two-phonon state and the 0+2 level the intruder band head; maximal mixing of these two levels
was required to account for the enhancement of the B(E2; 0+2 → 0+
gs) value and the cancellat ion of
the matrix elements contribut ing to the B(E2; 0+3 → 0+
gs). However, since this st rong-mixing scenario
was rejected, a new interpretat ion was required. From the decay pat terns, the underlying structure of
the non-intruder has the appearance that is associated with a γ-soft potent ial, or Wilets-Jean model,
whose key signature is an enhanced decay of the excited 0+ state to the second excited 2+ state, as
observed in the Cd isotopes as shown in Fig. 2.
In addit ion to this paradigm shift in the 110Cd structure, it was also suggested that the propert ies
of the 0+4 level, previously assigned as a three-phonon 0+ , was actually the head of a deformed proton
4p − 6h int ruder band. This suggest ion was based on its strongly favored decay to the 2+ int ruder
band level, which has theproton 2p− 4h assignment. Figure3 displays a port ion of theγ-ray spectrum
of coincidences with a 1397-keV γ ray from the 3475-keV I = 1 → 2079-keV 0+4 level, clearly showing
the dominance of the 295-keV 0+4 → 2+
3 (i ) γ ray feeding the 2+ int ruder level. Also noted is the
locat ion of a potent ial 603-keV 0+4 → 2+
2 t ransit ion (the expected enhanced transit ion if the 0+4 level
were a three-phonon state); the extracted upper limit for the branch is < 0.18. With a sensit ivity
to individual branches at the 10− 4 level, the β-decay data provides an unprecedented view into the
collect ive nature of low-lying states.
2
Deformed band head 0+ states: strong E2 decay to “one-phonon” 2+ states
“Two-phonon” 0+ states: very weak E2 decay to “one-phonon” 2+ states;but strong E2 decay to “two-phonon” 2+ states
Introduction to mid-shell collectivityin Z = 48, 52 (N = 66) isotones
0+
2+
4+
0+2+
2+
3+
(4)+
4+6+
8+
(5)+
6+
0+
0+
2+
2+
2+
4+
4+
4+
3+
6+
5+ 6+
8+
0
1
2
3
118Te 114Cd
MIX
E(MeV)
0+
2+
0+3-
other states
.
otherstates
3356
691115
801014
312
624
11936
π (4p-2h) ?
π (2p-4h)
0+
Differences exist for 03+ and higher-lying states
Demise of quadrupole vibrations in 110-116Cd: low-energy 0+ states are shell and subshell excitations
0
1
2
0d+
2d+
4d+
6d+
01+
21+
22+
41+
0+,3+,4+,6+
02+
23+
trans. 110Cd 112Cd 114Cd 116Cd harm.vib.
π 2p-4h
π 2h g9/2-2
π 2h p1/2-
2
P.E. Garrett and J.L. Wood, J.Phys. G37, 064028 (2010) J.L. Wood, J.Phys. Conf. Ser. 403, 012011 (2012)
E(MeV)
2302 242 278 175 3510 42
2341 < 5 < 0.4 < 0.3 < 7 31
2322 < 0.76 < 2 2.84 2.06 17
0221 < 7.9 0.009944 0.00264 0.554 60
2101 27 30 31 34 30 (norm)
B(E2)’s (W.u.) from lifetime measurements @ Univ. of Kentucky using (n,n’γ).
High-lying, low-energy transitions are difficult to observe: used 8Pi array @TRIUMF-ISAC and ultrahigh statistics β-decay scheme studies.
4d2d 11535 11912
Coexisting deformed bands in the even-mass Pb isotopes
Figure from Heyde & Wood Heavy arrows indicate E0+M1+E2 transitions:G.D. Dracoulis et al., PR C67 R 051301 2003