isomers and shape transitions in the n-rich a~190 region: phil walker university of surrey prolate k...
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Isomers and shape transitionsin the n-rich A~190 region:
Phil WalkerUniversity of Surrey
prolate K isomers vs.oblate collective rotation
the influence of angular momentum
Segre chart with isomers
adapted from Walker and Dracoulis, Nature 399 (1999) 35
K isomers(A ~ 170-190)
Z=72 (Hf)
prolate-oblate shape transition
Robledo et al., J. Phys. G: Nucl. Part. Phys. 36, 115104 (2009).
0
n-rich hafnium ground states
60
γ
30
N = 116critical point
Hilton and Mang
[PRL43 (1979) 1979]
prolate
oblate
HFB calculations
180Hf oblate band?
Tandel et al.,Phys. Rev. Lett. 101(2008) 182503with Gammasphere
three 20+ statespre-Gammaspherehigh-K yrast isomers:d'Alarcao et al.,Phys. Rev. C59(1999) 1227(R)
3600
cranked n-rich hafnium: 3 well-deformed minima
collective prolate
non-collective prolate
182Hf example: Xu, Walker and Wyss, Phys. Rev. C62 (2000) 014301
ћω = 0.2 ћω = 0.3 ћω = 0.4
collective oblate
190Hf TRS 190Hf TRSoblate rotor
ħω = 0 MeV ħω = 0.15 MeV
ħω = 0.3 MeV ħω = 0.45 MeV
prolate
oblate
I=32
Xu et al., unpublished
beyond the critical point
Hf prolate vs oblate182Hf186Hf
prolate
oblate
mqpprolate
[Xu et al., Phys. Rev. C62 (2000) 014301]
prolateoblate
Nilsson single-particle diagram N = 116 (188Hf, 190W, 192Os)
oblate prolate
data for even-even A~190 nuclei
190W
10- ~1ms
192Os
10- 6s
186W16+ >3ms
7- 20μs
190Os
10- 10m
188W
182Hf13+ 40μs
8- 62m
184Hf
8- 48s
184W15 0.2μs
5- 8μs
188Os
7- 14ns
186Os
7- 8ns
Z=76
Z=74
Z=72
N = 110 112 114 116
?
188Hf 186Hf
new data new data
critical point
W-190 gammas
190W
delayed gamma rays from 208Pb fragmentation at 1 GeV per nucleon
~1 ms
a critical point nucleus
isomer energies, potential energy surfaces
190Os114 192Os116 190W116
(calc)
(exp)
0+
10-
1633
2360±25
2015 6s
19201705 10m
1700
~1ms
190W: prolate
10- isomer PES
ground state PES
10-
(keV)
[Walker and Xu, PLB636 (2006) 286]
190W with Gammasphere
Lane et al.,Phys. Rev. C82(2010) 051304
190W with Gammasphere
Lane et al.,Phys. Rev. C82(2010) 051304
10- isomer at 1839 keV
isomer energies, potential energy surfaces
190Os114 192Os116 190W116
(calc)
(exp)
0+
10-
1633
2360±25
2015 6s
19201705 10m
1700
~1ms
190W: prolate
10- isomer PES
ground state PES
10-
(keV)
1839 240µs
[Walker and Xu, PLB636 (2006) 286]
190W with Gammasphere
Lane et al.,Phys. Rev. C82(2010) 051304
That was thehigh-K isomer.What about the oblate rotation?
190W with Gammasphere
Lane et al.,Phys. Rev. C82(2010) 051304
That was thehigh-K isomer.What about the oblate rotation?
(12+) yrast at 2653 keV
190W TRS: prolate to oblate
ħω = 0.216 MeVħω = 0.200 MeV
I = 4prolate
I = 14oblate
rotation alignment of 2 i13/2 neutrons with oblate shape
γ=0o
γ=-60o
[Walker and Xu, PLB636 (2006) 286]
N=116
74W 76Os 78Pt 80Hg0+
2+
(i 13/2)2
12+
2653
207 206
2451
412
2439
329
9 ns 5 ns
?200 ns
194 P
t and
196 H
g: L
evon
et a
l., N
ucl.
Phy
s. A
764
(200
6) 2
4
experimental energies, spins and half-lives
190W Lane et al.
192 O
s: V
alie
nte-
Dob
on e
t al.,
Phy
s. R
ev. C
69 (
2004
) 02
4316
projected shell model(angular momentum basis)
Sun et al., PLB659 (2008) 165
summary
- oblate-prolate competition in N = 116 188Hf – 190W – 192Os - N = 116 seems to be the critical-point neutron number- focus on angular momentum effects- 10- prolate K isomers- 12+ isomers: bandheads of collective oblate bands??- giant backbending candidates: cf. Hilton and Mang 1979- oblate rotation becomes yrast over a wide spin range- more data needed!! (188Hf, 190W and/or 192Os)