Results from the RISING Stopped Beam Campaign 2006 Andrea Jungclaus Universidad Autónoma de Madrid...
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![Page 1: Results from the RISING Stopped Beam Campaign 2006 Andrea Jungclaus Universidad Autónoma de Madrid NUSTAR Meeting 2007 introduction the RISING setup nuclear.](https://reader036.fdocuments.in/reader036/viewer/2022062301/56649e445503460f94b388fc/html5/thumbnails/1.jpg)
Results from the RISING Stopped Beam Campaign 2006
Andrea JungclausUniversidad Autónoma de Madrid
NUSTAR Meeting 2007
• introduction• the RISING setup• nuclear structure results• summary and outlook
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Rare ISotope INvestigations at GSI
relativistic radioactive beams(selected by the FRS)
highly efficient -ray detection(15 EUROBALL cluster detectors)+
fast beam campaign (2003-2005)g-RISING (fall 2005)stopped beam campaign (2006-2007) passive stopper - -decays from isomeric states active stopper - ß-decay studies
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Ion-by-ion identification with the FRS
TOF
E
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The setup at the focal plane S4
energy loss Z
x,y tracking
time-of-flight A/qtrigger signal (SC41)veto signal (SC43)
deceleration
ionizationchambers
(MUSIC41,42)scintillators(SC41,SC42)
multiwirechambers
(MW41,MW42)
SC43
stopperdegrader
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Best -spectrometer ever used in isomer spectroscopy !
The RISING -ray spectrometer
15 EUROBALL Cluster (105 Ge crystals)digital signal processing via 30 XIA DGF modules
Ab
solu
te e
ffic
ien
cy [
%]
-energy [keV]200 600 1000 14000
10
0
20
30
40
DGFTDC
MSU GSI
detection efficiency
very high -ray efficiencyhigh granularity (prompt flash problem)
S. Pietri et al., NIM
Thanks to Cluster owners !
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Physics aims of the RISINGstopped beam campaign 2006
82Nb,86Tc
54Ni
130Cd
204Pt
106Zr
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Is there evidence for a N=82 shell quenching ?
Assumption of a N=82 shell quenching leads to a considerableimprovement in the global abundance fit in r-process calculations !
r-p
roce
ss a
bu
nd
ance
s
mass number A
exp.pronounced shell gapshell structure quenched
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132Sn
N=82
Z=50
130Cd
A closer look to the region ...
known mass
known half-live
r-process waiting point(ETFSI-Q)
no direct experimentalsignature for N=82 quenching
most N=82 waiting-point nucleiexperimentally not accessible
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70 72 74 76 78 80 820
500
1000
1500
60Nd
58Ce
56Ba
54Xe
52Te
48Cd
Ene
rgy
of 2
+ sta
te
Neutron number N
Indirect evidence for a N=82 shell quenching ?
Kautzsch et al., Eur. Phys. J. A9 (2000) 201
from ß-decay studiesat ISOLDE
Can the anomalous behaviour of 2+ energies in the Cd isotopestowards N=82 be attributed to a change in the N=82 shell gap ?
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g9/2
Search for the 8+ (g9/2)-2 seniority isomer in 130Cd
two proton holes in the g9/2 orbit
6-proton-knockout from 136Xe: A. Jungclausfission of 238U: M. Górska, M. Pfützner June/July 2006
M. Górska et al., Phys. Rev. Lett. 79 (1997)
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A/q
pos
itio
n a
t S
4
S4 position
Identification of 130Cd in the fragmentation of 136Xe
A/q
pos
itio
n a
t S
2
Z1
Z2
MUSIC42 vs. MUSIC41 S2 position
Z=48130Cd
4000 identified 130Cd Ionen in fragmentation (2300 in fission)
750 MeV/u
136Xe
4 g/cm2
Be
meas(130Cd)~150 pb
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Gamma energy - time correlations
0.5
1.0
1.5
0.0DGF time (arb. units)
E
(MeV
)
0.5
1.0
1.5
0.0DGF time (arb. units)
6.300 ions 260.000 ions130Cd 128Cd
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Singles -spectrum in delayed coincidencewith implanted 130Cd ions
T1/2=220(30) ns
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coincidence spectra
128 138 539 1325
Gate: 128 keV
Gate: 138 keV
Gate: 539 keV
Gate: 1325 keV0+
(2+)
(4+)(6+)(8+)
SM130Cd8248
1346
1889
2094
2207
0+
2+
4+6+8+
1325
539
Decay of the 8+ isomer in 130Cd
T1/2=173nsT1/2=220(30)ns
New results give no evidence for a N=82 shell quenching !A. Jungclaus, L. Cáceres et al., subm. to Nature
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0+
(2+)
(4+)
(6+)(8+)
0+
(2+)
(4+)(6+)(8+)
0+
(2+)
(4+)(6+)(8+)
1
0
2
Ex (
MeV
)
76Ni482898Cd5048
130Cd8248
g9/2-2 g9/2
-2 g9/2-2
992
1922
2276
2420
1395
2083
2281
2428
1325
18641992/2002
2130
Unexpected scaling of (g9/2)2 two-body interaction
2+-8+ levels arepure (g9/2)-2 states
2+-8+ energy spread
scales with A-1
not with ħ=41·A-1/3
as commonly assumed
idea of H. GraweC. Mazzocchi et al.,PLB 622 (2005) 45
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What about the 2+ anomaly in the Cd isotopes ?
T. Rodríguez, J.L. Egido
Different behaviour inZ=48 Cd and Z=52 Tecan be attributed todeformation effects !
Symmetry conservingconfiguration mixingcalculations with theGogny force.
48Cd80 52Te80
x0.7 x0.7
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Physics aims of the RISINGstopped beam campaign
82Nb,86Tc
54Ni
130Cd
204Pt
106Zr
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Shell structure south of 208PbSpokesperson: Zsolt Podolyak, Surrey
cold fragmentationof 208Pb@1 GeV/u
main aim:spectroscopy of N=126 isotones206Hg, 204Pt and 202Os
204Pt
202Os
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204Pt populated via 4-proton-knockout from 208Pb
T1/2=8.41(16) s
T1/2=152(16) ns
short isomer:
long isomer:
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N=126 isotones: (h11/2)-2,4 I=10+ isomers
206Hg Z=80 204Pt Z=78
B. Fornal et al.PRL 87 (2001)212501
s1/2-1d3/2
-1
s1/2-1h11/2
-1
d3/2-1h11/2
-1
h11/2-2
SM
92(8) ns
152(16) ns
2.15(21) s8.41(16) s
d3/2-1d5/2
-1
d5/2-1h11/2
-1
?
Results require modification ofSPE and/or interactions !
SM
Z. Podolyak, S. Steer et al., PRL, in preparation
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Physics aims of the RISINGstopped beam campaign
82Nb,86Tc
54Ni
130Cd
204Pt
106Zr
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nn ppnp
T=1, S=0
T=0, S=1
TZ: +1 0 -1
even-even mirror nuclei (TZ=1)
Studies of the isospin symmetry at N=Z
"search for isospin breaking effects"od
d-o
dd
N=
Z n
ucl
ei"
T=
1 vs
. T=
0 co
mp
etit
ion
"
54Ni
82Nb,86Tc
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Isospin symmetry and eff. charges near 56NiSpokesperson: Dirk Rudolph, Lund
main aim:observe I =10+ isomer in 54Ni
A. Gadea et al., Phys. Rev. Lett. 97 (2006) 152501
24Mg(32S,2n)54Ni EUROBALL IV54Ni
58Ni @ 550 MeV/u
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coincidence spectra
gate on 54Ni50 ns < t < 1 s
Identification of 54Ni
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A=54, T=1 isospin symmetry
VBM: charge symmetry breaking component in the NN force
J=2 anomaly !
A. Zuker et al., PRL89 (2002) 142502
0 2 4 6 8 10spin (ħ)
ME
D (
keV
)
0
100
-100
0
100
-100
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Delayed -spectrum for 54Ni (50ns-1s)
The big surprise ...
Where does the 1327 keV line come from ???
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Proton radioactivity from the I=10+ isomer in 54Ni
First observation of excitedstate proton emission (compe-ting with -decay) followingfragmentation !
D. Rudolph, R. Hoischen et al., PRL, in preparation
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Physics aims of the RISINGstopped beam campaign
82Nb,86Tc
54Ni
130Cd
204Pt
106Zr
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T=0 - T=1 competition in heavy odd-odd N=Z nuclei
Spokesperson: Paddy Regan, Surrey
main aim:low-spin level structurein odd-odd 82Nb, 86Tc
43
41
41 43
107Ag @ 750 MeV/u
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86Tc
82Nb
20.000 ions
Identification of odd-odd N=Z 82Nb and 86Tc
Z
A/q
4.500 ions
Setting on 86Tc
N=Z
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82Nb 86Tc
T1/2= 133(20) ns T1/2= 1.59(20) s
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T=1 (T=0) T=1 (T=0)T=1 T=1
82Nb 86Tc82Zr 86Mo
Level structure of 82Nb and 86Tc comparedto their TZ=+1 isobars
A. Garnsworthy, P. Regan et al., PRL, in preparation
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T=0 and T=1 competition in odd-odd N=Z nuclei
Nb,Tc
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Physics aims of the RISINGstopped beam campaign
82Nb,86Tc
54Ni
130Cd
204Pt
106Zr
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S. Lalkovski, A. Bruce
Shape coexistence and the possibility of X(5)behaviour in A~110 nuclei
Spokesperson: Alison Bruce, Brighton
preliminary
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Summary
Isomers identified in 54Ni, 82Nb, 86Tc, 130Cd and 204Pt first proton-emitting state following fragmentation established in 54Ni
first isomeric decay observed after 6-proton-knockout: 130Cd
Additional observation of more than 25 new isomeric states
New information with respect to the reaction mechanism new world record in fragmentation: 27+ high-spin isomer in 148Tb isomeric ratios cross-section measurement
2006 has been a very successful year for the RISINGstopped-beam collaboration !
And the sun will continue to shine ...
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Physics aims of the RISINGactive stopper experiments 2007
collective evolution"south" of 208PbBenlliure, Regan
shape evolution from190W to 170Dy
Regan, Benlliure
isospin symmetry54Ni, 50Fe, and 46Cr
Fujita, Gelletly, Rubio
p-n pairing effects62Ge, 70Kr
Gadea, Algora
100Sn GT strengthT. Fästermann
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-decay of 190Ta 190W
2+0+
T1/2 ~16 sec
A. Garnsworthy
Online spectrum
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L.-L.Andersson, K. Andgren, L.Atanasova, D.L.Balabanski, F.Becker, P.Bednarczyk,J. Benlliure, M.A.Bentley, G.Benzoni, B.Blank, A.Blazhev, C.Brandau, J.Brown,
A.M.Bruce, E. Casarejos, L.Cáceres, F.Camera, W.N.Catford, B. Cederwall, F.C.L.Crespi, I.J.Cullen, P. Detistov, Zs.Dombradi, P.D.Doornenbal, E.Estevez, C.Fahlander,G.F.Farrelly, A.B.Garnsworthy, H.Geissel, W.Gelletly, J.Gerl, M.Górska, H. Grawe,
J.Grębosz, B. Hadinia, A.Heinz, M.Hellström, C. Hinke, R.Hoischen, G.Ilie, G. Jaworski, E.K.Johansson, J.Jolie, G.A.Jones, A.Jungclaus, A.Kelic, A. Khaplanov, M.Kmiecik,
I.Kojouharov, F.G. Kondev, R. Kumar, T.Kurtukian-Nieto, N.Kurz, S. Lalkovski,Z.Liu, A.Maj, S. Mandal, V. Modamio, F.Montes, S.Myalski, M.Pfützner, M. Palacz,S.Pietri, Zs.Podolyák, W.Prokopowicz, P.H.Regan, D.Rudolph, T.Saito, H.Schaffner,S.Schwertel, T.Shizuma, A.J.Simons, G. Simpson, S.J.Steer, S.Tashenov, J. Walker,
P.M.Walker, E.Werner-Malento, O. Wieland & H.J.Wollersheim
Argonne National Laboratory, Bordeaux, University of Brighton, Universitá di Camerino,Craków, Debrecen, ILL Grenoble, GSI, Japan Atomic Energy Agency, Universität zu Köln,
Lund University, Universidad Autónoma de Madrid, Universitá degli Studi di MilanoTechnische Universität München, University of New Delhi, Universidad de Santiagode Compostela, University of Sofia, KTH Stockholm, University of Surrey, Warsaw
University, Yale University, University of York
The RISING isomeric decay collaboration
Special thanks to the GSI accelerator group (2x108 p/sec 238U etc.) !
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Workshop on RISING PhysicsMadrid 6-8 November 2006
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100.000 ions 340.000 ions
T1/2=73(2) ns
T1/2 ~ 20 ns
134Sn
What is the lifetime limit of the current setup ?
no trace !