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108 Sn studied with intermediate-energy Coulomb excitation. Dissertation zur Erlangung des Grades “Doktor der Naturwissenschaften” am Fachbereich Physik der Johannes Gutenberg-Universit ät in Mainz Leontina Adriana Banu. Outline. Motivation Why to study 108 Sn ? - PowerPoint PPT Presentation
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108Sn studied with intermediate-energy Coulomb excitation
Dissertation zur Erlangung des Grades “Doktor der Naturwissenschaften”
am Fachbereich Physikder Johannes Gutenberg-Universität
in Mainz
Leontina Adriana Banu
OutlineOutline
Motivation Why to study Why to study 108108Sn ?Sn ? Why to study it with Coulomb excitation ?Why to study it with Coulomb excitation ?
Experimental method description Most significant features of intermediate-energyMost significant features of intermediate-energy Coulomb excitationCoulomb excitation Experimental set-up
Data analysis
Experimental results Theoretical interpretation
Why to study Why to study 108108Sn ?Sn ?
• magic numbers shell closuresmagic numbers shell closures
Nuclear shell modelNuclear shell model
• 100100Sn (N=Z=50)Sn (N=Z=50) principle test groundprinciple test ground
• insight into the structure of insight into the structure of 100100SnSn by by studying the nuclei in its vicinitystudying the nuclei in its vicinity
• how rigid is the the doubly-magic core how rigid is the the doubly-magic core when valence neutrons are being when valence neutrons are being added ?added ? ((studying A=102-130 Sn isotopesstudying A=102-130 Sn isotopes))
• investigation on quadrupole investigation on quadrupole polarization ofpolarization of the doubly-magic corethe doubly-magic core ((E2 core polarization effectE2 core polarization effect))
• B(E2;0B(E2;0++->2->2++)=|<)=|<ff||||OOE2E2||||ii>|>|22 is the is the mostmost sensitive to E2 collective effectssensitive to E2 collective effects
108108SnSn
5858
112112SnSn
6262
N=ZN=Z
Number of neutrons (N)
Num
ber
of
pro
tons
(Z)
Z = 2,8,20,28,50,82Z = 2,8,20,28,50,82 N = N = 2,8,20,28,50,82,1262,8,20,28,50,82,126
100Sn
Sn(N,Z) = B(N,Z) – B(N-1,Z)N oddZ even
22 88 2020 2828 5050 8282 126126
Neutr
on s
epara
tion e
nerg
y [
MeV
]
Avera
ge e
nerg
y o
f th
e fi
rst
exci
ted s
tate
s in
even
- even n
ucl
ei
Why Coulomb excitation to study Why Coulomb excitation to study 108108Sn ?Sn ?
• B(E2) determination:B(E2) determination:Lifetime measurement B(E2) valueB(E2) value
( ~ 7 ns) isomeric state( ~ 7 ns) isomeric state
B(E2;6B(E2;6++->4->4++) = 3 W.u.) = 3 W.u.
Z. Phys. A352 (1995) 373Z. Phys. A352 (1995) 373
E2E2
00++
22++
44++
66++
108108SnSn
905905
253253
12061206
(HI,xn(HI,xn) reaction) reaction
(< 0.5 ps)(< 0.5 ps)
• Electromagnetic decay of lowest excited 2Electromagnetic decay of lowest excited 2++state:state:
transition probability
τ1
secB(E2)ET(E2) 15γ
lifetime
22++
00++
EE(())
Coulomb excitation B(E2) valueB(E2) value
cross section
((E2) ~ B(E2))
66++
E2E2
2+
0 keV0 keV
1207 keV
Intermediate-energy Coulomb Intermediate-energy Coulomb excitationexcitation
~ ~ 3%3%
E=1.3 MeVD = 70 cm
1 Ge-Cluster 1 Ge-Cluster detectordetector
Composite
Composite
detector
detector
E/E
0 [%
]
Detector opening angle Detector opening angle =3°=3°
lab
[deg]
= 0.57= 0.57
= 0.43= 0.43
= 0.11= 0.11
• Nuclear excitation (±)
• Lorentz boost (+)
• Doppler broadening (-)
• Atomic background
radiation (-)
n
Nuclear excitationNuclear excitation
Coulomb excitationCoulomb excitation
target1.5θmax( in our case ) = 0.43
UNILACSIS
ESR
FRSFRS
GSI accelerator facilityGSI accelerator facility
Experimental set-upExperimental set-up
Primary beam
124Xe @ 700 A•MeV
9Be, 4 g/cm2
• projectile fragmentation (production method)
• in-flight fragment separation
(Bρ-E-Bρ method)
βγBρ
uce
ZA
(~ 150 A•MeV)
Secondary beam @ reaction target:108Sn/112Sn
197Au, 0.4 g/cm2
Beam directionBeam direction
CATE (Si) CATE (CsI)
Fragment identification Fragment identification beforebefore//afterafter targettarget
108108SnSn
Selection with FRSSelection with FRS Selection with CATESelection with CATE
βγBρ
uce
ZA
res
2
EΔEAZ
ΔE
Scattering angle measurementScattering angle measurement
p
MW MW CATE
Si CsITarget
Beam trackingBeam tracking
• Event–by–event Doppler shift correction:Event–by–event Doppler shift correction:
• Impact parameter determination:Impact parameter determination:
γ
20γγ βcosΘ1
β1EE
[rad]Θ1
MeV]}[AT2ucMeV])[A{(TA
MeV])[AT(ucZZ~b[fm]
plab22
labp
lab2
tp
511 keV
40K
~ 50%
rest
in-flight
Analysis of intermediate-energy Coulomb Analysis of intermediate-energy Coulomb excitationexcitation
• Fragment selectionFragment selection beforebefore secondary secondary targettarget
• Fragment selectionFragment selection afterafter secondary secondary targettarget
• Scattering angle selection (1°- 2°)Scattering angle selection (1°- 2°)
• Prompt Prompt time ‘window’ time ‘window’
• Ge-Cluster multiplicity: MGe-Cluster multiplicity: M(E(E > 500 keV) > 500 keV) = 1= 1
Elastic scattering dominates
Nuclear excitation contributiongrazzing = 1.5° ± 0.5°
Experimental resultsExperimental results
B(E2; 0B(E2; 0+ + -> 2-> 2++) = 0.230 (57) e) = 0.230 (57) e22bb22
A. Banu et al.A. Banu et al., submitted to Phys. Rev. C (2005), submitted to Phys. Rev. C (2005)
0.88I
N
N
I)B(E2)B(E2 112
γ
112p
108p
108γ112108
• Measure:Measure:-particle coinc.-particle coinc.
particle singles
II
Np
• Deduce B(E2) for Deduce B(E2) for 108108Sn as follows:Sn as follows:
)(atom/cmNN
/εIσ(E2) 2
tp
γγ
)B(E2)f(bσ(E2) min
exp.exp.
theorytheory
0.240 (14) e0.240 (14) e22bb22 --- previous work
Theoretical interpretationTheoretical interpretation
Neutron numberNeutron number
B(E
2 )
eB
(E2
) e
2 2 bb
22
This workThis work
theory (theory (neutron valenceneutron valence and and 100100SnSn as closed-shell core)as closed-shell core)
••••••••
5810850Sn
Neutron/proton single-particle statesin a nuclear shell-model potential:
theory (theory (neutron valenceneutron valence + proton core excitations+ proton core excitations and and
9090ZrZr as closed-shell core)as closed-shell core)
t=0
t=2t=4
t=4
Proton np-nh core excitations (t=n)&
100Sn core is open
Conclusion and OutlookConclusion and Outlook
• 108108Sn the heaviest Z-nucleus studied with Sn the heaviest Z-nucleus studied with intermediate-energy Coulomb excitationintermediate-energy Coulomb excitation
• B(E2;0B(E2;0++->2->2++) measured for the first time) measured for the first time
• The experimental result is in agreementThe experimental result is in agreement with latest large scale shell model calculationswith latest large scale shell model calculations
• This work brings more insight into the investigation ofThis work brings more insight into the investigation of E2 correlations related to E2 correlations related to 100100Sn core polarizationSn core polarization
• 108108Sn further step towards Sn further step towards 100100SnSn
““Art is I, Science is We.” - Claude BernardArt is I, Science is We.” - Claude Bernard
Thanks to…Thanks to…
J. Gerl (GSI), J. Pochodzalla (Uni. Mainz) - thesis advisorsJ. Gerl (GSI), J. Pochodzalla (Uni. Mainz) - thesis advisors
C. Fahlander (Lund), M. GC. Fahlander (Lund), M. Górska (GSI) - spokespersonsórska (GSI) - spokespersons
H. Grawe, T.R. Saito, H.-J. Wollersheim (GSI) H. Grawe, T.R. Saito, H.-J. Wollersheim (GSI)
M. Horth-JensenM. Horth-Jensen et al. (Oslo Uni.), et al. (Oslo Uni.), F.NowackiF.Nowacki et.al et.al (IRES)(IRES)
and last but not least…and last but not least…
The local RISING team
Seniority scheme in Sn isotopes:Seniority scheme in Sn isotopes:
E(E(jj22J) ~ VJ) ~ V00tan(tan(/2)/2) for T=1, J even for T=1, J even
-residual interaction in a -residual interaction in a jjnn configuration configuration
00++
22++
44++
66++
jjnn00
22
22
22
= 2= 2
= 0= 0
= 0= 0
22++
44++
66++
00++
(V(V1212(() = -V) = -V00((rr11--rr22))))
minmin
ener
gy a
xis
jj
j
j
j
j
j j
JJ
JJJJ
JJ
Data SummaryData Summary
Primary beamPrimary beam
SIS energySIS energy (MeV/nucleon)
Primary beam intensityPrimary beam intensity (s-1)
124124XeXe
700700
6 6 × 10× 1077
124124XeXe
700700
6 6 × 10× 1077
Secondary beamSecondary beam
Sec. beam abundance Sec. beam abundance (%)
Sec. beam rate Sec. beam rate (s-1)
Sec. beam energy @ target Sec. beam energy @ target (MeV/nucleon)
112112SnSn
6060
24002400
147147
108108SnSn
6262
24802480
142142
EE(2(211++->0->0++) ) (keV)
Data collection timeData collection time (h)
12571257
3333
12061206
5858
Single-particle states in shell-model Single-particle states in shell-model potentialpotential
2j+12j+1 nnjjll
Spectrsoscopic notation:Spectrsoscopic notation:
ll -> orbital angular momentum
jj -> total angular momentum
l= 0, 1, 2, 3, 4, 5, 6
s, p, d, f, g, h, is, p, d, f, g, h, i
jj = = ll + s + s
s = 1/2s = 1/2j = l ± ½
2j+1 2j+1 nucleons /orbitalnucleons /orbital
inertinert core
+activeactive valencenucleons
••••••••
5810850Sn
Single-particle states in shell-model Single-particle states in shell-model potentialpotential
2j+12j+1 nnjjll
Spectrsoscopic notation:Spectrsoscopic notation:
ll -> orbital angular momentum
l= 0, 1, 2, 3, 4, 5, 6
s, p, d, f, g, h, is, p, d, f, g, h, i
jj -> total angular momentum
jj = = ll + s + s
s = 1/2s = 1/2j = l ± ½
2j+1 2j+1 nucleons /orbitalnucleons /orbital
B(E2;0B(E2;0++ -> 2 -> 2++) ) ~ f(1-f)~ f(1-f) wherewhere
Generalized seniority scheme:Generalized seniority scheme:
f = (N – 50)/ 32f = (N – 50)/ 32