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Invariant-mass spectroscopy of neutron halo nuclei. Takashi Nakamura 中村隆司 Tokyo Institute of Technology 東京工業大学. 中日 NP 06 , Shanghai. Coulomb Breakup of 11 Li Submitted to Phys.Rev.Lett. Collaborators. T.Nakamura, A.M. Vinodkumar, T.Sugimoto, N.Fukuda, M.Miura, Y.Kondo, N.Aoi, N.Imai, - PowerPoint PPT Presentation
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Invariant-mass spectroscopy of neutron halo nuclei
Takashi Nakamura中村隆司
Tokyo Institute of Technology東京工業大学
中日 NP 06 , Shanghai
T.Nakamura, A.M. Vinodkumar,T.Sugimoto,N.Fukuda, M.Miura, Y.Kondo, N.Aoi, N.Imai,T.Kubo, T.Kobayashi, T.Gomi, A.Saito, H.Sakurai, S.Shimoura,D.Bazin, H.Hasegawa, H.Baba, T. Motobayashi, T.Yakushiji, Y. Yanagisawa,K.Yoneda, K. Watanabe, Y.X.Watanabe, M.Ishihara
Collaborators
Coulomb Breakup of 11LiSubmitted to Phys.Rev.Lett.
Invariant Mass Method (unbound excited states)
RadioactiveIon beam
BreakupKinematicFocusing
Well-defined Energy by Invariant Mass
ThickTarget
Ex
12Be vs. 14Be
12Be0+
2+0+
1-
2.24
2.70 MeV
2.10
14Be Drip line
11Be+n3.169 MeV
0+
1.264 MeV
? 2+
12Be+2nBound RegionInbeam spectroscopy
Unbound RegionInvariant massspectroscopy
14Be + 12C 12Be + n + n + 12C
Eex = S2n + Erel = 1.56 0.13 MeV
Erel (MeV)
d/d
Ere
l(mb/
MeV
)
T.Sugimoto, TN et al., (2006)
1.56MeV
N=8MagicityLoss
HHe
LiBeBC
NO
FNe
Neutron Dripline
N=8
N=20
11Be19C
N
Z Neutron halosStudied by InvariantMass Method by our group
11Li
11Li11Be
2n halo nucleus1n halo nucleus
Neutron Halo Nuclei– Nuclei at the stability limit
9Li
n
n10Ben
Sn=504 keV S2n=300 keV
14Be
11Li
High-Z Target (Pb)
9Li
n
= NE1(Ex)dB(E1)dEx
dCD
dEx 9hc163
Cross section = (Photon Number)xTransition Probability)
Invariant Mass
Equivalent Photon Method
relx , EE
)Li(),(),( 9PnPnP
11Li*
n
Coulomb Breakup of 11Li
11Be : E1 Response of one-neutron Halo
Ex10~20MeV
1~2MeV
N.Fukuda, TN et al., PRC70, 054606 (2004) TN et al.,PLB 331,296(1994)
core n
dB(E1)dEx
)W.u06.029.3(
fm06.005.1)1( 22
eEB
11Be
dB(E1)dEx
exp(iqr)| rY1m|gs
|2
ZA
-Sn
~ |exp(-r/)/r|2
Fourier Transform
Low-lying E1 Strength Halo State
exp(iqr)| rY1m|s1/2 |2Z
A
Direct Breakup Mechanism
Sn=504keV
= 0.72
One neutron halo nucleus vs. Two neutron halo nucleus
9Li
n
n10Ben
Motion between core and 1 valence neutron
Motion between 1. Core and neutron2. Core and neutron3. Two valence neutrons (neutron-neutron correlations)
S2n=300 keVSn=504 keV
Coulomb Dissocitaion of 11Li (Summary of Previous Results)
RIKEN @ 43MeV/nucleonPLB348 (1995) 29.
GSI @280MeV/nucleonNPA 619 (1997) 151.
MSU@ 28MeV/nucleonPRL 70 (1993) 730.PRC 48(1993) 118.
• RIPS@RIKEN• Primary Beam
18O 100 AMeV• Projectile Frag
mentation• Secondary Bea
m11Li ~70 AMeV~20 kcps
RIKENProjectile-fragment Separator
18O 100 AMeV
11Li ~70 AMeV
11Li
9Li
nn
Experimental Setup@RIPS at RIKEN
Pb Target
NEUT
HOD
BOMAG
DC
DALI
70MeV/nucleon
Examine Different Wall Events
t1
t2
1
2
12
Condition: 121 Almost no bias
Eth=6MeVee to avoid any gamma related events
Elimination of Cross-Talk events
Coulomb Dissociation Spectrum of 11Li
MeV3for
b.)(28.0.)(05.034.2
rel
E
syststat
Angular Distribution
Calculation:H.Esbensen et al.,NPA542(1992)310. Private Communication
“Soft dipole excitations in 11Li”
Present Result
Comparison with the 3-bodytheorykeV3002 nS
= NE1(Ex)dB(E1)dEx
dCD
dEx 9hc163
B(E1) Distribution
MeV3
18.042.1)1(
rel
22
E
fmeEB
Non-energy weightedE1 Cluster Sum Rule
22
2
212
22
1
2
0
3
)(24
3)1()1(
nc
xx
rA
Ze
rrrrA
ZedE
dE
EdBEB
r1
r2 n
9Li
rc-2n
fm32.001.5
)22(78.1
)3MeV(18.042.1)1(
2
2
22
rel22
ncr
fme
EfmeEB
(Extrapolated cluster strength)
~70% larger than non-correlatedstrength 021 rr
deg50~12
H.Esbensen et al.,NPA542(1992)310.
Experimental Result
E(9Li-n)
E(9
Li-n
)
1MeV
1MeV
Simulation (Phase-space decay)
E(9Li-n)
E(9
Li-n
)
1MeV
1MeV
Correlation?
Summary
11Li(2n halo)+Pb (Coulomb Breakup)
Low-lying B(E1) Strength Could be used to see the nn correlation & 9Li-n correlation in 11Li (E1 Non-energy weighted sum rule)
Strong B(E1) at very low excitation energy 2218.042.1)1( fmeEB
c.f. B(E1)=1.05(6) e2fm2 for 11Be
Invariant Mass Spectroscopy ----Powerful Spectroscopic tool