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Introduction In experiment, more than 80 SD bands have been observed in A~190 mass region. For even-even nuclei, the dynamical moment of inertia (J (2) ) exhibits a gradual increase with the increasing rotational frequency ћω. A. V. Afanasjev, P. Ring, J. König, Nucl. Phys A 676 (2000) Y. Sun, J. Y. Zhang, and M. Guidry, Phys. Rev. Lett. 78 (1997) 2321; Phys. Rev. C 63 (2001) For the odd-odd nuclei, quite a part of the moments of inertia for SD bands keep constant. X. T. He, S. X. Liu, S. Y. Yu, E. G. Zhao HEP & NP 27 (2003) 124 X. T. He, S. Y. Yu, S. X. Liu, Y. X. liu, E. G. Zhao Chin. Phys. Lett. 21 (2004) 813 X. T. He, S. X. Liu, S. Y. Yu, J. Y. Zeng, E. G. Zhao J. Phys. G: Nucl. Part. Phys. (submited)
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The The ii13/2 13/2 Proton and Proton and jj15/215/2 Neutron Orbital and the Neutron Orbital and the
SD Band in A~190 SD Band in A~190 RegionRegion
Xiao-tao He Xiao-tao He En-guang ZhaoEn-guang Zhao
Institute of Theoretical Physics, CAS, Beijing, Institute of Theoretical Physics, CAS, Beijing, ChinaChina
Summer school • Peking University •2004 Summer school • Peking University •2004
Outline• Introduction• Particle-number conserving method• Numerical result• Summary
Introduction• In experiment, more than 80 SD bands have
been observed in A~190 mass region.
• For even-even nuclei, the dynamical moment of inertia (J(2)) exhibits a gradual increase with the increasing rotational frequency ћω.
A. V. Afanasjev, P. Ring, J. König, Nucl. Phys A 676
(2000) 196.. Y. Sun, J. Y. Zhang, and M. Guidry, Phys. Rev. Lett. 78
(1997) 2321; Phys. Rev. C 63 (2001)
047306.
For the odd-odd nuclei, quite a part of the moments of inertia for SD bands keep constant.
X. T. He, S. X. Liu, S. Y. Yu, E. G. Zhao HEP & NP 27 (2003) 124
X. T. He, S. Y. Yu, S. X. Liu, Y. X. liu, E. G. Zhao Chin. Phys. Lett. 21 (2004) 813
X. T. He, S. X. Liu, S. Y. Yu, J. Y. Zeng, E. G. Zhao J. Phys. G: Nucl. Part. Phys. (submited)
Some different methods:
HF method B. -Q. Chen, et al., Phys. Rev. C 46 (1992) R1582.
J. Terasaki, et al,. Phys. Rev. C 55 (1997) 1231.
RMF J. D. Walecka, Ann. Phys. 83 491 (1974)
PRM X.Q.Chen and Z Xing J.Phys.G:Nucl.Part.Phys.19(1993)1869
PSM Y. Sun, J. Y. Zhang, and M. Guidry, Phys. Rev. Lett. 78 (1997) 2321
IBM (IBFM) Y. X. Liu, et al., Phys. Rev. C 63, (2001) 054314 Phys. Rev. C 59 (1999)
2511
CSM D. R. Inglis, Phys. Rev. 95, (1954) 1059
Particle-number conserving (PNC)
methodadvantage:• Particle number is conserved • A cranked many-particles configuration
(CMPC) truncation is adopted instead of the single-particle level (SPL) truncation.
• The blocking effects is taken into account strictly and consistently.
disadvantage:• Angular momentum is not conserved
FormulaCSM Hamiltonian : H0 : single particle part Hp : pairing interaction part
ppxSPCSM HHHJHH 0
ii hH ))(( 00 xNil jhh )(0
)2()0( ppp HHH
1. Nilsson level single-particle Nilsson hamiltonian : good quantum number : (parity),
[N,nz,L] : is the good quantum number of H0 ,Hz ,lz and jz under the extreme large deformation
degeneracy: ( ± )。
'22
2VV
Mh oscNil
0 anN z 0 anN z
2. Cranked Nilsson levelCranked Nilsson hamiltonian
: signatureThe eignstate of Rx() and j2z :
diagonalize h0() in space|, we get | :
xNil jhh )(0
xjix eR )(
)(12
1x
i Re 0 b
0C
3. Many-body systemn particles system , the configuration |i :
According to configuration |i, the system
possess certain energy Ei 、 parity Pi 、 signaturei and particle number N:
02121
niiiniiii
)(occupied
ii
iE
)(occupied
ii
iP
2mod)()(
occupied
ii
i
4 .paring interactionIn Nilsson single particle space :
In | space :
In | space : Similar to HP(0), we can get HP(2)
0,
)0(
aaaaGH p
,)()()2( 222,1,0
2
aaaaqqGHP
bbbbGHP0,
'''
'''
ffGHP
b
aa N
21
C
bC )(
In | space : Diagonalize HCSM in the CMPC
space, we get the solution of CSM Hamiltonian :
Di: interger
pCSM HHH 0
i
i iD
5 . moment of inertia
The angular momentum alignment in | :
Dynamic :Kinematic :
ji
xjii
xixx jJiDDiJiDJJ 22
xJJ )1(
dJd
J x)2(
Result The cranked Nilsson orbital
in A~190 mass region
-0.1 0.0 0.1 0.2 0.3 0.4 0.5 0.66.5
6.6
6.7
6.8
6.9
7.0
7.1
7.2
-0.1 0.0 0.1 0.2 0.3 0.4 0.5 0.65.7
5.8
5.9
6.0
6.1
6.2
6.3
6.4
6.5
114
[651]1/2
[761]1/2
[633]5/2
[512]3/2
[510]1/2
[631]3/2
[752]5/2
[514]7/2
[624]9/2
[512]5/2[505]11/2
[761]3/2
[642]3/2
[640]1/2
[770]1/2
cran
ked
neut
ron
Nils
son
leve
l (0)
/Mev
80
[651]1/2[633]7/2
[521]3/2
[402]5/2
[523]5/2
[404]7/2
[514]9/2
[642]5/2
[530]1/2
[651]3/2
[532]3/2
[411]1/2
[660]1/2
cr
anke
d pr
oton
Nils
son
leve
l (0)
/Mev
Parameters• The Nilsson parameters (κ) are taken from Lund
systematics. T.Bengtsson and I. Ragnarsson, Nucl. Phys. A436, 14
(1985)
• The deformation parameters 2=0.46 , 4=0.03. M. A. Riley et al., Nucl. Phys. A512
178 (1990) • The effective pairing interaction strengths ( G0
for monopole pairing and G2 for quadrupole pairing ) in unite of MeV are given as follow:
G0p=0.3, G2p=0.01, G0n=0.2, G2n=0.013
Experimental and calculated J(1) and J(2) of the yrast SD band in even-even
nuclei 192Hg
0.00 0.05 0.10 0.15 0.20 0.25 0.30 0.35 0.40 0.4580
90
100
110
120
130
140
150
80
90
100
110
120
130
140
150
J(2)
J(1)
(MeV)
192Hg(1)
mom
ents
of i
nerti
a (
2 MeV
-1)
Experimental and calculated J(1) and J(2) of the SD bands in odd-A
nuclei 193Tl and 195Tl
90
100
110
120
130
140
150
90
100
110
120
130
140
150
0.0 0.1 0.2 0.3 0.480
90
100
110
120
130
140
150
0.0 0.1 0.2 0.3 0.480
90
100
110
120
130
140
150
J(2)
J(1)
193Tl(1) =-1/2([642]5/2,a=-1/2)
mom
ent o
f ine
rtia
(2 M
eV-1)
J(2)
J(1)
193Tl(2) =+1/2([642]5/2,a=+1/2)
J(1)
J(2)
195Tl(2) =+1/2([642]5/2,a=+1/2)
(MeV)
J(1)
J(2)
195Tl(1) =-1/2([642]5/2,a=-1/2)
Occupation probability of each proton cranked orbital near the
Fermi surface in 193Tl
0
1
2
0
1
2
0.0 0.1 0.2 0.3 0.40
1
2
0.0 0.1 0.2 0.3 0.40
1
20
1
20
1
2193Tl(1) proton N=6
[651]1/2
[642]5/2 =-1/2
[651]3/2
proton N=5
[514]9/2
[532]3/2[530]1/2
prot
on o
ccup
atio
n pr
obab
lity
proton N=4
[404]7/2
[411]1/2proton N=4
[404]7/2
[411]1/2
(MeV)
proton N=5
[514]9/2
[530]1/2
193Tl(2) proton N=6
[633]7/2
[642]5/2 =+1/2
[651]3/2
The separate contributions to J(2) from each cranked proton orbitals
near the Fermi surface
-20
0
20
40
60
0.0 0.1 0.2 0.3 0.4
-20
0
20
40
60
-20
0
20
40
60
0.0 0.1 0.2 0.3 0.4
-20
0
20
40
60[633] 7/2 [642] 5/2
193Tl(1) Proton
[651] 1/2 [642] 5/2[651] 1/2
[642] 5/2
[651] 3/2
[660] 1/2
Sep
arat
e co
ntrib
utio
ns to
J(2
) (2 M
eV-1)
[532] 3/2
[523] 7/2
[541] 1/2
[532] 5/2
[541] 3/2
[550] 1/2
[651] 1/2 [651] 3/2[642] 5/2 [651] 3/2
[633] 7/2 [642] 5/2
193Tl(2) Proton
[642] 5/2
[651] 3/2
[660] 1/2
(MeV)
[532] 3/2
[523] 7/2
[541] 1/2
[532] 5/2
[541] 3/2
[550] 1/2
Experimental and calculated J(1) and J(2) of the six SD bands in odd-
odd nuclei 194Tl
90
100
110
120
130
140
150
90
100
110
120
130
140
150
0.0 0.1 0.2 0.3 0.490
100
110
120
130
140
150
0.0 0.1 0.2 0.3 0.4 0.0 0.1 0.2 0.3 0.490
100
110
120
130
140
150
J(2)
J(1)
194Tl(1a) =0([642]5/2+ [512]5/2-)
J(2)
J(1)
194Tl(2a) =0([642]5/2- [624]9/2+)
J(2)
J(1)
194Tl(3a) =0([642]5/2- [512]5/2=+)
J(2)
J(1)
194Tl(1b) =1([642]5/2+ [512]5/2+)
mom
ent o
f ine
rtia
(2 M
eV-1)
J(2)
J(1)
194Tl(2b) =1([642]5/2- [624]9/2-)
(MeV)
J(2)
J(1)
194Tl(3b) =1([642]5/2- [512]5/2=-)
Occupation probability of each neutron cranked orbital near the
Fermi surface in 194Tl
0.0 0.1 0.2 0.3 0.40
1
2
0.0 0.1 0.2 0.3 0.4 0.0 0.1 0.2 0.3 0.40
1
20
1
2
0
1
20
1
2
0
1
2
N=5
(MeV)
[514]7/2
[512]5/2
[505]11/2
N=5
[514]7/2
[512]5/2
[505]11/2
N=5
[514]7/2
[512]5/2
[505]11/2
N=6
[642]3/2
[624]9/2
occu
patio
n pa
obab
ility
n
N=6
[624]9/2
[642]3/2
N=6
[642]3/2
[624]9/2
N=7
[752]5/2
[761]3/2
N=7
[752]5/2
[761]3/2
N=7
[752]5/2
[761]3/2
Experimental and calculated J(1) and J(2) of the four SD bands in
odd-odd nuclei 192Tl
90
100
110
120
130
140
150
90
100
110
120
130
140
150
0.0 0.1 0.2 0.3 0.490
100
110
120
130
140
150
0.0 0.1 0.2 0.3 0.490
100
110
120
130
140
150
J(1)
J(2)
192Tl(a) [642]-5/2[761]-3/2
J(1)
J(2)
192Tl(b) [642]+5/2[761]-3/2
J(1)
J(2)
192Tl(c) [642]5/2[512]5/2
mom
ent o
f ine
rtia
(2 M
eV-1)
J(1)
J(2)
192Tl(d) [642]5/2[512]-5/2
/MeV
Occupation probability of each neutron cranked orbital near the
Fermi surface in 192Tl
0.0 0.1 0.2 0.3 0.40
1
2
0
1
20
1
2
0
1
20
1
2
0
1
2
[512] 5/2 [514] 7/2[512] 5/2
[505]11/2
/MeV
[640] 1/2[642] 3/2
[624] 9/2
occu
patio
n pa
obab
ility
n
[770] 1/2[761] 3/2
[752] 5/2
Summary• The PNC method in the frame of CSM is
one of the useful method to deal with the SD nuclei.
• The i13/2 Proton and j15/2 Neutron intruder Orbital plays a very important role in the variation in both kinematic and dynamical moments of inertia (MOI) with rotational frequency in A~190 Region.
Thank you !