evolution of n=50 towards 78 ni: recent inputs from experiments
DESCRIPTION
Workshop Espace de Structure Nucléaire Théorique Saclay 3-5 May 2010. Evolution of N=50 towards 78 Ni: recent inputs from experiments. D. Verney, IPN Orsay. Introduction: recent progress in experiment north north-east to 78 Ni. 0. - PowerPoint PPT PresentationTRANSCRIPT
Evolution of N=50 towards 78Ni: recent inputs from experiments
Workshop Espace de Structure Nucléaire Théorique Saclay 3-5 May 2010
Position of the problem : why should we worry about N=50 ?1
N=50 shell gap evolution: salient features from experimental data2
deeper into nuclear structure close to 78Ni : valence space, single particle state effective sequence
3
D. Verney, IPN Orsay
0 Introduction: recent progress in experiment north north-east to 78Ni
0 Introduction: recent progress in experiment north north-east to 78Ni
N=50 : recent experimental breakthrough
(d,3He)
-decay
« border » of the knowledge on nuclear structure
fission
(t,p)
Zendel et alInorg Nucl Chem 42, 1387 (1980)
Kratz et alNucl Phys A
250, 13 (1975)
Del Marmol et alNucl Phys A
194, 140 (1972)
Hoff -FogelbergNucl Phys A
368, 210 (1981)Ge83
Experimental status in year 2003
Sr88
Rb87
Kr86
Br85
Se84
As83
Ge82
Ga81
Zn80
Cu79
Ni78Ni77Ni71 Ni72 Ni73 Ni74 Ni75 Ni76Ni70Ni69Ni68Ni67Ni66Ni65Ni64
Ge76Ge74Ge72
Y89
Zr90 Z=40
28
N=40 50
Cu65
Zn66 Zn67 Zn68 Zn70
Ga69 Ga71
Ge70 Ge73
As75
Se76Se74 Se77 Se78 Se80 Se82
Br79 Br81
Kr78 Kr80 Kr82 Kr83 Kr84
Rb85
Sr86 Sr87Sr84
Zr91
Se75 Se79 Se81 Se83
Kr85
Cu74
Zn75 Zn76 Zn77 Zn78
Ga79 Ga80fra
gmentation
Winger et alPhys Rev C
36, 758 (1987)
Beginning of -decay studies at PARRNe
OSIRIS /Studsvik
TRISTAN /Brookhaven
On
-lin
e m
as
s
se
pa
rati
on
Ch
imic
al
se
pa
rati
on
First structure data (’s) came from -decay (for N=50)1
Fission + ISOL technique
ESNT Workshop – Saclay – 3-5 May 2010 D. Verney
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main nuclear mechanisms used :
-fragmentation of stable beams
-fission
Sr88
Rb87
Kr86
Br85
Se84
As83
Ge82
Ga81
Zn80
Cu79
Ni78Ni77Ni71 Ni72 Ni73 Ni74 Ni75 Ni76Ni70Ni69Ni68Ni67Ni66Ni65Ni64
Ge76Ge74Ge72
Y89
Zr90 Z=40
28
50
Cu65
Zn66 Zn67 Zn68 Zn70
Ga69 Ga71
Ge70 Ge73
As75
Se76Se74 Se77 Se78 Se80 Se82
Br79 Br81
Kr78 Kr80 Kr82 Kr83 Kr84
Rb85
Sr86 Sr87Sr84
Zr91
Ge84Ge83
isomeric decay: LISE-GANIL
radioactive beam: REX ISOLDECu77
Zn78 Zn79
As84
Se85 Se86
-decay Orsay direct reaction in inverse kinematics :
Oak Ridge
DIC at Legnaro
ISOLDE laser
Experimental status in year 2010
-decay is still in the competition, good complementarities with DIC2
Fission + ISOL technique + post acceleration
BE(2)
Spectroscopic factors
DIC at Legnaro
Fusion-fission
Spontaneous fission
JYFLTRAP IGISOL
-decay Orsay
N=50 : recent experimental breakthrough
main nuclear mechanisms used :
-fragmentation of stable beams
-fission
-deep inelastic collisions
ESNT Workshop – Saclay – 3-5 May 2010 D. Verney
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Position of the problem : why should we worry about N=50 ?1
Why should we worry about N=50 ?
Historically from astrophysical considerations (and -decay experiments)
By Kratz et al. PRC 38 (1988)
Waiting point nucleus at N=50 80Zn
By Winger et al. PRC 36 (1987)
« »
« it’s a joke » M. Bernas, private communication (2001)
1
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ground state of 42Si N=28 is observed deformedB. Bastin et al., Phys. Rev. Lett. 99 (2007) 022503
spin-orbit origin
Why should we worry about N=50 ?
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“A full treatment of Hm shows no magicity at30Ne and 32Mg, while 34Si (or any other Si isotope)exhibits a clear shell effect. It just so happens that the fullHm reproduces the observed robustness of the SO closures,and the fragility of those of other origins. Whetherthey survive or not depends mainly on the possibility ofdeveloping quadrupole coherence in a given space.”
A.P. Zuker PRL 91 (2003)
O. Sorlin, M. Porquet Prog. Part. Nucl. Phys. 61 (2008) 602
N=50 gap extrapolation → 78Ni =3.0(5) MeV
100Sn
78Ni
from binding energies of the states below and above Z=28 and N=50
78Ni
56Ni
Z=28 gap extrapolation → 78Ni =2.5 MeV
Why should we worry about N=50 ?
44 46 48 50
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T. Otsuka et al. PRL95, 232502 (2005)
Why should we worry about N=50 ?
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extracted from J. Van de Walle et al PRC 70 (2009) 014309
Their is a N=50 shell effect with strong influence on nuclear structure close to 78Ni
Now, the real question becomes : how the shell gap associated to the N=50 magic number evolves towards 78Nior is there any evolution at all ?
N=50 shell gap evolution: prominent features from experimental data2
Evolution of the N=50 shell gap
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A Prévost et al. EPJ A 22 (2004) 391Medium/high spin states obtained from fusion/fission at the Vivitron (Euroball IV)
conclusion : N=50 shell gap decrease : yes
-
f7/2
p3/2
p1/2
f5/2
g9/2
28
50
40
f7/2
p1/2
g9/2
d5/2
p3/2f5/2
protons neutrons
-
+
+ +
Yrast structure studies (fusion-fission mechanism)
Yrast structure studies (spontaneous fission mechanism)
2 levels added : one of the two “must be” 1p-1h across N=50
T. Rza˛ca-Urban et al. PRC 76 (2007) 027302Medium/high spin states fed in 248Cm spontaneous fission
conclusion : N=50 shell gap decrease : yes
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Evolution of the N=50 shell gap
32
Y.H. Zhang et al. PRC 70 (2004) 024301Medium/high spin states fed in DIC at Legnaro (GASP)conclusion : N=50 shell gap decrease : no(same conclusion as Kamila)
84Se
SM calculation proton valence space
SM calculation proton valence space + neutron 1ph
f7/2
p3/2
p1/2
f5/2
g9/2
28
p1/2
g9/2
d5/2
protons neutrons
504 MeV
The gap used in the calculation has the good size
Yrast structure studies (deep inelastic mechanism)
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Evolution of the N=50 shell gap
Mass measurements (IGISOL Jyvaskyla)
Evolution of the N=50 shell gap
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Local minimum at Z=32
=S2n(52)-S2n(50)
(this quantity is the one traditionnally used to extract shell gaps from mass measurements)
Mass measurements (IGISOL Jyvaskyla)
Evolution of the N=50 shell gap
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Koopmans theorem :
gap in the single particle levels
50
j’
j
j’= Sn(Z,N)
but Sn(Z,N+1) is not a good prescription
for for the evaluation of j
one has to estimate j’ and jin the same
nucleus
NPA466 (1987) 189
j—j’ = Sn(Z,N) —Sn(Z,Nextr) then the good prescription becomes :
Mass measurements : what quantity is truly relevant for nuclear structure
Evolution of the N=50 shell gap
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Z
Sn(Z,N)-Sn(Z,N+1)
Sn(Z,N)-Sn(Z,Nextr)
N N+1 N+3 N+5 N+7
neutron number
using data taken from mass evaluation 2010 with kind authorization by G. Audi (AME2010 unpublished - G. Audi private communication)
d5/
2 –
g9/
2 (M
eV)
Ni Zn Ge Se Kr Sr
Duflo Zuker gap PRC59 (1999) 90Zr =4,7 MeV
Duflo Zuker gap 78Ni =5,7 MeV
gap
« rough »
« prescripted »
gap
pairi
ng g
ain(
MeV
)
neutron pairing gain = 2Sn(Z,N+1) —S2n(Z,N+2)
Ni Zn Ge Se Kr Sr
AME2010 extrapolation
Mass measurements : what quantity is truly relevant for nuclear structure
Evolution of the N=50 shell gap
loca
l min
imu
m a
t Z
=3
2
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conclusion : N=50 becomes somewhat “porous” relative to pair promotions (towards 78Ni)• what will be the result on structure? • what is the microscopic mechanism at play which could explain this local minimum ?
Zr
32
Evolution of the N=50 shell gap
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in particular : could provide a simple explanation to the Yrast structure behavior
Local minimum, not at mid distance Z=28-40
REX-ISOLDE
J. Van de Walle et al.PRL 99, 142501 (2007)
80Zn 82Ge84Se
86Kr
88Sr
90Zr
Evolution of the N=50 shell gap
and also the peculiar evolution of the E(2+) of the even-even N=50 isotones
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from -decay at ALTO
Evolution of the N=50 shell gap
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52
N=42
0.1 0.2 0.3 0.40
N=44
0.1 0.2 0.3 0.40
N=46
0.1 0.2 0.3 0.40
N=48
0.1 0.2 0.3 0.40
Ge isotopic chain
Evolution of the N=50 shell gap
and connection with collectivity
N=50
0.1 0.2 0.3 0.40
N=52
0.1 0.2 0.3 0.40
N=54
0.1 0.2 0.3 0.40
O Perru thesis Paris-Sud XI (2004) & J. Libert and M. Girod
private communicationD1S Gogny HFB calculation
GCM Bohr dynamics
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Ge
HFB + GCM (GOA)
Evolution of the N=50 shell gap
and connection with collectivity
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Collectivity close to 78Ni N=52 even-even nuclei
Z=
28 s
hell
closu
re
Z=
40 s
ubsh
ell
eff
ect
N=52
Evolution of the N=50 shell gap
and connection with collectivity
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deeper into nuclear structure close to 78Ni : valence space, single particle state effective sequence
3
Proton structure above 78Ni
K. Flanagan et al.
N=40 N=42 N=44 N=46 N=48 N=50
but already hinted at in the 80’s !!(from shell model, empirical interaction)
E (MeV)
-14,386
-13,233
-11,831
-7,121
40
f5/2
p3/2
p1/2
g9/2
Proton single particles
From Ji et Wildenthal Phys. Rev. C 38, 2849
(1988)
28
50
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Proton structure above 78Ni
shell model calculation :
Ji et Wildenthal Phys. Rev. C 38, 2849 (1988)
TBME and SP energies fitted to the data
Proton structure above 78Ni
E (MeV)
-14,386
-13,233
-11,831
-7,121
40
f5/2
p3/2
p1/2
g9/2
Proton single particles
28
50
Zn GeSe
Kr
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A. Pfeiffer et al. NPA 455 (1986) 381
Proton structure above 78Ni
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E (MeV)
-14,386
-13,233
-11,831
-7,121
40
f5/2
p3/2
p1/2
g9/2
Proton single particles
From Ji et Wildenthal Phys. Rev. C 38, 2849
(1988)
28
50
1236(9/2-)
hot subject - -decay experiment redone at ISOLDE and Oak Ridge
(same lines as us)
observed in -decay at Orsay (PARRNe)
D. Verney et al PRC 76 (2007) 054312
observed in DIC experiments at LegnaroG. De Angelis et al. NPA 787
(2007) 74c
Zn81
Sr88
Rb87
Kr86
Br85
Se84
As83
Ge82
Ga81
Zn80
Cu79
Ni78
Y89
Zr90
50
Zr91 Zr93Zr92 Zr92 Zr93 Zr94 Zr95 Zr96
Se85 Se86
As84
Ge83 Ge84
3 protons out of a 78Ni core
PARRNe
Proton structure above 78Ni
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0
200
400
600
800
1000
1200
1400
1600
1800
keV
3/2-5/2- 64 keV
0 keV
679 keV3/2-
1279 keV1/2-5/2- 1368 keV
3/2- 1897 keV
81Ga Z=31 N=50
351.1 keV
0 keV
802.8 keV
1236 keV
Experiment
empirical effective interaction : fit on a series of carefully selected states
Valence space N=50 closed & Z=28 closed (the doubly magical nature of 78Ni is assumed)The valence space is reduced to proton orbitals
Theory
Ji & Wildenthal, PRC 40, 389 (1989)
306.51 keV
83As Z=33 N=50
0 keV
711.66 keV
1193.7 keV1196.53 keV1256.76 keV1329.87 keV1415.11 keV1434.92 keV1525.52 keV
1804.76 keV
1977.9 keV
Experiment
(3/2-)
(5/2-)
Winger et al, PRC 38, 285 (1988)
1/2-
0 keV
189 keV
353 keV
589 keV
990 keV
1115 keV
1253 keV
1382 keV1455 keV
1643 keV
1845 keV1857 keV1879 keV1985 keV
5/2-
3/2-1/2-
3/2-
7/2-5/2-3/2-1/2-
5/2-9/2-
3/2-7/2-
9/2-
Theory
351.
1 ke
V45
1.7
keV
(5/2-)
(3/2-)
(3/2-)
(9/2-)
Proton structure above 78Ni
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Proton structure above 78Ni
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what to do ?
remember the textbooks and assume 1f5/2 is indeed the first proton orbit filled above 78Ni
formule générale
V J j n a b c n an n 1( )
2 b J( ) J 1( ) n j j 1( )[ ] c
n 2
2 j 3 n Talmi : <VJ>=
single particle (binding) energy
number of particles in the configuration
seniority number
for identical particles in j<=7/2 there exists a closed formula expressing the configuration energy (by Talmi)
82Ge 81Ga 80Zn
n=4, =00+
5/2+
3/2+
0+
2+
n=3, =1
n=3, =31492 keV
803 keV
n=2, =2
n=2, =0
BE(f5/2)= -13.576 MeV………JW give -14.386 MeV
E(9/2-) in 81Ga=1250 keV ……experiment :1236 keV
E(4+) in 80Zn=1809 keV ………experiment :?
1f5/2)4 1f5/2)3 1f5/2)2
but also extract : <f5/2f5/2|V|f5/2f5/2>J=0
<f5/2f5/2|V|f5/2f5/2>J=2 <f5/2f5/2|V|f5/2f5/2>J=4
Proton structure above 78Ni
f5/2 f5/2 f5/2 f5/2
f5/2 f5/2 f5/2 f5/2
f5/2 f5/2 f5/2 f5/2
pairing looks small !
back to the Ji Wildenthal proton-proton residual interaction :
Is it possible to find a simple cure to the interaction ?
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A.F. Lisetskiy et al.,
PRC 70 (2004)
Ji & Wildenthal,
PRC 40, 389 (1989)Z=31 N=50
JW+rustine
Proton structure above 78Ni
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1qp f5/2
1qp p3/2
v=3(f5/2)3
A.F. Lisetskiy et al.,
PRC 70 (2004)
Ji & Wildenthal,
PRC 40, 389 (1989)
Z=33 N=50
711 keV
JW+rustine
Proton structure above 78Ni
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1qp f5/2
1qp p3/2
1qp p1/2
Z=35 N=50
JW+rustineESNT Workshop – Saclay – 3-5 May 2010
D. Verney Page 34/52
1qp f5/2
1qp p3/2
1qp p1/2
Proton structure above 78Ni
2p3/2
1f5/2
81Ga Z=31 N=50
2p3/2
1f5/2
83As Z=33 N=50
2p3/2
1f5/2
85Br Z=35 N=50
2p1/22p1/2 2p1/2
the conclusion is : this proton sequence is confirmed
E (MeV)
-14,386
-13,233
-11,831
-7,121
40
f5/2
p3/2
p1/2
g9/2
Proton single particles
From Ji et Wildenthal Phys. Rev. C 38, 2849
(1988)
28
50
and the observed structure of the odd-proton N=50 isotones simply (and naturally) reflects the change of the Fermi level
Proton structure above 78Ni
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Neutron structure above 78Ni
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O. Sorlin, M. Porquet Prog. Part. Nucl. Phys. 61 (2008) 602
centroides from (d,p)
g7/2 goes up
91Zr
89Srg7/2 nearly constant
K. Sieja et al. PRC 79, 064310 (2009)EXPERIMENT
THEORY (SM)
g7/2 goes down
SM calculations in valence space above 78Ni
From Duflo Zuker
PRC 59, R2347 (1999)
E (MeV)
0.00
1.00
2.453.04
82
Neutron single particles
From T.A. Hughes
Phys. Rev. 181, 1586 (1969)
d5/2
d3/2
s1/2
g7/2
50
in 89Sr
? h11/2
but in fact the problem of the position of h11/2 remains unsolved → need for the observation of negative parity Yrast states in N=51
Neutron structure above 78Ni
ESNT Workshop – Saclay – 3-5 May 2010 D. Verney
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experiment and theory agree close to stability
Ga84
247.81/2+
observé en2H(82Ge,p)83Ge à Oak
RidgeThomas et al.
PRC 71 (2005) 021302
observé en décroissance -decay à PARRNe
O. Perru et al.EPJ A 28 (2006) 307
et thèse Paris 11
Ga83
Sr88
Rb87
Kr86
Br85
Se84
As83
Ge82
Ga81
Zn80
Cu79
Ni78
Y89
Zr90
50
Zr91 Zr93Zr92 Zr92 Zr93 Zr94 Zr95 Zr96
Se85 Se86
As84
Ge83 Ge84
4 protons + 1 neutron au dessus de 78Ni
observé en décroissance n avec ALTO
M. Lebois et al.PRC 80 (2009) 044308
et thèse Paris 11
2d5/2
3s1/2
(3/2,5/2+)
7/2+
Neutron structure above 78Ni
experiment and theory agree close to stability ?
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(1/2+)?
E(2+) of the even-even core(semi-magic N=50)
Neutron structure above 78Ni
systematics for the odd-neutron N=51 isotones
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Even-even semi-magic core
single particle
Q>0Q=0 Q<0
2+1 2d5/2
J=1/2
J=3/2 J=9/2
J=5/2
J=7/2
Neutron structure above 78Ni
ESNT Workshop – Saclay – 3-5 May 2010 D. Verney
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(1/2+)?
N=51
E(2+) of the even-even core(semi-magic N=50)
Neutron structure above 78Ni
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(1/2+)?
S=0.84
non-stripped
S=0.49
S=0.016
d3/2
g7/2
S=0.06±0.02S=0.77±0.27
from J. S. Thomas et al. PRC 76, 044302 (2007)
not observed in (d,p)
Neutron structure above 78Ni
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first 7/2 state is 2+*d5/2 coupled state, g7/2 is higher in energy
(1/2+)?
s1/2
d’après J. S. Thomas et al. PRC 76, 044302 (2007)
S=0.905
S=0.46S=0.31
S=0.18non-stripped
not observed (dp)
S=0.52s1/2 s1/2
s1/2
down sloping of the s1/2 is firmly established
Neutron structure above 78Ni
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Core – particle coupling model
Even-even semi-magic core
L. S. Kisslinger & R. A. Sorensen Rev. Mod. Phys., 35, 853, (1963)
Thankappan & TruePhys. Rev. B, 137, 793 (1965)
Neutron single particle
Core excitation energies taken from experiment : E(2+)
Parameters :
Vector space :0+1 2d5/22+1 2d5/22+1 3s1/2Etc…
= =
Quadrupole moment of the 2+ state
Phenomenological model with a clear underlying physical image. All parameters with straightforward interpretation:
Example : harmonic vibrator : Q2+=0 2=0
how to extract (at least approximately) effective single particle energies when no direct reaction data is available ? use a simple empirical model
Neutron structure above 78Ni
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unperturbed theory experiment
0+ d5/2
0+ s1/2
2+ d5/2
0+ d3/2
0+ g7/2
02+ d5/2
22+ d5/2
2+ s1/2
52
12
32
72
52
12
32
52
72
92
52
52
72
12
72
72
52
52
32
92 3
2
92
32
32
12
72
12
32
52
72
92
12
0.26ps
0.19ps0.10ps0.21ps
0.11ps
0.16ps
0.02ps0.09ps
1.85ps
S=0.79
S=0.905
S=0.091
S=0.46
S=0.34
S=0.74
S=0.88
S=0.78
S=0.016
S=0.053S=0.64
S=0.15
S=0.84
89Sr3
25
2
>1 ps
1/2 calculated assuming only M1 and E2 transitions
e()=1 and gs=0.6 gsfree
2=0.56 (M1+E2)
2=0.87 (M1+E2)
Qexp= -0.28(3) eb / -0.32(2) eb exp= -1.1481 n.m.
Qcalc= -0.27 eb calc= -1.020 n.m.
experimentcore-particle couplingnot included in the model space
unperturbed theory experiment
0+ d5/2 52
52
52S=0.90 S=0.56
0+ s1/2 12
2+ d5/2 12
32
52
72
92
0+ d3/2 32
0+ g7/2 72
4+ d5/2 32
52
72
92 2
112
13
22+ d5/2 1
23
25
27
29
2
2+ s1/23
25
2
12
32
92
72
52
32
12
72
52
S=0.68
S=0.20
S=0.02
S=0.06
S=0.43
S=0.27
S=0.84
S=0.03
72
32
52
92
S=0.4612
S=0.23
92
32
52S=0.02
32
52
S=0.0912S=0.18
112
32
52S=0.3
S=0.49 72
87Kr
85Se
0+ d5/2
0+ s1/2
2+ d5/2 12
32
52
72
92
02+ d5/2
12
52
52
4+ d5/2 32
52
72
92 2
112
13
2+ s1/2 32
52
0+ d3/2
0+ g7/2
32 7
2
12
52
unperturbed theory experiment
72
92
52
32
32
72
12
52
12
72
92
32
52
12 ?
12
92
72 ?-
112
32
52
32
12
92
32
52
72
112
132
32
52
72?
?
?
S=0.38
S=0.31
S=0.77 or 0.06
S=0.90
S=0.86
S=0.09
g7/2
d3/2
d5/2
s1/2
Neutron structure above 78Ni
on the overall neutron single particle sequence appears to be :
ESNT Workshop – Saclay – 3-5 May 2010 D. Verney
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d5/2
s1/2
d3/2
g7/2
MeV
N=
58
?
if we extract the effective single particle energies using the core-particle coupling model :
Neutron structure above 78Ni
ESNT Workshop – Saclay – 3-5 May 2010 D. Verney
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conclusion : appearance of a new neutron subshell gap close to 78Ni ?
d5/2
s1/2
d3/2
g7/2
MeV
?
N=
58
?
is there a simple explanation to the s1/2 down sloping ?
Neutron structure above 78Ni
ESNT Workshop – Saclay – 3-5 May 2010 D. Verney
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80 10060is there a simple explanation to the s1/2 down sloping ?
Neutron structure above 78Ni
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s1/2 s1/2s1/2
s1/2s1/2
g7/2
d3/2
Neutron structure above 78Ni
K. Sieja private communication (yesterday)
ESNT Workshop – Saclay – 3-5 May 2010 D. Verney
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Proton single particles
d5/2
d3/2
s1/2
g7/2
Neutron single particles
f5/2
p3/2
p1/2
g9/2
Single particle sequence in 78Ni mean-
field
Conclusion
What we think we have understood :
1
2 the N=50 shell gap is effective towards 78Nithough it varies a little in amplitude impact on collectivity
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