Insights into Seniority Isomers in Nuclear Physics

 
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Ashok Kumar Jain
Department of Physics
Indian Institute of Technology,
 
Roorkee
 
O
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Atlas of Nuclear Isomers ~2450 Isomers
Seniority isomers: Where and why??
Semi-magic seniority isomers
Similar excitation energy systematics
Similar half-life systematics
Will large scale shell model calculations be able to explain this??
Alignment properties of the intruder orbital
Neutron-rich Sn-isomers beyond 
132
Sn and the effective
interactions
How a small change in TBME changes seniority mixing?
Summary
 
2
 
3
Lower limit of the
half-life : 
10 ns
 
Total no. of isomers =
2448
 
Even-even = 414
Odd- odd = 800
Even-odd = 640
Odd-even = 594
 
4
 
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Any interaction between
identical fermions in single-
j
shell conserves seniority if
j
7/2.
The seniority is conserved up
to j=11/2 in Sn-isomers after
the mid-shell, where the
mixing of other orbitals is
negligible.
 Particle number
independent energy
variation.
 Constant pairing gap.
 
5
In the 1940s Racah had
introduced the concept in
the atomic context. 
The
third of his seminal series
contains the first mention
of seniority.
It has been adopted in
nuclear physics in a
similar fashion.
Seniority (
v
) may be
defined as the number of
unpaired nucleons.
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?
Seniority: number of unpaired nucleons
Semi-magic isomers : good place to find seniority isomers.
E2 transitions between same seniority states vanish,
when the valence shell is close to the half-filled.
     [
Ref
: A. De Shalit and I. Talmi, Nuclear Shell Theory (Dover
Publications, New York, 1963). ]
6
7
Same spin-parity isomers
11/2
, 10
+
 and 27/2
Same available valence-space
(50-82)
Observed similar kind of
systematic
Half-life
Excitation energies
High-j h
11/2
 orbital plays the
dominant role.
Fascinating to explore their
structural properties……
W
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Z
=
5
0
,
N
=
8
2
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?
?
 
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Z
=
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s
Nushell  
[Ref.: B. A. Brown and W. D. M. Rae, Nushell @MSU, MSU-NSCL report (2007). ]
SN100PN: 
0g
7/2
, 1d
5/2
, 0h
11/2
, 1d
3/2
, and 2s
1/2 
 orbitals 
[Ref.: 
B. A. Brown, 
et al., Phys. Rev. C 71, 044317 (2005). ]
 
8
 
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N
=
8
2
 
i
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s
To be published.
 
g
7/2
, d
5/2
 
h
11/2
 
v
=
1
 
v
=
4
, 
5
 
v
=
2
, 
3
 
v
=
1
SN100PN: 
0g
7/2
, 1d
5/2
, 0h
11/2
, 1d
3/2
, and 2s
1/2 
 orbitals 
[Ref.: 
B. A. Brown, 
et al., Phys. Rev. C 71, 044317 (2005). ]
 
9
 
0
 
Z
=
5
0
 
a
n
d
 
N
=
8
2
 
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.
 
10
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e
n
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g
i
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s
h
11/2
 orbital comes
late in the N=82
isomers compared to
the Z=50 isomers.
Therefore, the change
in the seniority takes
place at different
neutron/proton
numbers in the two
chains.
11
 
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12
 
Expt.
 
Theo.
Sn-isotopes
 
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N
=
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2
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13
 
Theo.
On the basis of the similar behavior in the Z=50 and the N=82 chains,
we can make reliable predictions for some new isomers.
 
Z
=
5
0
 
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Z
=
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2
 
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i
13/2
 orbital
 
h
11/2
 orbital
 
14
 
High seniority
 
High seniority
 
low seniority
 
low seniority
 
f
5/2, 
p
3/2, 
p
1/2 
and i
13/2
 
g
7/2, 
d
5/2 
and h
11/2
 
 Different intruder orbitals
 Mirror experimental energy systematics
 Will large scale scale shell model calculations be able to explain this?
 
Nushell
  
[Ref.: B. A. Brown and W. D. M.
Rae, Nushell @MSU, MSU-NSCL report
(2007). ]
 
SN100PN: 
0g
7/2
, 1d
5/2
, 0h
11/2
, 1d
3/2
,
and 2s
1/2 
 orbitals
 
[Ref.: 
B. A. Brown,
et al., Phys. Rev. C 71, 044317 (2005). ]
KHHE:
 
1h
9/2
, 2f
7/2
, 1i
13/2,
 3p
3/2
, 2f
5/2
,
and 3p
1/2
 
orbitals 
[Ref.: 
E. K.
Warburton and B. A. Brown, Phys. Rev.
C 43, 602 (1991). 
]
 
Our calculations are able to
reproduce the experimental
systematics quite well except for the
fact that the relative gap of the
isomeric states is systematically
smaller due to the applied
truncations for both the chains.
 
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To be published.
 
15
 
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1
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136,138
Sn measured
for the first time.
 
Interpretation in
terms of 
v
=2 and
v
=4 seniority
mixing.
 
6
+
 isomer has been
assigned as 
v
=2
isomer.
 
16
 
Simpson 
et al.
 PRL 113, 132502 (2014)
 
Realistic V
lowk
 interaction
does not reproduce the expt.
BE2 value for 
136
Sn, even
when the core excitations are
included.
 
A reduction of diagonal and
non-diagonal 
υ
f
7/2
2 
TBME by
150 keV generates a seniority-
mixed 4
+ 
state equivalent to
the reduced pairing, and
reproduces the expt. data.
 
17
 
S
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m
p
s
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t
 
a
l
.
 
P
R
L
 
1
1
3
,
 
1
3
2
5
0
2
 
(
2
0
1
4
)
 
6
+
 
i
s
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e
r
s
 
i
n
 
1
3
4
-
1
3
8
S
n
 
18
B. Maheshwari, A. K. Jain and P. C. Srivastava, Phys. Rev. C 
91
, 024321 (2015)
 
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m
i
x
i
n
g
?
Large nonzero
value =  
Seniority
mixing
If the seniority is
conserved then the BE2
should be almost zero at
the mid-shell, 
136
Sn.
 
On modifying the
interaction , BE2
increases 
seniority
mixing increases.
 
Active orbital: f
7/2
 orbital
 
19
 
RCDBMO: modified RCDB by reducing the diagonal and non-diagonal 
υ
f
7/2
2  
TBME by 25 keV.
 
S
u
m
m
a
r
y
 
Data of about 
2450
 isomers with lower limit as 
10 ns
 have been
collected and systematized in different ways.
This helps us in understanding many universal and novel features of
nuclear isomers.
It is interesting to observe that the semi-magic seniority isomers show
identical energy and half-life systematics.
Large scale shell model calculations are able to reproduce the
systematics quite well.
Their systematic studies provide a global understanding of the known
isomers and predictions of unknown isomers.
The systematic studies in long chain of isomers are also able to shed
light on the nature of the effective interactions, particularly in
neutron/proton-rich regions.
 
 
 
 
20
 
T h a n k s
 
21
Slide Note

Good evening to all!!

The title of my presentation is “atlas of nuclear isomers and the role of seniority”, under the supervision of Prof. A. K. Jain.

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Explore the concept of seniority isomers in nuclear physics, delving into topics like semi-magic isomers, alignment properties of intruder orbitals, and the role of seniority mixing. Discover the significance of Z=50, N=82 isomers and the structural properties associated with them. Uncover the essence of seniority as the number of unpaired nucleons and its conservation up to specific shell models.

  • Seniority Isomers
  • Nuclear Physics
  • Semi-Magic Isomers
  • Intruder Orbitals
  • Z=50 N=82

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  1. Semi Semi- -magic seniority isomers magic seniority isomers and and the effective interactions the effective interactions Ashok Kumar Jain Department of Physics Indian Institute of Technology, Roorkee

  2. Outline Atlas of Nuclear Isomers ~2450 Isomers Seniority isomers: Where and why?? Semi-magic seniority isomers Similar excitation energy systematics Similar half-life systematics Will large scale shell model calculations be able to explain this?? Alignment properties of the intruder orbital Neutron-rich Sn-isomers beyond 132Sn and the effective interactions How a small change in TBME changes seniority mixing? Summary 2

  3. Fission/ Shape isomers K- isomers Spin isomers Shape isomers 3

  4. Lower limit of the half-life : 10 ns Total no. of isomers = 2448 Even-even = 414 Odd- odd = 800 Even-odd = 640 Odd-even = 594 4 To be published in Nuclear Data Sheets

  5. What is seniority? In the 1940s Racah had introduced the concept in the atomic context. The third of his seminal series contains the first mention of seniority. It has been adopted in nuclear physics in a similar fashion. Seniority (v) may be defined as the number of unpaired nucleons. Particle number independent energy variation. Constant pairing gap. Any identical fermions in single-j shell conserves seniority if j 7/2. The seniority is conserved up to j=11/2 in Sn-isomers after the mid-shell, where the mixing of other orbitals is negligible. interaction between 5

  6. Seniority isomers: Where to find and why?? Seniority: number of unpaired nucleons Semi-magic isomers : good place to find seniority isomers. E2 transitions between same seniority states vanish, when the valence shell is close to the half-filled. [Ref: A. De Shalit and I. Talmi, Nuclear Shell Theory (Dover Publications, New York, 1963). ] C.T. Zhang et al., PRC 62, 057305 6

  7. Why Z=50, N=82 isomers?? Same spin-parity isomers 11/2 , 10+ and 27/2 Same available valence-space (50-82) Observed similar kind of systematic Half-life Excitation energies High-j h11/2 orbital plays the dominant role. Fascinating to explore their structural properties 7

  8. Calculated and experimental excitation energies for the Z=50 isomers Energy transition ~ 4 MeV ~ 3 MeV v=4, 5 g7/2, d5/2 h11/2 v=2, 3 v=1 v=1 SN100PN: 0g7/2, 1d5/2, 0h11/2, 1d3/2, and 2s1/2 orbitals [Ref.: B. A. Brown, et al., Phys. Rev. C 71, 044317 (2005). ] 8 Nushell [Ref.: B. A. Brown and W. D. M. Rae, Nushell @MSU, MSU-NSCL report (2007). ]

  9. Calculated and experimental excitation energies for the N=82 isomers Energy transition To be published. ~ 4 MeV ~ 3 MeV 0 g7/2, d5/2 v=4, 5 h11/2 v=2, 3 v=1 v=1 SN100PN: 0g7/2, 1d5/2, 0h11/2, 1d3/2, and 2s1/2 orbitals [Ref.: B. A. Brown, et al., Phys. Rev. C 71, 044317 (2005). ] 9

  10. Z=50 and N=82 seniority isomers the configuration lists the unpaired neutrons in the respective orbitals. 10+ 11/2- Isotope Seniority Configuration Isotope Seniority 27/2- Seniority Configuration Configuration 102Sn 104Sn 106Sn 108Sn 110Sn 112Sn 2 4 4 2 2 2 2 h11/22 g7/22, d5/22 g7/22, d5/22 h11/22 h11/22 h11/22 h11/22 103Sn 105Sn 107Sn 109Sn 111Sn 113Sn 1 1 1 1 1 1 1 h11/21 h11/21 h11/21 h11/21 h11/21 h11/21 h11/21 3 5 5 5 5 3 3 h11/23 g7/22, d5/22, h11/21 g7/22, d5/22, h11/21 g7/22, d5/22, h11/21 g7/22, d5/22, h11/21 h11/23 h11/23 114Sn 115Sn 10+ Seniority 11/2- Seniority 27/2- Seniority Isotone Configuration Isotone Configuration Configuration 134Te 136Xe 138Ba 140Ce 142Nd 144 Sm 146Gd 2 4 4 4 4 4 2 h11/22 g7/22, d5/22 g7/22, d5/22 g7/22, d5/22 g7/22, d5/22 g7/22, d5/22 h11/22 135I 137Cs 139La 141Pr 143Pm 145Eu 147Tb 1 1 1 1 1 1 1 h11/21 h11/21 h11/21 h11/21 h11/21 h11/21 h11/21 3 5 5 5 5 5 3 h11/23 g7/22, d5/22, h11/21 g7/22, d5/22, h11/21 g7/22, d5/22, h11/21 g7/22, d5/22, h11/21 g7/22, d5/22, h11/21 h11/23 10

  11. Single-particle energies h11/2 orbital comes late in the N=82 isomers compared to the Z=50 isomers. N=82 isomers Therefore, the change in the seniority takes place at different neutron/proton numbers in the two chains. Z=50 isomers 11

  12. Alignment of the h11/2 orbital after the mid-shell Isotope E (2+ 0+) E (12+ 10+) Isotope E (15/2- 11/2-) E (31/2- 27/2-) R (15: 2) R (31: 12) 112 Sn 1.257 113 Sn 1.168 0.9295 Sn-isotopes 114 Sn 1.300 115 Sn 1.312 1.0089 116 Sn 1.294 117 Sn 1.279 0.9887 Expt. 118 Sn 1.230 1.237 119 Sn 1.220 1.179 0.9921 0.953 120 Sn 1.171 1.190 121 Sn 1.151 1.083 0.9827 0.910 122 Sn 1.141 1.103 123 Sn 1.107 1.043 0.9706 0.946 124 Sn 1.132 1.047 125 Sn 1.088 0.924 0.9614 0.883 Isotope E (2+ 0+) E (12+ 10+) Isotope E (15/2- 11/2-) E (31/2- 27/2-) R (15: 2) R (31: 12) 114Sn 1.508 0.878 0.988 0.939 0.888 1.093 1.123 1.197 0.853 1.12 1.007 0.905 0.822 0.937 0.919 0.977 115Sn 1.463 0.889 0.942 0.872 0.827 0.994 1.014 1.152 0.782 0.921 1.011 0.871 0.841 0.905 0.871 0.970 1.012 0.953 0.928 0.931 0.910 0.903 0.962 0.916 0.822 1.004 0.962 1.023 0.966 0.948 Theo. 116Sn 117Sn 118Sn 119Sn 120Sn 121Sn 122Sn 123Sn 124Sn 125Sn 126Sn 128Sn 127Sn 129Sn 12 ~1 value

  13. Similar alignments in the N=82 isotones Isotone E (2+ 0+) E (12+ 10+) Isotone E (15/2- 11/2-) E (31/2- 27/2-) R (15: 2) R (31: 12) 146 Gd 2.212 0.994 147 Tb 2.152 0.920 0.972 0.925 148 Dy 1.088 1.293 149 Ho 1.182 1.501 1.086 1.160 150 Er 1.162 1.090 151 Tm 1.067 1.000 0.918 0.917 152 Yb 1.102 0.981 153 Lu 1.006 0.902 0.913 0.919 154 Hf 1.068 0.923 155 Ta 0.974 0.845 0.912 0.915 156 W 1.279 1.035 157 Re 1.135 0.878 0.887 0.848 Theo. 158 Os 1.279 1.002 ~1 value On the basis of the similar behavior in the Z=50 and the N=82 chains, we can make reliable predictions for some new isomers. 13

  14. Z=50 and Z=82 seniority isomers coming from their respective intruder orbitals High seniority i13/2 orbital f5/2, p3/2, p1/2 and i13/2 low seniority High seniority h11/2 orbital g7/2, d5/2 and h11/2 low seniority Different intruder orbitals Mirror experimental energy systematics Will large scale scale shell model calculations be able to explain this? 14

  15. Large scale shell model calculations Nushell[Ref.: B. A. Brown and W. D. M. Rae, Nushell @MSU, MSU-NSCL report (2007). ] SN100PN: 0g7/2, 1d5/2, 0h11/2, 1d3/2, and 2s1/2orbitals [Ref.: B. A. Brown, et al., Phys. Rev. C 71, 044317 (2005). ] To be published. KHHE:1h9/2, 2f7/2, 1i13/2, 3p3/2, 2f5/2, and 3p1/2 orbitals Warburton and B. A. Brown, Phys. Rev. C 43, 602 (1991). ] [Ref.: E. K. Our reproduce systematics quite well except for the fact that the relative gap of the isomeric states is systematically smaller due to truncations for both the chains. calculations are able to the experimental the applied 15

  16. Neutron-rich seniority isomers beyond 132Sn and the effective interactions 136,138Sn measured for the first time. Interpretation in terms of v=2 and v=4 seniority mixing. 6+ isomer has been assigned as v=2 isomer. Simpson et al. PRL 113, 132502 (2014) 16

  17. Simpson et al. PRL 113, 132502 (2014) Realistic Vlowk interaction does not reproduce the expt. BE2 value for 136Sn, even when the core excitations are included. A reduction of diagonal and non-diagonal f7/22 TBME by 150 keV generates a seniority- mixed 4+ state equivalent to the reduced pairing, and reproduces the expt. data. 17

  18. 6+ isomers in 134-138Sn B. Maheshwari, A. K. Jain and P. C. Srivastava, Phys. Rev. C 91, 024321 (2015) 18

  19. How a small change in TBME changes seniority mixing? If the seniority is conserved then the BE2 should be almost zero at the mid-shell, 136Sn. Large nonzero value = Seniority mixing On modifying the interaction , BE2 increases seniority mixing increases. Active orbital: f7/2 orbital RCDBMO: modified RCDB by reducing the diagonal and non-diagonal f7/22 TBME by 25 keV. 19

  20. Summary Data of about 2450 isomers with lower limit as 10 ns have been collected and systematized in different ways. This helps us in understanding many universal and novel features of nuclear isomers. It is interesting to observe that the semi-magic seniority isomers show identical energy and half-life systematics. Large scale shell model calculations are able to reproduce the systematics quite well. Their systematic studies provide a global understanding of the known isomers and predictions of unknown isomers. The systematic studies in long chain of isomers are also able to shed light on the nature of the effective interactions, particularly in neutron/proton-rich regions. 20

  21. T h a n k s 21

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