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E. Sahin, G. de Angelis

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Title: E. Sahin, G. de Angelis


1
Breaking of the Isospin Symmetry and CED in the
A?70 mass region the Tz-1 70Kr
E. Sahin, G. de Angelis
2
NZ A70 Nuclei 70Se, 70Br, 70KrCharacteristic
features can be extracted through CED?
  • Strong Collective Effects (NpNn)
  • Shape co-existence
  • Strong Collective Effects (NpNn) (Shape
    co-existence)
  • Nuclear Isospin Symmetry
  • A70 isobaric nuclei has an unusual behavior of
    the CED, a negative tendency with increasing spin.

3
Mirror Nuclei Properties
Charge symmetry ?pp?nn Charge independence ?
pp?nn?pn Ground state masses!!! i)n-p mass
difference ii)Coulomb energy difference
When the Coulomb interactions between protons are
ignored, the nuclear force is perfectly
charge-symmetric and charge-independent
4
Mirror Nuclei Properties
Charge symmetry ?pp?nn Charge independence ?
pp?nn?pn Ground state masses!!! i)n-p mass
difference ii)Coulomb energy difference
When the Coulomb interactions between protons are
ignored, the nuclear force is perfectly
charge-symmetric and charge-independent
5
Coulomb Energy Difference (CED)
CED(Jp)EJp(Tzlt)-EJp(Tzgt)
TzgtTzlt1
But in reality, Isospin non-conserving
interactions with Coulomb force break the isospin
symmetry!!
A plot of CED with increasing angular momentum
will be a good tool to study the collective
properties of the nuclei N?/Z
M.A. Bentley, S. Lenzi, Prog.Part.Nucl.Phys.
(2006)
D.D. Warner et al.,Nature Physics 2, 311 (2006)
6
Coulomb Energy Difference (CED)
Negatif CED values in A70 isobars
CED(6)-37 keV
CED(4)-36 keV
CED(2)-11 keV
Tzlt
Tzgt
N. Singh et al., Phys.Rev.C75, 061301 (2007)
70BrG.de Angelis Eur. Phys.J.A.12,51 (2001)
70SeJ. Ljungvall et al., PRL 100, 102502 (2008)
7
Calculated CED Values
Deformed liquid drop model
S.E. Larsson, Phys.Scri. 8,17 (1973)
If ?2 changes from -0.3 to 0.35 ?CED ? -7 keV
R.Sahu et al, JPG 13, 603 (1987)
Def. Shell Model Calculations Stretch in ?2 from
0.18 to 0.33 ?CED ? -75 keV
Assume that the shape changes in the analogue
nuclei are the same
8
Excited Vampire Predictions
Microscopic description of mirror nuclei in the
A70 mass region Shape coexistence and mixing
Isospin symmetric G-matrix(A) Coulomb
Interaction between valence protons
Mixing ratios
p/o
o/p
95/4
81/18
70/29
84/16
Exp. data 66As G. de Angelis (to be submitted)
70BrG.de Angelis Eur.Phys.J.A.12,51 (2001)
A.Petrovici Nuc.Phy. A 728, 396 (2003)
70SeJ. Ljungvall et al., PRL 100, 102502 (2008)
9
Excited Vampire Predictions
Vampire Calculations First minimum is
predominantly prolate in 70Br First minimum is
predominantly oblate in 70Se
Mixing ratios
p/o
o/p
80/20
39/61
58/41
64/36
59/41
59/41
64/36
57/42
A.Petrovici Nuc.Phy. A 728, 396 (2003)
10
Excited Vampire Predictions
The comparison of the microscopic structure of
the mirror nuclei 70Se and 70Kr
The Coulomb interaction is included for the
valence protons The mirror nuclei 70Se-70Kr have
different shapes in their ground state
A.Petrovici private comm.
11
Excited Vampire Predictions
B(E2) Values e2fm4
Ji ?Jf 70Kr 70Se
2 ????0 603 492
4 ????? 864 713
6 ????? 933 779
342
Exp.
J. Ljungvall et al.
12
Experiment
1neutron-knockout reaction 71Kr 9Be ?70Kr
Target
1neutron
70Kr
71Kr
9Be
56Fe
Identification of the 2?0 transition 71Kr
9Be ? 70Kr Lifetime measurement 71Kr
56Fe ? 70Kr
13
Beam Production
LISE calculations
Secondary beam 71Kr 100 pps at 170 MeV/u
AGATA
Primary beam 78Kr 1.3x1010 pps
LISE calculations
LISE calculations
Be target 5000 mg/cm2
Be target 1000 mg/cm2
14
Identification of the 2 ? 0 transition
  • 71Kr on 9Be target
  • dtarget1 g/cm2
  • Ibeam100 pps
  • ?2 mb (for 1n knock-out)
  • ??20 (1 MeV)
  • N?200 day-1

1-2 days of beamtime
15
Lifetime determination
2
950
  • 71Kr on 56Fe target
  • dtarget700 mg/cm2
  • Ibeam100 pps
  • ?2.7 mb (for 1n knock-out)
  • ??20 (1 MeV)
  • N?35 day-1

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18
955 keV
19
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