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E. Sahin, G. de Angelis Breaking of the Isospin Symmetry and CED in the A70 mass region: the T z =-1 70 Kr

E. Sahin, G. de Angelis

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Breaking of the Isospin Symmetry and CED in the A  70 mass region: the T z =-1 70 Kr. E. Sahin, G. de Angelis. N~Z A=70 Nuclei: 70 Se, 70 Br, 70 Kr Characteristic features can be extracted through CED?. Strong Collective Effects (N p =N n ) Shape co-existence. - PowerPoint PPT Presentation

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Page 1: E. Sahin, G. de Angelis

E. Sahin, G. de Angelis

Breaking of the Isospin Symmetry and CED in the A70 mass region: the T

z=-1 70Kr

Page 2: E. Sahin, G. de Angelis

N~Z A=70 Nuclei: 70Se, 70Br, 70KrCharacteristic features can be extracted through CED?

Strong Collective Effects (Np=Nn) (Shape co-existence)Nuclear Isospin Symmetry

A=70 isobaric nuclei has an unusual behavior of the CED, a negative tendency with increasing spin.

Strong Collective Effects (Np=Nn)

Shape co-existence

Page 3: E. Sahin, G. de Angelis

Coulomb Energy Difference (CED)

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

D.D. Warner et al.,Nature Physics 2, 311 (2006)

M.A. Bentley, S. Lenzi, Prog.Part.Nucl.Phys. (2006)

Tz>=Tz<+1CED(Jπ)=E

Jπ(T

z<)-E

Jπ(T

z>)

Page 4: E. Sahin, G. de Angelis

Negatif CED values in A=70 isobars

CED(2+)=-11 keV

CED(4+)=-36 keV

CED(6+)=-37 keV

Tz< Tz>70Br:G.de Angelis Eur. Phys.J.A.12,51 (2001)

N. Singh et al., Phys.Rev.C75, 061301 (2007)

Coulomb Energy Difference (CED)

70Se:J. Ljungvall et al., PRL 100, 102502 (2008)

Page 5: E. Sahin, G. de Angelis

Excited Vampire Predictions Microscopic description of mirror nuclei in the A=70 mass region

Shape coexistence and mixing

70/29

p/o o/p

81/18

95/4

84/16

Mixing ratios

A.Petrovici Nuc.Phy. A 728, 396 (2003)70Br:G.de Angelis Eur.Phys.J.A.12,51 (2001)

Isospin symmetric G-matrix(A) + Coulomb Interaction between valence protons

70Se:J. Ljungvall et al., PRL 100, 102502 (2008)

Exp. data 66As: G. de Angelis (to be submitted)

Page 6: E. Sahin, G. de Angelis

Excited Vampire Predictions

Vampire Calculations:

First minimum is predominantly prolate in 70BrFirst minimum is predominantly oblate in 70Se

A.Petrovici Nuc.Phy. A 728, 396 (2003)

59/41

p/o o/p

58/41

80/20

64/36

Mixing ratios

59/41

64/36

39/61

57/42

Page 7: E. Sahin, G. de Angelis

Excited Vampire Predictions

The Coulomb interaction is included for the valence protons

The mirror nuclei 70Se-70Kr have different shapes in their ground state

The comparison of the microscopic structure of the mirror nuclei 70Se and 70Kr

A.Petrovici private comm.

Page 8: E. Sahin, G. de Angelis

Excited Vampire Predictions

B(E2) Values B(E2) Values ee22fmfm44

Ji J

f

70Kr 70Se

2+ 0+ 603 492

4+ + 864 713

6+ + 933 779

342 Exp.J. Ljungvall et al.

Page 9: E. Sahin, G. de Angelis

Experiment1neutron-knockout reaction: 71Kr + 9Be →70Kr

71Kr 9Be70Kr

1neutronTarget

56Fe

Identification of the 2+→0+ transition : 71Kr + 9Be → 70Kr Lifetime measurement : 71Kr + 56Fe → 70Kr

Page 10: E. Sahin, G. de Angelis

Beam Production

LISE++ calculations: LISE++ calculations: Primary beam78Kr 1.3x1010 pps

Be target5000 mg/cm2

Secondary beam 71Kr ~ 100 pps at 170 MeV/u

Be target1000 mg/cm2

AGATA

Page 11: E. Sahin, G. de Angelis

Identification of the 2+ → 0+ transition

71Kr on 9Be targetd

target=1 g/cm2

Ibeam

=100 pps=2 mb (for 1n knock-out) =20% (1 MeV) N=200 day-1

1-2 days of beamtime

Page 12: E. Sahin, G. de Angelis

Lifetime determination

71Kr on 56Fe targetd

target=700 mg/cm2

Ibeam

=100 pps=2.7 mb (for 1n knock-out) =20% (1 MeV) N=35 day-1

2+

0+

950

Page 13: E. Sahin, G. de Angelis
Page 14: E. Sahin, G. de Angelis
Page 15: E. Sahin, G. de Angelis

955 keV

Page 16: E. Sahin, G. de Angelis