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Sarah Naimi Nuclear structure oddities from ISOLTRAP mass measurements CSNSM Orsay & ISOLTRAP/ISOLDE CERN ISOLDE Workshop 2009

Sarah Naimi

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ISOLDE Workshop 2009. Nuclear structure oddities from ISOLTRAP mass measurements. Sarah Naimi. CSNSM Orsay & ISOLTRAP/ISOLDE CERN. ISOLDE Workshop 2009. Plan Experimental setup Shell closure at N = 40 Mn isotopes masses Kr isotopes : deformation from N = 60? Summary and outlook. - PowerPoint PPT Presentation

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Page 1: Sarah Naimi

Sarah Naimi

Nuclear structure oddities from ISOLTRAP mass measurements

CSNSM Orsay & ISOLTRAP/ISOLDE CERN

ISOLDE Workshop 2009

Page 2: Sarah Naimi

ISOLDE Workshop 2009

Plan • Experimental setup

• Shell closure at N = 40

• Mn isotopes masses

• Kr isotopes : deformation from N = 60?

• Summary and outlook

Page 3: Sarah Naimi

B = 4.7 T

B = 5.9 T

2 m

G. Bollen, et al., NIM A 368, 675 (1996)F. Herfurth, et al., NIM A 469, 264 (2001)

Bunching of thecontinuous beam

ISOLTRAP: Experimental setup

Page 4: Sarah Naimi

B = 4.7 T

B = 5.9 T

2 m

G. Bollen, et al., NIM A 368, 675 (1996)F. Herfurth, et al., NIM A 469, 264 (2001)

removal of contaminant ions

(R = 105)

Removal of isobaric contaminants

Buffer gas cooling with QP excitation:Savard et al., Phys. Lett. A 158, 247 (1991)

Page 5: Sarah Naimi

B = 4.7 T

B = 5.9 T

2 m

determination of cyclotron frequency

(R = 107)

ISOLTRAP: Experimental setup

Bmq

c

21

97Kr : 63(3) ms (preparation trap)66Mn : 64.4(1.8) ms (Record at Isoltrap!!!)

66Mn

Page 6: Sarah Naimi

Introduction : Masses and nuclear structure

Page 7: Sarah Naimi

Shell closure at N = 40 ?

O. Sorlin et al, PRL. 88, 092501 (2002): 68Ni

possibility of new magic number at N = 40

C. Guénaut et al, PRC 75, 044303 (2007) :

neutron rich Ni, Cu, Ga mass measurements at Isoltrap

No evidence of shell closure at N = 40

Harmonic oscillator : 2, 8, 20, 40, 70…

Spin orbit : 2, 8, 20, 28, 50, 82…

40

50

Page 8: Sarah Naimi

Shell closure at N = 40 ?

Page 9: Sarah Naimi

A ≈ 100 Region

Large deformation in the Zr region

Quantum nuclear phase transition Iachello, PRL, 87, 5 (2001) D. A. Arseniev et al, Nucl. Phys. A139, 269 (1969)

P. Federman and S. Pittel, PRC, 20, 820 (1979)

N = 60

4039383736

Z =

Page 10: Sarah Naimi

Kr: deformation from N = 60 ?

Page 11: Sarah Naimi

Kr: deformation from N = 60 ?

S2n and charge radii correlation

95–101Y,101–107Nb mass measurements by JYFL group: U. Hager et al, Nuclear Physics A 793 (2007) 20–39

86–90,92–102Y, isomeric states 87–90,93,96,97,98Y Laser spectroscopy: B. Cheal, et al., Phys. Lett. B 645 (2007) 133

Page 12: Sarah Naimi

AME 2008 - includes some JYFL data:

Hakala et al. (2008)& ISOLTRAP data:

Delahaye et al. (2006)Baruah et al. (2008)

?

Kr: deformation from N = 60 ?

#

Zn

Kr

Ge

Se

Page 13: Sarah Naimi

Kr: deformation from N = 60 ?

HFB17 : S. Goriely, N. Chamel, and J.M. Pearson

Page 14: Sarah Naimi

Kr: deformation from N = 60 ?Experimental results

spectra from CLARA and PRISMA spectrometer

N. Mărginean et al. PHYSICAL REVIEW C 80, 021301(R) (2009)

241-keV gamma ray : 2+1 0+

g.s transition

Moderate deformation

Page 15: Sarah Naimi

Kr: deformation from N = 60 ?Mass measurements experimental results

Kr97_118.DAT

x []

y []

750860 750880 750900 750920 750940 750960

0

5

10

15

20

25

30

35

40

Freq [Hz]#

of io

ns

96Kr

Time of flight resonance in the precision trap

97Kr

Cooling resonance in the preparation trap

Page 16: Sarah Naimi

Kr: deformation from N = 60 ?Mass measurements experimental results

Page 17: Sarah Naimi

ISOLDE Workshop 2009

Summary

• From the Mn isotopes masses

No evidence on shell closure at N = 40

• Mass measurements of 96Kr and 97Kr showed no strong sudden deformation at N = 60

The end of quantum nuclear phase transition in the N = 60 region

Page 18: Sarah Naimi

ISOLDE Workshop 2009

Outlook • Re-measure the 97Kr in the precision trap to reduce the error bars

• Go further 98Kr proposal 2009 on noble gases INTC-P-263

• More study on the n-rich medium masses

Page 19: Sarah Naimi

ISOLDE Workshop 2009

Collaborators:G. Audi, D. Beck, K. Blaum, Ch. Böhm, Ch. Borgmann, M. Breitenfeldt, D. Fink, S.George, A. Herlert, F. Herfurth, A. Kellerbauer, H.-J. Kluge,

M. Kowalska, S. Kreim, D. Lunney, E. Minaya Ramirez, S. Naimi,D.Neidherr, M. Rosenbusch, S. Schwarz,

L. Schweikhard, R. Wolf

Funding:BMBF, GSI, EU, IN2P3, MPI, CERN, ISOLDE