rare isotope investigation at gsi experimental set-up sub-shell closure (n=32 gap) for cr nuclei...

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Rare ISotope INvestigation at GSI experimental set-up sub-shell closure (N=32 gap) for Cr nuclei pairing interaction in semi-magic Sn nuclei shapes and shape coexistence: 136 Nd, 134 Ce

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Page 1: Rare ISotope INvestigation at GSI experimental set-up sub-shell closure (N=32 gap) for Cr nuclei pairing interaction in semi-magic Sn nuclei shapes and

Rare ISotope INvestigation at GSI experimental set-up

sub-shell closure (N=32 gap) for Cr nuclei pairing interaction in semi-magic Sn nuclei shapes and shape coexistence: 136Nd, 134Ce Pygmy dipole resonance in 68Ni T=2 mirrors 36Ca and 36S

future: PreSPEC

Page 2: Rare ISotope INvestigation at GSI experimental set-up sub-shell closure (N=32 gap) for Cr nuclei pairing interaction in semi-magic Sn nuclei shapes and

Rare ISotope INvestigation at GSI

Nuclear structure of exotic nuclei studied by secondary fragmentation and relativistic Coulomb excitation

g-factor measurements

Isomeric γ- and β-decay studies

FRS → secondary radioactive ion beams:

• Fragmentation or fission of primary beams

• High secondary beam energies (100 - 400 AMeV)

• Fully stripped ions

• Reactions on a secondary target

• Implantation inside a stopper

The Accelerators:UNILAC (injector) - E<15 AMeV

SIS 18Tm 238U 1 AGeVBeam currents:

238U 109 ppsmedium mass nuclei 1010 pps

Page 3: Rare ISotope INvestigation at GSI experimental set-up sub-shell closure (N=32 gap) for Cr nuclei pairing interaction in semi-magic Sn nuclei shapes and

The Accelerators:UNILAC (injector) - E<15 AMeV

SIS 18Tm 238U 1 AGeVBeam currents:

238U 109 ppsmedium mass nuclei 1010 pps

Fast beam campaign (2003-2005)

g-factor campaign (2005)

Stopped beam campaign (2006-2009)

Rare ISotope INvestigation at GSI

Rare ISotope INvestigation at GSI

• FRS: excellent in-flight A and Z selection energy resolution: ~ 1 GeV • EUROBALL: excellent γ-ray spectrometer intrinsic energy resolution: ~ 2 keV

131Sn 132Sn

Page 4: Rare ISotope INvestigation at GSI experimental set-up sub-shell closure (N=32 gap) for Cr nuclei pairing interaction in semi-magic Sn nuclei shapes and

FRagment Separator

86Kr, 480 MeV/u

CATEMWPC

• 15 EUROBALL Clusters (105 Ge crystals)• ΔEγ=1.6% (1.3 MeV, d = 70 cm)

• εγ = 2.8%

Ring angular range

1 10.50-21.30

2 27.60-38.40

3 30.60-41.40

Experimental set-up

56Cr

Page 5: Rare ISotope INvestigation at GSI experimental set-up sub-shell closure (N=32 gap) for Cr nuclei pairing interaction in semi-magic Sn nuclei shapes and

70cm

20cm

beam

target

γ-ray set-up with higher efficiency

Page 6: Rare ISotope INvestigation at GSI experimental set-up sub-shell closure (N=32 gap) for Cr nuclei pairing interaction in semi-magic Sn nuclei shapes and

Atomic Background RadiationBremsstrahlung

Bremsstrahlung: slowing down of a moving point-charge

Radiative electron capture (REC) capture of target electrons into bound states of the projectile:

Primary Bremsstrahlung (PB)capture of target electrons into continuum states of the projectile:

Secondary Bremsstrahlung (SB)Stopping of high energy electrons in the target: 22~ tp ZZ

tp ZZ 2~

tp ZZ 2~

Page 7: Rare ISotope INvestigation at GSI experimental set-up sub-shell closure (N=32 gap) for Cr nuclei pairing interaction in semi-magic Sn nuclei shapes and

EUROBALL Cluster Detectors Miniball: HPGe segmented detectors

HECTOR Large 14.5 x 17 cm BaF2 Detectors

CATE : ΔE-E telescope event by event beam identification

Coulomb Excitation at Relativistic Energy

New Shell structure at N>>Z Relativistic Coulomb excitation of nuclei near 100Sn Triaxiality in even-even core nuclei of N=75 isotones E1 Collectivity in neutron rich nuclei 68Ni

nucleus σ (mb)

56Cr 91

108Sn 314

136Nd 338 / 2180

beam

Rare ISotope INvestigation at GSI

H.J. Wollersheim NIM A537, 637(2005)

Page 8: Rare ISotope INvestigation at GSI experimental set-up sub-shell closure (N=32 gap) for Cr nuclei pairing interaction in semi-magic Sn nuclei shapes and

Relativistic Coulomb Excitationof 54,56,58Cr → 197Au

Identification before the secondary target

after secondary target

γ-efficiency = 2.8% , ΔEγ = 1.6% (1.3 MeV, d=70 cm)

Page 9: Rare ISotope INvestigation at GSI experimental set-up sub-shell closure (N=32 gap) for Cr nuclei pairing interaction in semi-magic Sn nuclei shapes and

Relativistic Coulomb Excitationof 54,56,58Cr → 197Au

A. Bürger et al., Phys. Lett B622, 29 (2005)

E [keV] B(E2) [Wu]

54Cr 835 14.6 (6)56Cr 1006 8.7 (3.0)58Cr 880 14.8 (4.2)

Indication for N=32 sub-shell closure

Page 10: Rare ISotope INvestigation at GSI experimental set-up sub-shell closure (N=32 gap) for Cr nuclei pairing interaction in semi-magic Sn nuclei shapes and

The 100Sn / 132Sn region

d5/2

g7/2

Naïve single particle filling

s1/2 d3/2

h11/2

Z = 50

N=50g7/2

s1/2

d3/2

h11/2

00.5

1.62.22.6

MeV

d5/2

Single particle energies

N=82

Pairing interaction:Large spin-orbit splitting implies a jj-coupling scheme

mid shell

Page 11: Rare ISotope INvestigation at GSI experimental set-up sub-shell closure (N=32 gap) for Cr nuclei pairing interaction in semi-magic Sn nuclei shapes and

Relativistic Coulomb Excitationof 108Sn → 197Au

Seniority: a broken-pair model

Constant 2+ energy Simple B(E2) trend as function of shell filling

22++

44++

66++

00++

minmin

ener

gy a

xis

jj

j

j

j

j

j jJJ

JJJJ

=0

=2

=2

=2

Seniority scheme:

Emerging discrepancy:Do we need to open the proton space near 100Sn or do we need to improve the effective interaction?

A. Banu, Phys Rev C72, 061305 (2005)

B(E2) ~ Nparticles* Nholes

mid shell

Page 12: Rare ISotope INvestigation at GSI experimental set-up sub-shell closure (N=32 gap) for Cr nuclei pairing interaction in semi-magic Sn nuclei shapes and

Relativistic Coulomb Excitationof 136Nd → 197Au

2 1+

0+

2 2+

0+

2 2+

2 1

+

136136NdNd

energy [keV]

cou

nts

First observation of a second excited 2+ state populated in a Coulomb experiment at 100 AMeV using EUROBALL and MINIBALL Ge detectors.

collective strength shape symmetry triaxiality (in N=76) in even-even core nuclei of the odd-odd chiral isotones

T.R. Saito, Phys.Lett B669, 19 (2008)

Page 13: Rare ISotope INvestigation at GSI experimental set-up sub-shell closure (N=32 gap) for Cr nuclei pairing interaction in semi-magic Sn nuclei shapes and

Pygmy Dipole ResonanceCollective oscillation of neutron skin against the core

Excess Yield

Statistical model (Cascade) calculation of -rays following statistical equilibration of excited target nuclei (197Au) and of the excited beam nuclei (68Ni) folded with RF and in the CM system

NP-Core

N-Skin

O.Wieland et al. PRL 102, 092502 (2009)

Page 14: Rare ISotope INvestigation at GSI experimental set-up sub-shell closure (N=32 gap) for Cr nuclei pairing interaction in semi-magic Sn nuclei shapes and

40

80

120

(,n)

10-1

100

101

102

103 VP VP and R

[m

b]

8 10 12 14 16 18 200.1

1

GDR PDR Total

d/

dE

[mb/M

eV

]

E [MeV]

GDR

PDR

PDR5% +/-1 GDR

Folded with the detector response function

O.Wieland et al. PRL 102, 092502 (2009)without pygmy

virtual photonsvirtual photons

branching

Photonuclear Photonuclear cross sectioncross section

Pygmy Dipole Resonance

Page 15: Rare ISotope INvestigation at GSI experimental set-up sub-shell closure (N=32 gap) for Cr nuclei pairing interaction in semi-magic Sn nuclei shapes and

Mirror symmetry at the proton drip-line: 36Ca – 36SDeviations from the classical shell model

34Si

32Mg

36S

40Ca36Ca

Z

N

d5/2 s1/2 d3/2

d5/2

s1/2

d3/2

34Ca32Ca

20

20 CLUSTER

MINIBALL

HECTOR

Double fragmentation reaction: Primary: 40Ca, 420 A·MeV, 3·108 ions/s, 4 mg/cm2 9Be

Secondary: 37Ca, 196·A MeV, 2·103 ions/s, 0.7 mg/cm2 9Be

E2+ (36Ca) - E2+ (36S) = -276(16) keV

too large to result from Coulomb corrections

P. Doornenbal et al., Phys. Lett. B647, 237 (2007)

Page 16: Rare ISotope INvestigation at GSI experimental set-up sub-shell closure (N=32 gap) for Cr nuclei pairing interaction in semi-magic Sn nuclei shapes and

*H. Herndl et al., Phys. Rev. C 52 (1995) 1078P. Doornenbal et al., Phys. Lett. B647, 237 (2007).A. Gade et al. Phys. Rev. C 76, 024317 (2007)

Mirror energy differences for T=1,2 nuclei Deviations from the classical shell model

Page 17: Rare ISotope INvestigation at GSI experimental set-up sub-shell closure (N=32 gap) for Cr nuclei pairing interaction in semi-magic Sn nuclei shapes and

Future: PreSPEC and AGATA

LYCCA

BeamDirection

Detectorat rear

10 ATC+ 5 double Cluster detectors beam pipe diameter = 12cm

chamber diameter = 46 cm

S2´-configuration:10 AGATA Triple Cluster+ 5 double Cluster detectors

γ-efficiency = 17.5% γγ-efficiency = 2.5%

resolution (FWHM)

intrinsic spatial

resolution

8.5 keV 5 mm

4 keV 2 mm

Page 18: Rare ISotope INvestigation at GSI experimental set-up sub-shell closure (N=32 gap) for Cr nuclei pairing interaction in semi-magic Sn nuclei shapes and

PreSPEC fast-beam campaign great perspectives …

AGATA increases-sensitivity ≈ 10x

LYCCA-0 provides mass resolution up to A ≈ 100

SIS/FRS intensitiesincrease up to ≈ 10x

Tracking det. and EDAQ upgrade increase max. rate and throughput 10x

PreSPEC Fast Beam Campaignconvener: W. Korten

Very attractive and competitivespectroscopy themes

Unique combination of beams, set-up and people

Page 19: Rare ISotope INvestigation at GSI experimental set-up sub-shell closure (N=32 gap) for Cr nuclei pairing interaction in semi-magic Sn nuclei shapes and