introduction shell evolution along ni isotopic chain, towards 78 ni. focus on 74 ni existing data....
TRANSCRIPT
Shell evolution in exotic Ni isotopes
T. Marchi11th INTERNATIONAL SPRING SEMINAR ON NUCLEAR PHYSICS
SHELL MODEL AND NUCLEAR STRUCTURE: achievements of the past two decades Ischia, May 12 – 16 2014
Shell evolution in exotic Ni isotopes
T. Marchi
Introduction
• Shell evolution along Ni isotopic chain, towards 78Ni.
Focus on 74Ni• Existing data.• Intermediate energy Coulomb excitation (NSCL 09031):
Exotic Beam production; Experimental setup; Data analysis and B(E2)↑ extraction; Comparison with SM calculations.
Conclusion and Outlook
11th INTERNATIONAL SPRING SEMINAR ON NUCLEAR PHYSICSSHELL MODEL AND NUCLEAR STRUCTURE: achievements of the past two decades
Ischia, May 12 – 16 2014
[B. P
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at. A
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. Tab
. 98,
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[N. Shimizu et al, Progr. Theo. Exp. Phys (2012) 01A205 ]
Introduction
T. Marchi 11th INTERNATIONAL SPRING SEMINAR ON NUCLEAR PHYSICS Ischia, May 12 – 16 2014
[N. Shimizu et al, Progr. Theo. Exp. Phys (2012) 01A205 ]
Introduction
T. Marchi 11th INTERNATIONAL SPRING SEMINAR ON NUCLEAR PHYSICS Ischia, May 12 – 16 2014
[B. P
rityc
henk
o et
al,
At. D
at. A
nd N
ucl.
Dat
. Tab
. 98,
4 (2
012)
798
]
[N. Shimizu et al, Progr. Theo. Exp. Phys (2012) 01A205 ]
Introduction
T. Marchi 11th INTERNATIONAL SPRING SEMINAR ON NUCLEAR PHYSICS Ischia, May 12 – 16 2014
[B. P
rityc
henk
o et
al,
At. D
at. A
nd N
ucl.
Dat
. Tab
. 98,
4 (2
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798
]
Motivation:1-Study the evolution of nuclear Shells far from stability, towards 78Ni.2-Test model space and interactions far from stability.
0
Shell Evolution
[T. O
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a, P
hys
Rev
Lett
104
.012
501] Proton ESPE for Ni isotopes
[K. Sieja and F. Nowacki, Phys Rev C 85, 051301]
Neutron ESPE for N=50 isotones and for Ni isotopes
See also: H. L. Crawford, PRL 110, 242701 (2013) on Fe/Cr isotopes. “twin experiment”. And S. M. Lenzi, PRC 82, 054301 (2010)
Introduction
T. Marchi 11th INTERNATIONAL SPRING SEMINAR ON NUCLEAR PHYSICS Ischia, May 12 – 16 2014
[B. P
rityc
henk
o et
al,
At. D
at. A
nd N
ucl.
Dat
. Tab
. 98,
4 (2
012)
798
]
74Ni Existing data – 74Co β-decay
T. Marchi 11th INTERNATIONAL SPRING SEMINAR ON NUCLEAR PHYSICS Ischia, May 12 – 16 2014
Existing data - proton scattering(p,p’) extracted from proton inelastic scattering cross section using distorted wave theory. (ECIS97 code)
[N. Aoi et al, Phys. Lett. B 602, 302 (2010)][B. Pritychenko et al, At. Dat. And Nucl. Dat. Tab. 98, 4 (2012) 798]
Assuming comparable deformation lengths also for the neutron rich part of the chain: (p,p’) C B(E2) = 1270(380) e2fm4
N=46
T. Marchi 11th INTERNATIONAL SPRING SEMINAR ON NUCLEAR PHYSICS Ischia, May 12 – 16 2014
74Ni
Radioactive ion beam production
86Kr34+ @ 140 AMeV74Ni ≈ 0.7 pps
dp/p = 3%9Be 399 mg/cm2
T. Marchi 11th INTERNATIONAL SPRING SEMINAR ON NUCLEAR PHYSICS Ischia, May 12 – 16 2014
74Ni
Experimental setup
Object scintillator
Secondary target position
197Au 640 mg/cm2
S800 Analysis line
S800 Spectrometer
Focal Plane detectors
CAESAR array
T. Marchi 11th INTERNATIONAL SPRING SEMINAR ON NUCLEAR PHYSICS Ischia, May 12 – 16 2014
74Ni
The S800 spectrometer and the CAESAR array
CAESAR array
CAESAR array + S800 spectrometer
T. Marchi 11th INTERNATIONAL SPRING SEMINAR ON NUCLEAR PHYSICS Ischia, May 12 – 16 2014
74Ni
Beam Tagging and Particle Identification
Focal plane PID Beam Tagging
Runs without target
T. Marchi 11th INTERNATIONAL SPRING SEMINAR ON NUCLEAR PHYSICS Ischia, May 12 – 16 2014
74Ni
Data analysis: particle and gamma ray time gates
Energy-time gamma-rays gate:
T. Marchi 11th INTERNATIONAL SPRING SEMINAR ON NUCLEAR PHYSICS Ischia, May 12 – 16 2014
74NiImpact parameter selection:
Two main issues
T. Marchi 11th INTERNATIONAL SPRING SEMINAR ON NUCLEAR PHYSICS Ischia, May 12 – 16 2014
Beam contaminationUngated PID
Gated PID
Background modeling
74Ni
EPAX: 76Cu 1p-1n K.O. : σ = 29 mb NK.O. =18±9 Ng = 9 ±5
E (keV)
E (keV)
Event by event analysis and gamma-ray spectra
Fit: GEANT4 +exponential bkg
[A. Winther and K. Alder, Nucl. Phys. A319, 518 (1979)]
= 148+50-52 mb B(E2; 0+ -> 2+) = 642+216
-226 e2 fm4
T. Marchi 11th INTERNATIONAL SPRING SEMINAR ON NUCLEAR PHYSICS Ischia, May 12 – 16 2014
74Ni
Ng = 99 ± 28
The B(E2; 0+ →2+) value obtained in the intermediate energy Coulomb excitation provides new important information for the understanding of the Ni isotopic chain towards the 78Ni doubly magic nucleus.1-The collectivity enhancement suggested by the (p,p’) experiment seems quenched when using purely electromagnetic probes;2-The obtained values can be used to benchmark the Model Space and Interactions used for Shell Model Calculations far from stability.
Resultsp n
LNPS pf p, f5/2, g9/2 d5/2 [1]
Vlow_k f7/2, p3/2 p, f5/2, g9/2,d5/2 [2]
A3DA pf g9/2d5/2 [3]
[1] K. Sieja, F. Nowacki, Phys Rev C 85, 051301(R) (2012) K. Sieja, F. Nowacki, arXiv:1201.0373v1 (2012) S. M. Lenzi et al, Phys Rev C 82, 054301 (2010)[2] L. Coraggio, PRC 89, 024319 (2014) L. Coraggio et al., Prog. Part. Nucl. Phys 62, 135 (2009)[3] N. Shimizu et al., Progr Theor Exp. Phys, 01A205 (2012) Y. Tsunoda et al., PRC 89, 031301(R) (2014)
T. Marchi 11th INTERNATIONAL SPRING SEMINAR ON NUCLEAR PHYSICS Ischia, May 12 – 16 2014
Discussion and outlookInelastic scattering data compared to Coulex results allow to disentangle the proton/neutron excitation matrix elements. For the 74Ni isotope, their difference could be an indication of the relative proton/neutron cores polarization leading to different deformation. A higher degree of accuracy is needed to constrain the B(E2) error bar and provide quantitative Mn/Mp ratio information.
T. Marchi 11th INTERNATIONAL SPRING SEMINAR ON NUCLEAR PHYSICS Ischia, May 12 – 16 2014
Exp 2.4±0.8
LNPS 1.8
Discussion and outlookInelastic scattering data compared to Coulex results allow to disentangle the proton/neutron excitation matrix elements. For the 74Ni isotope, their difference could be an indication of the relative proton/neutron cores polarization leading to different deformation. A higher degree of accuracy is needed to constrain the B(E2) error bar and provide quantitative Mn/Mp ratio information.
T. Marchi 11th INTERNATIONAL SPRING SEMINAR ON NUCLEAR PHYSICS Ischia, May 12 – 16 2014
Exp 2.4±0.8
LNPS 1.8
Outlook:
72Ni and 76Ni become key nuclei to understand the evolution of collectivity along the Ni chain. 76Ni still represents a challenge in terms of RIB production.Two different experiments are under analysis:-68 – 70 - 72Ni (p,p’) inelastic scattering at NSCL (GRETINA) – NSCL E12016-74Ni Coulex at RIKEN with higher beam intensity (~150 counts in the 2+ peak).
Collaboration
T. Marchi,1, 2 G. De Angelis,1 J.J. Valiente-Dobón,1 V. Bader3, T. Baugher,3 D. Bazin,3 J. Berryman,3 A. Bonaccorso,4 R. Clark,5 L. Coraggio,6 E. L. Crawford,5 M. Doncel,7
E. Farnea,8 A. Gade,3 A. Gadea,9 A. Gargano,6 T. Glasmacher,3 A. Gottardo,1, 2 F. Gramegna,1 N. Itaco,10,6 P.R. John,8,2 R. Kumar,11 S. M. Lenzi,8,2 S. Lunardi,8,2 S. McDaniel,3 C. Michelagnoli,8,2 D. Mengoni,8,2 V. Modamio,1 D.R. Napoli,1
B. Quintana,12 A. Ratkiewicz,3 F. Recchia,8,2 E. Sahin,1 R. Stroberg,3
D. Weisshaar,3 K. Wimmer,3 and R. Winkler3
1INFN Legnaro National Laboratories, Legnaro (Pd), Italy2Department of Physics, Padua University, Padua, Italy3National Superconducting Cyclotron Laboratory , Michigan State University, East Lansing, Michigan, USA4INFN Sezione di Pisa, Pisa, Italy5Nuclear Science Division, Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA6INFN Sezione di Napoli, Napoli, Italy7Ionizing Radiations Laboratory, University of Salamanca, Spain8INFN Sezione di Padova, Padova, Italy9CSIC-IFIC, Valencia, Spain10Dipartimento di Fisica, Università “Federico II”, Napoli, Italy11Deenbandhu Chhoturam University of Science and Technology, Haryana, 131039 India12Grupo de Fisica Nuclear, Universidade de Salamanca, Spain
Thank you!
CAESAR scintillator array[D
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CAESAR Resolution CAESAR EfficiencyExperimental gamma-rays
multiplicity
T. Marchi 11th INTERNATIONAL SPRING SEMINAR ON NUCLEAR PHYSICS Ischia, May 12 – 16 2014
74Ni
S800 Focal Plane Detectors[D
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80% CF4 20% C4H10
P10500 Torr
T. Marchi 11th INTERNATIONAL SPRING SEMINAR ON NUCLEAR PHYSICS Ischia, May 12 – 16 2014
74Ni
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[T. Otsuka, A. Schwenk, Nucl Phys News 22-4 (2012) 12]
T. Marchi 11th INTERNATIONAL SPRING SEMINAR ON NUCLEAR PHYSICS Ischia, May 12 – 16 2014