Resonance in Iron neutron rich exotic isotopes R.Avigo 1,2 A.Bracco - - PowerPoint PPT Presentation

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Resonance in Iron neutron rich exotic isotopes R.Avigo 1,2 A.Bracco - - PowerPoint PPT Presentation

Investigation of Pygmy Dipole Resonance in Iron neutron rich exotic isotopes R.Avigo 1,2 A.Bracco 1,2 , O.Wieland 1 , F.Camera 1,2 on behalf of the AGATA collaborations 1 INFN sezione di Milano 2 Universit degli Studi di Milano Outlines


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SLIDE 1

Investigation of Pygmy Dipole Resonance in Iron neutron rich exotic isotopes

R.Avigo1,2 A.Bracco1,2, O.Wieland1, F.Camera1,2

  • n behalf of the AGATA collaborations

1 INFN sezione di Milano 2 Università degli Studi di Milano

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SLIDE 2

Outlines

COMEX5, Krakow, September 14 - 18, 2015

Pygmy Dipole Resonance in neutron rich nuclei E1 strength investigation of 62,64Fe nuclei with relativistic coulomb excitation PreSPEC-AGATA setup at GSI Experimental gamma ray spectra from 62,64Fe Preliminary results Conclusions

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SLIDE 3

Pygmy Dipole Resonance in neutron rich nuclei

E1 strength response measured in neutron rich stable nuclei

  • A. Zigles et al. Journ. of Phys. 580 (2015) 012052

Accumulation of strength around and above neutron separation energy interpret as a collective motion called Pygmy Dipole Resonance (PDR)

COMEX5, Krakow, September 14 - 18, 2015

Experimental effort over 40 years to investigate this strength accumulation in different mass region towards exotic nuclei

  • P. Aldrich et al. PRL 95 (2005) 132501
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SLIDE 4

Pygmy Dipole Resonance in Iron

COMEX5, Krakow, September 14 - 18, 2015

This low energy region contribution of PDR has attracted interest and it was measured in different region of mass

  • R. Massarczyk et al.,PRL 112, 072501
  • A. C. Larsen et al.,PRL 111,242504 (2013)

OSLO experiment

62-64Fe region

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SLIDE 5

Iron isotopes

Theoretical predictions show dipole strenght around 10 MeV and also below the threshold for 62,64Fe For the first time E1 strength distribution below the threshold will be studied for exotic isotopes at varying of the neutron number

62Fe

62Fe:expected dipole strength

  • Arb. Un.

80 40

COMEX5, Krakow, September 14 - 18, 2015

Carbone - Colò

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SLIDE 6

Relativistic coulomb excitation

b>bmin

virtual photon

γ emission

Relativistic coulomb excitation of Pygmy Dipole Strength High selectivity No neutron-threshold effect Pygmy Dipole Strength measured for the first time in exotic nuclei:

62,64Fe coulomb excitation experiment in GSI

COMEX5, Krakow, September 14 - 18, 2015

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SLIDE 7

PreSPEC-AGATA setup to investigate exotic nuclei

AGATA FRS production and selection of exotic nuclei LYCCA selection of coulomb excitation events on secondary target

EPJ Web of Conferences 66, 02083 (2014)

COMEX5, Krakow, September 14 - 18, 2015

AGATA – HECTOR Measurement of gamma decay of: first 2+ state High energy levels

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SLIDE 8

PreSPEC-AGATA setup

22° 68° 95° 142°

AGATA coupled with HECTOR allows to cover a wide angular range. This can be used to get informations on the multipolarity of gamma rays detected In addition backward scintillators can be used for the estimation of background

COMEX5, Krakow, September 14 - 18, 2015

AGATA From 15° to 60° HECTOR 22°, 68°, 95°, 142°

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SLIDE 9

Relativistic coulomb excitation selection @ GSI

Identification of beam of interest Identification of reaction products Scattering angle mrad ΔE (arb. Un.) E (arb. Un.) A/Q Z COMEX5, Krakow, September 14 - 18, 2015

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SLIDE 10

Low energy spectra @ GSI

AGATA 64Fe*

Ground State 2+ 746 keV Thick target and relativistic (440 MeV/nucl.) beam required a fine tuning of PreSPEC and AGATA detectors to observe 2+ state decay for both iron isotopes B(E2) of 2+ decay is known and it is used to provide a normalization for the cross section essential to deduce B(E1) from the high energy γ-transition

400 500 600 700 800 900 1000 1100 1200 1300 1400 5 10 15 20

Counts E [keV]

GEAN T

GEANT

Ground State 2+ 877 keV

COMEX5, Krakow, September 14 - 18, 2015

877 keV 2+ @877 keV  g.s. 746 keV 2+ @ 746 keV  g.s.

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SLIDE 11

High energy spectra

4000 8000 12000 1 10 100

Counts E [keV] AGATA

62Fe*

4000 8000 12000 1 10 100

Counts E [keV] AGATA

64Fe*

COMEX5, Krakow, September 14 - 18, 2015

0,80 0,90 1,00 1,10 1,20 1,30 1,40 1,50 1,60 1,70 1,80 15 30 45 60 75

Θ(degree)

Ratio E2 yield/E1 yield Angular distribution was used to deduce the E1 character of the γ-ray data above 6 MeV.

expected

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SLIDE 12

 yield in the pygmy region

COMEX5, Krakow, September 14 - 18, 2015

How would be the spectrum if the GDR response is pure lorentzian? Pure Lorentzian GDR shape and spectrum of virtual photons used to obtain excitation spectrum

GDR lorentzian shape Spectrum of virtual photons Number of excitations

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SLIDE 13

 yield in the pygmy region

COMEX5, Krakow, September 14 - 18, 2015

GEMINI code used to deduce de-excitation gamma yield from the excitation spectrum AGATA response function applied to de-excitation gamma yield

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SLIDE 14

 yield from GDR  yield from GDR+background experimental data  yield from GDR  yield from GDR+background experimental data

High energy spectra show statistics accumulations above the background (evaluated with backward angle LaBr) and the GDR tail contribution

62Fe AGATA spectrum 64Fe AGATA spectrum

COMEX5, Krakow, September 14 - 18, 2015

High energy spectra

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SLIDE 15

Conclusions and Perspectives

COMEX5, Krakow, September 14 - 18, 2015

E1 strenght accumulation at one particle separation energy has attracted interest because it is relevant for both nuclear structure and astrophysics A lot of data available for stable nuclei, data about exotic nuclei very scarce Measurement of E1 response of 64,62Fe by relativistic coulomb scattering at GSI laboratories The advanced features of the setup allowed to collect interesting data for both Iron isotopes Gamma ray energy spectra show interesting structures over the GDR tail: the analysis showed the possibility to get an estimation of B(E1) value related to high energy  ray transitions E1 response just below the threshold is under investigation

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SLIDE 16
  • O. Wieland, R. Avigo, A. Bracco, F. Camera, S. Ceruti, G. Benzoni, N. Blasi, S. Brambilla, F.C.L. Crespi, S. Leoni,

B.Million, A. Morales, L. Pellegri, A. Giaz et al., Università degli Studi di Milano and INFN, Sezione di Milano, Italy

  • A. Maj, M. Kmiecik, P. Bednarczyk, J. Grebosz , M. Kmiecik,M. Krzysiek et al.,

The Niewodniczanski Institute of Nuclear Physics, PAN, Krakow, Poland

  • G. de Angelis, D.R. Napoli, et al.,

INFN, Laboratori Nazionali di Legnaro, Italy

  • D. Bazzacco, E. Farnea, S.M. Lenzi, S. Lunardi, et al.,
  • Dip. di Fisica and INFN, Sezione di Padova, Italy
  • J. Gerl, M. Gorska, H.J. Wollersheim, T. Aumann, N. Pietralla, P. Boutachkov, G. Guastalla, E.Gregor, N. Goel,F. Ameil, P.

Singh, A. Ghivechev, M. Reese, D. Ralet, N. Lalovic, S. Pietri, M. Lettman, R. Stegmann, T. Arici, L. Cortes, Ch. Bauer, Th. Moller, A. Ghivechev, C.Sthal, H. Schnaffer, I. Khojouharov et al., TU Darmstadt and GSI, Germany

  • G. Duchene, F. Didierjean

IPHC Strasbourg

  • K. Moschner, P. Thole

University of Cologne

  • D. RudolphP. Golubev

University of Lund

  • Z. Podolyak, T. Alexander

University of Surrey

  • A. Gadea, T. Huyuk, R. Perez

Universidat de Valencia

  • G. Rainovsky

University of Sofia

  • K. Kezzar

King Saud University

Special thanks to all AGATA - PreSPEC collaboration:

COMEX5, Krakow, September 14 - 18, 2015

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SLIDE 17

Thank you for your kind attention