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Level Densities and ray Strength Functions in Sm Isotopes

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Zakopane 2006. Level Densities and -ray Strength Functions in Sm Isotopes ... The M1 pygmy resonance observed in several deformed nuclei vanishes in the Sm ... – PowerPoint PPT presentation

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Title: Level Densities and ray Strength Functions in Sm Isotopes


1
Level Densities and ?-ray Strength Functions in
Sm Isotopes
  • Sunniva Siem
  • University of Oslo

2
Spin energy diagram
In our experiments spin 2-6 h
Bn
Excitation energy
Yrast
Spin
3
CACTUS- experimental setup
  • Reactions (3He,?) and (3He,3He)
  • Beam 30-45 MeV
  • Targets Yb, Dy, Er, Sm, Nd, Si, Mo, Fe, Sn, V,
    Pb,Ti,Ni
  • 8 Si particle telescopes at ? 45
  • Spin 2-6 h
  • CACTUS detector array (28 NaI 2Ge) has 15
    efficiency

4
  • Energy distribution of primary ? rays contains
    info on
  • level density ?(Ef)
  • -ray transmission coefficient T(E?)
  • Brink-Axel
  • P(Ex,E?) T(E?) ?(Ef)

Ex
5
147Sm
146Sm
6
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7
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8
Microcanonical Temperature
9
148Sm strength function
  • Circles our data
  • Squares from photoabsorpsjon cross sections
    P.Carlos et al. NPA 225 (1974)
  • Filled triangle is based on neutron capture in
    147Sm

10
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12
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13
Radiative strength function of 57Fe
A.Voinov et al. Phys.Rev.Lett.93, 142504 (2004)
14
M.Guttormsen et al. Phys.Rev.C 71,044307(2005)
?-strength functions in Mo isotopes
Filled circles (3He,a) Open circles (3He,3He)
15
A workshop onLevel density and ?-strength in
continuum
21-24 May 2007 in Oslo http//ocl.uio.no
16
Collaborators
  • R.Chankova, M.Guttormsen, F.Ingebretsen, S.
    Messelt, J.Rekstad, A.C.Larsen, N.U.H.Syed,
    S.Ødegård, University of Oslo
  • A.Voinov, Dubna, Russia
  • U.Agvaanluvsan, G.Mitchell, TUNL, USA
  • J.A.Becker, L.Bernstein, LLNL, USA
  • A.Schiller, MSU,USA
  • T.Lønnroth, Ã…bo,Finland
  • T.Belgya, Budapest, Hungary
  • E.Algin, Turkey

17
Summary
  • Unique technique to extract level densities and
    ?-strength function experimentally
  • New Sm data show that the level density continues
    to decrease as one approaches the N82 closed
    shell
  • The M1 pygmy resonance observed in several
    deformed nuclei vanishes in the Sm nuclei as one
    approaches N82
  • We dont understand the large enhancement in
    strength function for low E? in Fe, Mo and V
    isotopes

18
Microcanonical Temperature
19
strength functions in Mo as a function of the
initial excitation energy of the nucleus.
20
Strength functions as a function of the final
excitation energy feed by the decay, i.e. only
feeding 1.1 MeV or 1.8 MeV etc.
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