Title: Level Densities and ray Strength Functions in Sm Isotopes
1Level Densities and ?-ray Strength Functions in
Sm Isotopes
- Sunniva Siem
- University of Oslo
2Spin energy diagram
In our experiments spin 2-6 h
Bn
Excitation energy
Yrast
Spin
3CACTUS- 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
5147Sm
146Sm
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8Microcanonical Temperature
9148Sm 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
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13Radiative strength function of 57Fe
A.Voinov et al. Phys.Rev.Lett.93, 142504 (2004)
14M.Guttormsen et al. Phys.Rev.C 71,044307(2005)
?-strength functions in Mo isotopes
Filled circles (3He,a) Open circles (3He,3He)
15A workshop onLevel density and ?-strength in
continuum
21-24 May 2007 in Oslo http//ocl.uio.no
16Collaborators
- 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, Åbo,Finland
- T.Belgya, Budapest, Hungary
- E.Algin, Turkey
17Summary
- 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
18Microcanonical Temperature
19strength functions in Mo as a function of the
initial excitation energy of the nucleus.
20Strength 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.