Puzzling γ-ray strength functions in 44,45Sc and 50,51V

Details Puzzling γ-ray strength functions in 44,45Sc and 50,51V Puzzling γ-ray strength functions in 44,45Sc and 50,51V

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1012..380l&link_type=abstract

FRONTIERS IN NUCLEAR STRUCTURE, ASTROPHYSICS, AND REACTIONS: FINUSTAR 2. AIP Conference Proceedings, Volume 1012, pp. 380-382 (

Astronomy and Astrophysics

Astrophysics

Level Density, Thermal And Statistical Models, Elastic And Inelastic Scattering

Scientific paper

The nuclear physics group at the Oslo Cyclotron Laboratory (OCL) has developed a method to extract nuclear level density and γ-ray strength function simultaneously from primary γ-ray spectra. The resulting γ-ray strength functions of 44,45Sc and 50,51V show an unexpected, large enhancement at low γ-ray energies, indicating an increased probability of emitting low-energy γ rays in the quasi-continuum.

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