Energy spectrum of gamma rays produced in the decay of a giant dipole resonance in Iron

Details Energy spectrum of gamma rays produced in the decay of a giant dipole resonance in Iron Energy spectrum of gamma rays produced in the decay of a giant dipole resonance in Iron

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989svjnp..49.1005m&link_type=abstract

Soviet Journal of Nuclear Physics, vol. 49, p. 1005-1008

Physics

Nuclear Physics

Scientific paper

The energy spectrum and mean multiplicity of gamma rays produced in the decay of a giant dipole resonance in the Fe56 nucleus are calculated on the basis of the statistical model of nuclear reactions. It is shown that the maximum mean multiplicity (two photons per event of photoabsorption) is reached at the maxima of the photoabsorption cross section, the yield of the secondary gamma rays being I>120 mb. The results obtained indicate that relativistic nuclei are an efficient source of cosmic gamma radiation of super high energy and provide quantitative information for astrophysical calculations.

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