The γ-ray Strength Function in Nuclear Astrophysics

Details The γ-ray Strength Function in Nuclear Astrophysics The γ-ray Strength Function in Nuclear Astrophysics

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1120..183u&link_type=abstract

PERSPECTIVE IN NUCLEAR PHYSICS: Proceedings of the 6th Japan-Italy Symposium on Heavy-Ion Physics. AIP Conference Proceedings,

Physics

Nuclear Physics

Giant Resonances, Beta Decay, Double Beta Decay, Electron And Muon Capture, Atomic Scattering, Cross Sections, And Form Factors, Compton Scattering, Compound Nucleus

Scientific paper

The γ-ray strength function is a key statistical nuclear ingredient to the s-, r- and p-process nucleosynthesis of heavy elements. It has recently become apparent that extra γ-ray strengths that appear near neutron threshold on top of the low-energy tail of GDR play an important role in neutron capture and photodisintegration. We discuss extra γ-ray strengths of pigmy E1 and giant M1 nature based on the latest experimental photoneutron cross sections measured with laser Compton scattering γ-rays.

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