Electrodisintegration and photodisintegration of nuclei

Details Electrodisintegration and photodisintegration of nuclei Electrodisintegration and photodisintegration of nuclei

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...254..688s&link_type=abstract

Astrophysical Journal, Part 1, vol. 254, Mar. 15, 1982, p. 688-698.

Astronomy and Astrophysics

Astrophysics

3

Astronomical Models, Astrophysics, Electron Impact, High Energy Interactions, Nuclear Astrophysics, Nuclear Reactions, Photodecomposition, Bremsstrahlung, Gamma Ray Astronomy, High Energy Electrons, Photonics, Pulsars, Quasars, Scattering, Supernova Remnants

Scientific paper

Relevant excitation functions for electron-induced spallation are presented for use in models of various astrophysical sites such as pulsars, supernova remnants, and in particular for the evaluation of the B/C ratio in quasars. The cross-sections for nuclear gamma-ray lines are evaluated that are due to high energy photons produced by bremsstrahlung emissions resulting from high-energy electrons. The disintegration of nuclei is discussed in terms of the Coulomb scattering process and the giant dipole nuclear state excitation process.

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