Spallative nucleosynthesis in supernova remnants II . Time-dependent numerical results

@inproceedings{Parizot1999SpallativeNI,
  title={Spallative nucleosynthesis in supernova remnants II . Time-dependent numerical results},
  author={Etienne Parizot and Luke Drury},
  year={1999}
}
We calculate the spallative production of light elements associated with the explosion of an isolated supernova in the interstellar medium, using a time-dependent model taking into account the dilution of the ejected enriched material and the adiabatic energy losses. We first derive the injection function of energetic particles (EPs) accelerated at both the forward and the reverse shock, as a function of time. Then we calculate the Be yields obtained in both cases and compare them to the value… CONTINUE READING
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A&A, accepted (Paper I

  • E. Parizot, L. Drury
  • Parizot E., Kn̈odlseder J.,
  • 1999
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