The endpoint of the rp-process on accreting neutron stars

@article{Schatz2001TheEO,
  title={The endpoint of the rp-process on accreting neutron stars},
  author={H. Schatz and A. Aprahamian and V. Barnard and L. Bildsten and A. Cumming and M. Ouellette and T. Rauscher and F. Thielemann and M. Wiescher},
  journal={Physical Review Letters},
  year={2001},
  volume={86},
  pages={150-153}
}
We calculate the rapid proton (rp) capture process of hydrogen burning on the surface of an accreting neutron star with an updated reaction network that extends up to Xe, far beyond previous work. In both steady-state nuclear burning appropriate for rapidly accreting neutron stars (such as the magnetic polar caps of accreting x-ray pulsars) and unstable burning of type I x-ray bursts, we find that the rp process ends in a closed SnSbTe cycle. This prevents the synthesis of elements heavier than… Expand

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