Parameter study of r-process lanthanide production and heating rates in kilonovae

@article{Lippuner2015ParameterSO,
  title={Parameter study of r-process lanthanide production and heating rates in kilonovae},
  author={Jonas Lippuner and Luke F Roberts},
  journal={Bulletin of the American Physical Society},
  year={2015},
  volume={2015}
}
r-Process nucleosynthesis in material ejected during neutron star mergers may lead to radioactively powered transients called kilonovae. The timescale and peak luminosity of these transients depend on the composition of the ejecta, which determines the local heating rate from nuclear decays and the opacity. Kasen et al. (2013, ApJ, 774, 25) and Tanaka & Hotokezaka (2013, ApJ, 775, 113) pointed out that lanthanides can drastically increase the opacity in these outflows. We use the new general… 

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