Estimating the core compactness of massive stars with Galactic supernova neutrinos

@article{Horiuchi2017EstimatingTC,
  title={Estimating the core compactness of massive stars with Galactic supernova neutrinos},
  author={S. Horiuchi and Ko Nakamura and T. Takiwaki and K. Kotake},
  journal={arXiv: High Energy Astrophysical Phenomena},
  year={2017}
}
We suggest the future detection of neutrinos from a Galactic core-collapse supernova can be used to infer the progenitor's inner mass density structure. We present the results from 20 axisymmetric core-collapse supernova simulations performed with progenitors spanning initial masses in the range 11--30Msun, and focus on their connections to the progenitor compactness. The compactness is a measure of the mass density profile of the progenitor core and recent investigations have suggested its… Expand

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