# Neutrino emissions in all flavors up to the pre-bounce of massive stars and the possibility of their detections

@article{Kato2017NeutrinoEI,
title={Neutrino emissions in all flavors up to the pre-bounce of massive stars and the possibility of their detections},
author={C. Kato and H. Nagakura and S. Furusawa and K. Takahashi and H. Umeda and T. Yoshida and K. Ishidoshiro and S. Yamada},
journal={arXiv: High Energy Astrophysical Phenomena},
year={2017}
}
• C. Kato, +5 authors S. Yamada
• Published 2017
• Physics
• arXiv: High Energy Astrophysical Phenomena
This paper is a sequel to our previous one (Kato et al.2015), which calculated the luminosities and spectra of electron-type anti-neutrinos ($\bar{\nu}_e$'s) from the progenitors of core-collapse supernovae. Expecting that a capability to detect electron-type neutrinos ($\nu_e$'s) will increase dramatically with the emergence of liquid-argon detectors such as DUNE, we broaden the scope in this study to include all-flavors of neutrinos emitted from the pre-bounce phase. We pick up three… Expand
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