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Neutrino Emissions in All Flavors up to the Pre-bounce of Massive Stars and the Possibility of Their Detections

  • Authors: Chinami Kato, Hiroki Nagakura, Shun Furusawa, Koh Takahashi, Hideyuki Umeda, Takashi Yoshida, Koji Ishidoshiro, and Shoichi Yamada

2017 The Astrophysical Journal 848 48.

  • Provider: AAS Journals

Caption: Figure 12.

Time evolutions of the event rates (top panels) and cumulative numbers of events (bottom panels) for the 15 ﹩{M}_{\odot }﹩ progenitor model. The upper half of each panel shows the results for the normal mass hierarchy, while the lower half presents those for the inverted mass hierarchy. Colors specify the neutrino detectors. We consider ﹩{\nu }_{e}﹩ for DUNE (dotted line) and ﹩{\bar{\nu }}_{e}﹩ for other detectors (solid lines).

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