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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 1.

Evolutionary paths of the central density and temperature for three progenitors. The red, blue, and green curves correspond to the 15, 12, and ﹩9\ {M}_{\odot }﹩ models, respectively. The evolutions in both the progenitor phase (solid lines) and collapse phase (dotted lines) are presented. The initiation points of some major nuclear burnings as well as the evolutionary stages defined by Takahashi et al. (2013) for the ONe-core progenitors are marked with labels.

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