Boron Synthesis in Type Ic Supernovae
Ko Nakamura, Takashi Yoshida, Toshikazu Shigeyama, and Toshitaka, Kajino

TL;DR
This study explores how Type Ic supernovae can produce boron through neutrino interactions and spallation, highlighting their potential role in galactic chemical evolution.
Contribution
First hydrodynamic simulation of boron production via neutrino-process in SN Ic, demonstrating significant 11B synthesis and its implications for galactic chemical evolution.
Findings
SN Ic can produce significant 11B via neutrino-process.
Neutrino interactions in SN Ic enhance light element synthesis.
Produced boron ratios align with meteorite observations.
Abstract
We investigate the neutrino-process in an energetic Type Ic supernova (SN Ic) and resultant productions of the light elements including boron and its stable isotopes. SN Ic is a very unique boron source because it can produce boron through not only spallation reactions as discussed in Nakamura & Shigeyama (2004) but also the neutrino-process. The neutrino-process is considered to occur in core-collapse supernovae and previous studies were limited to Type II supernovae (SNe II). Although the progenitor star of an SN Ic does not posses a He envelope so that 7Li production via the neutrino-process is unlikely, 11B can be produced in the C-rich layers. We demonstrate a hydrodynamic simulation of SN Ic explosion and estimate the amounts of the light elements produced via the neutrino-process for the first time, and also the subsequent spallation reactions between the outermost layers of…
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