Boron synthesis in type ic supernovae

Ko Nakamura, Takashi Yoshida, Toshikazu Shigeyama, Toshitaka Kajino

Research output: Contribution to journalArticle

15 Citations (Scopus)

Abstract

We investigate the ν-process in an energetic Type Ic supernova (SN Ic) and the 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 not only through spallation reactions as discussed in Nakamura & Shigeyama but also the ν-process. The ν-process is considered to occur in core-collapse supernovae and previous studies were limited to SNe II. Although the progenitor star of an SN Ic does not posses an He envelope so that 7Li production via the ν-process is unlikely, 11B can be produced in the C-rich layers.We demonstrate a hydrodynamic simulation of a SN Ic explosion and estimate the amounts of the light elements produced via the ν-process for the first time, and also the subsequent spallation reactions between the outermost layers of the compact SN Ic progenitor and the ambient medium. We find that the ν-process in the current SN Ic model produces a significant amount of 11B, which is diluted by 10B from spallation reactions to get closer to B isotopic ratios observed in meteorites. We also confirm that high-temperature μ and τ neutrinos and their anti-neutrinos, reasonably suggested from the compact structure of SN Ic progenitors, enhance the light-element production through the neutral current reactions, which may imply an important role of SNe Ic in the Galactic chemical evolution.

Original languageEnglish
JournalAstrophysical Journal Letters
Volume718
Issue number2 PART 2
DOIs
Publication statusPublished - 2010 Aug 1
Externally publishedYes

Fingerprint

boron
supernovae
light elements
spallation
synthesis
neutrinos
isotopic ratio
meteorite
explosion
chemical evolution
neutral currents
galactic evolution
stable isotope
meteorites
energetics
hydrodynamics
explosions
envelopes
isotopes
stars

Keywords

  • Abundances-stars
  • Abundances-supernovae
  • General
  • Nuclear reactions
  • Nucleosynthesis

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Nakamura, K., Yoshida, T., Shigeyama, T., & Kajino, T. (2010). Boron synthesis in type ic supernovae. Astrophysical Journal Letters, 718(2 PART 2). https://doi.org/10.1088/2041-8205/718/2/L137

Boron synthesis in type ic supernovae. / Nakamura, Ko; Yoshida, Takashi; Shigeyama, Toshikazu; Kajino, Toshitaka.

In: Astrophysical Journal Letters, Vol. 718, No. 2 PART 2, 01.08.2010.

Research output: Contribution to journalArticle

Nakamura, K, Yoshida, T, Shigeyama, T & Kajino, T 2010, 'Boron synthesis in type ic supernovae', Astrophysical Journal Letters, vol. 718, no. 2 PART 2. https://doi.org/10.1088/2041-8205/718/2/L137
Nakamura K, Yoshida T, Shigeyama T, Kajino T. Boron synthesis in type ic supernovae. Astrophysical Journal Letters. 2010 Aug 1;718(2 PART 2). https://doi.org/10.1088/2041-8205/718/2/L137
Nakamura, Ko ; Yoshida, Takashi ; Shigeyama, Toshikazu ; Kajino, Toshitaka. / Boron synthesis in type ic supernovae. In: Astrophysical Journal Letters. 2010 ; Vol. 718, No. 2 PART 2.
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