Supernova neutrino nucleosynthesis of the radioactive 92Nb observed in primitive meteorites

T. Hayakawa, K. Nakamura, T. Kajino, S. Chiba, N. Iwamoto, M. K. Cheoun, G. J. Mathews

    研究成果: Article査読

    29 被引用数 (Scopus)

    抄録

    The isotope 92Nb decays to 92Zr with a half-life of 3.47 × 107 yr. Although this isotope does not exist in the current solar system, initial abundance ratios for 92Nb/ 93Nb at the time of solar system formation have been measured in primitive meteorites. The astrophysical origin of this material, however, has remained unknown. In this Letter, we present new calculations which demonstrate a novel origin for 92Nb via neutrino-induced reactions in core-collapse supernovae (ν-process). Our calculated result shows that the observed ratio of 92Nb/93Nb ∼ 10-5 can be explained by the ν-process.

    本文言語English
    論文番号L9
    ジャーナルAstrophysical Journal Letters
    779
    1
    DOI
    出版ステータスPublished - 2013 12月 10

    ASJC Scopus subject areas

    • 宇宙惑星科学
    • 天文学と天体物理学

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