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    Nonthermal axino as cool dark matter in the supersymmetric standard model without R parity

    Eung Jin Chun*

    Hang Bae Kim†

    • Korea Institute for Advanced Study, 207-43 Cheongryangri-dong, Dongdaemun-gu, Seoul 130-012, Korea

    • Department of Physics and Institute of Basic Science, Sungkyunkwan University, Suwon 440–746, Korea

    • *Email address: ejchun@kias.re.kr
    • †Email address: hbkim@newton.skku.ac.kr

    Phys. Rev. D 60, 095006 – Published 7 October, 1999

    DOI: https://doi.org/10.1103/PhysRevD.60.095006

    Abstract

    We point out that the axino predicted as the supersymmetric partner of the axion is a good candidate for the recently proposed sterile neutrino cool dark matter. The axino mass falls into the right range (≲keV) in the context of gauge-mediated supersymmetry breaking. A sizable mixing of the axino with active neutrinos arises when R-parity violation is allowed and the resulting neutrino masses and mixing accommodate the atmospheric and solar neutrino oscillations simultaneously.

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