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We calculate the solar neutrino and antineutrino flux in the keV energy range.
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M. Pospelov, A. Ritz and M. B. Voloshin, Bosonic super-WIMPs as keV-scale dark matter,
2008
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2012
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H. An, M. Pospelov and J. Pradler, New stellar constraints on dark photons,
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J. Redondo and G. Raffelt, Solar constraints on hidden photons re-visited,
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J. Redondo, Solar axion flux from the axion-electron coupling,
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E. Hardy and R. Lasenby, Stellar cooling bounds on new light particles: Plasma mixing effects,
2017
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2017
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2017
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