We searched for antideuterons (d̄'s) in the 4.7×10⁹ cosmic-ray events observed during the BESS-Polar II flight at solar minimum in 2007--2008 but found no candidates. The resulting 95% C.L. upper limit on the d̄ flux is 6.7×10^-5 (m² s sr GeV/n)^-1 in an energy range from 0.163 to 1.100 GeV/n. The result has improved by more than a factor of 14 from the upper limit of BESS97, which had a potential comparable to that of BESS-Polar II in the search for cosmic-origin d̄'s and was conducted during the former solar minimum. The upper limit of d̄ flux from BESS-Polar II is the first result achieving the sensitivity to constrain the latest theoretical predictions.
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Sakai et al. (2024) studied this question.
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