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Measurement of cosmic-ray low-energy antiproton spectrum with the first BESS-Polar Antarctic flight

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arxiv 0805.1754 v2 pith:VQDCTLND submitted 2008-05-12 astro-ph

K. Abe , H. Fuke , S. Haino , T. Hams , A. Itazaki , K. C. Kim , T. Kumazawa , M. H. Lee
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Y. Makida S. Matsuda K. Matsumoto J. W. Mitchell A. A. Moiseev Z. Myers J. Nishimura M. Nozaki R. Orito J. F. Ormes M. Sasaki E. S. Seo Y. Shikaze R. E. Streitmatter J. Suzuki Y. Takasugi K. Takeuchi K. Tanaka T. Yamagami A. Yamamoto T. Yoshida K. Yoshimura
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The BESS-Polar spectrometer had its first successful balloon flight over Antarctica in December 2004. During the 8.5-day long-duration flight, almost 0.9 billion events were recorded and 1,520 antiprotons were detected in the energy range 0.1-4.2 GeV. In this paper, we report the antiproton spectrum obtained, discuss the origin of cosmic-ray antiprotons, and use antiprotons to probe the effect of charge sign dependent drift in the solar modulation.

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  1. Constraints on Primordial Black Holes

    astro-ph.CO 2020-02 accept novelty 4.0 of 10

    Updated compilation shows PBHs are tightly constrained across 55 orders of magnitude in mass, ruling out dominant dark matter contributions except in narrow windows, with many limits carrying observational uncertainties.

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