Observation of Cosmic-Ray Antiprotons at Energies below 500 MeV

K. Yoshimura, S. Orito, I. Ueda, K. Anraku, R. Golden, M. Imori, S. Inaba, B. Kimbell, N. Kimura, Y. Makida, H. Matsumoto, H. Matsunaga, J. Mitchell, M. Motoki, J. Nishimura, M. Nozaki, J. Ormes, T. Saeki, R. Streitmatter, J. Suzuki, K. Tanaka, N. Yajima, T. Yamagami, A. Yamamoto, and T. Yoshida
Phys. Rev. Lett. 75, 3792 – Published 20 November 1995
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Abstract

A search for cosmic-ray antiprotons was performed using a balloon-borne experiment with a superconducting magnetic rigidity spectrometer (BESS). We have detected four antiprotons in the kinetic energy range between 300 and 500 MeV, the first antiprotons to be identified by a direct mass measurement. The corresponding p¯p flux ratio at the top of the atmosphere is found to be 1.20.65+1.0 × 105. No antiprotons were observed in the range between 175 and 300 MeV, resulting in a 90% C.L. upper limit on the flux ratio of 2.9 × 105.

  • Received 20 March 1995

DOI:https://doi.org/10.1103/PhysRevLett.75.3792

©1995 American Physical Society

Authors & Affiliations

K. Yoshimura1, S. Orito1, I. Ueda1, K. Anraku2, R. Golden3, M. Imori1, S. Inaba2, B. Kimbell3, N. Kimura2, Y. Makida2, H. Matsumoto4, H. Matsunaga1, J. Mitchell5, M. Motoki4, J. Nishimura6, M. Nozaki4, J. Ormes5, T. Saeki1, R. Streitmatter5, J. Suzuki2, K. Tanaka2, N. Yajima6, T. Yamagami6, A. Yamamoto2, and T. Yoshida1

  • 1University of Tokyo, Bunkyo-ku, Tokyo, 113, Japan
  • 2National Laboratory for High Energy Physics (KEK), Tsukuba, Ibaraki, Japan
  • 3New Mexico State University, Las Cruces, New Mexico 88003
  • 4Kobe University, Kobe, Hyogo, Japan
  • 5National Aeronautics and Space Administration, Goddard Space Flight Center (NASA/GSFC), Greenbelt, Maryland 20771
  • 6The Institute of Space and Astronautical Science (ISAS), Sagamihara, Kanagawa, 229, Japan

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Vol. 75, Iss. 21 — 20 November 1995

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