- icrc2007@icrc2007.unam.mx
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Contribution Oral
Speakers
- Dr. Thomas HAMS
Primary authors
- Dr. Thomas HAMS (CRESST/USRA/NASA/Goddard Space Flight Center, Greenbelt, MD 20771 USA)
Co-authors
- Dr. Reiko ORITO (Kobe University, Kobe, Hyogo, 657-8501 Japan)
- Mr. Kenichi SAKAI (The University of Tokyo, Bunkyo, Tokyo, 113-0033 Japan)
- Dr. Ko ABE (Kobe University, Kobe, Hyogo, 657-8501 Japan)
- Dr. Hideyuki FUKE (Institute of Space and Astronautical Science (ISAS/JAXA), Sagamihara, Kanagawa, 229-8510 Japan)
- Dr. Sadakazu HAINO (High Energy Accelerator Research Organization, Tsukuba, Ibaraki, 305-0801 Japan)
- Mr. Atsushi HORIKOSHI (High Energy Accelerator Research Organization, Tsukuba, Ibaraki, 305-0801 Japan)
- Mr. Ki-Chun KIM (IPST, University of Maryland, College Park, MD 20742 USA)
- Dr. Moo Hyun LEE (IPST, University of Maryland, College Park, MD 20742 USA)
- Dr. Yasuhiro MAKIDA (High Energy Accelerator Research Organization, Tsukuba, Ibaraki, 305-0801 Japan)
- Dr. Shinya MATSUDA (High Energy Accelerator Research Organization, Tsukuba, Ibaraki, 305-0801 Japan)
- Dr. John W. MITCHELL (NASA/Goddard Space Flight Center, Greenbelt, MD 20771 USA)
- Dr. Alexander A. MOISEEV (CRESST/USRA/NASA/Goddard Space Flight Center, Greenbelt, MD 20771 USA)
- Dr. Jun NISHIMURA (The University of Tokyo, Bunkyo, Tokyo, 113-0033 Japan)
- Dr. Mitsuaki NOZAKI (High Energy Accelerator Research Organization, Tsukuba, Ibaraki, 305-0801 Japan)
- Dr. Jonathan F. ORMES (University of Denver, Denver, CO 80208 USA)
- Dr. Makoto SASAKI (CRESST/USRA/NASA/Goddard Space Flight Center, Greenbelt, MD 20771 USA)
- Dr. Yoshiaki SHIKAZE (Kobe University, Kobe, Hyogo, 657-8501 Japan)
- Dr. Eun-Suk SEO (IPST, University of Maryland, College Park, MD 20742 USA)
- Dr. Robert E. STREITMATTER (NASA/Goddard Space Flight Center, Greenbelt, MD 20771 USA)
- Mr. Junichi SUZUKI (High Energy Accelerator Research Organization, Tsukuba, Ibaraki, 305-0801 Japan)
- Mr. Kenichi TANAKA (High Energy Accelerator Research Organization, Tsukuba, Ibaraki, 305-0801 Japan)
- Dr. Takamasa YAMAGAMI (Institute of Space and Astronautical Science (ISAS/JAXA), Sagamihara, Kanagawa, 229-8510 Japan)
- Dr. Akira YAMAMOTO (High Energy Accelerator Research Organization, Tsukuba, Ibaraki, 305-0801 Japan)
- Dr. Tetsuya YOSHIDA (Institute of Space and Astronautical Science (ISAS/JAXA), Sagamihara, Kanagawa, 229-8510 Japan)
- Dr. Koji YOSHIMURA (High Energy Accelerator Research Organization, Tsukuba, Ibaraki, 305-0801 Japan)
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Abstract content
The Search for Antimatter in the galactic cosmic radiation is one of the main scientific objectives of the BESS-Program. A flatter antiproton spectrum below the secondary production peak at 1 GeV would suggest novel antiproton source, such as evaporating black-holes or decaying super-symmetric particles. The BESS-Polar experiment is designed as a highly transparent magnetic rigidity spectrometer that can precisely detect antiprotons down to energies of 0.1 GeV where a potential excess of antiprotons over the secondary production might be more apparent. The BESS-Polar instrument had its first successful balloon flight in December 2004, from McMurdo Station in Antarctica. During the 8.5-day long flight 900 million events where recorded. In this paper, we discuss the spectra of antiproton and proton as well as the search for antihelium.
If this papers is presented for a collaboration, please specify the collaboration
BESS
Reference
Proceedings of the 30th International Cosmic Ray Conference; Rogelio Caballero, Juan Carlos D'Olivo, Gustavo Medina-Tanco, Lukas Nellen, Federico A. Sánchez, José F. Valdés-Galicia (eds.); Universidad Nacional Autónoma de México, Mexico City, Mexico, 2008; Vol. 2 (OG part 1), pages 67-70