Search for Cosmic-Ray Antiproton Origins and for Cosmological Antimatter with BESS

• Main Authors: Kim, K. C., Kumazawa, T., Itazaki, A., Yoshimura, K., Matsuda, S., Mitchell, J. W., Abe, K., Makida, M., Haino, S., Nozaki, M., Sasaki, M., Hasegawa, M., Moiseev, A. A., Streitmatter, R. E., Fuke, H., Lee, M. H., Matsumoto, K., Myers, Z., Yamamoto, A., Kusumoto, A., Hams, T., Horikoshi, A., Matsukawa, Y., Nishimura, J., Orito, R.
• Format: Other/Unknown Material
• Language: unknown
• Published: 2011
• Subjects: Astronomy; Antarctic; The Antarctic; Austral; Antarc*
• Online Access: http://hdl.handle.net/2060/20120014324

The balloon-borne experiment with a superconducting spectrometer (BESS) has performed cosmic-ray observations as a US-Japan cooperative space science program, and has provided fundamental data on cosmic rays to study elementary particle phenomena in the early Universe. The BESS experiment has measured the energy spectra of cosmic-ray antiprotons to investigate signatures of possible exotic origins such as dark matter candidates or primordial black holes. and searched for heavier antinuclei that might reach Earth from antimatter domains formed in the early Universe. The apex of the BESS program was reached with the Antarctic flight of BESS-Polar II, during the 2007- 2008 Austral Summer, that obtained over 4.7 billion cosmic-ray events from 24.5 days of observation. The flight took place at the expected solar minimum, when the sensitivity of the low-energy antiproton measurements to a primary source is greatest. Here, we report the scientific restults, focusing on the long-duration flights of BESS-Polar I (2004) and BESS-Polar II (2007-2008).