Cosmic Ray Positrons at High Energies: A New Measurement

Details Cosmic Ray Positrons at High Energies: A New Measurement Cosmic Ray Positrons at High Energies: A New Measurement

1995-05-30

arxiv.org/abs/astro-ph/9505141v1

Phys.Rev.Lett. 75 (1995) 390-393

Astronomy and Astrophysics

Astrophysics

14 pages, 3 figures, tarred-compressed-uuencoded-postscript file; heatprl_preprint.tar_z (227 kbytes); Physical Review Letters

Scientific paper

We present a new measurement of the cosmic-ray positron fraction e+/(e+ + e-) obtained from the first balloon flight of the High Energy Antimatter Telescope (HEAT). Using a magnet spectrometer combined with a transition radiation detector, an electromagnetic calorimeter, and time-of-flight counters we have achieved a high degree of background rejection. Our results do not indicate a major contribution to the positron flux from primary sources. In particular, we see no evidence for the significant rise in the positron fraction at energies above ~10 GeV previously reported.

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