Low energy antiprotons in the cosmic rays: A new upper limit View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

1989-03

AUTHORS

S. P. Ahlen, S. Barwick, J. J. Beatty, C. R. Bower, G. Gerbier, R. M. Heinz, D. Lowder, S. McKee, S. Mufson, J. A. Musser, P. B. Price, M. H. Salamon, G. Tarle, A. Tomasch, B. Zhou

ABSTRACT

Kinematics predicts the severe suppression of low-energy (<1 GeV) secondary antiprotons in the Galactic cosmic rays. Thus the observation several years ago of a finite flux of low-energy antiprotons could not be explained with existing models of cosmic ray propagation, which led to a plethora of theoretical speculation. We have recently flown a balloon-borne instrument to measure the energy spectrum of cosmic-ray, and have found no antiprotons in the energy interval 200–640 MeV (corrected to the top of the atmosphere). This yields an upper limit to the ratio of 5.5×10−5 (90% confidence level), well below and hence contradicting the earlier result. More... »

PAGES

97-103

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/bf02398661

DOI

http://dx.doi.org/10.1007/bf02398661

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1014672436


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