Energy dependence of charm production cr
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I.N. Rakobolskaya; T.M. Roganova; L.G. Sveshnikova
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Article
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2003
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Elsevier Science
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English
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Charm production cross-sections estimated from data obtained in the "Pamir" and other cosmic ray experiments are compared with accelerator data. The strong increase of the charm production cross-section with energy, essential for the explanation of cosmic ray data, is analyzed from a theoretical poi