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Titolo:
Fluxes of cosmic-ray muons and atmospheric neutrinos at high energies
Autore:
Volkova, LV; Zatsepin, GT;
Indirizzi:
Russian Acad Sci, Inst Nucl Res, Moscow 117312, Russia Russian Acad Sci Moscow Russia 117312 st Nucl Res, Moscow 117312, Russia
Titolo Testata:
PHYSICS OF ATOMIC NUCLEI
fascicolo: 2, volume: 64, anno: 2001,
pagine: 266 - 274
SICI:
1063-7788(200102)64:2<266:FOCMAA>2.0.ZU;2-J
Fonte:
ISI
Lingua:
ENG
Soggetto:
HEAVY-QUARK PRODUCTION; HADRONIC COLLISIONS; QCD CORRECTIONS; SPECTRUM; PARTICLE; RATIO;
Tipo documento:
Article
Natura:
Periodico
Settore Disciplinare:
Physical, Chemical & Earth Sciences
Citazioni:
34
Recensione:
Indirizzi per estratti:
Indirizzo: Volkova, LV Russian Acad Sci, Inst Nucl Res, Pr Shestidesyatiletiya Oktyabrya 7A, Moscow 117312, Russia Russian Acad Sci Pr Shestidesyatiletiya Oktyabrya 7A Moscow Russia 117312
Citazione:
L.V. Volkova e G.T. Zatsepin, "Fluxes of cosmic-ray muons and atmospheric neutrinos at high energies", PHYS ATOM N, 64(2), 2001, pp. 266-274

Abstract

The problem of charm generation in the interactions of nucleons with nuclei of air atoms at energies inaccessible at present-day accelerators is discussed. Both experimental data on cosmic-ray muons and the predictions of QCD-based theoretical models are used in analyzing the behavior of the differential cross sections for charmed-particle production at high energies. Thecalculated fluxes of muons and neutrinos arriving at sea level both along the vertical and along the horizontal direction are presented, together with their approximations for the interval 2 x 10(2)-10(10) GeV. (C) 2001 MAIK"Nauka/Interperiodica".

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Documento generato il 07/04/20 alle ore 21:05:44