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Naslov:Measurement of the proton-air cross section with Telescope Array's Black Rock Mesa and Long Ridge fluorescence detectors, and surface array in hybrid mode
Avtorji:ID Abbasi, R. U. (Avtor)
ID Abe, Mitsuhiro (Avtor)
ID Abu-Zayyad, T. (Avtor)
ID Allen, M. (Avtor)
ID Azuma, R. (Avtor)
ID Barcikowski, E. (Avtor)
ID Belz, J. W. (Avtor)
ID Bergman, Douglas R. (Avtor)
ID Blake, S. A. (Avtor)
ID Lundquist, Jon Paul (Avtor)
Datoteke: Gradivo nima datotek, ki so prostodostopne za javnost. Gradivo je morda fizično dosegljivo v knjižnici fakultete, zalogo lahko preverite v COBISS-u. Povezava se odpre v novem oknu
Jezik:Angleški jezik
Vrsta gradiva:Neznano
Tipologija:1.01 - Izvirni znanstveni članek
Organizacija:UNG - Univerza v Novi Gorici
Opis:Ultra high energy cosmic rays provide the highest known energy source in the universe to measure proton cross sections. Though conditions for collecting such data are less controlled than an accelerator environment, current generation cosmic ray observatories have large enough exposures to collect significant statistics for a reliable measurement for energies above what can be attained in the lab. Cosmic ray measurements of cross section use atmospheric calorimetry to measure depth of air shower maximum (Xmax), which is related to the primary particle’s energy and mass. The tail of the Xmax distribution is assumed to be dominated by showers generated by protons, allowing measurement of the inelastic proton-air cross section. In this work the proton-air inelastic cross section measurement, σ_inel_p−air, using data observed by Telescope Array’s Black Rock Mesa and Long Ridge fluorescence detectors and surface detector array in hybrid mode is presented. σ_inel_p−air is observed to be 520.1 ± 35.8 [Stat.] +25.0 −40 [Sys.] mb at √s = 73 TeV. The total proton-proton cross section is subsequently inferred from Glauber formalism and is found to be σ_tot_pp = 139.4 +23.4−21.3[Stat.] +15.0−24.0[Sys.] mb.
Ključne besede:cosmic rays, astroparticles, proton-air cross section
Leto izida:2020
Št. strani:str. 1-13
Številčenje:Vol. 102, 6
PID:20.500.12556/RUNG-6246 Novo okno
COBISS.SI-ID:50289923 Novo okno
UDK:524
ISSN pri članku:2470-0010
DOI:10.1103/PhysRevD.102.062004 Novo okno
NUK URN:URN:SI:UNG:REP:CR5MVANS
Datum objave v RUNG:04.02.2021
Število ogledov:2330
Število prenosov:0
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Gradivo je del revije

Naslov:Physical review
Skrajšan naslov:Phys. rev., D
Založnik:American Physical Society
ISSN:2470-0010
COBISS.SI-ID:29757223 Novo okno

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