Feasibility Studies of Charge Exchange Measurements in pp Collisions at the LHC

Author:

Fehérkuti AnnaORCID,Veres Gábor I.ORCID,Ulrich Ralf,Pierog TanguyORCID

Abstract

(1) Pions produced in the development of extended atmospheric cosmic ray air showers subsequently decay to muons. The measured yield of those muons is generally underestimated by current phenomenological models and event generators optimized for cosmic ray physics. The importance of those disagreements motivates the feasibility studies for testing these models at the Large Hadron Collider (LHC) energies, at the highest center-of-mass energies achievable in a laboratory. The interaction of a nucleus and a virtual pion created in a charge exchange reaction at the LHC is a similar process to those contributing to the development of air showers in case of cosmic rays. The crucial problem of such an analysis is the selection of charge exchange events with the highest possible efficiency and high purity from proton–proton collisions at the LHC. (2) For this we consider distributions of various measurable quantities given by event generators commonly used in cosmic ray physics. (3) We examine the expected distributions of energy deposited in different calorimeters of an LHC experiment. We consider the geometrical acceptance and energy resolution of the detectors at the Compact Muon Solenoid (CMS) experiment, as an example. We determine a working point cut from the various options for event selection, and compare signal and background predictions using different models for a representative simple observable, such as average transverse momentum or charge particle yield. (4) A set of event selection cuts along these considerations is proposed, with the aim of achieving optimal efficiency and purity.

Funder

Hungarian Scientific Research Fund

New National Excellence Program

Publisher

MDPI AG

Subject

General Physics and Astronomy

Reference14 articles.

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2. The Pierre Auger Collaboration (2015). The Pierre Auger Cosmic Ray Observatory. Nucl. Instrum. Methods Phys. Res., 798, 172–213.

3. Baur, S., Dembinski, H., Pierog, T., Ulrich, R., and Werner, K. (2020). The ratio of electromagnetic to hadronic energy in high energy hadron collisions as a probe for collective effects, and implications for the muon production in cosmic ray air showers. arXiv.

4. Farrar, G.R., and Allen, J.D. (2013). A new physical phenomenon in ultra-high energy collisions. arXiv.

5. Direct measurement of the muonic content of extensive air showers between 2 × 1017 and 2 × 1018 eV at the Pierre Auger Observatory;Eur. Phys. J. C,2020

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