Modeling Strangeness Enhancements to resolve the Muon Excess in Cosmic Ray Extensive Air Shower Data

نویسندگان

چکیده

Experimental observations of extensive air showers have revealed an excess the muon content with respect to their theoretical simulations, which we refer as puzzle. This puzzle hampers a precise determination ultra-high-energy cosmic ray mass composition. We investigate potential producing states dense quark-gluon matter (which call fireballs) resolve quantified data from Pierre Auger Observatory on depth shower maximum and number muons at ground. Adopting phenomenological fireball model, find that inelasticity enhancement associated formation plasma state is in tension electromagnetic longitudinal development. Instead, restrict model only enhance strangeness produced Standard Model hadronic interactions, dub this strangeball model. With analytic approach based Heitler-Matthews then explicit sets parameters Constraints shower-to-shower fluctuations require enhancements already energies accessible current-generation collider experiments. At Tevatron LHC estimate 40% interactions produce strangeballs, corresponding 5-9% increase average fraction energy retained cascade compared predictions current interaction models. A comparison relevant measurements LHCf LHCb detectors does not directly exclude scenario, though obtained suggests stringent test 14 TeV.

برای دانلود باید عضویت طلایی داشته باشید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

30TH INTERNATIONAL COSMIC RAY CONFERENCE Muon Production Height in the Air-Shower Experiment KASCADE-Grande

A large area (128m) Muon Tracking Detector (MTD), located within the KASCADE experiment, has been built with the aim to identify muons (Eμ >0.8GeV) and their directions in extensive air showers by track measurements under more than 18 r.l. shielding. The orientation of the muon track with respect to the shower axis is expressed in terms of the radialand tangential angles. By means of triangulat...

متن کامل

Cosmic Ray Results from the IceTop Air Shower Array

IceTop, the surface component of the IceCube neutrino telescope at the South Pole, is an air-shower array which will finally consist of 160 ice Cherenkov tanks at 80 stations spread over an area of 1 km. Currently 40 stations are deployed and taking data. The detector is designed to cover the energy range above the knee up to about 10 eV and study the mass composition of primary cosmic rays. In...

متن کامل

KASCADE extensive air shower experiment

The main aim of the KASCADE extensive air shower (EAS) experiment is the determination of the chemical composition of cosmic rays in the energy range around and above the knee at Ek ≈ 3 PeV. A large number of observables is measured simultaneously for each individual event, by the combination of various detection techniques for the electromagnetic, the muonic, and the hadronic component of the ...

متن کامل

Study of the Extensive Air Shower Size and the Energy Spectra of Cosmic Ray Muons at Sea Level

In this paper I presented the results obtained for the differential energy spectra of muons at sea level determined as a function of three zenith angles. I calculated the shower size and the number of muons per square meter as a function of the lateral distance from the center of the shower. The data interpretation provide the most significant physical information for understanding the main pro...

متن کامل

Cosmic Ray Muon Physics

We present a review of atmospheric and underground muon flux measurements. The relevance of these data for the atmospheric neutrino flux computation is emphasized. Possible sources of systematic errors in the measurements are discussed, focusing on the sea level muon data. Underground muon data are also reported.

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: Journal of Cosmology and Astroparticle Physics

سال: 2022

ISSN: ['1475-7516', '1475-7508']

DOI: https://doi.org/10.1088/1475-7516/2023/02/017