The high-energy muon flux at sea level up to 8 TeV derived from the observed burst size spectrum

1971 ◽  
Vol 4 (2) ◽  
pp. 177-196 ◽  
Author(s):  
S. Chin ◽  
Y. Hanayama ◽  
T. Hara ◽  
S. Higashi ◽  
T. Kitamura ◽  
...  
Keyword(s):  
Sea Level ◽  
Burst Size ◽  
High Energy ◽  
Muon Flux ◽  
Size Spectrum ◽  
High Energy Muon ◽  
8 Tev

The high-energy muon flux at sea level obtained from an observation of the burst-size spectrum

1964 ◽  
Vol 32 (1) ◽  
pp. 1-13 ◽  
Author(s):  
S. Higashi ◽  
T. Kitamura ◽  
Y. Watase ◽  
M. Oda ◽  
Y. Tanaka
Keyword(s):  
Sea Level ◽  
Burst Size ◽  
High Energy ◽  
Muon Flux ◽  
Size Spectrum ◽  
High Energy Muon

The high–energy muon flux at sea level up to 10 TeV derived from an observation of the burst-size spectrum

1968 ◽  
Vol 46 (10) ◽  
pp. S297-S300 ◽  
Author(s):  
S. Chin ◽  
Y. Hanayama ◽  
T. Hara ◽  
S. Higashi ◽  
T. Kitamura ◽  
...  
Keyword(s):  
Energy Spectrum ◽  
Size Distribution ◽  
Sea Level ◽  
Burst Size ◽  
High Energy ◽  
Muon Flux ◽  
Size Spectrum ◽  
High Energy Muon ◽  
Relativistic Particles

Bursts produced by high-energy muons in rock have been observed at a depth of 40 m.w.e. underground by the use of two layers of scintillator 20 m2 in area and 2 m apart. The size distribution of bursts with several hundreds to 30 000 relativistic particles was obtained during an observing time of 11 424.13 hours. Following the method of Christy and Kusaka (1941), the energy spectrum of muons up to 10 TeV was derived from the burst-size distribution.

scholarly journals Variations of the high energy muon flux and space-time structure of the temperature profile in the atmosphere

2013 ◽  
Vol 409 ◽  
pp. 012231
Author(s):  
M G Kostyuk ◽  
V B Petkov ◽  
R V Novoseltseva ◽  
M M Boliev ◽  
M D Berkova ◽  
...  
Keyword(s):  
Temperature Profile ◽  
High Energy ◽  
Space Time ◽  
Muon Flux ◽  
Time Structure ◽  
High Energy Muon ◽  
Space Time Structure

The high-energy muon flux in air showers from Cygnus X-3

1985 ◽  
Vol 44 (7) ◽  
pp. 491-496 ◽  
Author(s):  
A. Castellina ◽  
B. D’Ettorre Piazzoli ◽  
G. Mannocchi ◽  
P. Picchi ◽  
S. Vernetto ◽  
...  
Keyword(s):  
High Energy ◽  
Muon Flux ◽  
Air Showers ◽  
High Energy Muon

Electromagnetic interactions of high-energy muons

1968 ◽  
Vol 46 (10) ◽  
pp. S361-S364 ◽  
Author(s):  
F. Ashton ◽  
R. B. Coats ◽  
D. A. Simpson
Keyword(s):  
Energy Transfer ◽  
Sea Level ◽  
High Energy ◽  
Muon Flux ◽  
Electromagnetic Interactions ◽  
Significant Divergence

The nearly horizontal muon flux at sea level has been used to study the interactions of high-energy (34–520 GeV) muons in an iron absorber producing energy transfer in the range 3–240 GeV. No significant divergence from accepted theory has been found.

A Tiny Telescope of Si-Detectors for High Energy Muon Flux Measurement with Electron Rejection

1980 ◽  
Vol 27 (1) ◽  
pp. 272-275 ◽  
Author(s):  
E. H. M. Heijne ◽  
P. Jarron ◽  
P. Lazeyras ◽  
W. R. Nelson ◽  
G. R. Stevenson
Keyword(s):  
Flux Measurement ◽  
High Energy ◽  
Muon Flux ◽  
High Energy Muon

scholarly journals ATMOSPHERIC MUON FLUX AT PEV ENERGIES

2010 ◽  
Vol 25 (18n19) ◽  
pp. 3733-3740 ◽  
Author(s):  
S. I. SINEGOVSKY ◽  
A. A. KOCHANOV ◽  
T. S. SINEGOVSKAYA ◽  
A. MISAKI ◽  
N. TAKAHASHI
Keyword(s):  
Cross Sections ◽  
Production Cross ◽  
High Energy ◽  
Muon Flux ◽  
Muon Spectrum ◽  
High Energy Muon ◽  
Very High Energy ◽  
Atmospheric Muon ◽  
Near Future ◽  
Very High

In the near future, the energy region above few hundreds of TeV may really be accessible for measurements of the atmospheric muon spectrum with IceCube array. Therefore, one expects that muon flux uncertainties above 50 TeV, related to a poor knowledge of charm production cross-sections and insufficiently examined primary spectra and composition, will be diminished. We give predictions for the very high-energy muon spectrum at sea level, obtained with the three hadronic interaction models, taking into account also the muon contribution due to decays of the charmed hadrons.

scholarly journals HIGH-ENERGY ATMOSPHERIC MUON FLUX EXPECTED AT INDIA-BASED NEUTRINO OBSERVATORY

2008 ◽  
Vol 23 (19) ◽  
pp. 2933-2942 ◽  
Author(s):  
SUKANTA PANDA ◽  
SERGEI I. SINEGOVSKY
Keyword(s):  
Cross Sections ◽  
Zenith Angle ◽  
High Energy ◽  
Muon Flux ◽  
Angle Dependence ◽  
High Energies ◽  
High Energy Muon ◽  
Atmospheric Muon ◽  
Low X ◽  
Very High

We calculate the zenith-angle dependence of conventional and prompt high-energy muon fluxes at India-Based Neutrino Observatory (INO) depth. This study demonstrates a possibility to discriminate models of the charm hadroproduction including the low-x QCD behavior of hadronic cross-sections relevant at very high energies.

scholarly journals WIMPs at high energy muon colliders

2021 ◽  
Vol 103 (7) ◽  
Author(s):  
Tao Han ◽  
Zhen Liu ◽  
Lian-Tao Wang ◽  
Xing Wang
Keyword(s):  
High Energy ◽  
High Energy Muon ◽  
Muon Colliders

Uncertanties of atmospheric high-energy muon fluxes and spectrum of primary cosmic rays

2007 ◽  
Vol 50 (9) ◽  
pp. 891-897
Author(s):  
A. A. Kochanov ◽  
T. S. Sinegovskaya ◽  
S. I. Sinegovskii
Keyword(s):  
Cosmic Rays ◽  
High Energy ◽  
High Energy Muon ◽  
Primary Cosmic Rays
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