Radiative corrections to the average bremsstrahlung energy loss of high-energy muons

High-energy muons can travel large thicknesses of matter. For underground neutrino and cosmic ray detectors the energy loss of muons has to be known accurately for simulations. In this article the next-to-leading order correction to the average energy loss of muons through bremsstrahlung is calculat...

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Main Authors: A. Sandrock, S.R. Kelner, W. Rhode
Format: Article
Language:English
Published: Elsevier 2018-01-01
Series:Physics Letters B
Subjects:
QED
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269317309395
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spelling doaj-b9bf6a40f2fb46eab7bec7412dbc8dc02020-11-24T21:27:18ZengElsevierPhysics Letters B0370-26931873-24452018-01-01776C35035410.1016/j.physletb.2017.11.047Radiative corrections to the average bremsstrahlung energy loss of high-energy muonsA. Sandrock0S.R. Kelner1W. Rhode2Department of Physics, TU Dortmund University, D-44221 Dortmund, GermanyNational Research Nuclear University (MEPhI), Kashirskoe Shosse 31, Moscow 115409, RussiaDepartment of Physics, TU Dortmund University, D-44221 Dortmund, GermanyHigh-energy muons can travel large thicknesses of matter. For underground neutrino and cosmic ray detectors the energy loss of muons has to be known accurately for simulations. In this article the next-to-leading order correction to the average energy loss of muons through bremsstrahlung is calculated using a modified Weizsäcker–Williams method. An analytical parametrisation of the numerical results is given.http://www.sciencedirect.com/science/article/pii/S0370269317309395Muon cross sectionsBremsstrahlungRadiative correctionsQED
collection DOAJ
language English
format Article
sources DOAJ
author A. Sandrock
S.R. Kelner
W. Rhode
spellingShingle A. Sandrock
S.R. Kelner
W. Rhode
Radiative corrections to the average bremsstrahlung energy loss of high-energy muons
Physics Letters B
Muon cross sections
Bremsstrahlung
Radiative corrections
QED
author_facet A. Sandrock
S.R. Kelner
W. Rhode
author_sort A. Sandrock
title Radiative corrections to the average bremsstrahlung energy loss of high-energy muons
title_short Radiative corrections to the average bremsstrahlung energy loss of high-energy muons
title_full Radiative corrections to the average bremsstrahlung energy loss of high-energy muons
title_fullStr Radiative corrections to the average bremsstrahlung energy loss of high-energy muons
title_full_unstemmed Radiative corrections to the average bremsstrahlung energy loss of high-energy muons
title_sort radiative corrections to the average bremsstrahlung energy loss of high-energy muons
publisher Elsevier
series Physics Letters B
issn 0370-2693
1873-2445
publishDate 2018-01-01
description High-energy muons can travel large thicknesses of matter. For underground neutrino and cosmic ray detectors the energy loss of muons has to be known accurately for simulations. In this article the next-to-leading order correction to the average energy loss of muons through bremsstrahlung is calculated using a modified Weizsäcker–Williams method. An analytical parametrisation of the numerical results is given.
topic Muon cross sections
Bremsstrahlung
Radiative corrections
QED
url http://www.sciencedirect.com/science/article/pii/S0370269317309395
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AT srkelner radiativecorrectionstotheaveragebremsstrahlungenergylossofhighenergymuons
AT wrhode radiativecorrectionstotheaveragebremsstrahlungenergylossofhighenergymuons
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