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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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 |
work_keys_str_mv |
AT asandrock radiativecorrectionstotheaveragebremsstrahlungenergylossofhighenergymuons AT srkelner radiativecorrectionstotheaveragebremsstrahlungenergylossofhighenergymuons AT wrhode radiativecorrectionstotheaveragebremsstrahlungenergylossofhighenergymuons |
_version_ |
1725975495391051776 |