[PDF] Top 20 Test of hadronic interaction models with the KASCADE-Grande muon data
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Test of hadronic interaction models with the KASCADE-Grande muon data
... of hadronic models employed in EAS simulations present discrepancies from the observed ...set-up KASCADE have shown that models such as QGSJET 98 and 01, EPOS ...the data on the hadron, ... See full document
5
Tests of the SIBYLL 2.3 high-energy hadronic interaction model using the KASCADE-Grande muon data
... Hadronic interaction models are an important element in the analysis of data from extensive air sho- wers (EAS) induced by cosmic rays in the ...the models that has been updated is ... See full document
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Testing of almost all the hadronic interaction models by comparing calculated muon energy spectrum with data
... partial muon spectra. Thus, with the help of any of the interaction models [1–9], the CORSIKA package and approximations of data on fluxes of the primary cosmic nuclei [21–31] one can predict ... See full document
6
Testing of the VENUS 4.12, DPMJET 2.55, QGSJET II-03 and SIBYLL 2.3 hadronic interaction models via help of the atmospheric vertical muon spectra
... these models should be thoroughly tested. Usually these models are tested with the help of the accelerator data at small values ( ∼ 0) of the pseudorapidity η where most of secondary particles ... See full document
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Recent results from the KASCADE-Grande data analysis
... the test of hadronic interaction models with KASCADE and KASCADE-Grande ...by KASCADE-Grande data, initial tests of SIBYLL ...by ... See full document
5
Confronting the EPOS-LHC model predictions on the charged particle and muon attenuation lengths of EAS with the measurements of the KASCADE-Grande observatory
... high-energy hadronic interaction models are ...the muon content of air showers using the MTD and the KASCADE muon array has been designed in order to search for clues that could ... See full document
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The cosmic ray energy spectrum in the range 1016–1018 eV measured by KASCADE-Grande
... In KASCADE-Grande, the all-particle energy spectrum is derived by means of different techniques: using only one component, such as the size of the charged (Kang et ...or muon (Arteaga et ...(iv) ... See full document
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The 〈 ln A 〉 study with the Muon tracking detector in the KASCADE-Grande experiment – comparison of hadronic interaction models
... the KASCADE-Grande Muon Tracking Detector it was possible to measure with high accuracy directions of EAS muons with energy above ...Reconstructed muon tracks allow investigation of ... See full document
5
Constraints of hadronic interaction models from the cosmic muon observations
... interaction models. In the case of “soft” interaction the generation of secondary particles emitted at mostly small angles with respect to the projectile particle (the highest values of ... See full document
5
KASCADE-Grande: Composition studies in the view of the post-LHC hadronic interaction models
... same data with different hadronic interaction models we deepened the analysis in the following way: For each interaction model separately a set of data was generated with the ... See full document
7
Summary of the main results of the KASCADE and KASCADE-Grande experiments
... the KASCADE operation great at- tention was devoted to a careful check of the hadronic interaction models used in the CORSIKA ...hadrons, hadronic energy sum) and of the KASCADE ... See full document
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Measurements and tests of hadronic interactions at ultra-high energies with the Pierre Auger Observatory
... logarithmic muon content h ln R µ i as a function of the average shower depth hX max i is plotted for data and the mass phase-space predicted by models at E = 10 19 ...in data differs from the ... See full document
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Hadronic Interactions and Air Showers: Where Do We Stand?
... LHC data contribute a lot to reducing the uncertainties in air shower simulations, providing better tools to analyze cosmic ray ...the hadronic models have been reduced but one should keep in mind ... See full document
8
On the Hadronic light-by-light contribution to the muon g – 2
... the hadronic vacuum polarization contribution (HVP) there are integrals over all photon momenta ...The hadronic part is thus not only at ...the muon Pauli ... See full document
8
Hadronic Leading Order Contribution to the Muon g-2
... those data points which have large ...accurate data. To do so, we gather near-by data points into a bin (which we call a ‘cluster’) and integrate over the clusters to evaluate the dispersive ... See full document
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Measurement of the muon content in air showers at the Pierre Auger Observatory
... Since the electromagnetic component of a shower is absorbed faster in the atmosphere than the muonic part, highly inclined showers deliver an almost pure muon “beam”, which is suitable for direct studies. Here we ... See full document
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Hadronic light-by-light scattering in the muon g − 2
... For the pseudoscalar-pole contribution to HLbL the double-virtual transition form factors are needed as input, see Figure 1. There exist already several measurements of the single-virtual tran- sition form factors in ... See full document
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Low energy exclusive e+e− → hadrons cross sections and g − 2 of the muon
... The data are collected with the initial-state radiation (ISR) ...reduced hadronic energy √ s is obtained by selecting events with a hard ISR photon radiated from either the incoming electron or incoming ... See full document
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Measuring aμHLO with space-like data
... scattering data to Monte Carlo (MC) predictions. The LO Bhabha cross section receives contributions from t- and s- channel photon exchange amplitudes. At NLO in QED, it is customary to distinguish corrections with ... See full document
6
e+e− hadronic cross section and the muon g − 2
... The topology of the events is such that the ISR photon is back-to-back with the hadron system which allows to reach, thanks to the boost, detection efficiencies greater then zero even at the produc- tion threshold of the ... See full document
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