2015
DOI: 10.1103/physrevd.92.114011
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Photoproduction total cross section and shower development

Abstract: The total photoproduction cross section at ultra-high energies is obtained using a model based on QCD minijets and soft-gluon resummation and the ansatz that infrared gluons limit the rise of total cross sections. This cross section is introduced into the Monte Carlo system AIRES to simulate extended air-showers initiated by cosmic ray photons. The impact of the new photoproduction cross section on common shower observables, especially those related to muon production, is compared with previous results.

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Cited by 7 publications
(16 citation statements)
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“…108 The maximum single gluon momentum allowed for soft gluon integration, q max in GeV, vs. √ s in GeV for γ p scattering, from [147]. Reprinted with permission from [147] √ s in GeV, from [450]. This is Fig.…”
Section: The Bn Model: Eikonal Mini-jet Model With Soft-gluon Resummamentioning
confidence: 99%
See 1 more Smart Citation
“…108 The maximum single gluon momentum allowed for soft gluon integration, q max in GeV, vs. √ s in GeV for γ p scattering, from [147]. Reprinted with permission from [147] √ s in GeV, from [450]. This is Fig.…”
Section: The Bn Model: Eikonal Mini-jet Model With Soft-gluon Resummamentioning
confidence: 99%
“…This is Fig. (2) from [450], ©(2015) by the American Physical Society for the protons, while two sets of photon PDFs were used. A comparison was made with predictions from some available models, such as indicated in the figure and discussed in [147].…”
Section: The Bn Model: Eikonal Mini-jet Model With Soft-gluon Resummamentioning
confidence: 99%
“…significantly into the region of ultra high energy cosmic rays. Therefore VHEeP data could be used to constrain cosmic-ray air-shower simulations and so will be of benefit to understanding the nature of cosmic rays at the highest energies (for example, see [24]). Figure 5: Total γp cross section versus photon-proton centre-of-mass energy, W , shown for data compared to various models.…”
Section: Total Photon-proton Cross Sectionmentioning
confidence: 99%
“…We address again the question of how different models for photo production affect the description of the development of photon-initiated cosmic ray showers and, consequently, how much the estimated photon composition of the showers depends from the models used in the simulation. In this way, we update a previous publication [1]. The simulation of the shower development is performed using the AIRES MC [2], linked to the hadronic models QGSJET-II-04 [3], QGSJET in the following, and EPOS-LHC 3.40 [4], EPOS in the following, that have recently been updated to take into account LHC results.…”
Section: Introductionmentioning
confidence: 99%
“…
We present post-LHC updates of estimates of the total photo-production cross section in a mini-jet model with infrared soft gluon resummation, and apply the model to study Cosmic Ray shower development, comparing the results with those obtained from other existing models.
KeywordsTotal photo-production cross section; mini-jet models; cosmic rays; shower development 1 The total photo production cross sectionWe address again the question of how different models for photo production affect the description of the development of photon-initiated cosmic ray showers and, consequently, how much the estimated photon composition of the showers depends from the models used in the simulation. In this way, we update a previous publication [1]. The simulation of the shower development is performed using the AIRES MC [2], linked to the hadronic models QGSJET-II-04 [3], QGSJET in the following, and EPOS-LHC 3.40 [4], EPOS in the following, that have recently been updated to take into account LHC results.
…”
mentioning
confidence: 99%