English

Importance of High pt Physics for simulating UHECR Air Showers

High Energy Astrophysical Phenomena 2012-06-11 v2

Abstract

Observational evidence from Auger and earlier experiments shows a deficit of signal in a surface detector compared to predictions, which increases as a function of zenith angle, when the energy of the event is fixed by fluorescence measurements. We explore three potential explanations for this: the "Cronin effect" (growth of high-transverse momentum cross sections with nuclear size), the need for more particles at high transverse momentum in p- p collisions than currently predicted by high energy hadronic models used for air shower simulations, and the possibility that secondary interactions in the target air nucleus produces additional soft pions not included in simulations. We report here on the differences between Pythia and QGSJet II, especially for high Pt particles. The possible impact of these effects on the predicted surface array signal and attenuation with zenith angle are also reported.

Keywords

Cite

@article{arxiv.1206.0625,
  title  = {Importance of High pt Physics for simulating UHECR Air Showers},
  author = {Jeff Allen and Glennys Farrar},
  journal= {arXiv preprint arXiv:1206.0625},
  year   = {2012}
}

Comments

3 pages, 6 figures. Proceedings of the 31st International Cosmic Ray Conference in Lodz, Poland, 2009