Very high energy proton-proton cross section
Creators
- 1. University of Lodz, Department of Physics (Poland)and Andrzej Soltan Institute for Nuclear Studies, Uniwersytecka 5, 90-950 Lodz (Poland)
Description
The recent Pierre Auger Observatory result suggesting a coincidence of extensive air showers arrival directions with 'nearby' active galactic nuclei and HiRes discovery of the Greisen-Zatsepin-Kuzmin cutoff indicates protons to be only or at least the strongly dominant component of primary extra galactic cosmic ray flux. However, showers initiated by these ultrahigh energy particles developed faster than predicted by the simulation calculations with conventional interaction models. This could be evidence of the substantial increase of the p-air cross section. The progress in understanding the proton-proton cross section description allows us to examine this possibility, and eventually reject it as an explanation of the ultrahigh energy cosmic ray 'pure proton' controversy.
Additional details
Identifiers
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 79
- Journal Issue
- 9
- Journal Page Range
- p. 094008-094008.8
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41052347
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- COSMIC RAY FLUX; CROSS SECTIONS; EXTENSIVE AIR SHOWERS; GALAXY NUCLEI; INTERACTIONS; PROTON-PROTON INTERACTIONS; SIMULATION
- Descriptors DEC
- BARYON-BARYON INTERACTIONS; COSMIC RADIATION; COSMIC SHOWERS; HADRON-HADRON INTERACTIONS; INTERACTIONS; IONIZING RADIATIONS; NUCLEON-NUCLEON INTERACTIONS; PARTICLE INTERACTIONS; PROTON-NUCLEON INTERACTIONS; RADIATION FLUX; RADIATIONS; SECONDARY COSMIC RADIATION; SHOWERS
Optional Information
- Notes
- (c) 2009 The American Physical Society