Pair Production from 10 GeV to 10 ZeV
arXiv:hep-ex/0402028 · doi:10.1016/j.radphyschem.2005.09.005
Abstract
At very high energies, pair production () exhibits many interesting features. The momentum transfer from the target is very small, so the reaction probes the macroscopic properties of the target, rather than individual nuclei. Interference between interactions with different atoms reduces the pair production cross section considerably below the Bethe-Heitler values. At very high energies, photonuclear interactions may outnumber pair production. In contrast, in crystals, the interaction amplitudes may add coherently, greatly increasing the cross sections. Pair production in matter-free magnetic fields is also possible. The highest energy pair production occurs at high energy particle colliders. This article will compare pair production in these very different regimes.
37 pages with 9 figures. Invited Review for "Radiation Physics and Chemistry" Version for publication, incorporating comments by the referee, and by Gerhard Baur and Roman Lee
References in corpus (6)
- Big Bang Nucleosynthesis (in "The Review of Particle Properties" 2004)
- Production of Pairs Accompanied by Nuclear Dissociation in Ultra-Peripheral Heavy Ion Collision
- Concept of Formation Length in Radiation Theory
- High-energy expansion of Coulomb corrections to the e+e- photoproduction cross section
- Ultra-High Energy Quenching of the LPM Effect: Implications for GZK-Violating Events
- Ultra-Peripheral Collisions with STAR at RHIC
Cited by in corpus (21)
- STARlight: A Monte Carlo simulation program for ultra-peripheral collisions of relativistic ions
- Upper limit on the cosmic-ray photon flux above 10^19 eV using the surface detector of the Pierre Auger Observatory
- IceCube: An Instrument for Neutrino Astronomy
- The ALICE experiment: a journey through QCD
- Search for ultra-high energy photons using air showers
- Electron and Photon Interactions in the Regime of Strong LPM Suppression
- Coherent Cherenkov radio pulses from hadronic showers up to EeV energies
- Report on Progress in Physics: Observation of the Breit-Wheeler Process and Vacuum Birefringence in Heavy-Ion Collisions
- Starburst and post-starburst high-redshift protogalaxies: The feedback impact of high energy cosmic rays
- Interactions between Ultra-High-Energy Particles and Protogalactic Environments
- ARIANNA: A radio detector array for cosmic neutrinos on the Ross Ice Shelf
- Generation of Ultrarelativistic Vortex Leptons with Large Orbital Angular Momenta
- Coherent photoproduction in bulk matter at high energies
- A Re-evaluation of Evidence for Light Neutral Bosons in Nuclear Emulsions
- Experimental characterisation of a single-shot spectrometer for high-flux, GeV-scale gamma-ray beams
- EmCa -- Electromagnetic-Cascades Simulation Package
- Energetic particles and high-energy processes in cosmological filaments and their astronomical implications
- Particle Interactions in Matter at the Terascale: the Cosmic-Ray Experience
- Inter-Comparison and Validation of Geant4 Photon Interaction Models
- Ultra high-energy cosmic rays from beyond the Greisen-Zatsepin-Kuz'min horizon
- Ultra-peripheral collisions of charged hadrons in extensive air showers