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Stochastic processes --- Electromagnetic theory --- Cosmic ray showers --- Processus stochastiques --- Théorie électromagnétique --- 519.218 --- #WWIS:STAT --- Auger showers --- Cosmic showers --- EAS (Cosmic rays) --- Extensive air showers --- Showers, Auger --- Showers, Cosmic --- Showers, Extensive air --- Cosmic rays --- Pair production --- Random processes --- Probabilities --- Light, Electromagnetic theory of --- Electric fields --- Magnetic fields --- Special stochastic processes --- Stochastic processes. --- Electromagnetic theory. --- Cosmic ray showers. --- 519.218 Special stochastic processes --- Théorie électromagnétique
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Extensive air showers are a very unique phenomenon. In the more than six decades since their discovery by Auger et al. we have learned a great deal about these extremely energetic events and gained deep insights into high-energy phenomena, particle physics and astrophysics. In this Tutorial, Reference Manual and Data Book Peter K. F. Grieder provides the reader with a comprehensive view of the phenomenology and facts of the various types of interactions and cascades, theoretical background, experimental methods, data evaluation and interpretation, and air shower simulation. He discusses astrophysical aspects of the primary radiation and addresses the questions that continue to puzzle researchers. The book is divided into two parts, each in its own separate volume: Part I in Volume I deals mainly with the basic theoretical framework of the processes that determine an air shower and ends with a summary of ways to extract information on the primary radiation from air shower observations. It also presents a compilation of data representing our current knowledge of the high-energy portion of the primary spectrum and composition. Part II in Volume II mainly contains compilations of experimental and theoretical data, as well as predictions from simulations of individual air shower constituents. Also included are chapters dedicated exclusively to special processes and detection methods: optical atmospheric Cherenkov and fluorescence phenomena that represent special observational windows and have proven to be successful alternatives to particle measurements, yielding three-dimensional insights into the shower process, as well as radio emission, which may develop into a useful future method of detection.
Cosmic rays. --- Physics --- Physical Sciences & Mathematics --- Nuclear Physics --- Light & Optics --- Cosmic ray showers. --- Astrophysics. --- Astronomical physics --- Auger showers --- Cosmic showers --- EAS (Cosmic rays) --- Extensive air showers --- Showers, Auger --- Showers, Cosmic --- Showers, Extensive air --- Physics. --- Space sciences. --- Nuclear physics. --- Particle and Nuclear Physics. --- Extraterrestrial Physics, Space Sciences. --- Astrophysics and Astroparticles. --- Astronomy --- Cosmic physics --- Cosmic rays --- Pair production --- Space Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics). --- Science and space --- Space research --- Cosmology --- Science --- Atomic nuclei --- Atoms, Nuclei of --- Nucleus of the atom
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This thesis offers the first laboratory validation of microscopic simulations of radio emission from particle showers, including a detailed description of the simulation study. It presents a potential future avenue for resolving the mass composition of cosmic rays via radio detection of air showers. Particle showers are created from cascading interactions when high-energy particles collide with matter, e.g. with air in the case of cosmic radiation, or with a particle detector in the case of experiments at CERN. These showers can consist of billions of particles, mostly electrons, positrons and photons. They emit radio waves when the absorbing medium is in a magnetic field, and this radio emission can be used as a novel means of detecting and drawing inferences on the shower and the primary particle. The new method is currently being established in cosmic ray research, where large antenna arrays may soon replace or complement traditional particle detectors. In thi s study, a complete microscopic simulation of a radio-emission experiment conducted at Stanford Linear Accelerator Center (SLAC), Stanford/USA, is performed, and the underlying physical models are validated. The model is subsequently applied to the Square Kilometre Array (SKA) project, which is a large interferometer for radio astronomy. It is demonstrated that the SKA, with some modifications, might also be used for cosmic ray research based on radio detection of high-energy particles from the cosmos.
Radio astronomy. --- Cosmic ray showers. --- Antenna arrays. --- Arrays, Antenna --- Auger showers --- Cosmic showers --- EAS (Cosmic rays) --- Extensive air showers --- Showers, Auger --- Showers, Cosmic --- Showers, Extensive air --- Radioastronomy --- Physics. --- Astrophysics. --- Physical measurements. --- Measurement. --- Astrophysics and Astroparticles. --- Numerical and Computational Physics, Simulation. --- Measurement Science and Instrumentation. --- Antennas (Electronics) --- Large space structures (Astronautics) --- Cosmic rays --- Pair production --- Astronomy --- Interstellar communication --- Measurement . --- Measuring --- Mensuration --- Mathematics --- Technology --- Metrology --- Physical measurements --- Measurements, Physical --- Mathematical physics --- Measurement --- Natural philosophy --- Philosophy, Natural --- Physical sciences --- Dynamics --- Astronomical physics --- Cosmic physics --- Physics
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