Astrophysical Sources of High Energy Particles and Radiation: NATO Science Series II: Mathematics, Physics and Chemistry, cartea 44
Editat de M.M. Shapiro, Todor Stanev, John P. Wefelen Limba Engleză Paperback – 31 dec 2001
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Specificații
ISBN-13: 9781402001741
ISBN-10: 1402001746
Pagini: 392
Ilustrații: XII, 380 p. 18 illus.
Dimensiuni: 160 x 240 x 21 mm
Greutate: 0.62 kg
Ediția:2001
Editura: SPRINGER NETHERLANDS
Colecția Springer
Seria NATO Science Series II: Mathematics, Physics and Chemistry
Locul publicării:Dordrecht, Netherlands
ISBN-10: 1402001746
Pagini: 392
Ilustrații: XII, 380 p. 18 illus.
Dimensiuni: 160 x 240 x 21 mm
Greutate: 0.62 kg
Ediția:2001
Editura: SPRINGER NETHERLANDS
Colecția Springer
Seria NATO Science Series II: Mathematics, Physics and Chemistry
Locul publicării:Dordrecht, Netherlands
Public țintă
ResearchCuprins
I. High Energy Processes.- Theory of Cosmic Ray and High-Energy Gamma-Ray Production in Supernova Remnants.- Hadronic Collisions at Very High Energies.- Electron Acceleration by Quasi-Parallel Shockwaves.- Magnetohydrodynamic Wind Driven by Cosmic Rays in a Rotating Galaxy.- II. Sources in Our Galaxy.- Supernovae, Superbubbles, Nonthermal Emission & Light Element Nucleosynthesis in the Galaxy.- Cosmic Ray Interactions in the Galactic Center Region.- Dark Matter Halo of Our Galaxy.- A New Model for the Thermal X-Ray Composites and the Proton Origin Y-Rays from Supernova Remnants.- Evolution of Isolated Neutron Stars.- High Energy Outburst of Recurrent Transient Pulsar A0535+26.- III. Extra-Galactic Sources and Cosmological Connections.- High Energy Particles in Active Galactic Nuclei.- Galactic Clues About the high-energy processesiIn BL LAC (AGN) Jets.- Nonthermal Phenomena in Clusters of Galaxies.- Correlation and Clustering: Statistical Properties of Galaxy Large Scale Structures.- The Sunyaev-Zeldovich Effect and Its Cosmological Significance.- IV. Cosmic Photons: X-Rays and ?-Rays.- An Overview on GEV-TEV Gamma Ray Astronomy: Past-Present-Future.- A Brief Introduction to the Study of Afterglows of Gamma Ray Bursts.- Searches for TEV ?-Ray Emission with the Hegra Cherenkov Telescopes.- Variables Gamma Ray Sources, 1: Interactions of Flare Energetic Particles with Solar and Stellar Winds.- Variable Gamma Ray Sources,2: Interactions of Galactic Cosmic Rays with Solar and Stellar Winds.- Comets as X-Ray Objects.- V. Cosmic Ray Particles.- Cosmic Ray Origin: General Overview.- Galactic Cosmic Ray Composition: From the Anomalous Component to the Knee.- Low Energy Cosmic Ray Nuclei and their Propagation in the Galaxy.- Reacceleration Of Galactic Cosmic Rays: SecondaryElectron Capture Isotopes Measured by the Cosmic Ray Isotope Spectrometer.- The Astrophysics of ULtra-Heavy Galactic Cosmic Rays (and how we can detect them).- EAS: N? — Ne Measurements with the EAS-TOP Array.- L3+Cosmics: An Atmospheric Muon Experiment at Cern.- VI. Future Prospects.- Nuclear Paleoastrophysics: Prospects and Perspectives.- H.E.S.S.—The High Energy Stereoscopic System.- Development of Atmospheric Cherenkov Detectors Atmilagro.- NEMO: Neutrino Mediterranean Observatory.- Participants.