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9789810245733

Very High Energy Cosmic Gamma Radiation : A Crucial Window on the Extreme Universe

by
  • ISBN13:

    9789810245733

  • ISBN10:

    9810245734

  • Format: Hardcover
  • Copyright: 2004-10-01
  • Publisher: World Scientific Pub Co Inc
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Summary

Gamma ray astronomy, the branch of high energy astrophysics that studies the sky in energetic A?gammaA"-ray photons, is destined to play a crucial role in the exploration of nonthermal phenomena in the Universe in their most extreme and violent forms.
This book presents the motivations and highlights the principal objectives of the field, as well as demonstrates its intrinsic links to other branches of high energy astrophysics. Preference is given to three topical areas: (i) origin of cosmic rays: (ii) physics and astrophysics of relativistic jets: (iii) observational gamma ray cosmology. Also, a significant part of the book is devoted to the discussion of the principal mechanisms of production and absorption of energetic A?gammaA"-rays in different astrophysical environments, as well as to the description of the detection methods of high energy cosmic A?gammaA"- radiation.

Table of Contents

Prefacep. v
Introductionp. 1
"The Last Electromagnetic Window"p. 1
Energy Domains of Gamma Ray Astronomyp. 4
Gamma Ray Astronomy: A Discipline in Its Own Rightp. 7
Status of the Fieldp. 23
Low Energy Gamma Ray Sourcesp. 24
The COMPTEL source catalogp. 25
High Energy Gamma Ray Sourcesp. 31
GeV blazarsp. 34
GeV pulsarsp. 36
Unidentified EGRET sourcesp. 39
The Status of Ground-Based Gamma Ray Astronomyp. 42
Brief historical reviewp. 42
Reported TeV sourcesp. 46
The Crab Nebulap. 47
Other plerionsp. 51
Gamma ray pulsarsp. 54
Gamma rays from supernova remnantsp. 54
Other galactic sourcesp. 63
TeV blazarsp. 67
Other extragalactic objectsp. 79
Next generation of IACT arraysp. 83
Atmospheric Cherenkov radiationp. 83
Stereoscopic detection of Cherenkov imagesp. 84
IACT arraysp. 87
Sub-10 GeV ground based detectors?p. 90
Large field-of-view detectorsp. 95
IACT arrays for probing PeV [gamma]-raysp. 96
Gamma Ray Production and Absorption Mechanismsp. 99
Interactions with Matterp. 100
Electron bremsstrahlung and pair-productionp. 101
Electron-positron annihilationp. 105
Gamma rays produced by relativistic protonsp. 106
[pi superscript 0]-decay gamma raysp. 106
Nuclear gamma ray line emissionp. 110
Interactions with Photon Fieldsp. 112
Inverse Compton scatteringp. 113
Photon-photon pair productionp. 117
Interactions of hadrons with radiation fieldsp. 121
Interactions with Magnetic Fieldsp. 123
Synchrotron radiation and pair-productionp. 123
Synchrotron radiation of protonsp. 126
Relativistic Electron-Photon Cascadesp. 130
Gamma Rays and Origin of Galactic Cosmic Raysp. 135
Origin of Galactic Cosmic Rays: General Remarksp. 135
What do we know about Cosmic Rays?p. 135
What we do not know about Cosmic Rays?p. 137
Common beliefs and "nasty" problemsp. 140
Searching for sites of production of GCRsp. 143
Giant Molecular Clouds as Tracers of Cosmic Rayp. 147
Proton fluxes in the ISM near the acceleratorp. 149
Impulsive sourcep. 149
Continuous sourcep. 151
The case of dense gas regionsp. 154
Gamma rays from a cloud near the acceleratorp. 155
Accelerator inside the cloudp. 159
On the level of the "sea" of galactic cosmic raysp. 161
Probing the Sources of VHE CR Electronsp. 165
Distributions of VHE electronsp. 166
Extended regions of IC gamma radiationp. 168
Diffuse Radiation from the Galactic Diskp. 173
CR spectra in the inner Galaxyp. 174
Diffuse radiation associated with cosmic ray electronsp. 177
IC gamma raysp. 177
Electron bremsstrahlungp. 181
Annihilation of CR positrons in flightp. 182
Gamma rays of nucleonic originp. 183
Overall gamma ray fluxesp. 185
Probing the diffuse [gamma]-ray background on small scalesp. 189
Concluding remarksp. 195
Gamma Ray Visibility of Supernova Remnantsp. 199
Gamma Rays as a Diagnostic Toolp. 199
Inverse Compton Versus [pi superscript 0]-Decay Gamma Raysp. 205
Synchrotron X-ray Emission of SNRsp. 208
TeV Gamma Radiation of SN 1006 and Similar SNRsp. 209
Inverse Compton models of TeV emissionp. 209
Hadronic origin of TeV emission?p. 215
Distinct features of electronic and hadronic modelsp. 217
Concluding remarksp. 219
Molecular Clouds Overtaken by SNRsp. 220
Bremsstrahlung X-rays from [gamma] Cygnip. 223
The case of RX J1713.7-3946p. 225
A Special Case: Gamma Rays from Cassiopeia Ap. 231
"PeV SNRs"p. 238
Pulsars, Pulsar Winds, Plerionsp. 243
Magnetospheric Gamma Raysp. 244
Polar cap versus outer gap modelsp. 247
Magnetospheric TeV gamma rays?p. 251
Gamma Rays from Unshocked Pulsar Windsp. 253
Characteristics of the KED windp. 254
The ejection rate and the particle spectrump. 255
IC Radiation of the pulsar wind in Crabp. 256
Gamma rays from winds of PSR B1706-44 and Vela?p. 261
IC [gamma]-rays from the binary pulsar PSR B1259-63p. 265
Gamma Rays from Pulsar Driven Nebulaep. 268
Broad-band nonthermal radiation of the Crab Nebulap. 268
Synchrotron and IC radiationp. 270
Second High Energy Synchrotron Componentp. 273
Bremsstrahlung and [pi superscript 0]-decay gamma rays?p. 275
The objectives of future gamma ray studiesp. 278
High Energy Gamma Rays from Other Plerionsp. 281
Time-evolution of electronsp. 283
Target photon fieldsp. 284
Effects of B-field, electron energy, and pulsar agep. 286
Synchrotron and IC nebulae around PSR B1706-44p. 289
Gamma Rays Expected from Microquasarsp. 293
Do We Expect Gamma Rays from X-Ray Binaries?p. 293
Nonthermal Phenomena in Microquasarsp. 295
Modelling of Radio Flares of GRS 1915+105p. 301
Expected Gamma Ray Fluxesp. 304
Searching for Gamma Ray Signals from Microquasarsp. 309
The Case of Microblazarsp. 311
Ultraluminous Sources as Microblazars?p. 313
Persistent Gamma Ray Emission from Extended Lobesp. 317
Large Scale Jets of Radio Galaxies and Quasarsp. 321
Synchrotron and IC Models of Large Scale AGN Jetsp. 323
Ultra High Energy Protons in Jetsp. 327
Secondary electronsp. 327
Synchrotron radiation of protonsp. 330
Pictor A, PKS 0637-752, and 3C 120p. 332
The case of 3C 273p. 339
Large Scale Jets Powered by Gamma Raysp. 347
Concluding Remarksp. 354
Nonthermal Phenomena in Clusters of Galaxiesp. 359
Nonthermal Particles and Magnetic Fieldsp. 359
Inverse Compton and Bremsstrahlung Modelsp. 364
Inverse Compton modelsp. 364
Nonrelativistic bremsstrahlungp. 368
Synchrotron X- and [gamma]-rays of "Photonic" Origin?p. 369
Nonthermal Radiation Components Associated with Very High and Extremely High Energy Protonsp. 378
High energy radiation from cores of clustersp. 379
Detectability of gamma raysp. 384
Detectability of X-raysp. 386
Nonthermal radiation beyond the cluster coresp. 388
Weak magnetic fieldp. 389
Intermediate magnetic fieldp. 390
Strong magnetic fieldp. 390
TeV Blazars and Cosmic Background Radiationp. 393
Cosmic Infrared Background Radiationp. 394
Intergalactic Absorption of Gamma Raysp. 397
TeV Blazarsp. 399
Leptonic Models of TeV Blazarsp. 402
Constraints on the SSC parameter spacep. 404
Time-dependent SSC treatmentp. 409
The case of 1ES 1426+428p. 415
Hadronic Modelsp. 417
Mass-loaded hadronic jet modelsp. 418
Photo-pion and synchrotron losses of protonsp. 419
Proton synchrotron modelsp. 422
Fitting the TeV spectrum of Mkn 501p. 423
X-rays from secondary electronsp. 425
Broad band SED of 1ES 1426+428 within the proton-synchrotron modelp. 427
"IR background-TeV Gamma Ray Crisis"?p. 432
High Energy Gamma Rays--Carriers of Unique Cosmological Informationp. 437
Probing DEBRA Through [gamma]-Ray Absorption Featuresp. 437
The Effect of Cascading in the CIBp. 447
Pair Halos as Unique Cosmological Candlesp. 450
Diffuse Extragalactic Background as Calorimetric Measure of the VHE Emissivity of the Universep. 460
Spherically symmetric diffusion from a single sourcep. 463
Evolution of relativistic electrons in an expanding magnetised mediump. 465
Kinetic equationp. 465
Time-independent energy lossesp. 467
Expanding cloudp. 470
Bibliographyp. 473
Indexp. 493
Table of Contents provided by Rittenhouse. All Rights Reserved.

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