Particles and astrophysics: a multi-messenger approach
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| Main Author: | |
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| Format: | Book |
| Language: | English |
| Published: |
Cham [u.a.]
Springer
2015
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| Series: | Astronomy and astrophysics library
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| Subjects: | |
| Online Access: | Inhaltsverzeichnis |
| Item Description: | Literaturangaben |
| Physical Description: | XVI, 491 S. Ill., graph. Darst. |
| ISBN: | 9783319080505 |
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Record in the Search Index
| _version_ | 1804152719349383168 |
|---|---|
| adam_text | Titel: Particles and Astrophysics
Autor: Spurio, Maurizio
Jahr: 2015
Contents
1 An Overview of Astroparticle Physics..........................................1
1.1 Introduction........................................................................1
1.1.1 Astrophysics and Astroparticle Physics......................3
1.1.2 Discoveries and Experiments Not Covered in
This Book..............................................................6
1.2 Cosmic Rays......................................................................7
1.3 Gamma-Rays of GeV and TeV Energies................................10
1.4 Neutrino Astrophysics..........................................................11
1.5 The Dark Universe..............................................................15
1.6 Laboratories and Detectors for Astroparticle Physics................16
1.6.1 Space Experiments..................................................16
1.6.2 Experiments in the Atmosphere................................17
1.6.3 Ground-Based Experiments ...................................18
1.7 Underground Laboratories for Rare Events..............................18
References....................................................................................21
2 The Cosmic Rays and Our Galaxy..............................................23
2.1 The Discovery of Cosmic Rays............................................23
2.2 Cosmic Rays and the Early Days of Particle Physics....... . 26
2.3 The Discovery of the Positron and Particle Detectors..............27
2.3.1 The Motion in a Magnetic Field
and the Particle Rigidity..........................................27
2.3.2 The Identification of the Positron..............................29
2.4 A Toy Telescope for Primary Cosmic Rays............................32
2.5 Differential and Integral Flux................................................34
2.6 The Energy Spectrum of Primary Cosmic Rays......................37
2.7 The Physical Properties of the Galaxy....................................40
2.7.1 The Galactic Magnetic Field....................................42
2.7.2 The Interstellar Matter Distribution............................44
2.8 Low-Energy Cosmic Rays from the Sun................................45
2.9 The Effect of the Geomagnetic Field......................................47
2.10 Number and Energy Density of the Cosmic Rays.......... 50
2.11 Energy Considerations on Cosmic Ray Sources......................52
References....................................................................................53
3 Direct Cosmic Rays Detection: Protons, Nuclei, Electrons
and Antimatter............................................................................55
3.1 Generalities on Direct Measurements......................................56
3.2 The Calorimetric Technique..................................................57
3.2.1 Hadronic Interaction Length and Mean Free Path .... 58
3.2.2 The Electromagnetic Radiation Length......................59
3.2.3 Hadronic Interaction Length and Mean Free Path
in the Atmosphere....................................................60
3.3 Balloon Experiments............................................................61
3.4 Satellite Experiments............................................................64
3.4.1 The IMP Experiments..............................................64
3.4.2 The PAMELA Experiment........................................66
3.5 The AMS-02 Experiment on the International Space Station. .. 67
3.6 Abundances of Elements in the Solar System and in CRs .... 70
3.6.1 Cosmic Abundances of Elements..............................73
3.7 Energy Spectrum of CR Protons and Nuclei............................76
3.8 Antimatter in Our Galaxy....................................................78
3.9 Electrons and Positrons........................................................80
3.9.1 The Positron Component..........................................82
3.9.2 Considerations on the e+,e~ Components..................84
References....................................................................................85
4 Indirect Cosmic Rays Detection: Particle Showers
in the Atmosphere . . .................................................................87
4.1 Introduction and Historical Information..................................88
4.2 The Structure of the Atmosphere..........................................89
4.3 The Electromagnetic (EM) Cascade........................................92
4.3.1 Heitler s Model of EM Showers................................93
4.3.2 Analytic Solutions....................................................95
4.4 Showers Initiated by Protons and Nuclei................................99
4.4.1 The Muon Component in a Proton-Initiated
Cascade..................................................................102
4.4.2 The EM Component in a Proton-Initiated Cascade ... 103
4.4.3 Depth of the Shower Maximum for a Proton
Shower..................................................................106
4.4.4 Showers Induced by Nuclei: The Superposition
Model ..................................................................107
4.5 The Monte Carlo Simulations of Showers..............................110
4.6 Detectors of Extensive Air Showers at the Energy
of the Knee........................................................................112
4.6.1 A Toy Example of an EAS Array..............................113
4.6.2 Some EAS Experiments............................................116
4.6.3 Cherenkov Light Produced by EAS Showers..............118
4.7 The Time Profile of Cascades...................................120
4.8 The Arrival Direction of CRs as Measured
with EAS Arrays................................................................121
4.9 The CR Flux Measured with EAS Arrays..............................124
4.10 Mass Composition of CRs Around the Knee..........................126
4.10.1 The Ne Versus Nß Method........................................127
4.10.2 Depth of the Shower Maximum . .............................128
References....................................................................................130
5 Diffusion of Cosmic Rays in the Galaxy........................................133
5.1 The Overabundance of Li, Be, and B in CRs..........................134
5.1.1 Production of Li, Be, and B During Propagation..........135
5.2 Dating of Cosmic Rays with Radioactive Nuclei......................139
5.2.1 Unstable Secondary-to-Primary Ratios........................141
5.3 The Diffusion-Loss Equation................................................142
5.3.1 The Diffusion Equation with Nuclear Spallation..........145
5.3.2 Numerical Estimate of the Diffusion Coefficient D . . . 146
5.4 The Leaky box Model and its Evolutions................................147
5.5 Energy-Dependence of the Escape Time xesc..........................149
5.6 Energy Spectrum of Cosmic Rays at the Sources....................151
5.7 Anisotropics due to the Diffusion..........................................152
5.7.1 The Compton-Getting Effect....................................155
5.8 The Electron Energy Spectrum at the Sources........................155
5.8.1 Synchrotron Radiation..............................................156
5.8.2 Measured Energy Spectrum of Electrons....................160
5.8.3 Average Distance of Accelerators of Electrons............161
References....................................................................................162
6 Acceleration Mechanisms and Galactic Cosmic Ray Sources..........165
6.1 Second-and First-Order Fermi Acceleration Mechanisms..........166
6.1.1 Magnetic Mirrors....................................................167
6.1.2 The Second-Order Fermi Acceleration Mechanism ... 169
6.1.3 The First-Order Fermi Acceleration Mechanism..........171
6.1.4 The Power-Law Energy Spectrum from the Fermi
Model ..................................................................174
6.2 Diffusive Shock Acceleration in Strong Shock Waves..............174
6.2.1 Supernova Explosions and Cosmic Rays
Acceleration ..........................................................176
6.2.2 Relevant Quantities in a Supernova Explosion............177
6.3 Maximum Energy Attainable in the Supernova Model ............180
6.4 The Spectral Index of the Energy Spectrum ..........................182
6.4.1 The Escape Probability...................................184
6.4.2 A Shock Front in a Mono-Atomic Gas . . .................185
6.5 Success and Limits of the Standard Model of Cosmic
Ray Acceleration................................188
6.6 White Dwarfs and Neutron Stars............................................190
6.6.1 White Dwarfs..........................................................191
6.6.2 Neutron Stars and Pulsars........................................193
6.7 Possible Galactic Sources of Cosmic Rays Above
the Knee.....................................................................197
6.7.1 A Simple Model Involving Pulsars............................198
6.7.2 A Simple Model Involving Binary Systems................199
References......................................................200
7 Ultra High Energy Cosmic Rays..................................................203
7.1 The Observational Cosmology and the Universe......................204
7.2 The Large-Scale Structure of the Universe..............................206
7.3 Anisotropy of UHECRs: The Extragalactic Magnetic Fields. . . 208
7.4 The Quest for Extragalactic Sources of UHECRs....................210
7.5 Propagation of UHECRs......................................................215
7.5.1 The Adiabatic Energy Loss......................................215
7.5.2 The Propagation in the CMB: The GZK Cut-Off .... 215
7.5.3 Pair Production by Protons on the CMB................218
7.5.4 Propagation in the Extragalactic Magnetic Field..........219
7.6 The Fluorescence Light and Fluorescence Detectors................220
7.7 UHECR Measurements with a Single Technique......................225
7.7.1 Results from HiRes and AGASA..............................226
7.8 Large Hybrid Observatories of UHECRs................................228
7.9 The Flux of UHECRs..........................................................233
7.10 The Chemical Composition of UHECRs................................234
7.11 Correlation of UHECRs with Astrophysical Objects................236
7.12 Constraints on Top-Down Models..........................................238
7.13 Summary and Discussion of the Results................................239
References....................................................................................241
8 The Sky Seen in y-rays................................................................243
8.1 The Spectral Energy Distribution (SED)
and Multiwavelength Observations........................................244
8.2 Astrophysical y-rays: The Hadronic Model............................246
8.2.1 Energy Spectrum of y-rays from n° Decay................247
8.3 Galactic Sources and y-rays..................................................249
8.3.1 A Simple Estimate of the y-ray Flux
from a Galactic Source......................................250
8.4 Astrophysical y-rays: The Leptonic Model................................251
8.4.1 The Synchrotron Radiation from a Power-Law
Spectrum................................................................252
8.4.2 Synchrotron Self-Absorption....................................254
8.4.3 Inverse Compton Scattering and SSC........................255
8.5 The Compton Gamma Ray Observatory Legacy......................259
8.5.1 The EGRET y-ray Sky............................................259
8.6 Fermi-LAT and Other Experiments for y-ray Astronom}..........262
8.6.1 The Fermi-LAT....................................................262
8.6.2 AGILE and Swift..................................................264
8.7 Diffuse y-rays in the Galactic Plane......................................264
8.7.1 An Estimate of the Diffuse y-ray Flux........................267
8.8 The Fermi-LAT Catalogs..........................................268
8.9 Gamma Ray Bursts..............................................................273
8.9.1 Classification of GRBs............................................276
8.10 Limits of y-ray Observations from Space................................279
References....................................................................................280
9 The TeV Sky and Multiwavelength Astrophysics..........................281
9.1 The Imaging Cherenkov Technique........................................282
9.1.1 Gamma-Ray Versus Charged CR Discrimination .... 284
9.1.2 HESS, VERITAS and MAGIC..................................285
9.2 EAS Arrays for y-astronomy................................................288
9.2.1 Sensitivity of y-ray Experiments................................289
9.3 TeV Astronomy: The Catalog..............................................290
9.4 Gamma-Rays from Pulsars ..................................................293
9.5 The CRAB Pulsar and Nebula...................... . 294
9.6 The Problem of the Identification of Galactic CR Sources .... 296
9.7 Extended Supernova Remnants..............................................297
9.7.1 The SED of Some Peculiar SNRs..............................299
9.8 Summary of the Study of Galactic Accelerators......................303
9.9 Active Galaxies..................................................................304
9.10 The Extragalactic y-ray Sky..................................................307
9.11 The Spectral Energy Distributions of Blazars..........................308
9.11.1 Quasi-Simultaneous SEDs of Fermi-LAT Blazars .... 309
9.11.2 Simultaneous SED Campaigns and Mrk 421..............311
9.12 Jets in Astrophysics............................................................313
9.12.1 Time Variability in Jets............................................314
9.13 The Extragalactic Background Light......................................315
References....................................................................................319
10 High-Energy Neutrino Astrophysics..............................................321
10.1 The CRs, y-rays and Neutrino Connection..............................322
10.1.1 Neutrino Detection Principle....................................323
10.2 Background in Large Volume Neutrino Detectors....................325
10.3 Neutrino Detectors and Neutrino Telescopes..............
10 3 1 Muon Neutrino Detection........................................328
Tin
10.3.2 Showering Events..........................
10.4 Cosmic Neutrino Flux Estimates...............................331
10.4.1 A Reference Neutrino Flux from a Galactic Source. . . 331
10.4.2 Extragalactic Diffuse Neutrino Flux..........................333
10.4.3 Neutrinos from GRBs..............................................335
10.4.4 Cosmogenic Neutrinos..............................................338
10.5 Why km3-Scale Telescopes..................................................338
10.5.1 The Neutrino Effective Area of Real Detectors............341
10.5.2 Number of Optical Sensors in a Neutrino
Telescope..............................................................342
10.6 Water and Ice Properties......................................................343
10.7 Operating Neutrino Telescopes..............................................345
10.7.1 A Telescope in the Antarctic Ice................................345
10.7.2 A Telescope in the Mediterranean Sea........................347
10.8 Results from Neutrino Telescopes..........................................349
10.8.1 Point-Like Sources..................................................349
10.8.2 Limits from GRBs and Unresolved Sources................352
10.9 The First Measurement of Cosmic Neutrinos..........................353
References....................................................................................357
11 Atmospheric Muons and Neutrinos..............................................359
11.1 Nucléons in the Atmosphere..................................................360
11.2 Secondary Mesons in the Atmosphere....................................363
11.3 Muons and Neutrinos from Charged Meson Decays................367
11.3.1 The Conventional Atmospheric Neutrino Flux............369
11.3.2 The Prompt Component in the Muon
and Neutrino Flux....................................................369
11.4 The Particle Flux at Sea Level..............................................370
11.5 Measurements of Muons at Sea Level....................................373
11.6 Underground Muons ..........................................................374
11.6.1 The Depth-Intensity Relation....................................375
11.6.2 Characteristics of Underground/Underwater Muons .. . 375
11.7 Atmospheric Neutrinos........................................................377
11.7.1 Early Experiments....................................................379
11.8 Oscillations of Atmospheric Neutrinos....................................381
11.9 Measurement of Atmospheric vß Oscillations
in Underground Experiments................................................382
11.9.1 Event Topologies in Super-Kamiokande....................382
11.9.2 The Iron Calorimeter Soudan 2 Experiment................387
11.9.3 Upward-Going Muons and MACRO..........................388
11.10 Atmospheric vµ Oscillations and Accelerator
Confirmations ....................................................................391
11.11 Atmospheric Neutrino Flux at Higher Energies........................393
References....................................................................................394
12 Connections Between Physics and Astrophysics of Neutrinos .... 397
12.1 Stellar Evolution of Solar Mass Stars....................................398
12.2 The Standard Solar Model and Neutrinos................................400
12.3 Solar Neutrino Detection......................................................405
12.4 The SNO Measurement of the Total Neutrino Flux..................409
12.5 Oscillations and Solar Neutrinos............................................412
12.6 Oscillations Among Three Neutrino Families..........................414
12.6.1 Three Flavor Oscillation and KamLAND ..................416
12.6.2 Measurements of O13...................................417
12.7 Matter Effect and Experimental Results..................................418
12.8 Summary of Experimental Results and Consequences
for Neutrino Astrophysics....................................................421
12.8.1 Effects of Neutrino Mixing on Cosmic Neutrinos . . . 422
12.9 Formation of Heavy Elements in Massive Stars......................424
12.10 Stellae Novae......................................................................425
12.11 Core-Collapse Supernovae (Type II)......................................426
12.11.1 GRB Supernovae....................................................431
12.12 Neutrino Signal from a Core-Collapse SN..............................431
12.12.1 Supernova Rate and Location....................................431
12.12.2 The Neutrino Signal................................................432
12.12.3 Detection of Supernova Neutrinos..............................433
12.13 The SN 1987A....................................................................436
12.14 Stellar Nucleosynthesis of Trans-Fe Elements ........................437
References....................................................................................438
13 Microcosm and Macrocosm..........................................................441
13.1 The Standard Model of the Microcosm: The Big Bang............442
13.2 The Standard Model of Particle Physics and Beyond................445
13.3 Gravitational Evidence of Dark Matter....................................446
13.4 Dark Matter........................................................................448
13.5 Supersymmetry....................................................................450
13.5.1 Minimal Standard Supersymmetrie Model..................451
13.5.2 Cosmological Constraints and WIMP........................452
13.6 Interactions of WIMPs with Ordinary Matter..........................454
13.6.1 WIMPs Annihilation................................................455
13.6.2 WIMPs Elastic Scattering........................................456
13.7 Direct Detection of Dark Matter: Event Rates..........................458
13.8 WIMPs Direct Detection......................................................461
13.8.1 Solid-State Cryogenic Detectors................................462
13.8.2 Scintillating Crystals................................................463
13.8.3 Noble Liquid Detectors............................................464
13.8.4 Present Experimental Results and the Future..............465
13.9 Indirect WIMPs Detection....................................................467
13.9.1 Neutrinos from WIMP Annihilation
in Massive Objects..................................................467
13.9.2 Gamma-Rays from WIMPs......................................470
13.9.3 The Positron Excess: A WIMP Signature?..................471
13.10 What s Next?......................................................................473
References....................................................................................475
Index................................................................................................477
|
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| id | DE-604.BV042201879 |
| illustrated | Illustrated |
| indexdate | 2024-07-10T01:15:11Z |
| institution | BVB |
| isbn | 9783319080505 |
| language | English |
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| physical | XVI, 491 S. Ill., graph. Darst. |
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| record_format | marc |
| series2 | Astronomy and astrophysics library |
| spelling | Spurio, Maurizio 1962- Verfasser (DE-588)1019317434 aut Particles and astrophysics a multi-messenger approach Maurizio Spurio Cham [u.a.] Springer 2015 XVI, 491 S. Ill., graph. Darst. txt rdacontent n rdamedia nc rdacarrier Astronomy and astrophysics library Literaturangaben Physics Particle acceleration Elementarteilchenphysik (DE-588)4014414-8 gnd rswk-swf Astrophysik (DE-588)4003326-0 gnd rswk-swf Astrophysik (DE-588)4003326-0 s Elementarteilchenphysik (DE-588)4014414-8 s DE-604 Erscheint auch als Online-Ausgabe 978-3-319-08051-2 HBZ Datenaustausch application/pdf http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=027640750&sequence=000002&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA Inhaltsverzeichnis |
| spellingShingle | Spurio, Maurizio 1962- Particles and astrophysics a multi-messenger approach Physics Particle acceleration Elementarteilchenphysik (DE-588)4014414-8 gnd Astrophysik (DE-588)4003326-0 gnd |
| subject_GND | (DE-588)4014414-8 (DE-588)4003326-0 |
| title | Particles and astrophysics a multi-messenger approach |
| title_auth | Particles and astrophysics a multi-messenger approach |
| title_exact_search | Particles and astrophysics a multi-messenger approach |
| title_full | Particles and astrophysics a multi-messenger approach Maurizio Spurio |
| title_fullStr | Particles and astrophysics a multi-messenger approach Maurizio Spurio |
| title_full_unstemmed | Particles and astrophysics a multi-messenger approach Maurizio Spurio |
| title_short | Particles and astrophysics |
| title_sort | particles and astrophysics a multi messenger approach |
| title_sub | a multi-messenger approach |
| topic | Physics Particle acceleration Elementarteilchenphysik (DE-588)4014414-8 gnd Astrophysik (DE-588)4003326-0 gnd |
| topic_facet | Physics Particle acceleration Elementarteilchenphysik Astrophysik |
| url | http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=027640750&sequence=000002&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA |
| work_keys_str_mv | AT spuriomaurizio particlesandastrophysicsamultimessengerapproach |