High Energy Astrophysics : An Introduction
High-energy astrophysics has unveiled a Universe very different from that only known from optical observations. It has revealed many types of objects in which typical variability timescales are as short as years, months, days, and hours (in quasars, X-ray binaries, and other objects), and even down...
שמור ב:
| מחבר ראשי: | |
|---|---|
| פורמט: | Livre numérique |
| שפה: | Anglais |
| יצא לאור: |
Berlin, Heidelberg :
Springer Berlin Heidelberg
[20..].
Cham : Springer Nature |
| מהדורה: | 1st ed. 2013. |
| סדרה: | Astronomy and Astrophysics Library
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| נושאים: | |
| גישה מקוונת: | Accès sur la plateforme de l'éditeur Accès sur la plateforme Istex Accès Université d'Orléans Accès INSA CVL |
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Archives Springer e-books (Licence nationale) Archives Springer e-books (Licence nationale) |
| Autres localisations: | Voir dans le Sudoc |
| Edition sous un autre format: | • High Energy Astrophysics, Texte imprimé, 9783642309717 • High Energy Astrophysics, Texte imprimé, 9783642436840 • High energy astrophysics, an introduction, Thierry J.-L. Courvoisier, 2013, Heidelberg, Springer, 1 vol. (XV-332 p.), Astronomy and astrophysics library, 978-3-642-30969-4 |
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| 100 | 1 | |a Courvoisier, Thierry J.-L., |d 1953- | |
| 245 | 1 | 0 | |a High Energy Astrophysics : |b An Introduction |c by Thierry J.-L. Courvoisier. |
| 250 | |a 1st ed. 2013. | ||
| 260 | |a Berlin, Heidelberg : |b Springer Berlin Heidelberg. | ||
| 260 | |a Cham : |b Springer Nature, |c [20..]. | ||
| 490 | 0 | |a Astronomy and Astrophysics Library |x 2196-9698 | |
| 500 | |a Archives Springer e-books (Licence nationale) | ||
| 500 | |a Archives Springer e-books (Licence nationale) | ||
| 505 | 1 | |a Part I Physical Processes 1 The framework 2 Radiation of an accelerated charge 3 Bremsstrahlung 4 Cyclotron line emission 5 Synchrotron emission 6 Compton processes 7 Comptonisation 8 Pair Processes 9 Particle acceleration 10 Accretion 11 Radiation inefficient accretion flows Part II Astrophysical Objects 12 Black holes and accretion efficiency 13 Neutron Stars 14 Pulsars 15 The Hulse Taylor pulsar and gravitational radiation 16 X-ray binaries 17 X-ray binaries evolution 18 Relativistic jets 19 Gamma ray bursts 20 Active galactic nuclei 21 The diffuse X-ray background and other cosmic backgrounds.- Index | |
| 506 | |a Accès en ligne pour les établissements français bénéficiaires des licences nationales | ||
| 506 | |a Accès soumis à abonnement pour tout autre établissement | ||
| 506 | |a Conditions particulières de réutilisation pour les bénéficiaires des licences nationales. https://www.licencesnationales.fr/springer-nature-ebooks-contrat-licence-ln-2017 | ||
| 520 | |a High-energy astrophysics has unveiled a Universe very different from that only known from optical observations. It has revealed many types of objects in which typical variability timescales are as short as years, months, days, and hours (in quasars, X-ray binaries, and other objects), and even down to milli-seconds in gamma ray bursts. The sources of energy that are encountered are only very seldom nuclear fusion, and most of the time gravitation, a paradox when one thinks that gravitation is, by many orders of magnitude, the weakest of the fundamental interactions. The understanding of these objects' physical conditions and the processes revealed by high-energy astrophysics in the last decades is nowadays part of astrophysicists' culture, even of those active in other domains of astronomy.This book evolved from lectures given to master and PhD students at the University of Geneva since the early 1990s. It aims at providing astronomers and physicists intending to be active in high-energy astrophysics a broad basis on which they should be able to build the more specific knowledge they will need. While in the first part of the book the physical processes are described and derived in detail, the second part studies astrophysical objects in which high-energy astrophysics plays a crucial role. This two-pronged approach will help students recognise physical processes by their observational signatures in contexts that may differ widely from those presented here | ||
| 650 | |a Astrophysique nucléaire | ||
| 650 | |a Particules (physique) | ||
| 650 | |a Physique des hautes énergies | ||
| 776 | 0 | |t High Energy Astrophysics |b Texte imprimé |z 9783642309717 | |
| 776 | 0 | |t High Energy Astrophysics |b Texte imprimé |z 9783642436840 | |
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