Description
In the last two decades, cosmology, particle physics, high energy astrophysics and gravitational physics have become increasingly interwoven. The intense activity taking place at the intersection of these disciplines is constantly progressing, with the advent of major cosmic ray, neutrino, gamma ray and gravitational wave observatories for studying cosmic sources, along with the construction of particle physics experiments using beams and signals of cosmic origin. This book provides an up-to-date overview of the recent advances and potential future developments in this area, discussing both the main theoretical ideas and experimental results. It conveys the challenges but also the excitement associated with this field. Written in a concise yet accessible style, explaining technical details with examples drawn from everyday life, it will be suitable for undergraduate and graduate students, as well as other readers interested in the subject. Colour versions of a selection of the figures are available at www.cambridge.org/9780521517003.
Chapter
2 The nuts and bolts of the Universe
2.1 The building blocks: elementary particles
2.1.2 Anti-matter, neutrinos and the particle explosion
2.1.3 Elementary, dear Watson
2.2 The forces: three easy pieces and a harder one
2.2.1 The electromagnetic force
2.2.4 The gravitational force
2.3 Beyond the Standard Model
3.1 The dynamics of the Universe
3.2 The primordial fireball: a particle cauldron
3.3 Into the unknown: the GUT and Planck eras
3.4 Inflation, dark energy and dark matter
4 Cosmic structure formation
4.1 The perturbed Universe
4.2 Large scale structure formation
4.3 Stars: the Universe’s worker bees
4.4 Stellar and galactic concentrates
4.5 Black hole characteristics
4.6 Black hole astrophysics
5.1 What makes a galaxy “active”?
5.2 MBH masses, masers and distances
5.3 An AGN garden, classified
6.1 Stellar high energy sources
6.2 White dwarfs and thermonuclear supernovae
6.2.1 White dwarf formation
6.2.2 White dwarf high energy sources
6.3 Core collapse supernovae
6.3.1 Core collapse and neutron stars
6.3.2 Core collapse and black holes
6.3.3 Diffuse supernova remnants
6.4 Neutron stars and pulsars
6.5 Accreting X-ray binaries
6.9 Micro-quasars: neutron stars or black holes?
7.1 What are gamma-ray bursts?
7.2 Phenomenology of gamma-ray bursts
7.3 The GRB prompt radiation
7.4.1 Long gamma-ray bursts
7.4.2 Long gamma-ray bursts and supernovae
7.4.3 Short gamma-ray bursts
7.6 Cosmological uses of GRBs
7.7 Very high energy gamma-rays
7.8 Non-photonic emission
7.9 Wider impact of GRB multi-channel studies
8.1 Importance of the GeV–TeV range
8.2 Galactic Gev–TeV sources
8.3 Extragalactic sources
8.4 Detectability of GeV–TeV sources
8.5 GeV and TeV detection techniques
9.1 Ripples in space-time
9.2 Astrophysical sources of gravitational waves
9.3 Stellar binary GW sources
9.4 Galaxies as gravitational wave sources
9.5 Gravitational wave detectors
10.1 Particles from Heaven
10.2 Ultra-high energy cosmic rays
10.3 Cosmic-ray observational techniques
11.1 The elusive neutrinos
11.2 Stellar and supernova neutrinos
11.3 Atmospheric neutrinos
11.4 VHE astrophysical neutrinos
11.5 Cosmogenic neutrinos
12 Dark dreams, Higgs and beyond
12.2 Indirect astrophysical WIMP searches
12.3 Direct WIMP searches
12.6 Beyond the Standard Model at the LHC
12.7 Underground astrophysics and particle physics