
Particle Astrophysics.
Title:
Particle Astrophysics.
Author:
Perkins, D.H.
ISBN:
9780191562808
Personal Author:
Edition:
2nd ed.
Physical Description:
1 online resource (356 pages)
Series:
Oxford Master Series in Physics ; v.No. 10
Oxford Master Series in Physics
Contents:
Contents -- Part 1 Particles and Interactions -- 1 Quarks and leptons and their interactions -- 1.1 Preamble -- 1.2 Quarks and leptons -- 1.3 Fermions and bosons: the spin-statistics theorem -- supersymmetry -- 1.4 Antiparticles -- 1.5 The fundamental interactions: boson exchange -- 1.6 The boson couplings to fermions -- 1.7 The quark-gluon plasma -- 1.8 The interaction cross section -- 1.9 Examples of elementary particle cross sections -- 1.10 Decays and resonances -- 1.11 Examples of resonances -- 1.12 New particles -- 1.13 Summary -- Problems -- 2 Relativistic transformations and the equivalence principle -- 2.1 Coordinate transformations in special relativity -- 2.2 Invariant intervals and four-vectors -- 2.3 The equivalence principle: clocks in gravitational fields -- 2.4 General relativity -- 2.5 The Schwarzschild line element, Schwarzschild radius, and black holes -- 2.6 The gravitational deflection of light by a point mass -- 2.7 Shapiro time delay -- 2.8 Orbital precession -- 2.9 The Robertson-Walker line element -- 2.10 Modifications to Newtonian gravity? -- 2.11 Relativistic kinematics: four-momentum -- the Doppler effect -- 2.12 Fixed-target and colliding-beam accelerators -- Problems -- 3 Conservation rules, symmetries, and the Standard Model of particle physics -- 3.1 Transformations and the Euler-Lagrange equation -- 3.2 Rotations -- 3.3 The parity operation -- 3.4 Parity conservation and intrinsic parity -- 3.5 Parity violation in weak interactions -- 3.6 Helicity and helicity conservation -- 3.7 Charge conjugation invariance -- 3.8 Gauge transformations and gauge invariance -- 3.9 Superstrings -- 3.10 Gauge invariance in the electroweak theory -- 3.11 The Higgs mechanism of spontaneous symmetry breaking -- 3.12 Running couplings -- 3.13 Vacuum structure in gauge theories -- 3.14 CPT theorem and CP and T symmetry.
3.15 CP violation in neutral kaon decay -- 3.16 CP violation in the Standard Model: the CKM matrix -- 3.17 Summary -- Problems -- 4 Extensions of the Standard Model -- 4.1 Neutrinoless double beta decay -- 4.2 Neutrino masses and flavour oscillations -- 4.3 Grand unified theories: proton decay -- 4.4 Grand unification and the neutrino see-saw mechanism -- 4.5 Hierarchies and supersymmetry -- 4.6 Summary -- Problems -- Part 2 The Early Universe -- 5 The expanding universe -- 5.1 The Hubble expansion -- 5.2 Olbers' paradox -- 5.3 The Friedmann equation -- 5.4 The sources of energy density -- 5.5 Observed energy densities -- 5.6 The age and size of the universe -- 5.7 The deceleration parameter -- 5.8 Cosmic microwave background radiation (CMB) -- 5.9 Anisotropies in the microwave radiation -- 5.10 Particles and radiations in the early universe -- 5.11 Photon and neutrino densities -- 5.12 Radiation and matter eras -- 5.13 The eras of matter-radiation equality -- 5.14 Summary -- Problems -- 6 Nucleosynthesis and baryogenesis -- 6.1 Primordial nucleosynthesis -- 6.2 Baryogenesis and matter-antimatter asymmetry -- 6.3 The baryon-photon ratio in the Big Bang -- 6.4 The Sakharov criteria -- 6.5 The baryon-antibaryon asymmetry: possible scenarios -- 6.6 Summary -- Problems -- 7 Dark matter and dark energy components -- 7.1 Preamble -- 7.2 Dark matter in galaxies and clusters -- 7.3 Gravitational lensing -- 7.4 Evidence for dark matter from gravitational lensing -- 7.5 Microlensing and MACHOs -- 7.6 The lensing probability: optical depth -- 7.7 Baryonic dark matter -- 7.8 Neutrinos -- 7.9 Axions -- 7.10 Axion-like particles -- 7.11 Weakly interacting massive particles -- 7.12 Expected WIMP cross-sections and event rates -- 7.13 Experimental WIMP searches -- 7.14 Dark energy: high redshift supernovae and Hubble plot at large z.
7.15 Vacuum energy: the Casimir effect -- 7.16 Problems with the cosmological constant and dark energy -- 7.17 Summary -- Problems -- 8 Development of structure in the early universe -- 8.1 Preamble -- 8.2 Galactic and intergalactic magnetic fields -- 8.3 Horizon and flatness problems -- 8.4 Inflation -- 8.5 Chaotic inflation -- 8.6 Quantum fluctuations and inflation -- 8.7 The spectrum of primordial fluctuations -- 8.8 Gravitational collapse and the Jeans mass -- 8.9 The growth of structure in an expanding universe -- 8.10 Evolution of fluctuations during the radiation era -- 8.11 Cosmological limits on neutrino mass from fluctuation spectrum -- 8.12 Growth of fluctuations in the matterdominated era -- 8.13 Temperature fluctuations and anisotropies in the CMB -- 8.14 The Angular spectrum of anisotropies: 'acoustic peaks' in the distribution -- 8.15 Experimental observation and interpretation of CMB anisotropies -- 8.16 Polarization of the cosmic microwave radiation -- 8.17 Summary -- Problems -- Part 3 Particles and Radiation in the Cosmos -- 9 Cosmic particles -- 9.1 Preamble -- 9.2 The composition and spectrum of cosmic rays -- 9.3 Geomagnetic and solar effects -- 9.4 Acceleration of cosmic rays -- 9.5 Secondary cosmic radiation: pions and muons -- 9.6 Passage of charged particles and radiation through matter -- 9.7 Development of an electromagnetic cascade -- 9.8 Extensive air showers: nucleon- and photon-induced showers -- 9.9 Detection of extensive air showers -- 9.10 Point sources of γ-rays -- 9.11 γ-Ray bursts -- 9.12 Ultra-high-energy cosmic ray showers: the GZK cut-off -- 9.13 Point sources of ultra high energy cosmic rays -- 9.14 Radio galaxies and quasars -- 9.15 Atmospheric neutrinos: neutrino oscillations -- 9.16 Solar neutrinos -- 9.17 Neutrino oscillations in matter -- 9.18 Point sources of high-energy neutrinos.
9.19 Gravitational radiation -- 9.20 The binary pulsar -- 9.21 Detection of gravitational waves -- 9.22 Summary -- Problems -- 10 Particle physics in stars and galaxies -- 10.1 Preamble -- 10.2 Stellar evolution-the early stages -- 10.3 Hydrogen burning: the p-p cycle in the Sun -- 10.4 Helium burning and the production of carbon and oxygen -- 10.5 Production of heavy elements -- 10.6 Electron degeneracy pressure and stellar stability -- 10.7 White dwarf stars -- 10.8 Stellar collapse: type II supernovae -- 10.9 Neutrinos from SN 1987A -- 10.10 Neutron stars and pulsars -- 10.11 Black holes -- 10.12 Hawking radiation from black holes -- 10.13 Summary -- Problems -- A: Table of physical constants -- B: Yukawa theory and the boson propagator -- C: Perturbative growth of structure in the early universe -- C.1 Growth in the matter-dominated era -- D: The MSW mechanism in solar neutrino interactions -- Answers to problems -- References -- Bibliography -- Index -- A -- B -- C -- D -- E -- F -- G -- H -- I -- J -- K -- L -- M -- N -- O -- P -- Q -- R -- S -- T -- U -- V -- W -- X -- Y -- Z.
Abstract:
How did our universe begin? An understanding of the development of the early universe brings together the subjects of particle physics, astrophysics, and cosmology. This text involves the student in this rapidly growing field of research. - ;The last years have seen a symbiosis of the fields of elementary particle physics and the astrophysics of the early universe. This text presents the background of the subjects and the latest developments at a level suitable for final year undergraduates and beginning graduate students. The first chapters cover the properties and interactions of elementary particles followed by discussion of the early universe, including inflation, dark matter and dark energy, and the growth of the. galactic structure. The final chapters discuss cosmic rays and particle physics in the stars. The close relation between particle interactions and large scale development of the cosmos is a constant theme in the text, with emphasis on the interplay between experiment and theory. This book is an enlarged and updated version of the first edition published five years ago. In a rapidly evolving field, emphasis has of course been placed on the most recent developments. However, the opportunity has also been taken to re-arrange the material and present it in more detail and at somewhat greater length. -.
Local Note:
Electronic reproduction. Ann Arbor, Michigan : ProQuest Ebook Central, 2017. Available via World Wide Web. Access may be limited to ProQuest Ebook Central affiliated libraries.
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