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The Fizeau effect in a flowing refractive medium is treated and extended to when light propagates at an angle to the medium velocity. The reflection optics with relativistically moving mirrors is examined. Using Stokes parameters, it is shown that polarization is preserved in Lorentz transformation between frames of reference.
The chapter commences with an introduction to the ideas of special relativity. A brief discussion of the life and work of Albert Einstein is presented. The propagation of light, relativistic time dilation, and length contraction followed by a simple explanation of the production of light by accelerating charges are presented.
The motion of single electrons in electromagnetic waves is determined. The propagation of light in plasma with many electrons is treated leading to ,for example, an expression for the refractive index of a plasma. Cherenkov radiation and incoherent and coherent Thomson scatter and Compton scatter of light are examined.
Equilibrium distribution functions are determined for fermions (e.g. electrons) and bosons (e.g. photons). The Saha–Boltzmann equation, the Maxwellian distribution, and relativistic Maxwell–Juttner distribution are derived. The relativistic equation of state for a distribution where particle velocities approach the speed of light is examined.
Radiative transfer, the Einstein A and B coefficients, emission and absorption coefficients, and Doppler line broadening are discussed. Continuum radiation emission coefficients are derived using the idea of virtual photon scattering. Inverse Compton scattering is treated in some detail. The radiation reaction force is examined.
The Lorentz invariance of the phase of light is discussed. The transformation between frames of electric and magnetic fields is determined. The transformation between frames of acceleration is determined. The effect on the angular range of light in a laboratory frame when emitted in a rapidly moving frame is discussed in some detail.
The chemical potential of electrons is discussed as a function of density and temperature, including effects of degeneracy and relativity. It is shown that the chemical potential at all but the highest densities is negative.
The Lagrangian for a charge in electric and magnetic fields is presented. The acceleration of charges in particle accelerators, in laser-produced plasmas and in the production of cosmic rays is described. Emission from charges in magnetic fields is treated in some detail. Synchrotron radiation, undulators, and free electron laser radiation output is examined.
This textbook introduces the topic of special relativity, with a particular emphasis upon light-matter interaction and the production of light in plasma. The physics of special relativity is intuitively developed and related to the radiative processes of light. The book reviews the underlying theory of special relativity, before extending the discussion to applications frequently encountered by postgraduates and researchers in astrophysics, high power laser interactions and the users of specialized light sources, such as synchrotrons and free electron lasers. A highly pedagogical approach is adopted throughout, and numerous exercises are included within each chapter to reinforce the presentation of key concepts and applications of the material.
All aspects of space plasmas in the Solar System are introduced and explored in this text for senior undergraduate and graduate students. Introduction to Space Physics provides a broad, yet selective, treatment of the complex interactions of the ionized gases of the solar terrestrial environment. The book includes extensive discussion of the Sun and solar wind, the magnetized and unmagnetized planets, and the fundamental processes of space plasmas including shocks, plasma waves, ULF waves, wave particle interactions, and auroral processes. The text devotes particular attention to space plasma observations and integrates these with phenomenological and theoretical interpretations. Highly coordinated chapters, written by experts in their fields, combine to provide a comprehensive introduction to space physics. Based on an advanced undergraduate and graduate course presented in the Department of Earth and Space Sciences at the University of California, Los Angeles, the text will be valuable to both students and professionals in the field.