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  1. Magnetic Fields in Galaxies

    Magnetic fields are a major agent in the interstellar medium. They contribute significantly to the total pressure which balances the gas disk against...
    Rainer Beck in Cosmic Magnetic Fields
    Chapter
  2. Magnetic Fields in Galaxy Systems, Clusters and Beyond

    The discovery of significant magnetic fields beyond our Milky Way was unwittingly made in the early 1950’s when new “discrete” cosmic radio sources...
    Philipp P. Kronberg in Cosmic Magnetic Fields
    Chapter
  3. Stellar Magnetic Fields

    Stellar magnetic fields are directly detected or inferred across the whole Hertzsprung--Russell Diagram. Attention in this chapter is concentrated on...
    Leon Mestel, John D. Landstreet in Cosmic Magnetic Fields
    Chapter
  4. Magnetic Fields in Diffuse HI and Molecular Clouds

    The diffuse interstellar HI is the matrix within which many molecular clouds reside and the medium that soaks up the energy injected by sources such...
    C. Heiles, R. Crutcher in Cosmic Magnetic Fields
    Chapter
  5. Magnetic Fields in the Early Universe

    A substantial magnetic field could conceivably have been generated in the ultra-early Universe. However, the relevant physics at those eras is very...
    Martin J. Rees in Cosmic Magnetic Fields
    Chapter
  6. Introduction

    We summarize the topics presented in this book, and when appropriate we enlighten cross–references among the different topics: high precision and...
    Nora Bretón, Jorge L. Cervantes–Cota, Marcelo Salgado in The Early Universe and Observational Cosmology
    Chapter
  7. Cosmological Applications of Loop Quantum Gravity

    After a brief introduction to classical and quantum gravity we discuss applications of loop quantum gravity in the cosmological realm. This includes...
    Martin Bojowald, Hugo A. Morales-Técotl in The Early Universe and Observational Cosmology
    Chapter
  8. Quantum Corrections to Scalar Quintessence Potentials

    We give a brief introduction into the formalism of the effective action. We use the effective action to investigate the stability of scalar...
    Michael Doran, Joerg Jaeckel in The Early Universe and Observational Cosmology
    Chapter
  9. The Accelerating Universe and Dark Energy: Evidence from Type Ia Supernovae

    I discuss the use of Type Ia supernovae (SNe Ia) for cosmological distance determinations. Low-redshift SNe Ia (...
    Chapter
  10. Infering Annihilation Channels of Neutralinos in Galactic Halos

    Applying the microcanonical definition of entropy to a weakly interacting and self–gravitating neutralino gas, we evaluate the change in the local...
    Luis G. Cabral–Rosetti, Xavier Hernández, Roberto A. Sussman in The Early Universe and Observational Cosmology
    Chapter
  11. Electroweak Baryogenesis and Primordial Hypermagnetic Fields

    The origin of the matter-antimatter asymmetry of the universe remains one of the outstanding questions yet to be answered by modern cosmology, and...
    Gabriella Piccinelli, Alejandro Ayala in The Early Universe and Observational Cosmology
    Chapter
  12. Inflation

    The optimistic picture for the explanation of the baryon-antibaryon asymmetry that we apparently obtain with grand unified theories has one serious...
    Dierck-Ekkehard Liebscher in Cosmology
    Chapter
  13. Standard Synthesis

    One of the two most important observations that indicate a hot past of the universe is the universal distribution of helium and deuterium. Deuterium,...
    Dierck-Ekkehard Liebscher in Cosmology
    Chapter
  14. Topological Concepts in Gauge Theories

    In these lecture notes, an introduction to topological concepts and methods in studies of gauge field theories is presented. The three paradigms of...
    Chapter
  15. 1 An Introduction to the Physics of the Early Universe

    We present an elementary introduction to the Early Universe. The basic features of the hot Big Bang are reviewed in the framework of the fundamental...
    Kyriakos Tamvakis in The Physics of the Early Universe
    Chapter
  16. Basics

    Telescopes of all kinds look deep into the sky and find planets, stars, the Milky Way, other galaxies, clusters of galaxies, the large-scale...
    Dierck-Ekkehard Liebscher in Cosmology
    Chapter
  17. Topological Quasi-Particles

    The subject of topology is the set of properties of relative positions that can be defined without the use of metric properties. A metric induces a...
    Dierck-Ekkehard Liebscher in Cosmology
    Chapter
  18. Anthropic Aspects

    Cosmology attempts to understand the observable metagalaxy as a representative part of the universe and as a necessary consequence of the laws that...
    Dierck-Ekkehard Liebscher in Cosmology
    Chapter
  19. Higher Dimensions

    The invariance group of mechanics and field theory tells us that space has three dimensions, and space-time four. Nearly all physical theory uses...
    Dierck-Ekkehard Liebscher in Cosmology
    Chapter
  20. Chiral Anomalies and Topology

    When a field theory has a symmetry, global or local like in gauge theories, in the tree or classical approximation formal manipulations lead to...
    Chapter
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