rdf-syntax-grammar
mods:
  schema location: http://www.loc.gov/mods/v3 http://www.loc.gov/standards/mods/v3/mods-3-2.xsd
  title info:
    title: Understanding the Epoch of Cosmic Reionization
    sub title: Challenges and Progress
  name:
    name part: Mesinger, Andrei.
    role:
      role term: editor.
  name:
    name part: SpringerLink (Online service)
  type of resource: text
  origin info:
    place:
      place term: gw
    date issued: 2016
    edition: 1st ed. 2016.
    issuance: monographic
  language:
    language term: eng
  physical description:
    form: electronic
    form: electronic resource
    reformatting quality: access
    form: remote
    extent: XI, 286 p. 59 illus., 49 illus. in color. online resource.
  abstract: The aim of this volume is to summarize the current status and future outlook of the reionization field on both the theoretical and observational fronts. It brings together leading experts in many sub-disciplines, highlighting the measurements that are likely to drive the growing understanding of reionization and the cosmic dawn, and lays out a roadmap to interpreting the wealth of upcoming observations. The birth of the first stars and galaxies, and their impact on the diffuse matter perme­ating the early Universe, is one of the final frontiers in cosmology. Recently, measure­ments of the fluctuations in the cosmic microwave background (CMB), sourced only a few hundred thousand years after the Big Bang, provided robust insight into the overall physical content of our Universe. On the other end of the timeline, groundbreaking telescopes provide us a picture of the complexities of the galaxy-rich universe in which we now live. However, we know almost nothing about the astrophysics of the first billion years. During this relatively brief epoch, a tiny fraction of matter condensed inside the first galaxies, forming the first stars. This culminated in the final major phase change of our universe, cosmological reionization, which lifted the cosmic fog and allowed visible light to spread throughout space. This mysterious ep­och of reionization corresponds to the transition between the relative simplicity of the early universe and the complexity of the present-day one. It is fundamental in understanding cosmic origins, and its impact on structure formation resonates even to this day. Until recently, there was very little observational insight into the epoch of reionization. Subsequent observational and theoretical advancements have begun to paint a picture of a complicated, extended, inhomogeneous process. At its core, the process of cosmological reionization involves understanding how stars and clumps of gas impact each other and eventually the entire Universe. The challen…
  table of contents: Chapter 1: Cosmic Reionization and the First Nonlinear Structures in the Universe, Zolt´an Haiman -- Chapter 2: Physics of the Intergalactic Medium during the Epoch of Reionization, Adam Lidz -- Chapter 3: Quasars as Probes of Cosmological Reionization, Daniel J. Mortlock -- Chapter 4: Observing the Epoch of Reionization with the Cosmic Microwave Background, Christian L. Reichardt -- Chapter 5: The 21-cm Line as a Probe of Reionization, Steven R. Furlanetto -- Chapter 6: Constraining Reionization with Lya Emitting Galaxies, Mark Dijkstra -- Chapter 7: Metal Enrichment in the Reionization Epoch, Andrea Ferrara.
  note: edited by Andrei Mesinger.
  subject:
    topic: Physics
  subject:
    topic: Astronomy
  subject:
    topic: Astrophysics
  subject:
    topic: Cosmology
  subject:
    topic: Physics
  subject:
    topic: Astronomy, Astrophysics and Cosmology
  classification: QB1-991
  classification: QB460-466
  classification: QB980-991
  classification: 520
  related item:
    title info:
      title: Springer eBooks
  related item:
    title info:
      title: Astrophysics and Space Science Library, 423
  identifier: 9783319219578
  identifier: http://dx.doi.org/10.1007/978-3-319-21957-8
  record info:
    record creation date: 151128
    record change date: 20170425141128.0
    record identifier: 978-3-319-21957-8