Though astrophysicists have developed a theoretical framework for understanding how the first stars and galaxies formed, only now are we able to begin testing those theories with actual observations of the very distant, early universe. We are entering a new and exciting era of discovery that will advance the frontiers of knowledge, and this book couldn't be more timely. It covers all the basic concepts in cosmology, drawing on insights from an astronomer who has pioneered much of this research over the past two decades. Abraham Loeb starts from first principles, tracing the theoretical foundations of cosmology and carefully explaining the physics behind them. Topics include the gravitational growth of perturbations in an expanding universe, the abundance and properties of dark matter halos and galaxies, reionization, the observational methods used to detect the earliest galaxies and probe the diffuse gas between them--and much more. Cosmology seeks to solve the fundamental mystery of our cosmic origins. This book offers a succinct and accessible primer at a time when breathtaking technological advances promise a wealth of new observational data on the first stars and galaxies. Provides a concise introduction to cosmology Covers all the basic concepts Gives an overview of the gravitational growth of perturbations in an expanding universe Explains the process of reionization Describes the observational methods used to detect the earliest galaxies
This book takes the reader on an exploration of the structure and evolution of our universe.
This book provides a comprehensive, self-contained introduction to one of the most exciting frontiers in astrophysics today: the quest to understand how the oldest and most distant galaxies in our universe first formed.
This is left as key science for future telecopes like the James Webb Space Telescope.
Together, they will revolutionize the study of the most distant objects in the Universe. This volume is aimed at beginning graduate students but can also serve as a reference work for active researchers in the field.
Galaxies are vast ensembles of stars, gas and dust, embedded in dark matter halos. They are the basic building blocks of the Universe, gathered in groups, clusters and super-clusters. They exist in many forms, either as spheroids or disks.
The purpose of First Stars and Galaxies: Challenges in the Coming Decade was to congregate theorists and observers to review recent developments in our understanding of the formation of primordial stars and protogalaxies in advance of key ...
Consequently, the flux in forbidden lines is not directly related to the UV luminosity produced by massive young stars. Despite of this, it is found that the [OII] ... (d) Far-Infrared Continuum Typically the ISM associated with a ...
A large number of the theoretical challenges posed by the Science Frontiers Panels are of a scale and complexity that require sustained, multi-institutional collaborations of theorists, computational astrophysicists, observers, ...
A comprehensive examination of nearly fourteen billion years of galaxy formation and evolution, from primordial gas to present-day galaxies.
This book looks at answers to the biggest questions in astronomy – the questions of how the planets, stars, galaxies and the universe were formed.