Martin Lemoine – författare

Some 25 years after the birth of inflationary cosmology this volume sets out to provide a both authoritative and pedagogical introduction and review of the state of the field. Cosmic inflation corresponds to an episode of accelerated expansion of the very early universe and solves nicely a collection of puzzles that had plagued standard cosmology so far. Different scenarios exist, though, and the reader will learn about the "ins" and "outs" as the subject and related issues are surveyed. With lectures written by eminent scientists in the field, many of them having made pioneering contributrions in the early hours of the field, "Inflationary Cosmology" addresses both senior and younger high-energy physicists, cosmologists and observational astrophysicists seeking both a readable account and reference in the field.

Some 25 years after the birth of inflationary cosmology this volume sets out to provide a both authoritative and pedagogical introduction and review of the state of the field. Cosmic inflation corresponds to an episode of accelerated expansion of the very early universe and solves nicely a collection of puzzles that had plagued standard cosmology so far. Different scenarios exist, though, and the reader will learn about the "ins" and "outs" as the subject and related issues are surveyed. With lectures written by eminent scientists in the field, many of them having made pioneering contributrions in the early hours of the field, "Inflationary Cosmology" addresses both senior and younger high-energy physicists, cosmologists and observational astrophysicists seeking both a readable account and reference in the field.

Relativistic objects in astrophysics present a diverse set of phenomena and cover vast ranges of time scales and spatial scales, but their descriptions rely on a similar backbone: production of a relativistic outflow in a central compact object and dissipation of the outflow at large radii, accompanied by acceleration of particles up to very high energies and production of secondary non-thermal electromagnetic radiation. This book provides a timely and comprehensive review of the main physical processes involved in the formation and dissipation of relativistic outflows. It will be particularly useful to postgraduate students and researchers active in various areas of astrophysics and space science​. Originally published in Space Science Reviews, Volume 207, Issue 1-4, July 2017

Relativistic objects in astrophysics present a diverse set of phenomena and cover vast ranges of time scales and spatial scales, but their descriptions rely on a similar backbone: production of a relativistic outflow in a central compact object and dissipation of the outflow at large radii, accompanied by acceleration of particles up to very high energies and production of secondary non-thermal electromagnetic radiation. This book provides a timely and comprehensive review of the main physical processes involved in the formation and dissipation of relativistic outflows. It will be particularly useful to postgraduate students and researchers active in various areas of astrophysics and space science​. Originally published in Space Science Reviews, Volume 207, Issue 1-4, July 2017