1st Edition

Introduction to Cosmic Inflation and Dark Energy

By Konstantinos Dimopoulos Copyright 2021
284 Pages
by CRC Press

284 Pages
by CRC Press

284 Pages
by CRC Press

Cosmic inflation and dark energy hold the key to the origin and the eventual fate of the Universe. Despite the increasing prominence of these subjects in research and teaching over the past decade or more, no introductory textbook dedicated to these topics has been previously published. Dr. Konstantinos Dimopoulos is a highly regarded expert in the field, and an experienced communicator of the... Read more

Chapter 1. Introduction

Chapter 2. Dynamics and Content of the Universe

Chapter 3. History of the Universe

Chapter 4. Inflation basics

Chapter 5. CMB Primordial Anisotropy and Structure in the Universe

Chapter 6. The Inflationary Paradigm

Chapter 7. Models of Inflation

Chapter 8. beyond Slow-roll Inflation

Chapter 9. Dynamic Dark Energy

Chapter 10. Epilogue

Biography

Konstantinos Dimopoulos, presently Reader in Physics at Lancaster University, obtained his undergraduate degree in Physics from the Aristotle University of Thessaloniki in 1992. He continued his studies in the Department of Applied Mathematics and Theoretical Physics (DAMTP) of the University of Cambridge (Darwin College), where he obtained the Certificate of Advanced Study in Mathematics in 1994 and his PhD in Particle Cosmology in 1998 under the supervision of Professor A.C. Davis. Dr. Dimopoulos had several post-doctoral appointments in the framework of EU Research Training Network Programmes, in the Instituto de Fisica Corpuscular (IFIC) in Valencia, Spain (1999–2001) and in the Physics Department of Lancaster University, Lancaster, UK (2001–2003). In 2003, he obtained a four-year Research Associate Fellowship in the Institute of Nuclear Physics of the National Centre for Scientific Research ‘Demokritos’ in Athens, Greece, which he interrupted in 2004 when he was offered a staff position in the Physics Department of Lancaster University. His research interests centre around the physics of the very early Universe, in particular on particle cosmology, cosmic inflation, quintessential inflation, and cosmic vector fields.