A Closer Look at Dark Energy
Seiten
2019
Nova Science Publishers Inc (Verlag)
978-1-5361-6348-3 (ISBN)
Nova Science Publishers Inc (Verlag)
978-1-5361-6348-3 (ISBN)
The universe is in a period of accelerated expansion; and the observational evidence such as supernova of Ia type, Cosmic Microwave Background radiation (CMB) and Baryon Acoustic Oscillations (BAO) confirm this accelerating expansion [1-3]. Despite the great number of observational evidence, the responsible mechanism for this accelerating expansion is still unknown, and thus several models have been proposed for this phenomenon[4-18]. The simplest proposed model in the general relativity is a cosmic model with a dominant component that is considered as a fluid with negative pressure and constant density[8] (means Dark Energy component) . In this book, we consider effects of Dark Energy content on the universe. Accordingly, structure of discussions in the present book was on four chapters as follows: chapter 1 : Dark Energy, Motivation and Candidates, chapter 2 : The Equivalence Principle Applicability Boundaries,Measurability, Gravity and Dark Energy Problem, chapter 3 : The Behaviors of a Candidate for Dark Energy from ur-Higgs Boson , and chapter 4 : Non-equilibrium Evolution of Quantum Fields During Inflation and Late Accelerating Expansion . However, I hope this collection of context will be useful for readers to understand more accurately the dark energy idea.
| Erscheinungsdatum | 04.12.2019 |
|---|---|
| Verlagsort | New York |
| Sprache | englisch |
| Gewicht | 420 g |
| Themenwelt | Naturwissenschaften ► Physik / Astronomie ► Astronomie / Astrophysik |
| ISBN-10 | 1-5361-6348-1 / 1536163481 |
| ISBN-13 | 978-1-5361-6348-3 / 9781536163483 |
| Zustand | Neuware |
| Informationen gemäß Produktsicherheitsverordnung (GPSR) | |
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