Cosmological Inflation, Dark Matter and Dark Energy

Various cosmological observations support not only cosmological inflation in the early universe, which is also known as exponential cosmic expansion, but also that the expansion of the late-time universe is accelerating. To explain this phenomenon, the existence of dark energy is proposed. In additi...

Full description

Saved in:
Bibliographic Details
Main Author: Bamba, Kazuharu (auth)
Format: Book Chapter
Published: MDPI - Multidisciplinary Digital Publishing Institute 2019
Subjects:
Online Access:Get Fullteks
DOAB: description of the publication
Tags: Add Tag
No Tags, Be the first to tag this record!
LEADER 04142naaaa2200853uu 4500
001 doab_20_500_12854_44151
005 20210211
020 |a books978-3-03921-765-6 
020 |a 9783039217649 
020 |a 9783039217656 
024 7 |a 10.3390/books978-3-03921-765-6  |c doi 
041 0 |a English 
042 |a dc 
100 1 |a Bamba, Kazuharu  |4 auth 
245 1 0 |a Cosmological Inflation, Dark Matter and Dark Energy 
260 |b MDPI - Multidisciplinary Digital Publishing Institute  |c 2019 
300 |a 1 electronic resource (236 p.) 
506 0 |a Open Access  |2 star  |f Unrestricted online access 
520 |a Various cosmological observations support not only cosmological inflation in the early universe, which is also known as exponential cosmic expansion, but also that the expansion of the late-time universe is accelerating. To explain this phenomenon, the existence of dark energy is proposed. In addition, according to the rotation curve of galaxies, the existence of dark matter, which does not shine, is also suggested. If primordial gravitational waves are detected in the future, the mechanism for realizing inflation can be revealed. Moreover, there exist two main candidates for dark matter. The first is a new particle, the existence of which is predicted in particle physics. The second is an astrophysical object which is not found by electromagnetic waves. Furthermore, there are two representative approaches to account for the accelerated expansion of the current universe. One is to assume the unknown dark energy in general relativity. The other is to extend the gravity theory to large scales. Investigation of the origins of inflation, dark matter, and dark energy is one of the most fundamental problems in modern physics and cosmology. The purpose of this book is to explore the physics and cosmology of inflation, dark matter, and dark energy. 
540 |a Creative Commons  |f https://creativecommons.org/licenses/by-nc-nd/4.0/  |2 cc  |4 https://creativecommons.org/licenses/by-nc-nd/4.0/ 
546 |a English 
653 |a de Sitter vacuum 
653 |a n/a 
653 |a Einstein-Aether theory of gravity 
653 |a Supernovae 
653 |a apparatus 
653 |a normal galaxies 
653 |a higher dimension gauged super-gravity black hole 
653 |a dark energy model 
653 |a cosmo-particle physics 
653 |a instruments 
653 |a Cosmic Microwave Background (CMB) temperature 
653 |a Dark Energy 
653 |a hyper-color 
653 |a quantum tunneling phenomenon 
653 |a spacetime symmetry 
653 |a parametrizations 
653 |a quantum gravity 
653 |a dynamical Chern-Simons modified gravity 
653 |a comparative planetology 
653 |a properties of specific particles 
653 |a particle physics 
653 |a dark matter 
653 |a Hawking radiation 
653 |a memory 
653 |a junction conditions 
653 |a cosmology 
653 |a composite dark matter 
653 |a dosmological parameters 
653 |a field theory 
653 |a Dark Matter 
653 |a cosmological model 
653 |a extragalactic objects and systems 
653 |a scalar-tensor gravity 
653 |a fundamental astronomy 
653 |a cosmoligical parameters 
653 |a cosmological parameters 
653 |a Baryon Acoustic Oscillation (BAO) 
653 |a dark atoms 
653 |a quantum optical systems 
653 |a brans-dicke theory 
653 |a dark energy models 
653 |a loop quantum cosmology 
653 |a dark energy 
653 |a galactic rotation curve 
653 |a astronomical and space-research instrumentation 
653 |a null hypersurfaces 
653 |a QCD 
653 |a quantum optics 
653 |a Hubble constant 
653 |a and components common to several branches of physics and astronomy 
653 |a statistical analysis 
856 4 0 |a www.oapen.org  |u https://mdpi.com/books/pdfview/book/1789  |7 0  |z Get Fullteks 
856 4 0 |a www.oapen.org  |u https://directory.doabooks.org/handle/20.500.12854/44151  |7 0  |z DOAB: description of the publication