TY  - GEN
AU  - Bamba,Kazuharu
TI  - Cosmological Inflation, Dark Matter and Dark Energy
SN  - books978-3-03921-765-6
PY  - 2019///
PB  - MDPI - Multidisciplinary Digital Publishing Institute
KW  - de Sitter vacuum
KW  - n/a
KW  - Einstein-Aether theory of gravity
KW  - Supernovae
KW  - apparatus
KW  - normal galaxies
KW  - higher dimension gauged super-gravity black hole
KW  - dark energy model
KW  - cosmo–particle physics
KW  - instruments
KW  - Cosmic Microwave Background (CMB) temperature
KW  - Dark Energy
KW  - hyper-color
KW  - quantum tunneling phenomenon
KW  - spacetime symmetry
KW  - parametrizations
KW  - quantum gravity
KW  - dynamical Chern–Simons modified gravity
KW  - comparative planetology
KW  - properties of specific particles
KW  - particle physics
KW  - dark matter
KW  - Hawking radiation
KW  - memory
KW  - junction conditions
KW  - cosmology
KW  - composite dark matter
KW  - dosmological parameters
KW  - field theory
KW  - Dark Matter
KW  - cosmological model
KW  - extragalactic objects and systems
KW  - scalar–tensor gravity
KW  - fundamental astronomy
KW  - cosmoligical parameters
KW  - cosmological parameters
KW  - Baryon Acoustic Oscillation (BAO)
KW  - dark atoms
KW  - quantum optical systems
KW  - brans-dicke theory
KW  - dark energy models
KW  - loop quantum cosmology
KW  - dark energy
KW  - galactic rotation curve
KW  - astronomical and space-research instrumentation
KW  - null hypersurfaces
KW  - QCD
KW  - quantum optics
KW  - Hubble constant
KW  - and components common to several branches of physics and astronomy
KW  - statistical analysis
N1  - Open Access
N2  - 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
UR  - https://mdpi.com/books/pdfview/book/1789
UR  - https://directory.doabooks.org/handle/20.500.12854/44151
ER  -