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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...

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Autor principal: Bamba, Kazuharu
Format: Online
Idioma:anglès
Publicat: MDPI - Multidisciplinary Digital Publishing Institute 2021
Matèries:
QA1-939
Q1-390
de Sitter vacuum
n/a
Einstein-Aether theory of gravity
Supernovae
apparatus
normal galaxies
higher dimension gauged super-gravity black hole
dark energy model
cosmo–particle physics
instruments
Cosmic Microwave Background (CMB) temperature
Dark Energy
hyper-color
quantum tunneling phenomenon
spacetime symmetry
parametrizations
quantum gravity
dynamical Chern–Simons modified gravity
comparative planetology
properties of specific particles
particle physics
dark matter
Hawking radiation
memory
junction conditions
cosmology
composite dark matter
dosmological parameters
field theory
Dark Matter
cosmological model
extragalactic objects and systems
scalar–tensor gravity
fundamental astronomy
cosmoligical parameters
cosmological parameters
Baryon Acoustic Oscillation (BAO)
dark atoms
quantum optical systems
brans-dicke theory
dark energy models
loop quantum cosmology
dark energy
galactic rotation curve
astronomical and space-research instrumentation
null hypersurfaces
QCD
quantum optics
Hubble constant
and components common to several branches of physics and astronomy
statistical analysis
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