Cosmological Inflation, Dark Matter and Dark Energy

• Hoofdauteur: Bamba, Kazuharu (auth)
• Formaat: Elektronisch Hoofdstuk
• Taal: Engels
• Gepubliceerd in: MDPI - Multidisciplinary Digital Publishing Institute 2019
• Onderwerpen: 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
• Online toegang: DOAB: download the publication; DOAB: description of the publication

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...