Cosmological Inflation, Dark Matter and Dark Energy

• Autore: Bamba Kazuharu
• Pubblicazione: MDPI - Multidisciplinary Digital Publishing Institute, 2019
• Descrizione fisica: 1 electronic resource (236 p.)
• Soggetto non controllato: de Sitter vacuum; 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
• Sommario/riassunto: 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.
• Titolo autorizzato: Cosmological Inflation, Dark Matter and Dark Energy
• ISBN: 3-03921-765-8
• Formato: Materiale a stampa
• Livello bibliografico: Monografia
• Lingua di pubblicazione: Inglese
• Record Nr.: 9910367746403321
• Lo trovi qui: Univ. Federico II