04061nam 2200889z- 450 991036774640332120231214132937.03-03921-765-8(CKB)4100000010106253(oapen)https://directory.doabooks.org/handle/20.500.12854/44151(EXLCZ)99410000001010625320202102d2019 |y 0engurmn|---annantxtrdacontentcrdamediacrrdacarrierCosmological Inflation, Dark Matter and Dark EnergyMDPI - Multidisciplinary Digital Publishing Institute20191 electronic resource (236 p.)3-03921-764-X 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.de Sitter vacuumEinstein-Aether theory of gravitySupernovaeapparatusnormal galaxieshigher dimension gauged super-gravity black holedark energy modelcosmo-particle physicsinstrumentsCosmic Microwave Background (CMB) temperatureDark Energyhyper-colorquantum tunneling phenomenonspacetime symmetryparametrizationsquantum gravitydynamical Chern-Simons modified gravitycomparative planetologyproperties of specific particlesparticle physicsdark matterHawking radiationmemoryjunction conditionscosmologycomposite dark matterdosmological parametersfield theoryDark Mattercosmological modelextragalactic objects and systemsscalar-tensor gravityfundamental astronomycosmoligical parameterscosmological parametersBaryon Acoustic Oscillation (BAO)dark atomsquantum optical systemsbrans-dicke theorydark energy modelsloop quantum cosmologydark energygalactic rotation curveastronomical and space-research instrumentationnull hypersurfacesQCDquantum opticsHubble constantand components common to several branches of physics and astronomystatistical analysisBamba Kazuharuauth1323469BOOK9910367746403321Cosmological Inflation, Dark Matter and Dark Energy3035588UNINA