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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 latetime 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.
bransdicke theory  dark energy model  cosmological parameters  Dark Energy  statistical analysis  Baryon Acoustic Oscillation (BAO)  Supernovae  cosmological model  Hubble constant  Cosmic Microwave Background (CMB) temperature  n/a  Dark Energy  Dark Matter  memory  dark matter  galactic rotation curve  cosmoligical parameters  dark energy models  loop quantum cosmology  dark energy  spacetime symmetry  de Sitter vacuum  quantum optical systems  astronomical and spaceresearch instrumentation  instruments, apparatus, and components common to several branches of physics and astronomy  normal galaxies, extragalactic objects and systems  field theory  comparative planetology  properties of specific particles  quantum optics  fundamental astronomy  EinsteinAether theory of gravity  dosmological parameters  dark energy models  cosmology  particle physics  cosmo–particle physics  QCD  hypercolor  dark atoms  composite dark matter  scalar–tensor gravity  junction conditions  null hypersurfaces  higher dimension gauged supergravity black hole  quantum gravity  quantum tunneling phenomenon  Hawking radiation  dynamical Chern–Simons modified gravity  parametrizations  cosmological parameters
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