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Within the second half of the last century, quantum cosmology concretely became one of the main research lines within gravitational theory and cosmology. Substantial progress has been made. Furthermore, quantum cosmology can become a domain that will gradually develop further over the next handful of decades, perhaps assisted by technological developments. Indications for new physics (i.e., beyond the standard model of particle physics or general relativity) could emerge and then the observable universe would surely be seen from quite a new perspective. This motivates bringing quantum cosmology to more research groups and individuals.This Special Issue (SI) aims to provide a wide set of reviews, ranging from foundational issues to (very) recent advancing discussions. Concretely, we want to inspire new work proposing observational tests, providing an aggregated set of contributions, covering several lines, some of which are thoroughly explored, some allowing progress, and others much unexplored. The aim of this SI is motivate new researchers to employ and further develop quantum cosmology over the forthcoming decades. Textbooks and reviews exist on the present subject, and this SI will complementarily assist in offering open access to a set of wide-ranging reviews. Hopefully, this will assist new interested researchers, in having a single open access online volume, with reviews that can help. In particular, this will help in selecting what to explore, what to read in more detail, where to proceed, and what to investigate further within quantum cosmology.
string cosmology --- quantum cosmology --- Wheeler-DeWitt equation --- loop quantum cosmology --- observations --- classical and quantum cosmology --- time --- quantum fields in curved spacetime --- Brans–Dicke theory --- bounce models --- de Broglie–Bohm interpretation --- quantum geometrodynamics --- extended theories of gravity --- dark energy singularities --- quantum gravity --- Hawking radiation --- entanglement entropy --- uniqueness of the quantization --- polymer quantum mechanics --- bounce --- no-boundary proposal --- instantons --- multiverse --- superspace --- third quantisation --- universe–antiuniverse pair --- weyl curvature hypothesis --- early universe cosmology --- singularity and bounce --- cyclic universe --- quantum fields --- backreaction effects --- supersymmetry --- noncommutativity --- generalized uncertainty principles --- canonical quantum gravity --- clocks --- noether symmetries --- ADM formalism --- exact solutions --- supersymmetric quantum mechanics --- shape invariant potentials --- supersymmetric quantum cosmology --- n/a --- Brans-Dicke theory --- de Broglie-Bohm interpretation --- universe-antiuniverse pair
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Following the fundamental insights from quantum mechanics and general relativity, geometry itself should have a quantum description; the search for a complete understanding of this description is what drives the field of quantum gravity. Group field theory is an ambitious framework in which theories of quantum geometry are formulated, incorporating successful ideas from the fields of matrix models, ten-sor models, spin foam models and loop quantum gravity, as well as from the broader areas of quantum field theory and mathematical physics. This special issue collects recent work in group field theory and these related approaches, as well as other neighbouring fields (e.g., cosmology, quantum information and quantum foundations, statistical physics) to the extent that these are directly relevant to quantum gravity research.
quantum-gravity phenomenology --- hypersurface deformation algebra --- loop quantum gravity --- black holes --- no-boundary proposal --- loop quantum cosmology --- LQC instanton --- quantum gravity --- computer simulations --- numerical methods --- renormalization group --- discrete quantum gravity models --- nonperturbative renormalization group --- random geometry --- mimetic gravity --- limiting curvature --- bouncing cosmology --- effective field theory --- quantum geometry --- quantum cosmology --- group field theory --- cosmological perturbation theory --- Lewis-Riesenfeld invariant --- Bogoliubov transformation --- adiabatic vacua --- Spin networks --- vertex amplitudes --- quantum computing --- background independence --- generalised statistical equilibrium --- entropy --- holographic entanglement --- random tensor networks --- quantum many-body physics
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This book celebrates the 80 years of the Professor Eugene P. Wigner paper “On Unitary Representations of the Inhomogeneous Lorentz Group", published in The Annals of Mathematics in 1939. We have collected several contributions divided into Research articles and Reviews. All contributions are technical, but the papers also bring a health element of didactic. Practitioners from several areas, from Gravity to Quantum Field Theory and Quantum Mechanics, as well as students, shall find a rich material in this Volume.
spinors in 4d --- regularization --- anomalies --- quantum gravity --- quantum mechanics --- symmetry --- quantum cosmology --- special relativity --- combination of velocities --- wigner angle --- quaternions --- gauge field theory --- Yang-Mills fields --- modified gravity --- non-Riemannian geometry --- spacetime symmetries --- gauge field theories --- gauge anomalies --- nonperturbative techniques --- ray representation --- strongly continuous --- continuity --- Hilbert space --- entanglement --- bispinors --- chirality --- n/a
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The multiverse is a concept that acknowledges the existence of a multiplicity of worlds or universes. The designs of these universes do not have to be the same as our universe, but we have no clear view of what the “other” designs might be. It is suspected that they can obey different laws of physics and different constants of physics, which further implies different chemistry, biology, and life. Some say that the universes within the multiverse allow for different mathematics or even for different metamathematical logic. This book discusses most of the above aspects of the multiverse concept starting with the philosophy, through all the mathematical and physical subtleties, finally exploring the origin of life and consciousness. This book provides a satisfying intellectual exploration of front-edge advances in contemporary cosmology.
multiverse --- Leibniz --- other worlds --- multiverse levels --- habitability --- stars --- quantum cosmology --- origin of the universe --- time reversal symmetry --- planets --- life --- varying constants --- anthropic principle --- multiverse entanglement --- multiverse tests --- mass extinctions --- string theory --- string landscape --- dark energy --- creation from nothing --- soft entry --- quantum gravity --- Wheeler-de Witt-equation --- Bohm-like interpretation --- volume-quantisation --- space atoms --- information storage and transfer --- philosophy of multiverse --- categories of multiverses --- different physics universes --- superstring multiverse --- dark multiverse --- universe-antiuniverse pair creation --- multiverse habitability: stars, planets, life, consciousness --- falsifiability of multiverses
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"The four volumes of the proceedings of MG14 give a broad view of all aspects of gravitational physics and astrophysics, from mathematical issues to recent observations and experiments. The scientific program of the meeting included 35 morning plenary talks over 6 days, 6 evening popular talks and 100 parallel sessions on 84 topics over 4 afternoons. Volume A contains plenary and review talks ranging from the mathematical foundations of classical and quantum gravitational theories including recent developments in string theory, to precision tests of general relativity including progress towards the detection of gravitational waves, and from supernova cosmology to relativistic astrophysics, including topics such as gamma ray bursts, black hole physics both in our galaxy and in active galactic nuclei in other galaxies, and neutron star, pulsar and white dwarf astrophysics. The remaining volumes include parallel sessions which touch on dark matter, neutrinos, X-ray sources, astrophysical black holes, neutron stars, white dwarfs, binary systems, radiative transfer, accretion disks, quasars, gamma ray bursts, supernovas, alternative gravitational theories, perturbations of collapsed objects, analog models, black hole thermodynamics, numerical relativity, gravitational lensing, large scale structure, observational cosmology, early universe models and cosmic microwave background anisotropies, inhomogeneous cosmology, inflation, global structure, singularities, chaos, Einstein-Maxwell systems, wormholes, exact solutions of Einstein's equations, gravitational wave detectors and data analysis, precision gravitational measurements, loop quantum gravity, quantum cosmology, self-gravitating systems, gamma ray astronomy, cosmic rays and the history of general relativity"--
Binary Systems --- Astrophysics --- Loop Quantum Gravity --- Gravitational Wave Detectors and Data Analysis --- Black Hole Thermodynamics --- Active Galactic Nuclei --- Observational Cosmology --- Gravitational Wave --- X-ray Sources --- Dark Matter --- General Relativity --- Cosmic Rays --- Inflation --- Numerical Relativity --- Neutrinos --- Theoretical Physics --- Large Scale Structure --- Inhomogeneous Cosmology --- Radiative Transfer --- Supernova --- Gravitation --- Black Hole --- White Dwarf --- Precision Gravitational Measurements --- Quantum Gravity --- Quantum Cosmology --- Einstein-Maxwell Systems --- String Theory --- Cosmic Microwave Background Anisotropies --- Accretion Disks --- Neutron Star --- Gravitational Lensing --- Exact Solutions of Einstein's Equations --- Early Universe Models --- Wormholes --- Cosmology --- Pulsar --- Gamma Ray Burst
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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 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 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 --- cosmo-particle physics --- dynamical Chern-Simons modified gravity --- scalar-tensor gravity
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