A new type of isotropic cosmological models without singularity
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The large-scale structure of the universe: Turbulence, intermittency, structures in a self-gravitating mediumBrane new worldDark matter from R2 gravityCosmological constraints from the SDSS luminous red galaxiesGeneral relativity as an effective field theory: The leading quantum correctionsPopulating the landscape: A top-down approachLinearized f ( R ) gravity: Gravitational radiation and Solar System testsTesting General Relativity with Low-Frequency, Space-Based Gravitational-Wave DetectorsSECOND ORDER SCALAR INVARIANTS OF THE RIEMANN TENSOR: APPLICATIONS TO BLACK HOLE SPACETIMESProbes and Tests of Strong-Field Gravity with Observations in the Electromagnetic Spectrum.Cosmology and Fundamental Physics with the Euclid Satellite.Stochastic Gravity: Theory and Applications.Is exponential gravity a viable description for the whole cosmological history?Palatini wormholes and energy conditions from the prism of general relativity.Symmetry behavior in curved spacetime: Finite-size effect and dimensional reduction.The Higgs field and the resolution of the Cosmological Constant Paradox in the Weyl-geometrical Universe.Case for an EeV Gravitino.Brane gas-driven bulk expansion as a precursor stage to brane inflation.Black hole relics and inflation: Limits on blue perturbation spectra.Critical Number of Fields in Stochastic Inflation.Cosmology based on f(R) gravity admits 1 eV sterile neutrinos.Sequestering the standard model vacuum energy.Primordial non-Gaussianities of gravitational waves in the most general single-field inflation model with second-order field equations.One gravitational potential or two? Forecasts and tests.Dark energy from primordial inflationary quantum fluctuations.GUT's in curved spacetime: Running gravitational constants, Newtonian potential, and the quantum-corrected gravitational equations.Perturbative method to solve fourth-order gravity field equations.Semiclassical equations for weakly inhomogeneous cosmologies.Einstein equation with quantum corrections reduced to second order.Stability of the semiclassical Einstein equation.Inflation in a renormalizable cosmological model and the cosmic no-hair conjecture.Solutions to the effective field equations for a proposed gravitational effective action.Asymptotically Friedmann and Friedmann-type solutions to Einstein's equations when quantum effects due to conformally invariant fields are taken into account.Did BICEP2 see vector modes? First B-mode constraints on cosmic defects.Frame-Independent Classification of Single-Field Inflationary Models.Decaying vacuum energy and deflationary cosmology in open and closed universes.Plane domain walls when coupled with the Brans-Dicke scalar field.AgravityInflation after false vacuum decay: Observational prospects after PlanckTIME IN QUANTUM GRAVITY
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P2860
A new type of isotropic cosmological models without singularity
description
article
@en
im März 1980 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована в березні 1980
@uk
ലേഖനം
@ml
name
A new type of isotropic cosmological models without singularity
@en
A new type of isotropic cosmological models without singularity
@nl
type
label
A new type of isotropic cosmological models without singularity
@en
A new type of isotropic cosmological models without singularity
@nl
prefLabel
A new type of isotropic cosmological models without singularity
@en
A new type of isotropic cosmological models without singularity
@nl
P1433
P1476
A new type of isotropic cosmological models without singularity
@en
P2093
A.A. Starobinsky
P304
P356
10.1016/0370-2693(80)90670-X
P577
1980-03-01T00:00:00Z