A transition between bouncing hyper-inflation to ΛCDM from diffusive scalar fields

DOI10.1142/S0217751X18501191zbMath1395.83136arXiv1710.10588OpenAlexW3105986221MaRDI QIDQ4577916

D. Benisty, Eduardo I. Guendelman

Publication date: 6 August 2018

Published in: International Journal of Modern Physics A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1710.10588

zbMATH Keywords

diffusiondark matterscalar fieldsdark energybig bangdynamical timenonconservative stress-energy-momentum tensortwo measure theories

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Space-time singularities, cosmic censorship, etc. (83C75) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Astrophysical cosmology (85A40)

Related Items (2)

Scalar field dark matter and dark energy: a hybrid model for the dark sector ⋮ Cosmology of fermionic dark energy coupled to curvature

Cites Work

• Cosmological models with fluid matter undergoing velocity diffusion
• Emergent cosmology, inflation and dark energy
• Absence of the fifth force problem in a model with spontaneously broken dilatation symmetry
• Radiation-like scalar field and gauge fields in cosmology for a theory with dynamical time
• GRAVITATIONAL THEORY WITH A DYNAMICAL SPACE–TIME
• Dynamical Systems in Cosmology
• Unified DE–DM with diffusive interactions scenario from scalar fields
• HODGE DUALITY AND COSMOLOGICAL CONSTANT
• Transition to zero cosmological constant and phantom dark energy as solutions involving change of orientation of spacetime manifold
• EXOTIC LOW DENSITY FERMION STATES IN THE TWO MEASURES FIELD THEORY: NEUTRINO DARK ENERGY
• Einstein's General Theory of Relativity

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