How likely are constituent quanta to initiate inflation?

DOI10.1016/j.physletb.2015.08.007zbMath1364.83064arXiv1504.01730OpenAlexW358087016WikidataQ60152582 ScholiaQ60152582MaRDI QIDQ2396550

Mark Trodden, Lasha Berezhiani

Publication date: 8 June 2017

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1504.01730

Mathematics Subject Classification ID

Relativistic cosmology (83F05)

Related Items (10)

String gas cosmology after Planck ⋮ The effects of potential shape on inhomogeneous inflation ⋮ Cyclic completion of the anamorphic universe ⋮ Bouncing cosmologies: progress and problems ⋮ A relativistic gas of inflatons as an initial state for inflation ⋮ Features and new physical scales in primordial observables: Theory and observation ⋮ Robustness of inflation to inhomogeneous initial conditions ⋮ The role of fluctuation-dissipation dynamics in setting initial conditions for inflation ⋮ Primordial gravitational waves and perturbations during an inhomogeneous inflation ⋮ Inhomogeneous initial data and small-field inflation

Cites Work

• A new type of isotropic cosmological models without singularity
• Wave function of the Universe
• Inflationary universe: A possible solution to the horizon and flatness problems

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