Results 31 to 40 of about 359,649 (249)

Observational constraints on warm inflation in loop quantum cosmology [PDF]

open access: yesJournal of Cosmology and Astroparticle Physics, 2019
By incorporating quantum aspects of gravity, Loop Quantum Cosmology (LQC) provides a self-consistent extension of the inflationary scenario, allowing for modifications in the primordial inflationary power spectrum with respect to the standard General ...
M. Benetti, L. Graef, R. O. Ramos
semanticscholar   +1 more source

Inflation in multidimensional quantum cosmology [PDF]

open access: yesPhysical Review D, 1996
We extend to multidimensional cosmology Vilenkin's prescription of tunnelling from nothing for the quantum origin of the observable Universe. Our model consists of a $D+4$-dimensional spacetime of topology ${\cal R}\times {\cal S}^3 \times{\cal S}^D$, with a scalar field (``chaotic inflaton'') for the matter component.
Giuseppe Pollifrone   +3 more
openaire   +3 more sources

Palatini R 2 quintessential inflation [PDF]

open access: yesJournal of Cosmology and Astroparticle Physics, 2022
We construct a model of quintessential inflation in Palatini R 2 gravity employing a scalar field with a simple exponential potential and coupled to gravity with a running non-minimal coupling.
K. Dimopoulos   +3 more
semanticscholar   +1 more source

How Generic Is Eternal Inflation?

open access: yesSci, 2022
Everlasting inflation has far-reaching implications for cosmology and the standing of self-localizing inferences made by observers, which have been subjects of renewed interest in light of the growing acceptance of theory landscapes and the attendant ...
Ross Greenwood, Anthony Aguirre
doaj   +1 more source

Massive neutrino self-interactions and inflation [PDF]

open access: yesJournal of Cosmology and Astroparticle Physics, 2022
Certain inflationary models like Natural inflation (NI) and Coleman-Weinberg inflation (CWI) are disfavoured by cosmological data in the standard ΛCDM+r model (where r is the scalar-to-tensor ratio), as these inflationary models predict the regions in ...
Shouvik Roy Choudhury   +2 more
semanticscholar   +1 more source

Pre-inflationary dynamics of Starobinsky inflation and its generization in loop quantum Brans-Dicke cosmology [PDF]

open access: yesJournal of Cosmology and Astroparticle Physics, 2018
Recently, the nonperturbative quantization scheme of loop quantum gravity has been extended to the Brans-Dicke theory and the corresponding loop quantum Brans-Dicke cosmology has been derived, which provides an essential platform to explore inflationary ...
Wei-Jian Jin, Yong-Liang Ma, Tao Zhu
semanticscholar   +1 more source

Reheating in holographic cosmology and connecting to Λ-MSSM constructions for particle physics

open access: yesJournal of High Energy Physics, 2021
In this paper we model the transition from the non-geometric holographic cosmology regime, to the usual radiation dominated (RD) cosmology, known as reheating in the case of (perturbative) inflation.
Horatiu Nastase
doaj   +1 more source

Inflation and precision cosmology [PDF]

open access: yesBrazilian Journal of Physics, 2004
A brief review of inflation is presented. After having demonstrated the generality of the inflationary mechanism, the emphasize is put on its simplest realization, namely the single field slow-roll inflationary scenario. Then, it is shown how, concretely, one can calculate the predictions of a given model of inflation.
openaire   +4 more sources

A built-in inflation in the $$f(T)$$ f ( T ) -cosmology [PDF]

open access: yesThe European Physical Journal C, 2014
LaTeX2e: 19 pages, 9 figures, 1 table.
Gamal G. L. Nashed   +2 more
openaire   +3 more sources

Singularities in Inflationary Cosmological Models

open access: yesUniverse, 2021
Due to the accelerated expansion of the universe, the possibilities for the formation of singularities has changed from the classical Big Bang and Big Crunch singularities to include a number of new scenarios. In recent papers it has been shown that such
Leonardo Fernández-Jambrina
doaj   +1 more source

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