Results 31 to 40 of about 978,154 (293)

Viscous warm inflation: Hamilton–Jacobi formalism [PDF]

open access: yesAstroparticle Physics, 2017
Using Hamilton-Jacobi formalism, The scenario of warm inflation with viscous pressure is considered. The formalism gives a way of computing the slow-rolling parameters without extra approximation, and it is well-known as a powerful method in cold inflation.
Akhtari, L.   +3 more
openaire   +4 more sources

D-brane and exponential potentials inspire warm inflation and swampland conjecture

open access: yesNuclear Physics B
This research explores the rapid expansion period of the early universe by applying the Chaplygin gas model, an alternative cosmological framework, to analyze the dynamics of inflationary processes.
Shama Sadiq   +6 more
doaj   +2 more sources

Minimal warm inflation [PDF]

open access: yesJournal of Cosmology and Astroparticle Physics, 2020
Slow-roll inflation is a successful paradigm. However we find that even a small coupling of the inflaton to other light fields can dramatically alter the dynamics and predictions of inflation. As an example, the inflaton can generically have an axion-like coupling to gauge bosons. Even relatively small couplings will automatically induce a thermal bath
Berghaus, Kim V.   +2 more
openaire   +2 more sources

Looking inside the Swampland from Warm Inflation: Dissipative Effects in De Sitter Expansion

open access: yesUniverse, 2023
This paper reviews the theoretical and phenomenological implications of the swampland conjectures from the perspective of inflationary cosmology, focusing on warm inflation.
Arjun Berera, Jaime CalderĂłn-Figueroa
doaj   +1 more source

Extended warm inflation [PDF]

open access: yesPhysical Review D, 1999
11 pages, 1 ...
Maia, J. M. F., Lima, J. A. S.
openaire   +2 more sources

Revisiting Barrow's graduated inflationary universe: A warm perspective

open access: yesPhysics Letters B, 2022
It is presumed that thermal fluctuations present during inflationary epoch can make inflaton scalar field to interact with other fields resulting in the existence of a thermal component during the inflationary period.
Subhra Bhattacharya
doaj   +1 more source

Warm vector inflation [PDF]

open access: yesPhysics Letters B, 2013
In this paper we introduce the "warm vector inflation" scenario. In warm inflation scenario radiation is produced during the inflation epoch and reheating is avoided. Slow-roll and perturbation parameters of this model are presented. We develop our model using intermediate inflation model.
Setare, M. R., Kamali, V.
openaire   +3 more sources

Is warm inflation possible? [PDF]

open access: yesPhysical Review D, 1999
22 pages ...
Yokoyama, Jun'ichi, Linde, Andrei
openaire   +2 more sources

Strengthening the de Sitter swampland conjecture in warm inflation

open access: yesJournal of High Energy Physics, 2020
The de Sitter constraint on the space of effective scalar field theories consistent with superstring theory provides a lower bound on the slope of the potential of a scalar field which dominates the evolution of the Universe, e.g., a hypothetical ...
Robert Brandenberger   +2 more
doaj   +1 more source

WarmSPy: a numerical study of cosmological perturbations in warm inflation [PDF]

open access: yesJournal of Cosmology and Astroparticle Physics, 2023
We present WarmSPy, a numerical code in Python designed to solve for the perturbations' equations in warm inflation models and compute the corresponding scalar power spectrum at CMB horizon crossing.
Gabriele Montefalcone   +3 more
semanticscholar   +1 more source

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