Results 11 to 20 of about 771,516 (312)

Warm Inflation [PDF]

open access: yesUniverse, 2016
I show here that there are some interesting differences between the predictions of warm and cold inflation models focusing in particular upon the scalar spectral index n s and the tensor-to-scalar ratio r.
Øyvind Grøn
doaj   +3 more sources

Monomial warm inflation revisited [PDF]

open access: yesJournal of Cosmology and Astroparticle Physics, 2023
We revisit the idea that the inflaton may have dissipated part of its energy into a thermal bath during inflation, considering monomial inflationary potentials and three different forms of dissipation rate.
G. Ballesteros   +2 more
semanticscholar   +5 more sources

Warm quintessential inflation [PDF]

open access: yesPhysics Letters B, 2019
We introduce warm quintessential inflation and study it in the weak dissipative regime. We consider the original quintessential inflation model, which approximates quartic chaotic inflation at early times and thawing quartic inverse-power-law ...
Konstantinos Dimopoulos   +1 more
doaj   +4 more sources

Reconstructing warm inflation [PDF]

open access: yesEuropean Physical Journal C: Particles and Fields, 2018
The reconstruction of a warm inflationary universe model from the scalar spectral index $$n_S(N)$$ nS(N) and the tensor to scalar ratio r(N) as a function of the number of e-folds N is studied.
Ramón Herrera
doaj   +4 more sources

Anisotropic warm inflation [PDF]

open access: yesPhysical Review D, 2022
Anisotropic inflation is a model succeeded in explaining statistical anisotropy. Warm inflation is a model succeeded in providing a mechanism of reheating during inflation. We study anisotropic warm inflation focusing on the cosmic no-hair conjecture. In
S. Kanno   +3 more
semanticscholar   +3 more sources

Shapes of non-Gaussianity in warm inflation [PDF]

open access: greenJournal of Cosmology and Astroparticle Physics, 2023
Sphaleron heating has been recently proposed as a mechanism to realize warm inflation when inflaton is an axion coupled to pure Yang-Mills. As a result of heating, there is a friction coefficient γ ∝ T 3 in the equation of motion for the inflaton, and a ...
Mehrdad Mirbabayi, Andrei Gruzinov
openalex   +3 more sources

Theoretical and observational prescription of warm-inflation in FLRW universe with torsion

open access: yesEuropean Physical Journal C: Particles and Fields, 2023
The paper deals with Warm Inflationary scenario in FLRW with torsion both from theoretical and observational point of view. In the background of flat FLRW model the Hubble parameter is found to be proportional to the torsion function and warm inflation ...
Madhukrishna Chakraborty   +3 more
doaj   +2 more sources

Primordial black-hole dark matter via warm natural inflation

open access: diamondPhysics Letters B, 2022
We report on a study of the natural warm inflationary paradigm (WNI). We show two important new results arise in this model. One is that the observational constraints on the primordial power spectrum from the cosmic microwave background (CMB) can be ...
Miguel Correa   +3 more
doaj   +4 more sources

Warm DBI inflation with constant sound speed [PDF]

open access: diamondEuropean Physical Journal C: Particles and Fields, 2019
We study inflation with the Dirac–Born–Infeld (DBI) noncanonical scalar field in both the cold and warm scenarios. We consider the Anti-de Sitter warp factor $$f(\phi )=f_{0}/\phi ^{4}$$ f(ϕ)=f0/ϕ4 for the DBI inflation and check viability of the quartic
S. Rasouli   +3 more
doaj   +2 more sources

Erratum: Minimal warm inflation [PDF]

open access: hybridJournal of Cosmology and Astroparticle Physics, 2023
We correct several minor mistakes in equations in section 4.1 and update the viable parameter range of the model quoted in section 4.2 accordingly.
Kim V. Berghaus   +2 more
openalex   +2 more sources

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