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Is warm inflation possible? [PDF]
22 pages ...
Andrei Linde+2 more
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Strengthening the de Sitter swampland conjecture in warm inflation
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
Multi-field cold and warm inflation and the de Sitter swampland conjectures [PDF]
We discuss under which conditions multi-field cold and warm inflationary models with canonical kinetic energy terms are compatible with the swampland conjectures about the emergence of de Sitter solutions in string theory.
O. Bertolami, Paulo M. Sá
semanticscholar +1 more source
Warming up cold inflation [PDF]
Abstract The axion is a well-motivated candidate for the inflaton, as the radiative corrections that spoil many single-field models are avoided by virtue of its shift symmetry. However, axions generically couple to gauge sectors. As the axion slow-rolls during inflation, this coupling can cause the production of a non-diluting thermal ...
Saarik Kalia+2 more
openaire +4 more sources
On the consistency of warm inflation [PDF]
7 pages, ReVTeX.
Moss IG, Xiong C
openaire +4 more sources
Warm-assisted natural inflation [PDF]
Abstract We consider natural inflation in a warm inflation framework with a temperature-dependent dissipative coefficient Γ∝ T3. Natural inflation can be compatible with the Planck 2018 results with such warm assistance. With no a priori assumptions on the dissipative effect's magnitude, we find that the Planck results prefer a weak ...
Yakefu Reyimuaji, Xinyi Zhang
openaire +3 more sources
11 pages, 2 figures (In press Physical Review Letters 1995)
openaire +3 more sources
Scalar Induced Gravitational Waves from Warm Inflation [PDF]
Stochastic gravitational waves can be induced from the primordial curvature perturbations generated during inflation, through scalar-tensor mode coupling at the second order of cosmological perturbation theory.
R. Arya, A. Mishra
semanticscholar +1 more source
In warm inflation models there is the requirement of generating large dissipative couplings of the inflaton with radiation, while at the same time, not de-stabilising the flatness of the inflaton potential due to radiative corrections. One way to achieve this without fine tuning unrelated couplings is by supersymmetry. In this paper we show that if the
Hiranmaya Mishra+2 more
openaire +3 more sources