Results 31 to 40 of about 10,536 (250)
11 pages, 2 figures (In press Physical Review Letters 1995)
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On the consistency of warm inflation [PDF]
7 pages, ReVTeX.
Moss IG, Xiong C
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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
Mishra, Hiranmaya +2 more
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Inflaton as a pseudo-Nambu-Goldstone boson
In the realistic model of cosmic inflation the inflaton potential should be flat and stable under quantum corrections. It is natural to imagine that there is some symmetry behind and an idea of the inflaton as a Nambu-Goldstone boson of spontaneous ...
Noriaki Kitazawa
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Scaling Behavior in Warm Inflation
7 pages, no figures, revtex4. To be published in the Proceedings of the Conference "Phi in the Sky. The Quest for Cosmological Scalar Fields"
Mimoso, Jose P. +2 more
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Non-minimal Higgs inflation in the context of warm scenario in the light of Planck data
We investigate the non-minimally Higgs inflaton (HI) model in the context of warm inflation scenario. Warm little inflaton (WLI) model considers the little Higgs boson as inflaton.
Vahid Kamali
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Nonminimally-coupled warm Higgs inflation: Metric vs. Palatini formulations
In this work, we study the non-minimally-coupled Higgs model in the context of warm inflation scenario on both metric and Palatini approaches. We particularly consider a dissipation parameter of the form Γ=CTT with CT being a coupling parameter and focus
Thammarong Eadkhong +3 more
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CURRENT STATUS OF WARM INFLATION [PDF]
9 pages, 3 figures; Slightly longer version of a brief review talk at the 18th Lomonosov Conference on Elementary Particle Physics at Moscow State University, August 24-30 ...
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In this presentation, we are going to explain the thermodynamic origin of warm inflation scenarios by using the effetive Stefan-Boltzmann law. In the warm inflation scenarios, radiation always exists to avoid the graceful exit problem, for which the ...
Gim Yongwan, Kim Wontae
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Warm Little Inflaton becomes dark energy
We present a model where the inflaton field behaves like quintessence at late times, generating the present phase of accelerated expansion. This is achieved within the framework of warm inflation, in particular the Warm Little Inflaton scenario, where ...
João G. Rosa, Luís B. Ventura
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