Results 51 to 60 of about 896,961 (328)
New limits on warm inflation from pulsar timing arrays [PDF]
Rocco D’Agostino, Matteo Califano
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Constraints of Anisotropy on Warm Power-Law Ination in Light of Planck Results [PDF]
In this article, we examine the effects of anisotropy on a model of canonical warm inflation with the power-law potential. And we have compared the limitations of this model with Planck's results.
Zahra Ghadiry +2 more
doaj +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
Mishra, Hiranmaya +2 more
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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 the anisotropic warm inflation, the condition for making anisotropy survived is clarified.
Sugumi Kanno +3 more
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Salvaging power-law inflation through warming
Power-law inflation with scale factor $$a \propto t^m$$ a ∝ t m is investigated in the context of warm inflation. The treatment is performed in the weak and strong dissipation limits.
M. Alhallak, N. Chamoun, M. S. Eldaher
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Warm pseudoscalar inflation [PDF]
5 pages, 3 figures, 1 table, comments ...
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Warm inflation in a Universe with a Weylian boundary [PDF]
Teodora Matei, Tiberiu Harko
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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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Particle creation and warm inflation [PDF]
During cosmological inflation, it has been suggested that fields coupled to the inflaton can be excited by the slow-rolling inflaton into a quasi-stable non-vacuum state.
Aarts +28 more
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