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相关论文: Large-scale Perturbations from the Waterfall Field…

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We study carefully the contribution of the waterfall field to the curvature perturbation at the end of hybrid inflation. In particular we clarify the parameter dependence analytically under reasonable assumptions on the model parameters.…

宇宙学与河外天体物理 · 物理学 2011-03-28 Jinn-Ouk Gong , Misao Sasaki

We investigate the parameter spaces of hybrid inflation model with special attention paid to the dynamics of waterfall field and curvature perturbations induced from its quantum fluctuations. Depending on the inflaton field value at the…

宇宙学与河外天体物理 · 物理学 2015-05-28 Ali Akbar Abolhasani , Hassan Firouzjahi , Misao Sasaki

In this paper the possibility of generating large scale curvature perturbations induced from the entropic perturbations during the waterfall phase transition of standard hybrid inflation model is studied. We show that whether or not…

高能物理 - 理论 · 物理学 2011-03-22 Ali Akbar Abolhasani , Hassan Firouzjahi

We introduce a new method for calculating density perturbations in hybrid inflation which avoids treating the fluctuations of the "waterfall" field as if they were small perturbations about a classical trajectory. We quantize only the…

宇宙学与河外天体物理 · 物理学 2012-11-01 Alan H. Guth , Evangelos I. Sfakianakis

We discuss the waterfall that ends hybrid inflation. Making some simplifying assumptions, that may be satisfied by GUT inflation models, two issues are addressed. First, the procedure of keeping the quantum fluctuation of the waterfall…

宇宙学与河外天体物理 · 物理学 2015-05-19 David H. Lyth

We consider a two-field hybrid inflation model, in which the curvature perturbation is predominantly generated at the end of inflation. By finely tuning the coupling of the fields to the waterfall we find that we can get a measurable amount…

天体物理学 · 物理学 2009-11-11 Laila Alabidi , David Lyth

The decay of massive particles during inflation generates characteristic signals in the squeezed limit of the primordial bispectrum. These signals are in particular distinctive in the regime of the quasi-single field inflation, where…

宇宙学与河外天体物理 · 物理学 2018-08-08 Yi Wang , Yi-Peng Wu , Jun'ichi Yokoyama , Siyi Zhou

Hybrid inflation models are especially interesting as they lead to a spike in the density power spectrum on small scales, compared to the CMB, while also satisfying current bounds on tensor modes. Here we study hybrid inflation with $N$…

宇宙学与河外天体物理 · 物理学 2015-07-28 Illan F. Halpern , Mark P. Hertzberg , Matthew A. Joss , Evangelos I. Sfakianakis

We carried out numerical calculations of a contribution of the waterfall field to the primordial curvature perturbation (on uniform density hypersurfaces) $\zeta$, which is produced during waterfall transition in hybrid inflation scenario.…

宇宙学与河外天体物理 · 物理学 2011-11-17 Edgar Bugaev , Peter Klimai

We discuss the hybrid inflation model where the inflaton field is nonminimally coupled to gravity. In the Jordan frame, the potential contains $\phi^4$ term as well as terms in the original hybrid inflation model. In our model, inflation…

高能物理 - 理论 · 物理学 2011-02-22 Seoktae Koh , Masato Minamitsuji

The observed power spectrum of the cosmic microwave background (CMB) is consistent with inflationary cosmology, which predicts a nearly scale-invariant power spectrum of quantum fluctuations of the inflaton field as they exit the Hubble…

高能物理 - 理论 · 物理学 2007-05-23 Leonard Parker

In the framework of chaotic inflation we study the case of a massive scalar field using a semiclassical approach. We derive the energy density fluctuations in the infrared sector generated by matter field and gauge-invariant metric…

广义相对论与量子宇宙学 · 物理学 2010-11-11 F. Lara , F. Astorga , M. Bellini

We identify a new inflationary regime for which more than 60 e-folds are generated classically during the waterfall phase occuring after the usual hybrid inflation. By performing a bayesian Monte-Carlo-Markov-Chain analysis, this scenario…

广义相对论与量子宇宙学 · 物理学 2011-03-22 Sebastien Clesse

We compute the power spectrum of super-horizon curvature perturbations generated during a late period of thermal inflation, taking into account fluctuation-dissipation effects resulting from the scalar flaton field's interactions with the…

高能物理 - 唯象学 · 物理学 2024-07-22 Mar Bastero-Gil , Joaquim M. Gomes , João G. Rosa

We consider a variant of hybrid inflation where the waterfall phase transition happens during inflation. By adjusting the parameters associated with the mass of the waterfall field we arrange that the phase transition is not sharp so…

宇宙学与河外天体物理 · 物理学 2015-05-20 Ali Akbar Abolhasani , Hassan Firouzjahi , Mohammad Hossein Namjoo

We propose a new version of the hybrid inflation scenario that produces a significantly tilted n>1 spectrum of curvature perturbations. This may happen in supersymmetric models where the inflaton field acquires a mass proportional to the…

天体物理学 · 物理学 2009-09-29 Juan Garcia-Bellido , Andrei Linde

We study the parametric amplification of super-Hubble-scale scalar metric fluctuations at the end of inflation in some specific two-field models of inflation, a class of which is motivated by hybrid inflation. We demonstrate that there can…

高能物理 - 唯象学 · 物理学 2010-04-06 F. Finelli , R. Brandenberger

We consider D-term inflation for small couplings of the inflaton to matter fields. Standard hybrid inflation then ends at a critical value of the inflaton field that exceeds the Planck mass. During the subsequent waterfall transition the…

高能物理 - 唯象学 · 物理学 2015-06-22 W. Buchmuller , V. Domcke , K. Schmitz

Without demanding a specific form for the inflaton potential, we obtain an estimate of the contribution to the curvature perturbation generated during the linear era of the hybrid inflation waterfall. The spectrum of this contribution peaks…

宇宙学与河外天体物理 · 物理学 2015-06-03 David H. Lyth

For the original hybrid inflation as well as the supersymmetric F-term and D-term hybrid models, we calculate the level of non-gaussianities and the power spectrum of curvature perturbations generated during the waterfall, taking into…

宇宙学与河外天体物理 · 物理学 2014-03-26 Sébastien Clesse , Björn Garbrecht , Yi Zhu
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