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相关论文: Construction of inflationary scenarios with the Ga…

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We investigate the cosmological inflation for the Einstein-Hilbert action plus the Higgs potential function and the Gauss-Bonnet term coupled with the Higgs scalar field through a dilaton-like coupling. Then, using the…

广义相对论与量子宇宙学 · 物理学 2026-05-29 Zahra Ahghari , Mehrdad Farhoudi

We consider the constant-roll condition in the model of the inflaton nonminimal coupling to the Gauss-Bonnet term. By assuming the first Gauss-Bonnet flow parameter $\delta_1$ is a constant, we discuss the constant-roll inflation with…

广义相对论与量子宇宙学 · 物理学 2020-12-02 Tie-Jun Gao

We study a nonminimal derivative inflationary model in the presence of the Gauss-Bonnet term. To have a complete treatment of the model, we consider a general form of the nonminimal derivative function and also the Gauss-Bonnet coupling…

宇宙学与河外天体物理 · 物理学 2016-06-29 Kourosh Nozari , Narges Rashidi

Models of cosmic inflation suggest that our universe underwent an early phase of accelerated expansion, driven by the dynamics of one or more scalar fields. Inflationary models make specific, quantitative predictions for several observable…

宇宙学与河外天体物理 · 物理学 2016-05-10 David I. Kaiser

We show that an inflationary background might be realized by using any p-form non-minimally coupled to gravity. Standard scalar field inflation corresponds to the 0-form case and vector inflation to the 1-form. Moreover, we show that the 2-…

宇宙学与河外天体物理 · 物理学 2009-11-13 Cristiano Germani , Alex Kehagias

We propose new slow-roll approximations for inflationary models with the Gauss-Bonnet term. We find more accurate expressions of the standard slow-roll parameters as functions of the scalar field. To check the accuracy of approximations…

广义相对论与量子宇宙学 · 物理学 2024-09-24 Ekaterina O. Pozdeeva , Maria A. Skugoreva , Alexey V. Toporensky , Sergey Yu. Vernov

We consider the dynamics of power-law inflation with a nonminimally coupled scalar field $\phi$. It is well known that multiple scalar fields with exponential potentials $V(\phi)=V_0 {\rm exp}(-\sqrt{16\pi/p m_{\rm pl}^2} \phi)$ lead to an…

高能物理 - 唯象学 · 物理学 2009-10-31 S. Tsujikawa

This article presents a possible inflation scenario as a consequence of non-minimal gravitational couplings in the Conformal Standard Model. The model consists, in comparison to the SM, of additional right-chiral neutrinos and complex…

广义相对论与量子宇宙学 · 物理学 2018-02-27 Jan Kwapisz , Krzysztof A. Meissner

We construct models with the Gauss-Bonnet term multiplied to a function of the scalar field leading to inflationary scenario. The consideration is related with the slow-roll approximation. The cosmological attractor approach gives the…

广义相对论与量子宇宙学 · 物理学 2020-07-29 E. O. Pozdeeva

We study inflation with the most general non-degenerate gravitational action that depends on the symmetric part of the Ricci tensor coupled to a scalar field in the Palatini formulation of gravity. We use field redefinitions to shift the…

宇宙学与河外天体物理 · 物理学 2021-09-24 Jaakko Annala , Syksy Rasanen

Non-abelian gauge field inflation is studied in the context of warm inflation scenario. We introduce this scenario as a mechanism that gives an end for gauge-flation model. Slow-roll parameters and perturbation parameters are presented for…

广义相对论与量子宇宙学 · 物理学 2015-06-17 M. R. Setare , V. Kamali

We derive a generalized expressions for the scalar power spectrum and the observational parameters of inflation (the scalar spectral index $n_{\rm s}$ and the tensor-to-scalar ratio $r$) for several single field scalar models minimally…

广义相对论与量子宇宙学 · 物理学 2024-09-25 Marko Stojanovic , Dragoljub D. Dimitrijevic , Milan Milosevic

We study a class of generalized inflation models in which the inflaton is coupled to the Ricci scalar by a general $f(\phi, R)$ term. The scalar power spectrum, the spectral index, the running of the spectral index, the tensor mode spectrum…

天体物理学 · 物理学 2008-11-26 Bin Chen , Miao Li , Tower Wang , Yi Wang

Picking out DBI scalar field as inflation, the slow-rolling inflationary scenario is studied by attributing an exponential time function to scale factor; known as intermediate inflation. The perturbation parameters of the model are…

广义相对论与量子宇宙学 · 物理学 2017-08-15 N. Nazavari , A. Mohammadi , Z. Ossoulian , Kh. Saaidi

It is well known that the non-minimal coupling $\xi\phi^2R$ between the inflaton and the Ricci scalar affects predictions of single field inflation models. In particular, the $\lambda\phi^4$ quartic inflation potential with…

宇宙学与河外天体物理 · 物理学 2019-10-11 Nilay Bostan , Vedat Nefer Şenoğuz

We argue that in models of inflation with two scalar fields and non-canonical kinetic terms there is a possibility of obtaining a red tilt of the power spectrum of curvature perturbations from noncanonicality-induced interactions between…

高能物理 - 理论 · 物理学 2015-03-17 Sera Cremonini , Zygmunt Lalak , Krzysztof Turzynski

An intermediate inflationary universe model within the context of non-minimally coupled to the scalar curvature is analyzed. We will conduct our analysis under the slow roll approximation of the inflationary dynamics and the cosmological…

广义相对论与量子宇宙学 · 物理学 2017-09-12 Carlos Gonzalez , Ramon Herrera

The radiative neutrino mass model with inert doublet dark matter is a promising model for the present experimental issues which cannot be explained within the standard model. We study an extension of this model focusing on cosmological…

高能物理 - 唯象学 · 物理学 2016-02-05 Romy H. S. Budhi , Shoichi Kashiwase , Daijiro Suematsu

Recent LHC data provides precise values of coupling constants of the Higgs field, however, these measurements do not determine its coupling with gravity. We explore this freedom to see whether Higgs field non-minimally coupled to…

宇宙学与河外天体物理 · 物理学 2016-08-17 Jose Mathew , S. Shankaranarayanan

We analyze a two-field inflationary model consisting of the Ricci scalar squared ($R^2$) term and the standard Higgs field non-minimally coupled to gravity in addition to the Einstein $R$ term. Detailed analysis of the power spectrum of…

宇宙学与河外天体物理 · 物理学 2018-06-13 Minxi He , Alexei A. Starobinsky , Jun'ichi Yokoyama