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相关论文: Semi-shifted hybrid inflation with B-L cosmic stri…

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String models can produce successful inflationary scenarios in the context of brane collisions and in many of these models cosmic strings may also be produced. In scenarios such as KKLMMT the string contribution is naturally predicted to be…

天体物理学 · 物理学 2009-11-11 Uros Seljak , Anze Slosar

We have proposed a new class of inflationary scenarios in which the first stage of expansion is driven by "old" false vacuum inflation. This ends by nucleation of a bubble, which then further inflates. Unlike the standard slow-roll…

高能物理 - 唯象学 · 物理学 2007-05-23 Gia Dvali , Shamit Kachru

We extend our previous study of supersymmetric Higgs inflation in the context of no-scale supergravity and grand unification, to include models based on the flipped SU(5) and the Pati-Salam group. Like the previous SU(5) GUT model, these…

高能物理 - 唯象学 · 物理学 2016-09-01 John Ellis , Hong-Jian He , Zhong-Zhi Xianyu

Theories with elementary scalar degrees of freedom seem nowadays required for simple descriptions of the Standard Model and of the Early Universe. It is then natural to embed theories of inflation in supergravity, also in view of their…

高能物理 - 理论 · 物理学 2015-09-30 S. Ferrara , A. Sagnotti

In this paper, we consider logarithmic radiative corrections and higher order terms to the supersymmetric hilltop F- and D-term hybrid inflation models. Conventional F- and D-term hybrid inflation only predicts $n_s \gae 0.98$. We show that…

高能物理 - 唯象学 · 物理学 2010-04-23 Chia-Min Lin , Kingman Cheung

A realistic tribrid model of sneutrino inflation is constructed in an $R$-symmetric $SU(5)$ grand unified theory (GUT). To avoid the monopole problem, a pseudosmooth inflationary trajectory is generated with the help of an additional $Z_5$…

高能物理 - 唯象学 · 物理学 2020-04-27 Muhammad Atif Masoud , Mansoor Ur Rehman , Qaisar Shafi

We reconsider a class of well motivated supersymmetric models in which inflation is associated with the breaking of a gauge symmetry G to H, with the symmetry breaking scale M~10^16 GeV. Starting with a renormalizable superpotential, we…

高能物理 - 唯象学 · 物理学 2008-11-26 V. N. Senoguz , Q. Shafi

We analyze various phases of inflation based on the anomaly-induced effective action of gravity (modified Starobinsky model), taking the cosmological constant Lambda and k=0, +/- 1 topologies into account. The total number of the…

高能物理 - 唯象学 · 物理学 2009-11-07 A. M. Pelinson , I. L. Shapiro , F. I. Takakura

We consider a cosmological set-up, based on renormalizable superpotential terms, in which a superheavy scale F-term hybrid inflation is followed by a Peccei-Quinn phase transition, resolving the strong CP and mu problems of the minimal…

高能物理 - 唯象学 · 物理学 2014-11-21 G. Lazarides , C. Pallis

We develop sequestered inflation models, where inflation occurs along flat directions in supergravity models derived from type IIB string theory. It is compactified on a ${\mathbb{T}^6 \over \mathbb{Z}_2 \times \mathbb{Z}_2}$ orientifold…

高能物理 - 理论 · 物理学 2021-10-18 Renata Kallosh , Andrei Linde , Timm Wrase , Yusuke Yamada

We propose a general scenario for moduli stabilization where low-energy supersymmetry can be accommodated with a high scale of inflation. The key ingredient is that the stabilization of the modulus field during and after inflation is not…

高能物理 - 理论 · 物理学 2015-07-24 Stefan Antusch , Koushik Dutta , Sebastian Halter

We study the cosmology of a string derived supersymmetric flipped $SU(5)$ model in the context of free-fermionic heterotic constructions that allow full calculability of the effective supergravity in perturbation theory around the fermionic…

高能物理 - 理论 · 物理学 2021-03-12 Ignatios Antoniadis , Dimitri V. Nanopoulos , John Rizos

${\rm B - L}$ cosmic strings form in a wide class of theories beyond the Standard Model which contain a ${\rm U}(1)_{{\rm B - L}}$ gauge symmetry. They can form at the end of hybrid inflation and explain, together with inflation, the Cosmic…

高能物理 - 唯象学 · 物理学 2007-05-23 R. Jeannerot

We propose a model for cosmic inflation which is based on an effective description of strongly interacting, nonsupersymmetric matter within the framework of dynamical Abelian projection and centerization. The underlying gauge symmetry is…

高能物理 - 唯象学 · 物理学 2009-11-07 Ralf Hofmann , Mathias Th. Keil

Within the MSSM we propose the chaotic inflationary scenario in which the inflaton field is a combination of sleptons and the Higgs field states evolving along the $D$-term flat direction. In the inflation and postinflation reheating…

高能物理 - 唯象学 · 物理学 2019-12-19 Zurab Tavartkiladze

We consider a cosmological inflation scenario based on a no-scale supergravity sector with $U(1)_R$ symmetry. It is shown that a tree level $U(1)_R$ symmetric superpotential alone does not lead to a slowly rolling scalar potential. A…

高能物理 - 唯象学 · 物理学 2019-05-29 Shaaban Khalil , Ahmad Moursy , Abhijit Kumar Saha , Arunansu Sil

In a recent paper (see https://doi.org/10.1103/PhysRevD.108.095053), we have demonstrated that the 2023 PTA results, which hint at a stochastic gravitational wave (GW) background at nanohertz frequencies, point towards a promising…

高能物理 - 唯象学 · 物理学 2024-09-18 Stefan Antusch , Kevin Hinze , Shaikh Saad

We discuss non-minimal quadratic inflation in supersymmetric (SUSY) and non-SUSY models which entails a linear coupling of the inflaton to gravity. Imposing a lower bound on the parameter cR, involved in the coupling between the inflaton…

高能物理 - 唯象学 · 物理学 2015-03-31 Constantinos Pallis , Qaisar Shafi

We consider a class of well motivated supersymmetric models of F-term hybrid inflation (FHI) which can be linked to the supersymmetric grand unification. The predicted scalar spectral index n_s cannot be smaller than 0.97 and can exceed…

高能物理 - 唯象学 · 物理学 2010-01-26 C. Pallis

The conventional slow-roll approximation is broken in the so-called "ultra slow-roll" models of inflation, for which the inflaton potential is exactly (or extremely) flat. The interesting nature of (canonical) ultra slow-roll inflation is…

宇宙学与河外天体物理 · 物理学 2016-11-18 Shin'ichi Hirano , Tsutomu Kobayashi , Shuichiro Yokoyama
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