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A second order pole in the scalar kinetic term can lead to a class of inflation models with universal predictions referred to as pole inflation or $\alpha$-attractors. While this kinetic structure is ubiquitous in supergravity effective…

高能物理 - 理论 · 物理学 2019-03-11 Mafalda Dias , Jonathan Frazer , Ander Retolaza , Marco Scalisi , Alexander Westphal

We consider a phenomenological model of inflation where the inflaton is the phase of a complex scalar field $\Phi$. Planck-suppressed operators of $\mathcal O(f^5/M_\mathrm{pl})$ modify the geometry of the vev $\langle \Phi \rangle$ at…

宇宙学与河外天体物理 · 物理学 2015-11-19 Layne C. Price

Minimal hybrid inflation in supergravity has been ruled out by the 2015 Planck observations because the spectral index of the produced curvature perturbation falls outside observational bounds. To resurrect the model, a number of…

高能物理 - 唯象学 · 物理学 2016-10-25 Konstantinos Dimopoulos , Charlotte Owen

In this paper, we study inflation with {\alpha}-attractor potential in the RS braneworlds where high energy corrections to the Friedmann equation facilitate slow roll. In this scenario, we numerically investigate the inflationary parameters…

广义相对论与量子宇宙学 · 物理学 2019-05-22 Nur Jaman , Kairat Myrzakulov

It is commonly believed that a successful period of inflation driven by a single or several scalar fields requires a specific hierarchy of masses given by $M_{inf}\ll H \ll M_{heavy}$, where $M_{inf}$ can correspond to several or a single…

高能物理 - 理论 · 物理学 2020-01-15 Dibya Chakraborty , Roberta Chiovoloni , Oscar Loaiza-Brito , Gustavo Niz , Ivonne Zavala

We generalize the embedding of induced-gravity inflation beyond the no-scale Supergravity presented in arXiv:1403.5486 employing two gauge singlet chiral superfields, a superpotential uniquely determined by applying a continuous R and a…

高能物理 - 唯象学 · 物理学 2014-10-24 C. Pallis

The BICEP2 collaboration has recently reported a large tensor fluctuation in the cosmic microwave background, which suggests chaotic inflation models. In this letter, we reconsider the chaotic inflation model in the supergravity. We…

高能物理 - 唯象学 · 物理学 2015-06-19 Keisuke Harigaya , Tsutomu T. Yanagida

A new family of inflation models is introduced and studied. The models are characterised by a scalar potential which, far from the origin, approaches an inflationary plateau in a power-law manner, while near the origin becomes monomial, as…

高能物理 - 唯象学 · 物理学 2015-11-20 Konstantinos Dimopoulos

In this paper we show that certain types of cosmological brane configurations may induce topological inflation. In generic models for topological inflation, there is a strict bound for the potential of the inflaton field. Naively, it seems…

高能物理 - 唯象学 · 物理学 2009-11-10 Tomohiro Matsuda

It is shown that, when the inflaton field modulates the gauge kinetic function of the gauge fields in supergravity realisations of inflation, the dynamic backreaction leads to a new inflationary attractor solution, in which the inflaton's…

宇宙学与河外天体物理 · 物理学 2016-01-15 Konstantinos Dimopoulos , George Lazarides , Jacques M. Wagstaff

We construct $\alpha$-attractor versions of hybrid inflation models. In these models, the potential of the inflaton field $\varphi$ is uplifted by the potential of the second field $\chi$. This uplifting ends due to a tachyonic instability…

高能物理 - 理论 · 物理学 2022-08-31 Renata Kallosh , Andrei Linde

With the growing consensus on simple power law inflation models not being favored by the PLANCK observations, dynamics for the non-standard inflation gain significant interest in the recent past. In this paper, we analyze in detail a class…

广义相对论与量子宇宙学 · 物理学 2019-03-08 Debaprasad Maity , Pankaj Saha

We present a two-field inflation model where inflaton field has a non-canonical kinetic term due to the presence of a dilaton field. It is a two-parameter generalization of one-parameter Brans-Dicke gravity in the Einstein frame. We show…

高能物理 - 唯象学 · 物理学 2016-08-03 Girish Kumar Chakravarty , Suratna Das , Gaetano Lambiase , Subhendra Mohanty

Supersymmetric hybrid inflation is an exquisite framework to connect inflationary cosmology to particle physics at the scale of grand unification. Ending in a phase transition associated with spontaneous symmetry breaking, it can naturally…

高能物理 - 唯象学 · 物理学 2014-07-31 Wilfried Buchmuller , Valerie Domcke , Kohei Kamada , Kai Schmitz

BICEP2 observations, interpreted most simply, suggest an era of inflation with energy densities of order ($10^{16}\, {\rm GeV})^4$, not far below the Planck density. However, models of TeV gravity with large extra dimensions might allow a…

高能物理 - 唯象学 · 物理学 2015-06-19 Chiu Man Ho , Stephen D. H. Hsu

Recently a broad class of superconformal inflationary models was found leading to a universal observational prediction $n_s=1-2/N$ and $r=12/N^2$. Here we generalize this class of models by introducing a parameter $\alpha$ inversely…

高能物理 - 理论 · 物理学 2015-06-17 Renata Kallosh , Andrei Linde , Diederik Roest

In conventional scenario of thermal inflation, the requirement that the reheating temperature must be larger than the temperature of the nucleosynthesis puts a lower bound on the mass of the inflaton field. At the same time, the mass of the…

高能物理 - 唯象学 · 物理学 2009-11-10 Tomohiro Matsuda

In this paper, we study two inflationary models, namely, monomial inflation and the simplest $\alpha$-attractor inflation, within extra-dimensional frameworks. We consider three extra-dimensional setups: Dark Dimension, which embeds one…

高能物理 - 唯象学 · 物理学 2026-01-07 Nicolás Bernal , Catarina Cosme , Andrea Donini , Nuria Rius

We propose a realisation of 'new inflation' in supergravity (SUGRA), where the flatness of the inflaton potential is protected by a Heisenberg symmetry. Inflation can be associated with a particle physics phase transition, with the inflaton…

高能物理 - 唯象学 · 物理学 2013-12-04 Stefan Antusch , Francesco Cefala

We analyze the generation of seed magnetic fields during de Sitter inflation considering a non-invariant conformal term in the electromagnetic Lagrangian of the form $-\frac14 I(\phi) F_{\mu \nu} \widetilde{F}^{\mu \nu}$, where $I(\phi)$ is…

天体物理学 · 物理学 2010-01-26 Leonardo Campanelli