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相关论文: Correlated curvature perturbations and magnetogene…

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A sizeable tensor-to-scalar ratio, such as recently claimed by BICEP2, would imply a scale of inflation at the typical scale of supersymmetric grand unification. This could be an accident, or strong support for supersymmetric theories.…

高能物理 - 唯象学 · 物理学 2015-06-19 Felix Brummer , Valerie Domcke , Veronica Sanz

We consider the possibility of inflationary magnetogenesis due to dynamical couplings of the electromagnetic fields to gravity. We find that large primordial magnetic fields can be generated during inflation without the strong coupling…

宇宙学与河外天体物理 · 物理学 2016-02-26 Peng Qian , Zong-Kuan Guo

We propose an alternative implementation of the curvaton mechanism for generating the curvature perturbations which does not rely on a late decaying scalar decoupled from inflation dynamics. In our mechanism the supersymmetric Higgs scalars…

高能物理 - 唯象学 · 物理学 2009-11-07 M. Bastero-Gil , V. Di Clemente , S. F. King

We show that simple strongly coupled supersymmetric gauge theories with quantum moduli spaces can naturally lead to hybrid inflation. These theories contain no input dimensionful or small parameters. The effective superpotential is linear…

高能物理 - 唯象学 · 物理学 2009-10-30 Savas Dimopoulos , Gia Dvali , Riccardo Rattazzi

We present a new general mechanism for generating curvature perturbations after inflation. Our model is based on the simple assumption that a field that starts to oscillate after inflation has a potential characterized by an underlying…

高能物理 - 唯象学 · 物理学 2008-11-26 Tomohiro Matsuda

We consider the gravitational generation of the massive Z-boson field of the standard model, due to the natural breaking of its conformal invariance during inflation. The electroweak symmetry restoration at the end of inflation turns the…

天体物理学 · 物理学 2008-11-26 K. Dimopoulos , T. Prokopec , O. Tornkvist , A. C. Davis

We propose a predictive $SO(10)$ Grand Unified Theory (GUT) framework for cosmic inflation in the Palatini $\mathcal{R}^2$ formulation of gravity. In this model, a GUT Higgs field both drives inflation and induces intermediate-scale…

宇宙学与河外天体物理 · 物理学 2026-03-10 Nilay Bostan , Rafid H. Dejrah , Anish Ghoshal

We explore the generation of large-scale magnetic fields in the so-called moduli inflation. The hypercharge electromagnetic fields couple to not only a scalar field but also a pseudoscalar one, so that the conformal invariance of the…

宇宙学与河外天体物理 · 物理学 2015-06-30 Kazuharu Bamba

The dominant contribution to the primordial curvature perturbation may be generated at the end of inflation. Taking the end of inflation to be sudden, formulas are presented for the spectrum, spectral tilt and non-gaussianity. They are…

天体物理学 · 物理学 2009-11-13 David H. Lyth

While during inflation a phase of increasing gauge coupling allows for a scale-invariant hyperelectric spectrum, when the coupling decreases a flat hypermagnetic spectrum can be generated for typical wavelengths larger than the effective…

广义相对论与量子宇宙学 · 物理学 2021-06-08 Massimo Giovannini

If the conformal invariance of electromagnetism is broken during inflation, then primordial magnetic fields may be produced. If this symmetry breaking is generated by the coupling between electromagnetism and a scalar field---e.g. the…

宇宙学与河外天体物理 · 物理学 2013-05-29 Robert R. Caldwell , Leonardo Motta , Marc Kamionkowski

We investigate the inflationary cosmology involving an SU(5) GUT (grand unified theory) singlet scalar with non-minimal coupling to the Ricci scalar. In this scenario the scale of grand unification is set by the inflaton vev when the…

高能物理 - 唯象学 · 物理学 2023-06-13 Anish Ghoshal , Ahmad Moursy , Qaisar Shafi

The interplay among the possible variation of gauge coupling and the inflationary dynamics is investigated in a simplified toy model. Depending upon various parameters (scalar mass, curvature scale at the end of inflation and at the onset…

天体物理学 · 物理学 2007-05-23 Massimo Giovannini

In order to gain new insights into the gauge field couplings in the early universe, we consider the constraints on gauge field production during inflation imposed by requiring that their effect on the CMB anisotropies are subdominant. In…

宇宙学与河外天体物理 · 物理学 2014-07-14 Sami Nurmi , Martin S. Sloth

It is investigated whether a massive Abelian vector field, whose gauge kinetic function is growing during inflation, can be responsible for the generation of the curvature perturbation in the Universe. Particle production is studied and it…

高能物理 - 唯象学 · 物理学 2008-11-26 Konstantinos Dimopoulos

A variant of hybrid inflation which is applicable in a wide class of supersymmetric grand unified models and reproduces the observed temperature perturbations of cosmic background radiation with natural values of the parameters is…

高能物理 - 唯象学 · 物理学 2009-10-30 G. Lazarides

The evolution of the gauge coupling is modelled using a scalar degree of freedom whose homogeneous and inhomogeneous modes evolve from an ordinary inflationary phase to the subsequent epochs. Depending upon various parameters (scalar mass,…

高能物理 - 唯象学 · 物理学 2007-05-23 Massimo Giovannini

We explore the novel possibility that the inflaton responsible for cosmological inflation is a gauge non-singlet in supersymmetric (SUSY) Grand Unified Theories (GUTs). For definiteness we consider SUSY hybrid inflation where we show that…

高能物理 - 唯象学 · 物理学 2015-03-13 Stefan Antusch , Mar Bastero-Gil , Jochen P. Baumann , Koushik Dutta , Steve F. King , Philipp M. Kostka

Primordial magnetic fields of cosmologically interesting field strengths can be generated from gravitationally coupled electrodynamics during inflation. As the cosmological constraints require this to be power law inflation it is not…

宇宙学与河外天体物理 · 物理学 2013-03-14 Kerstin E. Kunze

Inflationary models with a superheavy scale F-term hybrid inflation followed by an intermediate scale modular inflation are considered. The restrictions on the power spectrum P_R of curvature perturbation and the spectral index n_s from the…

高能物理 - 唯象学 · 物理学 2008-11-26 George Lazarides
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