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相关论文: Inflation Assisted by Heterotic Axions

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Protecting the inflationary potential from quantum corrections typically requires symmetries that constrain the form of couplings of the inflaton to other sectors. We will explore how these restrictions affect reheating in models with UV…

高能物理 - 理论 · 物理学 2008-11-26 Daniel Green

I investigate multi-field inflationary models with fields that decay during inflation, leading to staggered inflation. This feature is natural in many models motivated by string theory, for instance if inflatons are related to interbrane…

天体物理学 · 物理学 2010-01-08 Thorsten Battefeld

Axion fluctuations generated during inflation lead to isocurvature and non-Gaussian temperature fluctuations in the cosmic microwave background radiation. Following a previous analysis for the model independent string axion we consider the…

高能物理 - 理论 · 物理学 2008-11-26 Ben Kain

The spectrum of primordial gravitational waves is one of the most robust inflationary observables, often thought of as a direct probe of the energy scale of inflation. We present a simple model, where the dynamics controlling this…

高能物理 - 理论 · 物理学 2017-12-13 Federico Piazza , David Pirtskhalava , Riccardo Rattazzi , Olivier Simon

This paper is based on a talk in which I discussed how a component of the dynamical affine connection, that is independent of the metric, can drive inflation in agreement with observations. This provides a geometrical origin for the…

高能物理 - 唯象学 · 物理学 2023-11-07 Alberto Salvio

We study an inflationary model developed by Kaloper and Sorbo, in which the inflaton is an axion with a sub-Planckian decay constant, whose potential is generated by mixing with a topological 4-form field strength. This gives a 4d…

高能物理 - 理论 · 物理学 2011-03-18 Nemanja Kaloper , Albion Lawrence , Lorenzo Sorbo

We derive inflation from M-theory on S^1/Z_2 via the non-perturbative dynamics of N M5-branes. The open membrane instanton interactions between the M5-branes give rise to exponential potentials which are too steep for inflation individually…

高能物理 - 理论 · 物理学 2008-11-26 Katrin Becker , Melanie Becker , Axel Krause

A systematic analysis of possibilities for realizing single-field F-term axion monodromy inflation via the flux-induced superpotential in type IIB string theory is performed. In this well-defined setting the conditions arising from moduli…

高能物理 - 理论 · 物理学 2015-01-14 Ralph Blumenhagen , Daniela Herschmann , Erik Plauschinn

In models of natural inflation, the inflaton is an axion-like particle. Unfortunately, axion potentials in UV-complete theories appear to be too steep to drive inflation. We show that, even for a steep potential, natural inflation can occur…

高能物理 - 理论 · 物理学 2015-05-14 Mohamed M. Anber , Lorenzo Sorbo

The electric Weak Gravity Conjecture demands that axions with large decay constant $f$ couple to light instantons. The resulting large instantonic corrections pose problems for natural inflation. We explore an alternative argument based on…

高能物理 - 理论 · 物理学 2017-04-26 Arthur Hebecker , Philipp Henkenjohann , Lukas T. Witkowski

We consider inflation driven by an axion-like particle coupled to an SU(2) gauge sector via a Chern-Simons term. Known as chromo-natural inflation, this scenario is in tension with CMB observations. In order to remedy this fact and preserve…

宇宙学与河外天体物理 · 物理学 2023-03-21 Ema Dimastrogiovanni , Matteo Fasiello , Martino Michelotti , Lucas Pinol

The original axion natural inflation model predicts a tensor-to-scalar ratio exceeding experimental limits. Conversely, in aligned axion inflation, inflation can proceed along trajectories emerging from near a saddle point of the two-field…

宇宙学与河外天体物理 · 物理学 2025-10-21 Federico Greco

We provide a pedagogical overview of inflation in string theory. Our theme is the sensitivity of inflation to Planck-scale physics, which we argue provides both the primary motivation and the central theoretical challenge for the subject.…

高能物理 - 理论 · 物理学 2009-12-15 Daniel Baumann , Liam McAllister

We consider the spectrum of primordial fluctuations produced by inflationary models where the inflaton potential is the sum of two exponential terms. A wide range of spectra result, with the only constraint being that the scalar spectrum…

天体物理学 · 物理学 2009-09-25 Richard Easther

We study a particular supersymmetric realization of the Peccei-Quinn symmetry which provides a suitable candidate for the curvaton field. The class of models considered also solves the mu problem, while generating the Peccei-Quinn scale…

高能物理 - 唯象学 · 物理学 2008-11-26 K. Dimopoulos , G. Lazarides

We propose an inflationary scenario, M-flation, in which inflation is driven by three $N\times N$ hermitian matrices $\Phi_i, i=1,2,3$. The inflation potential of our model, which is strongly motivated from string theory, is constructed…

高能物理 - 理论 · 物理学 2010-10-13 Amjad Ashoorioon , Hassan Firouzjahi , M. M. Sheikh-Jabbari

In the simplest inflationary model $V=\frac12 m^2\phi^2$, we provide a prediction accurate up to $1\%$ for the spectral index $n_s$ and the tensor-to-scalar ratio $r$ assuming instantaneous reheating and a standard thermal history: $n_s =…

宇宙学与河外天体物理 · 物理学 2014-10-22 Paolo Creminelli , Diana López Nacir , Marko Simonović , Gabriele Trevisan , Matias Zaldarriaga

We study the inflation scenarios, in the framework of superstring theory, where the inflaton is an axion producing the adiabatic curvature perturbations while there exists another light axion producing the isocurvature perturbations. We…

高能物理 - 唯象学 · 物理学 2016-02-03 Kenji Kadota , Tatsuo Kobayashi , Hajime Otsuka

In this talk, I shall focus on theories beyond the Standard Model which predict massive neutrinos. Hybrid inflation emerges naturally in these theories: the slow-rolling inflaton field is a gauge singlet which couples with a GUT Higgs field…

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

Recent models of axion monodromy inflation in string theory link the inflationary potential and the moduli stabilization potential. Realistic inflationary models require mechanisms to moderately suppress the inflaton mass with respect to…

高能物理 - 理论 · 物理学 2015-06-19 Sebastian Franco , Daniele Galloni , Ander Retolaza , Angel Uranga