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Related papers: Accidental Inflation in the Landscape

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Natural inflation relies on the existence of an axion decay constant which is super-Planckian. In string theory only sub-Planckian axion decay constants have been found in any controlled regime. However in field theory it is possible to…

High Energy Physics - Theory · Physics 2015-08-10 Eran Palti

We develop analytic and numerical techniques for studying the statistics of slow-roll inflation in random Gaussian landscapes. As an illustration of these techniques, we analyze small-field inflation in a one-dimensional landscape. We…

High Energy Physics - Theory · Physics 2017-06-14 Ali Masoumi , Alexander Vilenkin , Masaki Yamada

Random, multifield functions can set generic expectations for landscape-style cosmologies. We consider the inflationary implications of a landscape defined by a Gaussian random function, which is perhaps the simplest such scenario. Many key…

High Energy Physics - Theory · Physics 2022-12-21 Lerh Feng Low , Richard Easther , Shaun Hotchkiss

We show that a moduli space of the form predicted by string theory, lifted by supersymmetry breaking, gives rise to successful inflation for large regions of parameter space without any modification or fine tuning. This natural realization…

High Energy Physics - Phenomenology · Physics 2009-11-10 Kenji Kadota , Ewan D. Stewart

We embed natural inflation in an explict string theory model and derive observables in cosmology. We achieve this by compactifying the type IIB string on a Calabi-Yau orientifold, stabilizing moduli via the Large Volume Scenario, and…

High Energy Physics - Theory · Physics 2021-11-17 Stephen Angus , Kang-Sin Choi , Chang Sub Shin

Assuming that inflation happened through a series of tunneling in the string theory landscape, it is argued that one can determine the structure of vacua using precise measurements of the scalar spectral index and tensor perturbations at…

High Energy Physics - Theory · Physics 2010-04-02 Amjad Ashoorioon

Recent developments on large scale string moduli stabilization via non-geometric fluxes are reviewed. In the framework of type IIB orientifolds on fluxed Calabi-Yau manifolds, the existence of so-called flux-scaling minima provides a good…

High Energy Physics - Theory · Physics 2015-10-15 Ralph Blumenhagen , Anamaria Font , Michael Fuchs , Daniela Herschmann , Erik Plauschinn

The discovery of the string theory landscape has recently brought attention to the eternal nature of inflation. In contrast to the common belief that eternal inflation may be a generic feature of most inflationary models, in this note we…

High Energy Physics - Theory · Physics 2007-05-23 L. Mersini-Houghton , L. Parker

We develop a numerical statistical method to study linear cosmological fluctuations in inflationary scenarios with multiple fields, and apply it to an ensemble of six-field inflection point models in string theory. The latter are concrete…

Cosmology and Nongalactic Astrophysics · Physics 2012-07-05 Sébastien Renaux-Petel

In this talk we describe recent progress in construction of inflationary models in the context of string theory with flux compactification and moduli stabilization. We also discuss a possibility to test string theory by cosmological…

High Energy Physics - Theory · Physics 2010-04-06 Renata Kallosh

In the landscape perspective, our Universe begins with a quantum tunneling from an eternally-inflating parent vacuum, followed by a period of slow-roll inflation. We investigate the tunneling process and calculate the probability…

High Energy Physics - Theory · Physics 2017-07-19 Ali Masoumi , Alexander Vilenkin , Masaki Yamada

Open inflation scenario is attracting a renewed interest in the context of string landscape. Since there are a large number of metastable de Sitter vacua in string landscape, tunneling transitions to lower metastable vacua through the…

High Energy Physics - Theory · Physics 2011-09-08 Daisuke Yamauchi , Andrei Linde , Atsushi Naruko , Misao Sasaki , Takahiro Tanaka

Fibre inflationary models are constructed in type-IIB string flux compactification. These models have been shown to be in agreement with the cosmological observations under appropriate choices of parameters, which originate from their…

High Energy Physics - Theory · Physics 2025-09-04 Dibya Chakraborty , Rudnei O. Ramos

We compute the distribution of minima that are reached dynamically on multi-field axionic landscapes, both numerically and analytically. Such landscapes are well suited for inflationary model building due to the presence of shift symmetries…

High Energy Physics - Theory · Physics 2016-04-19 Gaoyuan Wang , Thorsten Battefeld

We study a string theory inspired model for hybrid inflation in the context of a brane-antibrane system partially compactified on a compact submanifold of (a caricature of) a Calabi-Yau manifold. The interbrane distance acts as the…

High Energy Physics - Theory · Physics 2018-02-14 Debajyoti Choudhury , Debashis Ghoshal , Dileep P. Jatkar , Sudhakar Panda

The continuous shift symmetry of axions is at the heart of several realizations of inflationary models. In particular, axion monodromy inflation aims at achieving super-Planckian field ranges for the inflaton in the context of string…

High Energy Physics - Theory · Physics 2014-11-05 Fernando Marchesano , Gary Shiu , Angel M. Uranga

Motivated by the string landscape we examine scenarios for which inflation is a two-step process, with a comparatively short inflationary epoch near the string scale and a longer period at a much lower energy (like the TeV scale). We…

High Energy Physics - Theory · Physics 2009-11-11 C. P. Burgess , Richard Easther , Anupam Mazumdar , David F. Mota , Tuomas Multamaki

In this paper we present an initial exploration of the Calabi-Yau landscape in the context of Kahler moduli inflation. We review how the slow-roll requirement on the scalar potential translates to a geometric constraint on the Kahler…

High Energy Physics - Theory · Physics 2016-11-30 Richard Galvez

This paper represents an in-depth treatment of the chain inflation scenario. We fully determine the evolution of the universe in the model, the necessary conditions in order to have a successful inflationary period, and the matching with…

High Energy Physics - Theory · Physics 2014-11-18 Diego Chialva , Ulf H. Danielsson

An anthropic understanding of the cosmological constant requires that the vacuum energy at late time scans from one patch of the universe to another. If the vacuum energy during inflation also scans, the various patches of the universe…

High Energy Physics - Theory · Physics 2014-11-18 Brian Feldstein , Lawrence J. Hall , Taizan Watari