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Related papers: Flavored axion-monodromy inflation

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Axion inflation entails a coupling of the inflaton field to gauge fields through the Chern-Simons term. This results in a strong gauge field production during inflation, which backreacts on the inflaton equation of motion. Here we show that…

Cosmology and Nongalactic Astrophysics · Physics 2020-08-13 Valerie Domcke , Veronica Guidetti , Yvette Welling , Alexander Westphal

We study the production of fermions through a derivative coupling with a pseudoscalar inflaton and the effects of the produced fermions on the scalar primordial perturbations. We present analytic results for the modification of the scalar…

Cosmology and Nongalactic Astrophysics · Physics 2019-11-18 Peter Adshead , Lauren Pearce , Marco Peloso , Michael A. Roberts , Lorenzo Sorbo

In a previous paper, the standard model was generalized to include an electroweak axion which carries baryon plus lepton number, $B+L$. It was shown that such a model naturally gives the observed value of the dark energy, if the scale of…

High Energy Physics - Phenomenology · Physics 2015-06-23 Larry McLerran

We propose an extra-dimension framework on the orbifold $S^1/Z_2$ for understanding the origin of the fermion mass and mixing hierarchies. Introducing the flavor symmetry $G_F(=${\it non-Abelian}$\times${\it Abelian}) as well as the extra…

High Energy Physics - Phenomenology · Physics 2022-11-09 Y. H. Ahn , Sin Kyu Kang , Hyun Min Lee

The inflationary paradigm has enjoyed phenomenological success, however, a compelling particle physics realization is still lacking. The key obstruction is that the requirement of a suitably flat scalar potential is sensitive to…

High Energy Physics - Phenomenology · Physics 2011-05-12 Neil Barnaby , Marco Peloso

We investigate the quantum fluctuations of an inflaton field in a two-field model of one-bubble open inflation. One of the inflatons is assumed to be responsible for the first false vacuum stage of inflation and the other is assumed to be…

Astrophysics · Physics 2009-10-09 Misao Sasaki , Takahiro Tanaka

We study string inspired two-field models of large-field inflation based on axion monodromy in the presence of an interacting heavier modulus. This class of models has enough structure to approximate at least part of the backreaction…

High Energy Physics - Theory · Physics 2020-02-12 Francisco G. Pedro , Alexander Westphal

In warm inflation models there is the requirement of generating large dissipative couplings of the inflaton with radiation, while at the same time, not de-stabilising the flatness of the inflaton potential due to radiative corrections. One…

High Energy Physics - Phenomenology · Physics 2015-05-28 Hiranmaya Mishra , Subhendra Mohanty , Akhilesh Nautiyal

We explore the possibility of obtaining inflation in weakly coupled heterotic string theory, where the model dependent axions are responsible for driving inflation. This model can be considered as a certain extrapolation of…

High Energy Physics - Theory · Physics 2010-10-27 Martin E. Olsson

Models of axion inflation based on a single cosine potential require the axion decay constant $f$ to be super-Planckian in size. However, $f > M_{Pl}$ is disfavored by the Weak Gravity Conjecture (WGC). It is then pertinent to ask if one…

High Energy Physics - Phenomenology · Physics 2019-06-10 Pran Nath , Maksim Piskunov

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…

Cosmology and Nongalactic Astrophysics · Physics 2023-03-21 Ema Dimastrogiovanni , Matteo Fasiello , Martino Michelotti , Lucas Pinol

In this work, we show the effect of the non-minimal coupling $\xi \phi^2 R$ on the inflationary parameters by considering the single-field inflation and present the inflationary predictions of the appealing potential for the particle…

Cosmology and Nongalactic Astrophysics · Physics 2023-03-03 Nilay Bostan

We develop a supersymmetric bi-axion model of high-scale inflation coupled to supergravity, in which the axionic structure originates from, and is protected by, gauge symmetry in an extra dimension. While local supersymmetry (SUSY) is…

High Energy Physics - Phenomenology · Physics 2021-07-01 Kaustubh Deshpande , Raman Sundrum

Many models of dark matter QCD axion requires inflation at a scale $H_{\text{inf}} \lesssim 10^{6}$~GeV and hence does not allow for a detectable tensor mode fluctuation. This is because the domain wall problem forces the Peccei--Quinn…

High Energy Physics - Phenomenology · Physics 2025-12-11 Dan Kondo , Hitoshi Murayama

We consider dynamical models of supersymmetry breaking which naturally incorporate cosmological inflation. The inflaton plays an inevitable role in dynamical SUSY breaking and the hierarchical scales of inflation and SUSY breaking are…

High Energy Physics - Phenomenology · Physics 2009-10-30 K. -I. Izawa

We discuss model building in tribrid inflation, which is a framework for realising inflation in the matter sector of supersymmetric particle physics models. The inflaton is a D-flat combination of matter fields, and inflation ends by a…

High Energy Physics - Phenomenology · Physics 2013-10-16 Stefan Antusch , David Nolde

It is shown that, in the context of split supersymmetry, a simple model with a single complex scalar field can produce chaotic inflation and generate the observed amount of baryon asymmetry via the Affleck-Dine mechanism. While the inflaton…

High Energy Physics - Phenomenology · Physics 2009-11-06 Yeo-Yie Charng , Da-Shin Lee , Chung Ngoc Leung , Kin-Wang Ng

We study an extension of the natural inflation model comprising a non-Abelian gauge sector coupled to the axion-inflaton kinetic term. We show how such non-minimal coupling serves as a source of friction for the rolling inflaton granting…

Cosmology and Nongalactic Astrophysics · Physics 2024-12-02 Martino Michelotti , Rodrigo Gonzalez Quaglia , Ema Dimastrogiovanni , Matteo Fasiello , Diederik Roest

We show that a supersymmetric axion model naturally induces a hybrid inflation with the waterfall field identified as a Peccei-Quinn scalar. The Peccei-Quinn scale is predicted to be around 10^{15}GeV for reproducing the large-scale density…

High Energy Physics - Phenomenology · Physics 2011-02-02 Masahiro Kawasaki , Naoya Kitajima , Kazunori Nakayama

We consider an inflationary model in the hidden-sector broken supergravity with an effectively large cutoff. The inflaton decay into right-handed neutrinos naturally causes the observed baryon asymmetry of the universe with a reheating…

High Energy Physics - Phenomenology · Physics 2009-11-11 M. Ibe , K. -I. Izawa , Y. Shinbara , T. T. Yanagida