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Related papers: Dual inflation

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We study the dynamics of a homogeneous, isotropic, and positively curved universe in the presence of a SU(2) gauge field or a triplet of mutually orthogonal vector fields. In the SU(2) case we use the previously known ansatz for the…

General Relativity and Quantum Cosmology · Physics 2021-10-11 Tomoaki Murata , Tsutomu Kobayashi

We consider a non-standard model of gravity coupled to a neutral scalar "inflaton" as well as to SU(2)xU(1) iso-doublet scalar with positive mass squared and without self-interaction, and to SU(2)xU(1) gauge fields. The principal new…

High Energy Physics - Theory · Physics 2016-09-23 Eduardo Guendelman , Emil Nissimov , Svetlana Pacheva

We consider the supersymmetry breaking effects on typical inflation models with different types of K\"ahler potential. The critical size of supersymmetry-breaking scale, above which the flatness of the inflaton potential is spoiled,…

High Energy Physics - Theory · Physics 2015-06-22 Hiroyuki Abe , Shuntaro Aoki , Fuminori Hasegawa , Yusuke Yamada

A new class of gravity-matter model defined with an independent non-Riemannian volume form is studied, in the second order formalism. The action has a global scale invariance symmetry, which can be broken by the equation of motion of the…

General Relativity and Quantum Cosmology · Physics 2019-05-22 David Benisty , Eduardo I. Guendelman

We show that the vacuum expectation value of the inflaton at the Peccei-Quinn axion scale can generate the supersymmetric Higgs mass $\mu$ term. This provides an inflationary simultaneous solution to the strong CP problem and the $\mu$…

High Energy Physics - Phenomenology · Physics 2009-11-10 O. J. Eyton-Williams , S. F. King

High-scale string inflationary models are in well-known tension with low-energy supersymmetry. A promising solution involves models where the inflaton is the volume of the extra dimensions so that the gravitino mass relaxes from large…

High Energy Physics - Theory · Physics 2016-01-20 Michele Cicoli , Francesco Muia , Francisco Gil Pedro

We extend the `topological inflation' of Linde and Vilenkin to {\em unstable} monopoles. This allows the monopole to decay; not inflating eternally, as topological inflation demands. Such a situation happens naturally in some Grand Unified…

High Energy Physics - Phenomenology · Physics 2008-02-03 Nathan F. Lepora , Adrian Martin

We investigate the observational viability of a class of $\alpha$-attractors inflationary models in light of the most recent Cosmic Microwave Background (CMB) and Large-Scale Structure (LSS) data. By considering a double-well potential we…

Cosmology and Nongalactic Astrophysics · Physics 2021-03-04 J. G. Rodrigues , S. Santos da Costa , J. S. Alcaniz

The measurements of the Higgs mass and top Yukawa coupling indicate that we live in a very special Universe, at the edge of the absolute stability of the electroweak vacuum. If fully stable, the Standard Model (SM) can be extended all the…

High Energy Physics - Phenomenology · Physics 2015-10-27 Fedor Bezrukov , Javier Rubio , Mikhail Shaposhnikov

We revisit models of natural inflation and show that the single-field effective theory described by the potential $V(a)\sim \cos\frac{a}{f}$ breaks down as the inflaton $a$ makes large-field excursions, even for values of $f$ smaller than…

High Energy Physics - Theory · Physics 2021-01-13 Mohamed M. Anber , Stephen Baker

A {\it gauge invariant} combination of LLe {\it sleptons} within the Minimal Supersymmetric Standard Model is one of the few inflaton candidates that can naturally explain population of the observable sector and creation of matter after…

High Energy Physics - Phenomenology · Physics 2015-03-19 Rouzbeh Allahverdi , Andrea Ferrantelli , Juan Garcia-Bellido , Anupam Mazumdar

Cosmological inflation gives a natural answer for a variety of cosmological questions, including the horizon problem, the flatness problem, and others. However, inflation yields new questions relating to the flatness of the inflaton…

High Energy Physics - Phenomenology · Physics 2009-11-10 David E. Kaplan , Neal Weiner

We point out some of the outstanding challenges for embedding inflationary cosmology within string theory studying the process of reheating for models where the inflaton is a closed string mode parameterising the size of an internal cycle…

High Energy Physics - Theory · Physics 2011-05-31 Michele Cicoli , Anupam Mazumdar

Strong coupling in Higgs inflation at high energies hinders a joint description of inflation, reheating and low-energy dynamics. The situation may be improved with a proper UV completion of the model. A well-defined self-consistent way is…

High Energy Physics - Phenomenology · Physics 2019-07-17 Fedor Bezrukov , Dmitry Gorbunov , Chris Shepherd , Anna Tokareva

We consider F-term hybrid inflation and supersymmetry breaking in the context of a model which largely respects a global U(1) R symmetry. The Kaehler potential parameterizes the Kaehler manifold with an enhanced U(1)_Rx(SU(1,1)/U(1))…

High Energy Physics - Phenomenology · Physics 2025-04-04 C. Pallis

In this paper we demand that a successfull inflationary scenario should follow from a model entirely motivated by particle physics considerations. We show that such a connection is indeed possible within the framework of concrete…

High Energy Physics - Phenomenology · Physics 2009-10-30 Gia Dvali , Antonio Riotto

In scalaron-Higgs inflation the Standard Model Higgs boson is non-minimally coupled to gravity and the Einstein-Hilbert action is supplemented by the quadratic scalar curvature invariant. For the quartic Higgs self-coupling $\lambda$ fixed…

High Energy Physics - Theory · Physics 2019-12-12 Anirudh Gundhi , Christian F. Steinwachs

We consider general linear Higgs-sigma models as ultra-violet completions of the Higgs inflation. We introduce general higher curvature terms beyond Einstein gravity and recast them into a class of linear Higgs-sigma models in the…

High Energy Physics - Phenomenology · Physics 2021-08-17 Hyun Min Lee , Adriana G. Menkara

Motivated by trans-Planckian issues in inflation, we determine the Hilbert space and amplitudes of quantum perturbations in the general low-energy effective theory of (multi-)field inflation without relying on the sub-horizon limit. The…

High Energy Physics - Theory · Physics 2026-05-29 Andrea Ambrosi de Magistris , Alberto Salvio

We discuss inflationary cosmology in a five dimensional SO(10) model compactified on $S^1/(Z_2\times Z_2')$, which yields $SU(3)_c\times SU(2)_L\times U(1)_Y\times U(1)_X$ below the compactification scale. The gauge symmetry $SU(5)\times…

High Energy Physics - Phenomenology · Physics 2014-11-17 Bumseok Kyae , Qaisar Shafi