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Related papers: Moduli and Monopoles

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Typically the moduli fields acquire mass m =C H in the early universe, which shifts the position of the minimum of their effective potential and leads to an excessively large energy density of the oscillating moduli fields at the later…

High Energy Physics - Theory · Physics 2009-09-29 Andrei Linde

We estimate the abundance of the coherent oscillation of moduli, which linearly couple to matter fields through higher dimensional operators. During the (p)reheating after inflation, matter particles are efficiently produced and it can…

High Energy Physics - Phenomenology · Physics 2019-03-18 Daisuke Hagihara , Koichi Hamaguchi , Kazunori Nakayama

Moduli fields are generally present in superstring--inspired models. They are typically characterized by masses of the order of the supersymmetry breaking scale and by interactions of gravitational strength to ordinary matter. If stable,…

High Energy Physics - Phenomenology · Physics 2009-11-07 Marco Peloso , Lorenzo Sorbo

Moduli with flat or run-away classical potentials are generic in theories based on supersymmetry and extra dimensions. They mix between themselves and with matter fields in kinetic terms and in the nonperturbative superpotentials. As the…

High Energy Physics - Theory · Physics 2010-11-03 Zygmunt Lalak

Thermal fluctuations of the gauge field lead to monopole formation at the grand unified phase transition in the early Universe, even if the transition is merely a smooth crossover. The dependence of the produced monopole density on various…

High Energy Physics - Phenomenology · Physics 2007-05-23 A. Rajantie

We discuss effects of cosmological moduli fields on the cosmic microwave background (CMB). If a modulus field \phi once dominates the universe, the CMB we observe today is from the decay of \phi and its anisotropy is affected by the…

High Energy Physics - Phenomenology · Physics 2008-11-26 Takeo Moroi , Tomo Takahashi

In theories beyond the Standard Model, in particular in theories with extra spatial dimensions such as superstring theory, there are a large number of scalar fields which appear in the low energy effective action. These moduli fields must…

High Energy Physics - Theory · Physics 2021-09-29 Mesbah Alsarraj , Robert Brandenberger

We investigate effects of the radiation and the moduli oscillation around the stabilized values on the evolution of a 6-dimensional spacetime compactified on $S^2$. In order to see the transition from the 5-dimensional space to the…

High Energy Physics - Theory · Physics 2023-06-14 Hajime Otsuka , Yutaka Sakamura

Cosmological models arising from a generalized compactification of Einstein gravity are derived. It is shown that a redefinition of the moduli fields reduces the system to a set of massless fields and a single field with a single…

Astrophysics · Physics 2009-10-31 Anne M. Green , James E. Lidsey

We investigate the applicability of the moduli space approximation in theories with unbroken non-Abelian gauge symmetries. Such theories have massless magnetic monopoles that are manifested at the classical level as clouds of non-Abelian…

High Energy Physics - Theory · Physics 2009-11-07 Xingang Chen , Huidong Guo , Erick J. Weinberg

In gravity mediated models and in particular in models with strongly stabilized moduli, there is a natural hierarchy between gaugino masses, the gravitino mass and moduli masses: $m_{1/2} \ll m_{3/2} \ll m_{\phi}$. Given this hierarchy, we…

High Energy Physics - Phenomenology · Physics 2015-06-17 Jason L. Evans , Marcos A. G. Garcia , Keith A. Olive

We discuss effects of cosmological moduli fields on the cosmic microwave background (CMB). If a modulus field \phi once dominates the universe, the CMB we observe today is from the decay of \phi and its anisotropy is affected by the…

High Energy Physics - Phenomenology · Physics 2007-05-23 Takeo Moroi , Tomo Takahashi

An exploratory study of the cosmology of moduli in string theory. Moduli are argued to be natural inflaton fields and lead to a robust inflationary cosmology in which inflation takes place at the top of domain walls. The amplitude of…

High Energy Physics - Theory · Physics 2016-09-06 T. Banks , M. Berkooz , G. Moore , S. H. Shenker , P. J. Steinhardt

A scenario which overcomes the well-known cosmological overshoot problem associated with stabilizing moduli with steep potentials in string theory is proposed. Our proposal relies on the fact that moduli potentials are very steep and that…

High Energy Physics - Theory · Physics 2008-11-26 R. Brustein , S. P. de Alwis , P. Martens

It is shown that the coherent field oscillation of moduli fields with weak or TeV scale masses can dissipate its energy efficiently if they have a derivative coupling to standard bosonic fields in a thermal state. This mechanism may provide…

High Energy Physics - Phenomenology · Physics 2008-11-26 Jun'ichi Yokoyama

Magnetic monopole solutions naturally arise in the context of spontaneously broken gauge theories. When the unbroken symmetry includes a non-Abelian subgroup, investigation of the low-energy monopole dynamics by means of the moduli space…

High Energy Physics - Theory · Physics 2007-05-23 Erick J. Weinberg

We show that, contrary to the standard belief, primordial monopoles expand exponentially during inflation in the new inflationary universe scenario. Moreover, inflation of monopoles continues without an end even when inflation ends in the…

Astrophysics · Physics 2009-09-29 Andrei Linde

In this talk I shall try to give an elementary introduction to certain areas of mathematical physics where the idea of moduli space is used to help solve problems or to further our understanding. In the wide area of gauge theory, I shall…

High Energy Physics - Theory · Physics 2007-05-23 ST Tsou

We study the cosmological evolution of the volume moduli in a class of recently proposed Inflationary Universe models arising out of Type IIB string theory, where a number of the moduli fields have been stabilised through flux…

High Energy Physics - Phenomenology · Physics 2013-05-29 T. Barreiro , B. de Carlos , E. J. Copeland , N. J. Nunes

Existing theoretical and observational constraints on the abundance of magnetic monopoles are limited. Here we demonstrate that an ensemble of monopoles forms a plasma whose properties are well determined and whose collective effects place…

Cosmology and Nongalactic Astrophysics · Physics 2017-07-05 Mikhail V. Medvedev , Abraham Loeb
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