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A quantum field theory warm inflation model is presented that solves the horizon/flatness problems. The model obtains, from the elementary dynamics of particle physics, cosmological scale factor trajectories that begin in a radiation…

High Energy Physics - Phenomenology · Physics 2008-11-26 Arjun Berera , Marcelo Gleiser , Rudnei O. Ramos

We investigate an inflation model with the inflaton being identified with a Higgs boson responsible for the breaking of U(1)B-L symmetry. We show that supersymmetry must remain a good symmetry at scales one order of magnitude below the…

High Energy Physics - Phenomenology · Physics 2012-03-13 Kazunori Nakayama , Fuminobu Takahashi

In the framework of superstring compactifications with N=1 supersymmetry spontaneously broken, (by either geometrical fluxes, branes or else), we show the existence of new inflationary solutions. The time-trajectory of the scale factor of…

High Energy Physics - Theory · Physics 2008-11-26 Costas Kounnas , Herve Partouche

We study models of modular inflation of the form expected to arise from low energy effective actions of superstring theories. We argue on general grounds that the most likely models of modular slow-roll inflation are small field models in…

High Energy Physics - Theory · Physics 2009-12-15 Ido Ben-Dayan , Ram Brustein , Senarath P. de Alwis

Tribrid inflation is a class of supersymmetric inflation models where the scalar component of a matter superfield, or a $D$-flat direction of matter fields, drives inflation. Similar to Hybrid inflation, the end of inflation is reached when…

High Energy Physics - Phenomenology · Physics 2024-11-06 Stefan Antusch , Katarina Trailović

We probe the cosmological consequences of a recently proposed class of solutions to the cosmological constant problem. In these models, the universe undergoes a long period of inflation followed by a contraction and a bounce that sets the…

High Energy Physics - Phenomenology · Physics 2022-01-27 Lingyuan Ji , David E. Kaplan , Surjeet Rajendran , Erwin H. Tanin

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

The shortcomings of the Standard Big Bang Cosmological Model as well as their resolution in the context of inflationary cosmology are discussed. The inflationary scenario and the subsequent oscillation and decay of the inflaton field are…

High Energy Physics - Phenomenology · Physics 2007-05-23 G. Lazarides

We investigate the possibility of preheating in hybrid inflation. This scenario involves at least two scalar fields, the inflaton field $\phi$, and the symmetry breaking field $\sigma$. We found that the behavior of these fields after…

High Energy Physics - Phenomenology · Physics 2009-09-29 Juan Garcia-Bellido , Andrei Linde

The dilaton field in string theories (if exists) is expected to have a mass of the order of the gravitino mass $m_{3/2}$ which is in a range of $10^{-2}$keV--1GeV in gauge-mediated supersymmetry breaking models. If it is the case, the…

High Energy Physics - Phenomenology · Physics 2009-10-30 J. Hashiba , M. Kawasaki , T. Yanagida

The generic expectation in string/supergravity models is that there are multiple moduli fields with masses of the order of the supersymmetry breaking scale. We study the cosmology that arises as a result of vacuum misalignment of these…

High Energy Physics - Theory · Physics 2020-01-23 Bobby S. Acharya , Mansi Dhuria , Diptimoy Ghosh , Anshuman Maharana , Francesco Muia

We argue that strong dynamics at the Planck scale can solve the cosmological moduli problem. We discuss its implications for inflation models, and find that a certain type of multi-field inflation model is required for this mechanism to…

High Energy Physics - Phenomenology · Physics 2011-02-24 Fuminobu Takahashi , Tsutomu T. Yanagida

We study the cosmological inflation and reheating in a teleparallel model of gravity. Reheating is assumed to be due to the decay of a scalar field to radiation during its rapid oscillation. By using cosmological perturbations during…

General Physics · Physics 2019-07-26 P. Goodarzi , H. Mohseni Sadjadi

Starting from an initial classical four dimensional flat background of the heterotic or type II superstrings, we are able to determine at the string one-loop level the quantum corrections to the effective potential due to the spontaneous…

High Energy Physics - Theory · Physics 2010-05-12 Francois Bourliot , Costas Kounnas , Herve Partouche

The theory of reheating of the Universe after inflation is developed. The transition from inflation to the hot Universe turns out to be strongly model-dependent and typically consists of several stages. Immediately after inflation the field…

High Energy Physics - Theory · Physics 2009-09-29 Lev Kofman , Andrei Linde , Alexei Starobinsky

A quantum field theory warm inflation model is presented that solves the cosmological horizon/flatness problems. An interpretation of the model is given from supersymmetry and superstring theory.

High Energy Physics - Phenomenology · Physics 2009-10-31 Arjun Berera

We conduct a systematic search for a viable string/M-theory cosmology, focusing on cosmologies that include an era of slow-roll inflation, after which the moduli are stabilized and the Universe is in a state with an acceptably small…

High Energy Physics - Theory · Physics 2009-11-07 R. Brustein , S. P. de Alwis , E. G. Novak

We provide a taxonomy of dynamical supersymmetry breaking theories, and discuss the cosmological implications of the various types of models. Models in which supersymmetry breaking is produced by chiral superfields which only have…

High Energy Physics - Phenomenology · Physics 2008-11-26 Tom Banks , David B. Kaplan , Ann E. Nelson

In supergravity, the dynamics of the sgoldstino -- superpartner of the goldstino superfield associated with the breaking of supersymmetry at low energy -- can substantially modify the dynamics of inflation in the primordial Universe.…

High Energy Physics - Theory · Physics 2023-03-15 Lucien Heurtier , Ahmad Moursy , Lucien Wacquez

We investigate moduli field dynamics in supergravity/M-theory like set ups where we turn on fluxes along some or all of the extra dimensions. As has been argued in the context of string theory, we observe that the fluxes tend to stabilize…

High Energy Physics - Theory · Physics 2008-11-26 Tirthabir Biswas , Prashanth Jaikumar
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