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We study cosmological solutions in the dilatonic brane world models. The effective four-dimensional equations on the brane are analyzed for the models with one positive tension brane and two branes with tensions of opposite signs. Just as…

High Energy Physics - Theory · Physics 2009-10-31 Donam Youm

In Gauss-Bonnet braneworld cosmology, the Friedmann equation of our four-dimensional universe on 3-brane is modified in a high energy regime (Gauss-Bonnet regime), while the standard expansion law is reproduced in low energies (standard…

High Energy Physics - Phenomenology · Physics 2009-07-30 Nobuchika Okada , Satomi Okada

We present supersymmetric scenarios with gravitino LSP and stau NLSP in the case of a non-standard model of cosmology with the addition of a dark component in the pre-BBN era. In the context of the standard model of cosmology, gravitino LSP…

High Energy Physics - Phenomenology · Physics 2011-03-24 Sean Bailly

Gravity is so different from other fundamental forces that it is now essentially treated as a non-fundamental force of entropic origin. A number of good studies have been carried out in this direction. Quantum gravity has also significantly…

General Relativity and Quantum Cosmology · Physics 2020-12-11 M. Hameeda , Q. Gani , B. Pourhassan , M. C. Rocca

We consider hybrid inflation in the braneworld scenario. In particular, we consider inflation in global supersymmetry with the D-terms in the scalar potential for the inflaton field to be the dominant ones (D-term inflation). We find that…

High Energy Physics - Phenomenology · Physics 2009-11-11 G. Panotopoulos

An improved version of the well-known Peebles-Vilenkin model unifying early inflationary era to current cosmic acceleration, is introduced in order to match with the theoretical values of the spectral quantities provided by it with the…

General Relativity and Quantum Cosmology · Physics 2019-01-16 Jaume Haro , Weiqiang Yang , Supriya Pan

We propose the possibility that compact extra dimensions can obtain large size by higher dimensional inflation, relating the weakness of the actual gravitational force to the size of the observable universe. Solution to the horizon problem…

High Energy Physics - Phenomenology · Physics 2024-06-26 Luis A. Anchordoqui , Ignatios Antoniadis

It is known that gravitinos are non-thermally produced in inflaton decay processes, which excludes many inflation models for a wide range of the gravitino mass. We find that the constraints from the gravitino overproduction can be greatly…

High Energy Physics - Phenomenology · Physics 2015-06-11 Kazunori Nakayama , Fuminobu Takahashi , Tsutomu T. Yanagida

We investigate the cosmological moduli problem by studying a modulus decay in detail and find that the branching ratio of the gravitino production is generically of O(0.01-1), which causes another cosmological disaster. Consequently, the…

High Energy Physics - Phenomenology · Physics 2008-11-26 Motoi Endo , Koichi Hamaguchi , Fuminobu Takahashi

We conducted an investigation into Affleck-Dine baryogenesis within the context of D-term inflation, specifically focusing on its relationship with a recent reheating formalism. It was found that by considering a specific reheating…

High Energy Physics - Phenomenology · Physics 2023-07-31 K. El Bourakadi , M. Ferricha-Alami , Z. Sakhi , M. Bennai , H. Chakir

We reconsidered leptogenesis scenario from right-handed (s)neutrino produced by the decay of inflaton. Besides the well-investigated case that the neutrino decays instantaneously after the production, leptogenesis is possible if neutrino…

High Energy Physics - Phenomenology · Physics 2010-04-30 Masato Senami , Tsutomu Takayama

Affleck-Dine baryogenesis in models where the gravitino is both the lightest supersymmetric particle and the dark matter candidate is investigated. For a high enough reheating temperature to produce sufficient gravitinos by thermal…

High Energy Physics - Phenomenology · Physics 2009-11-11 Osamu Seto

We show that the gravitino-overproduction problem is prevalent among inflation models in supergravity. An inflaton field \phi generically acquires (effective) non-vanishing auxiliary field G_\phi, if the K\"ahler potential is non-minimal.…

High Energy Physics - Phenomenology · Physics 2009-11-11 Masahiro Kawasaki , Fuminobu Takahashi , T. T. Yanagida

We review recent attempts to address the cosmological constant problem and the late-time acceleration of the Universe based on braneworld models. In braneworld models, the way in which the vacuum energy gravitates in the 4D spacetime is…

Astrophysics · Physics 2009-06-23 Kazuya Koyama

We study the cosmological consequences of generic scalar fields like moduli which decay only through gravitationally suppressed interactions. We consider a new production mechanism of gravitinos from moduli decay, which might be more…

High Energy Physics - Phenomenology · Physics 2009-11-10 Kazunori Kohri , Masahiro Yamaguchi , Jun'ichi Yokoyama

The decays of massive gravitinos into neutralino dark matter particles and Standard Model secondaries during or after Big-Bang nucleosynthesis (BBN) may alter the primordial light-element abundances. We present here details of a new suite…

Cosmology and Nongalactic Astrophysics · Physics 2011-04-08 Richard H. Cyburt , John Ellis , Brian D. Fields , Feng Luo , Keith A. Olive , Vassilis C. Spanos

We consider the conditions for the decay products of perturbative inflaton decay to thermalize. The importance of considering the full spectrum of inflaton decay products in the thermalization process is emphasized. It is shown that the…

High Energy Physics - Phenomenology · Physics 2009-10-31 John McDonald

Gravitons are described by the propagator in Teleparallel gravity in nearly flat space-time. Finite temperature is introduced by using Thermo Field Dynamics formalism. The Gravitational Casimir effect and Stefan-Boltzmann law are calculated…

High Energy Physics - Theory · Physics 2019-04-02 S. C. Ulhoa , A. F. Santos , T. F. Furtado , F. C. Khanna

A successful implementation of thermal leptogenesis requires the re-heat temperature after inflation T_R to exceed ~2\times 10^9 GeV. Such a high T_R value typically leads to an overproduction of gravitinos in the early universe, which will…

High Energy Physics - Phenomenology · Physics 2015-05-20 Howard Baer , Sabine Kraml , Andre Lessa , Sezen Sekmen

In this article we study a constant-roll inflationary model in the context of brane-world cosmology caused by a quintessence scalar field for warm inflation with a constant dissipative parameter Q =$\Gamma$/3H. We determine the analytical…

General Relativity and Quantum Cosmology · Physics 2022-01-11 Mohammad Reza Setare , Arvin Ravanpak , Karam Bahari , Golnaz Farpour Fadakar
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