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Related papers: Comments on SUSY inflation models on the brane

200 papers

In this paper, we study two inflationary models, namely, monomial inflation and the simplest $\alpha$-attractor inflation, within extra-dimensional frameworks. We consider three extra-dimensional setups: Dark Dimension, which embeds one…

High Energy Physics - Phenomenology · Physics 2026-01-07 Nicolás Bernal , Catarina Cosme , Andrea Donini , Nuria Rius

In this paper we quantise scalar perturbations in a Randall-Sundrum-type model of inflation where the inflaton field is confined to a single brane embedded in five-dimensional anti-de Sitter space-time. In the high energy regime,…

High Energy Physics - Theory · Physics 2010-10-27 Kazuya Koyama , Andrew Mennim , V. A. Rubakov , David Wands , Takashi Hiramatsu

"Brane supersymmetry breaking" occurs in String Theory when the only available combinations of D-branes and orientifolds are not mutually BPS and yet do not introduce tree-level tachyon instabilities. It is characterized by the emergence of…

High Energy Physics - Theory · Physics 2015-06-18 N. Kitazawa , A. Sagnotti

Motivated by recent cosmological observations of a possibly unsuppressed primordial tensor component $r$ of inflationary perturbations, we reanalyse in detail the 5D conformal SUGRA originated natural inflation model of Ref. [1]. The model…

High Energy Physics - Phenomenology · Physics 2015-07-15 Filipe Paccetti Correia , Michael G. Schmidt , Zurab Tavartkiladze

It was pointed out that brane-anti-brane inflation without warped geometry is not viable due to compactification effects (in the simplified scenario where the inflaton is decoupled from the compactification moduli). We show that the…

High Energy Physics - Theory · Physics 2009-11-10 Sarah Shandera , Benjamin Shlaer , Horace Stoica , S. -H. Henry Tye

We consider higher-dimensional uniform inflation, in which the extra dimensions expand at the same rate as three-dimensional non-compact space during inflation. We compute the cosmological perturbation in $D+4$ dimensions and derive the…

High Energy Physics - Phenomenology · Physics 2025-01-24 Takuya Hirose

We consider a supersymmetric (SUSY) Grand Unified Theory (GUT) based on the gauge group G_PS=SU(4)_C x SU(2)_L x SU(2)_R, which incorporates non-minimal chaotic inflation, driven by a quartic potential associated with the Higgs fields…

High Energy Physics - Phenomenology · Physics 2011-12-06 C. Pallis , N. Toumbas

The effect of including a Gauss-Bonnet contribution in the bulk action is investigated within the context of the steep inflationary scenario. When inflation is driven by an exponential inflaton field, this Gauss-Bonnet term allows the…

Astrophysics · Physics 2009-11-07 James E. Lidsey , N. J. Nunes

We propose the unified models of cosmological inflation, spontaneous SUSY breaking, and the dark energy (de Sitter vacuum) in $N=1$ supergravity with the dilaton-axion chiral superfield $T$ in the presence of an $N=1$ vector multiplet with…

High Energy Physics - Theory · Physics 2019-08-28 Yermek Aldabergenov , Auttakit Chatrabhuti , Sergei V. Ketov

We consider DBI inflation with a quadratic potential and the effect of trapped branes on the inflationary fluctuations. When going through a trapped brane the effective potential of the inflaton receives a contribution whose effect is to…

High Energy Physics - Theory · Physics 2011-03-09 Philippe Brax , Emeline Cluzel

We present a new mechanism for slow-roll inflation based on higher dimensional supersymmetric gauge theory compactified to four dimensions with twisted (supersymmetry breaking) boundary conditions. These boundary conditions lead to a…

High Energy Physics - Theory · Physics 2011-01-27 Joshua L. Davis , Thomas S. Levi , Mark Van Raamsdonk , Kevin R. L. Whyte

We discuss string corrections to the effective potential in various models of brane inflation. These corrections contribute to the mass of the inflaton candidate and may improve its slow-roll properties. In particular, in orientifold string…

High Energy Physics - Theory · Physics 2007-05-23 Marcus Berg , Michael Haack , Boris Kors

The potential during inflation must be very flat in, at least, the direction of the inflaton. In renormalizable global supersymmetry, flat directions are ubiquitous, but they are not preserved in a generic supergravity theory. It is known…

High Energy Physics - Theory · Physics 2009-09-29 Mary K. Gaillard , David H. Lyth , Hitoshi Murayama

In their minimal form both supersymmetric and smooth hybrid inflation yield a scalar spectral index n_s close to 0.98, to be contrasted with the result n_s=0.951+0.015-0.019 from WMAP3. To realize better agreement, following hep-ph/0604198,…

High Energy Physics - Phenomenology · Physics 2008-11-26 Mansoor ur Rehman , V. N. Senoguz , Qaisar Shafi

We consider a class of well motivated supersymmetric models of F-term hybrid inflation (FHI) which can be linked to the supersymmetric grand unification. The predicted scalar spectral index n_s cannot be smaller than 0.97 and can exceed…

High Energy Physics - Phenomenology · Physics 2010-01-26 C. Pallis

We discuss a supersymmetric version of DBI (Dirac-Born-Infeld) inflation, which is a typical inflation model in string cosmology. The supersymmetric DBI action together with a superpotential always leads to correction terms associated with…

High Energy Physics - Theory · Physics 2015-06-05 Shin Sasaki , Masahide Yamaguchi , Daisuke Yokoyama

We investigate in the context of brane inflation the possibility of additional light scalar fields generating significant power spectrum and non-Gaussianities at the end of inflation affecting the CMB scale observations. We consider the…

High Energy Physics - Theory · Physics 2008-11-26 Heng-Yu Chen , Jinn-Ouk Gong , Gary Shiu

We examine a non-Abelian SUSY $SU(2) \times U(1)$ gauge theory and a SUSY U(1) theory originally used to investigate the microphysics of cosmic strings in supersymmetric theories. We show that both theories automatically include hybrid…

High Energy Physics - Phenomenology · Physics 2009-10-31 A. C. Davis , M. Majumdar

We study a gravitational model with curvature-squared $R^2$ and curvature-quartic $R^4$ nonlinearities. The effective scalar degree of freedom $\phi$ (scalaron) has a multi-valued potential $U(\phi)$ consisting of a number of branches.…

High Energy Physics - Theory · Physics 2014-11-20 Tamerlan Saidov , Alexander Zhuk

A Randall-Sundrum type brane-cosmological model in which slow-roll inflation on the brane is driven solely by a bulk scalar field was recently proposed by Himemoto and Sasaki. We analyze their model in detail and calculate the quantum…

General Relativity and Quantum Cosmology · Physics 2009-10-09 Norichika Sago , Yoshiaki Himemoto , Misao Sasaki