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Related papers: F_D-Term Hybrid Inflation with Electroweak-Scale L…

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Considering hybrid F-term inflation in RSII model and using the most recent data from Planck 2018 and in comparison with Planck 2015and WMAP 9-year , we can obtain some interesting constraints on main parameters of the model. Also, we…

General Relativity and Quantum Cosmology · Physics 2018-08-22 M. Roostaee , Amir M. Abbassi

A sizeable tensor-to-scalar ratio, such as recently claimed by BICEP2, would imply a scale of inflation at the typical scale of supersymmetric grand unification. This could be an accident, or strong support for supersymmetric theories.…

High Energy Physics - Phenomenology · Physics 2015-06-19 Felix Brummer , Valerie Domcke , Veronica Sanz

We consider the construction of inverted hybrid inflation models in which the vacuum energy during inflation is at the TeV scale, and the inflaton couples to the Higgs field. Such models are of interest in the context of some recently…

High Energy Physics - Phenomenology · Physics 2009-11-07 Edmund J. Copeland , David Lyth , Arttu Rajantie , Mark Trodden

In sneutrino hybrid inflation the superpartner of one of the right-handed neutrinos involved in the seesaw mechanism plays the role of the inflaton field. It obtains its large mass after the "waterfall" phase transition which ends hybrid…

High Energy Physics - Phenomenology · Physics 2010-10-27 Stefan Antusch , Jochen P. Baumann , Valerie F. Domcke , Philipp M. Kostka

We use present cosmological data from the cosmic microwave background, large-scale structure and deuterium at high redshifts to constrain supersymmetric F- and D-term hybrid inflation scenarios including possible contributions to the CMB…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-20 Richard Battye , Bjorn Garbrecht , Adam Moss

We propose a variant of hybrid inflation which is applicable in a wide class of supersymmetric grand unified models. The observed temperature perturbations of cosmic background radiation can be reproduced with natural values of the…

High Energy Physics - Phenomenology · Physics 2019-08-15 G. Lazarides , C. Panagiotakopoulos

We argue that the mass of the inflaton can be much smaller than the Hubble constant in supergravity models in which inflation is driven by D--terms and not F--terms. We investigate a supergravity toy model which leads to hybrid inflation…

High Energy Physics - Phenomenology · Physics 2009-10-28 Edi Halyo

Comparisons of cosmological models to current data show that the presence of a non-trivial feature in the primordial power spectrum of fluctuations, around the scale k=0.05 h/Mpc, is an open and exciting possibility, testable in a near…

High Energy Physics - Phenomenology · Physics 2009-10-31 Julien Lesgourgues

Inflation, as currently understood, requires the presence of fields with very flat potentials. Supersymmetric models in which supersymmetry breaking is communicated by supergravity naturally yield such fields, but the scales are typically…

High Energy Physics - Phenomenology · Physics 2009-10-30 Michael Dine , Antonio Riotto

We show that Supersymmetric models with Type I seesaw neutrino masses support slow roll inflection point inflation. The inflaton is the D-flat direction labelled by the chiral invariant HLN composed of the Higgs(H), slepton(L) and conjugate…

High Energy Physics - Phenomenology · Physics 2015-06-11 Charanjit S. Aulakh

We consider supersymmetric inflation models in which inflation occurs at an intermediate scale and which provide a solution to the $\mu$ problem and the strong CP problem. Such models are particularly attractive since inflation,…

High Energy Physics - Phenomenology · Physics 2008-11-26 G. L. Kane , S. F. King

Recently a new model of "Affleck-Dine inflation" was presented, that produces the baryon asymmetry from a complex inflaton carrying baryon number, while being consistent with constraints from the cosmic microwave background. We adapt this…

High Energy Physics - Phenomenology · Physics 2020-06-24 James M. Cline , Matteo Puel , Takashi Toma

We study the consistency of hybrid inflation and moduli stabilization, using the Kallosh--Linde model as an example for the latter. We find that F-term hybrid inflation is not viable since inflationary trajectories are destabilized by…

High Energy Physics - Theory · Physics 2015-06-17 Wilfried Buchmuller , Valerie Domcke , Clemens Wieck

Inflation ends with the formation of a Bose condensate of inflatons. We show that in hybrid inflation models this condensate is typically unstable with respect to spatial perturbations and can fragment to condensate lumps. The case of…

High Energy Physics - Phenomenology · Physics 2009-11-07 John McDonald

The onset of inflation in hybrid models require fine tuning in the initial conditions. The inflaton field should have an initial value close to the Planck scale $M_{P}$, whereas the auxiliary "orthogonal" field must be close to zero with an…

High Energy Physics - Phenomenology · Physics 2009-11-07 Zurab Berezhiani , Anupam Mazumdar , Abdel Pérez-Lorenzana

We consider the well motivated model of the (standard) supersymmetric F-term hybrid inflation (FHI) which can be realized close to the grand unification scale. The predicted scalar spectral index $n_s$ cannot be smaller than 0.98 and can…

High Energy Physics - Phenomenology · Physics 2015-05-13 C. Pallis

We study a minimal scenario to realize non-thermal leptogenesis and UV freeze-in of a Standard Model (SM) gauge singlet fermionic dark matter (DM) simultaneously, with inflaton field playing a non-trivial role in their yields. The…

High Energy Physics - Phenomenology · Physics 2021-09-01 Basabendu Barman , Debasish Borah , Rishav Roshan

We consider D-term hybrid inflation in the framework of superconformal supergravity. In part of the parameter space, inflation continues for subcritical inflaton field value. Consequently, a new type of inflation emerges, which gives…

Cosmology and Nongalactic Astrophysics · Physics 2018-06-04 Koji Ishiwata

We present a concrete supersymmetric grand unified model based on the Pati-Salam gauge group SU(4)_c x SU(2)_L x SU(2)_R and leading naturally to smooth hybrid inflation, which avoids the cosmological disaster encountered in the standard…

High Energy Physics - Phenomenology · Physics 2008-11-26 R. Jeannerot , S. Khalil , G. Lazarides

We propose a model of inflation based on a simple variant of the NMSSM, called $\phi$NMSSM where the additional singlet $\phi$ plays the role of the inflaton in hybrid (or inverted hybrid) type models. The $\phi$NMSSM solves the $\mu$…

High Energy Physics - Phenomenology · Physics 2009-10-31 M. Bastero-Gil , S. F. King
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