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Related papers: Inflation caused by a potential valley with CP vio…

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We consider the dynamics of power-law inflation with a nonminimally coupled scalar field $\phi$. It is well known that multiple scalar fields with exponential potentials $V(\phi)=V_0 {\rm exp}(-\sqrt{16\pi/p m_{\rm pl}^2} \phi)$ lead to an…

High Energy Physics - Phenomenology · Physics 2009-10-31 S. Tsujikawa

CP violation and the violation of baryon-minus-lepton number B-L do not necessarily have to occur simultaneously in order to accomplish successful leptogenesis. Instead, it suffices if new CP-violating interactions at high energies result…

High Energy Physics - Phenomenology · Physics 2023-02-07 Valerie Domcke , Kohei Kamada , Kyohei Mukaida , Kai Schmitz , Masaki Yamada

In the vanilla type-I seesaw leptogenesis scenario, CP violation required to generate the lepton asymmetries in the heavy Majorana neutrino decays stem from complex Dirac-type Yukawa couplings. In this paper we explore the case in which…

High Energy Physics - Phenomenology · Physics 2023-01-25 D. M. Barreiros , H. B. Câmara , R. G. Felipe , F. R. Joaquim

We propose a model for combining the Standard Model (SM) with gravity. It relies on a non-minimal coupling of the Higgs field to the Ricci scalar and on the Palatini formulation of gravity. Without introducing any new degrees of freedom in…

High Energy Physics - Theory · Physics 2021-05-31 Mikhail Shaposhnikov , Andrey Shkerin , Sebastian Zell

We explore the dynamics and observational predictions of the Warm Little Inflaton scenario, presently the simplest realization of warm inflation within a concrete quantum field theory construction. We consider three distinct types of scalar…

Cosmology and Nongalactic Astrophysics · Physics 2018-10-10 Mar Bastero-Gil , Arjun Berera , Rafael Hernandez-Jimenez , Joao G. Rosa

We explore the inflationary phase of a scalar field with a kinetic term non-minimally coupled to gravity. We find that one of the slow-roll conditions is naturally consequence of the equation of motion of the scalar field. Thus, slow-roll…

Cosmology and Nongalactic Astrophysics · Physics 2014-09-16 Amir Ghalee

We investigate for viable models of inflation that can successfully produce dark matter (DM) from inflaton decay process, satisfying all the constraints from Cosmic Microwave Background (CMB) and from some other observations. In particular,…

High Energy Physics - Phenomenology · Physics 2022-10-19 Anish Ghoshal , Gaetano Lambiase , Supratik Pal , Arnab Paul , Shiladitya Porey

Inflation can occur in the cores of topological defects, where the scalar field is forced to stay near the maximum of its potential. This topological inflation does not require fine-tuning of the initial conditions.

High Energy Physics - Theory · Physics 2010-11-01 Alexander Vilenkin

We consider the introduction of a complex scalar field carrying a global lepton number charge to the Standard Model and the Higgs inflation framework. The conditions are investigated under which this model can simultaneously ensure Higgs…

High Energy Physics - Phenomenology · Physics 2020-11-10 Neil D. Barrie , Akio Sugamoto , Tatsu Takeuchi , Kimiko Yamashita

We examine whether F-term supersymmetric hybrid inflation can be embedded within the minimal SO(10) model, in a natural way. We show that none of the singlets of the Standard Model symmetries in the minimal set of SO(10) representations can…

High Energy Physics - Phenomenology · Physics 2015-06-16 Giacomo Cacciapaglia , Mairi Sakellariadou

We suggest a new type of hill-top inflation originating from the initial conditions in the form of the microcanonical density matrix for the cosmological model with a large number of quantum fields conformally coupled to gravity. Initial…

High Energy Physics - Theory · Physics 2016-01-27 A. O. Barvinsky , A. Yu. Kamenshchik , D. V. Nesterov

We present a unified model where the same scalar field can drive inflation and account for the present dark matter abundance. This scenario is based on the incomplete decay of the inflaton field into right-handed neutrino pairs, which is…

High Energy Physics - Phenomenology · Physics 2025-02-14 Antonio Torres Manso , Joao G. Rosa

We propose a new class of inflationary models in which inflation takes place while the inflaton is climbing up a potential hill due to a coupling to gravity. We study their attractor behavior, and investigate its relation with known…

High Energy Physics - Phenomenology · Physics 2017-08-30 Ryusuke Jinno , Kunio Kaneta

The necessary complex structures needed for CP violation are not easy to generate and, indeed, CP can be a symmetry in higher dimensional theories. In 4-dimensions CP violation argues for the existence of a scalar sector and, in its…

High Energy Physics - Phenomenology · Physics 2007-05-23 R. D. Peccei

The inclusion of two triplet scalars in the Standard Model (SM) enables to accommodate neutrino mass generation as well as baryogenesis through leptogenesis. One of the essential ingredients of leptogenesis is the violation of charge…

High Energy Physics - Phenomenology · Physics 2024-07-17 Sreerupa Chongdar , Sasmita Mishra

Warm Inflation seems to be the most befitting single-field slow-roll inflation scenario in the context of the recently proposed Swampland Criteria. We investigate the constraints these Swampland Criteria impose on Warm Inflation parameters…

High Energy Physics - Theory · Physics 2019-03-27 Suratna Das

Attention has been recently drawn towards models in which inflation and quintessence schemes are unified. In such `quintessential inflation' models, a unique scalar field is required to play both the role of the inflaton and of the…

High Energy Physics - Phenomenology · Physics 2016-09-06 Marco Peloso , Francesca Rosati

We propose a model of inflation driven by minimal extension of SUSY, commonly known as MSSM. Starting from gauge invariant flat directions in the n = 4 level comprising of QQQL,QuQd,QuLe and uude, we construct the inflaton potential and…

High Energy Physics - Phenomenology · Physics 2012-04-19 Sayantan Choudhury , Supratik Pal

During hybrid inflation, the slowly-rolling inflaton field has a significant coupling to the trigger field which is responsible for most of the potential. Barring a fine-tuned accidental cancellation, this coupling induces a minimal…

High Energy Physics - Phenomenology · Physics 2009-10-31 David H Lyth

We present a new inflation model in which the inflationary scenario including subsequent reheating is determined in part by a U(1)_R\times Z_n symmetry. A preinflation epoch can be introduced to yield, among other things, a running spectral…

High Energy Physics - Phenomenology · Physics 2008-11-26 V. N. Senoguz , Q. Shafi
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