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Scalar fields in the minimal supersymmetric standard model may have large field values during inflation. Because of approximate global symmetry, it is plausible that the phase directions of them are nearly massless during inflation and…

High Energy Physics - Phenomenology · Physics 2020-12-30 Keisuke Harigaya , Masaki Yamada

The nonminimal coupling (NMC) of the scalar field to the Ricci curvature is unavoidable in many cosmological scenarios. Inflation and quintessence models based on nonminimally coupled scalar fields are studied, with particular attention to…

General Relativity and Quantum Cosmology · Physics 2008-11-26 Valerio Faraoni

The possibility to have an infinite open inflationary universe inside a bubble of a finite size is one of the most interesting realizations extensively discussed in the literature. The original idea was based on the theory of tunneling and…

Astrophysics · Physics 2009-09-29 Andrei Linde , Misao Sasaki , Takahiro Tanaka

We present a model where the inflaton can naturally account for all the dark matter in the Universe within the warm inflation paradigm. In particular, we show that the symmetries of the Warm Little Inflaton scenario (i) avoid large thermal…

High Energy Physics - Phenomenology · Physics 2019-05-10 Joao G. Rosa , Luis B. Ventura

Within the framework of the Minimal Supersymmetric Standard Model (MSSM), we explore a decoupling of the parameters into separate sectors that determine consistency with collider data, the abundance of dark matter, and potential signatures…

High Energy Physics - Phenomenology · Physics 2016-07-27 Pearl Sandick

The minimal gauge group extension to the standard model (SM) by the local $U(1)_{B-L}$ (MBLSM) is well known as the minimal model to understand neutrino mass origins via the seesaw mechanism, following the gauge principle. This "small"…

High Energy Physics - Phenomenology · Physics 2018-08-22 Chengfeng Cai , Zhaofeng Kang , Hong-Hao Zhang , Yupan Zeng

The existence of dark matter provides compelling evidence for physics beyond the Standard Model. Minimal extensions of the Standard Model with additional scalars or fermions allow to explain the observed dark matter relic density in an…

High Energy Physics - Phenomenology · Physics 2014-08-27 M. Klasen

We investigate the production of non-thermal fermionic dark matter particles during the reheating era following slow roll inflation, driven by inflaton $\varphi$ non-minimally coupled to the curvature scalar, $\mathcal{R}$. Two types of…

High Energy Physics - Phenomenology · Physics 2025-04-03 Anish Ghoshal , Maxim Yu. Khlopov , Zygmunt Lalak , Shiladitya Porey

We consider the modified gravity non-minimally coupled with matter Lagrangian for the description of early-time and late-time universe. Such $F(R)$ ($F(G)$) gravity in the absence of non-minimal coupling is viable theory which passes the…

High Energy Physics - Theory · Physics 2008-11-26 Shin'ichi Nojiri , Sergei D. Odintsov , Petr V. Tretyakov

Dark matter and cosmic inflation represent two of the major puzzles in cosmology. They are typically addressed by introducing separate fields with independent dynamics. On the other hand, extra dimensions might play an important role for…

High Energy Physics - Phenomenology · Physics 2023-10-23 Hansel Gordillo-Ruiz , Cesar Morales-Mena , Saul Ramos-Sanchez

The minimal warm inflation model was constructed as a warm inflation setup with direct interaction between inflaton and (non-Abelian) gauge fields. The model was shown to be compatible with observation for some forms of potential. As a…

General Relativity and Quantum Cosmology · Physics 2021-11-24 Vahid Kamali , Hossein Moshafi , Saeid Ebrahimi

It is very much intriguing if the Planck scale $M_{\rm{Pl}}$ is not a fundamental parameter. The Brans-Dicke gravity is nothing but the theory where the Planck scale $M_{\rm{Pl}}$ is indeed an illusional parameter. The theory predicts a…

High Energy Physics - Phenomenology · Physics 2026-02-10 Muzi Hong , Kyohei Mukaida , Tsutomu T. Yanagida

The $\beta$-exponential inflation is driven by a class of primordial potentials, derived in the framework of braneworld scenarios, that generalizes the well-known power law inflation. In this paper we update previous constraints on the…

Cosmology and Nongalactic Astrophysics · Physics 2022-06-23 Felipe Bruno Medeiros dos Santos , Simony Santos da Costa , Raimundo Silva , Micol Benetti , Jailson Alcaniz

The radiative neutrino mass model with inert doublet dark matter is a promising model for the present experimental issues which cannot be explained within the standard model. We study an extension of this model focusing on cosmological…

High Energy Physics - Phenomenology · Physics 2016-02-05 Romy H. S. Budhi , Shoichi Kashiwase , Daijiro Suematsu

The Conformal Standard Model (CSM) is a minimal extension of the Standard Model of Particle Physics based on the assumed absence of large intermediate scales between the TeV scale and the Planck scale, which incorporates only right-chiral…

High Energy Physics - Phenomenology · Physics 2018-03-07 Adrian Lewandowski , Krzysztof A. Meissner , Hermann Nicolai

If cosmic inflation was driven by an electrically neutral scalar field stable on cosmological time scales, the field necessarily constitutes all or part of dark matter (DM). We study this possibility in a scenario where the inflaton field…

High Energy Physics - Phenomenology · Physics 2019-03-13 Juan P. Beltrán Almeida , Nicolás Bernal , Javier Rubio , Tommi Tenkanen

A cosmological model with total density close to critical (and flat geometry), dominated by dark matter and dark energy of unknown nature, and consistent with the basic predictions of the inflationary scenario is a very good fit to a…

Astrophysics · Physics 2007-05-23 A. Balbi

Inert Doublet Model (IDM) is a minimal extension of the Standard Model with the second scalar doublet that may provide a Dark Matter candidate. In this paper we consider the different variants of the evolution of the Universe after…

High Energy Physics - Phenomenology · Physics 2016-02-03 Maria Krawczyk , Dorota Sokolowska

Constraints on inflationary models typically assume only the standard models of cosmology and particle physics. By extending the neutrino sector to include a new interaction with a light scalar mediator ($m_{\phi}\sim$MeV), it is possible…

Cosmology and Nongalactic Astrophysics · Physics 2019-04-18 Gabriela Barenboim , Peter B. Denton , Isabel M. Oldengott

After the observation in 2012 of a new scalar particle closely resembling the Higgs boson of the Standard Model of particle physics, there is a general consensus that there must be Physics Beyond the Standard Model, with present experiments…

High Energy Physics - Phenomenology · Physics 2025-09-24 Rafael Boto
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