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Neutrino masses and quantum gravity are strong reasons to extend the standard model of particle physics. A large extra dimension can be motivated by quantum gravity and can explain the small neutrino masses with new singlet states that…

High Energy Physics - Phenomenology · Physics 2024-10-08 David McKeen , John Ng , Michael Shamma

Dark matter and inflation are two key elements to understand the origin of cosmic structures in modern cosmology, and yet their exact physical models remain largely uncertain. The Weyl scaling invariant theory of gravity may provide a…

High Energy Physics - Phenomenology · Physics 2022-07-08 Qing-Yang Wang , Yong Tang , Yue-Liang Wu

The quintessence field coupled to the cosmic neutrino background (CNB) has been widely discussed as an alternative mechanism to address the coincidence problem. As it is well known, it is possible to extend such models to obtain…

Cosmology and Nongalactic Astrophysics · Physics 2021-04-01 Zurab Kepuladze , Michael Maziashvili

We present a TeV scale model for leptogenesis where the origin of neutrino masses are independent of the scale of leptogenesis. As a result, the model could be extended to explain {\it dark matter, neutrino masses and leptogenesis at the…

High Energy Physics - Phenomenology · Physics 2008-11-26 Narendra Sahu

We propose an extension of the standard model (SM) by two SU(2) triplet scalars and an inert SU(2) doublet. We demonstrate that this setup can simultaneously produce an inflaton and baryon asymmetry in the early universe, provide a dark…

High Energy Physics - Phenomenology · Physics 2025-10-09 Sin Kyu Kang , Raymundo Ramos

We study a simple extension of the standard model to simultaneously explain neutrino masses, dark matter and the matter-antimatter asymmetry of the Universe. In our model, the baryon asymmetry is achieved by the leptogenesis mechanism,…

High Energy Physics - Phenomenology · Physics 2010-03-26 Chuan-Hung Chen , Chao-Qiang Geng , Dmitry V. Zhuridov

We investigate whether interaction between massive neutrinos and quintessence scalar field is the origin of the late time accelerated expansion of the universe. We present explicit formulas of the cosmological linear perturbation theory in…

High Energy Physics - Phenomenology · Physics 2009-09-01 Kiyotomo Ichiki , Yong-Yeon Keum

We consider a simple extension of the Standard Model to consistently explain the observation of a peak in the galactic X-ray spectrum at 3.55 keV and the light neutrino masses along with the baryon asymmetry of the universe. The baryon…

High Energy Physics - Phenomenology · Physics 2018-01-17 Sin Kyu Kang , Ayon Patra

We consider the mechanism of thermal leptogenesis at the TeV scale in the context of an extension of the Standard Model with 4 generations and the inclusion of four right-handed Majorana neutrinos. We obtain a value for the baryon asymmetry…

High Energy Physics - Phenomenology · Physics 2016-09-06 Asmaa Abada , Habib Aissaoui , Marta Losada

Origin of baryon asymmetry is studied in the framework of extra dimensional approach. Baryon excess production and the symmetrization of extra-space are performed simultaneously. Baryon number is conserved long after the inflationary stage…

General Relativity and Quantum Cosmology · Physics 2013-12-09 A. V. Grobov , S. G. Rubin

A simple TeV scale model for baryon and lepton number violation is presented, where neutrino mass arises via a one-loop radiative seesaw effect and B-violation obeys $\Delta B=2$ selection rule. The stability of proton is connected to the…

High Energy Physics - Phenomenology · Physics 2015-07-29 P. S. Bhupal Dev , Rabindra N. Mohapatra

The $super$-$weak$ force combines three simple extensions of the Standard Model, one in gauge sector, one in fermion sector and one in scalar sector. Each of these extensions are well motivated by their rich phenomenology. Combined to a…

High Energy Physics - Phenomenology · Physics 2021-11-16 Timo J. Kärkkäinen , Zoltán Trócsányi

We propose a unified setup for dark matter, inflation and baryon asymmetry generation through the neutrino mass seesaw mechanism. Our scenario emerges naturally from an extended gauge group containing $B-L$ as a non-commutative symmetry,…

High Energy Physics - Phenomenology · Physics 2019-04-03 P. V. Dong , D. T. Huong , Daniel A. Camargo , Farinaldo S. Queiroz , José W. F. Valle

Neutrino physics is going through a revolutionary progress. In this talk I review what we have learned and why neutrino mass is so important. Neutrino masses and mixings are already shedding new insight into the origin of flavor. Given the…

High Energy Physics - Phenomenology · Physics 2009-09-29 Hitoshi Murayama

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

The asymmetric dark matter scenario is known to give an interesting solution for the cosmic coincidence problem between baryon and dark matter densities. In the scenario, the dark matter asymmetry, which is translated to the dark matter…

High Energy Physics - Phenomenology · Physics 2015-05-27 Naoyuki Haba , Shigeki Matsumoto , Ryosuke Sato

We suggest a minimal extension of the standard model, which can explain current experimental data of the dark matter, small neutrino masses and baryon asymmetry of the universe, inflation, and dark energy, and achieve gauge coupling…

High Energy Physics - Phenomenology · Physics 2015-06-17 Naoyuki Haba , Kunio Kaneta , Ryo Takahashi

A brief review is made of some of the experimental signatures that may be associated to a certain class of extensions of the standard model. The material of these lectures is divided into two sections. After briefly sketching the present…

High Energy Physics - Phenomenology · Physics 2016-09-01 José W. F. Valle

The basic workings of inflationary models are summarized, along with the arguments that strongly suggest that our universe is the product of inflation. I describe the quantum origin of density perturbations, giving a heuristic derivation of…

Astrophysics · Physics 2007-05-23 Alan H. Guth

We review the current standard model for the evolution of the Universe from an early inflationary epoch to the complex hierarchy of structure seen today. We summarize and provide key references for the following topics: observations of the…

Astrophysics · Physics 2009-06-23 Bharat Ratra , Michael S. Vogeley