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The simplest explanation for early time acceleration (inflation) and the late time acceleration indicated by recent data is that they have a common origin. We investigate another generic cosmological implication of this possiblity, that the…

High Energy Physics - Phenomenology · Physics 2009-11-07 Antonio De Felice , Salah Nasri , Mark Trodden

The thermal inflation is the most plausible mechanism that solves the cosmological moduli problem naturally. We discuss relic abundance of superheavy particle $X$ in the presence of the thermal inflation assuming that its lifetime is longer…

High Energy Physics - Phenomenology · Physics 2009-10-31 T. Asaka , M. Kawasaki , T. Yanagida

A minimal extension of the standard model to naturally generate small neutrino masses and provide a dark matter candidate is proposed. The dark matter particle is part of a new scalar doublet field that plays a crucial role in radiatively…

High Energy Physics - Phenomenology · Physics 2014-07-03 Michael Gustafsson , Jose Miguel No , Maximiliano A. Rivera

We present a unified theory of inflation, neutrino mass, baryogenesis and dark matter where global lepton number symmetry and its breaking play a crucial role. The basic idea is to use a lepton number carrying complex scalar field as the…

High Energy Physics - Phenomenology · Physics 2022-03-14 Rabindra N. Mohapatra , Nobuchika Okada

Cosmological production of scalar, non-minimally coupled dark matter depends on the specifics of the inflationary model under consideration. We analyze both Starobinsky inflation and a quadratic potential, solve the full background…

General Relativity and Quantum Cosmology · Physics 2026-02-24 Jose A. R. Cembranos , Luis J. Garay , Álvaro Parra-López , Javier Ortega del Río

In a unified picture both inflation and present dynamical dark energy arise from the same scalar field. The history of the Universe describes a crossover from a scale invariant "past fixed point" where all particles are massless, to a…

High Energy Physics - Theory · Physics 2015-12-09 C. Wetterich

Quintessential inflation provides a unified description of the early and late accelerated phases of the Universe, linking the inflationary epoch to the present-day dark energy-dominated era through a single scalar degree of freedom. In this…

Cosmology and Nongalactic Astrophysics · Physics 2026-02-25 Jamerson Rodrigues , Gabriel Rodrigues , Felipe B. M. dos Santos , Simony Santos da Costa , Jailson Alcaniz

We present a scalar triplet extension of the standard model to unify the origin of inflation with neutrino mass, asymmetric dark matter and leptogenesis. In presence of non-minimal couplings to gravity the scalar triplet, mixed with the…

High Energy Physics - Phenomenology · Physics 2015-06-05 Chiara Arina , Jinn-Ouk Gong , Narendra Sahu

In this talk I begin with a brief review of the status of approaches to understanding the origin of the baryon asymmetry of the universe (BAU). I then describe a recent model unifying three seemingly-distict problems facing particle…

High Energy Physics - Phenomenology · Physics 2008-11-26 Mark Trodden

Recent observations of the cosmic microwave background (CMB) and baryon acoustic oscillations (BAO) show some tension with a $\Lambda$CDM cosmology. For one, the cosmological parameters determined by the CMB are at odds with the expansion…

Cosmology and Nongalactic Astrophysics · Physics 2026-02-23 Peter W. Graham , Daniel Green , Joel Meyers

This study reviews the advances made in inflationary theory, especially regarding the seeming disparity between inflation energy and dark energy, and their significance to cosmic evolution as a whole. I attempt to connect the two sources of…

General Relativity and Quantum Cosmology · Physics 2018-12-17 Anantya Bhatnagar

Cosmological and astrophysical observations suggest that both energy densities of baryon and dark matter take the same order values in the present Universe. We propose a scenario to give an answer for this problem in a scotogenic model and…

High Energy Physics - Phenomenology · Physics 2024-05-29 Daijiro Suematsu

In this work, we explain three beyond standard model (BSM) phenomena, namely neutrino masses, the baryon asymmetry of the Universe and Dark Matter, within a single model and in each explanation the right handed (RH) neutrinos play the prime…

High Energy Physics - Phenomenology · Physics 2019-06-26 Anirban Biswas , Sandhya Choubey , Laura Covi , Sarif Khan

Over the past three years we have determined the basic features of our Universe. It is spatially flat; accelerating; comprised of 1/3 a new form of matter, 2/3 a new form of energy, with some ordinary matter and a dash of massive neutrinos;…

Astrophysics · Physics 2008-11-26 Michael S. Turner

We study a seesaw-type extension of the Standard Model in which the symmetry group is enlarged by a global U(1). We introduce adequate scalar and fermion representations which naturally explain the smallness of neutrino masses. With the…

High Energy Physics - Phenomenology · Physics 2011-12-19 François-Xavier Josse-Michaux , Emiliano Molinaro

The observational evidence for the inflationary cosmology with baryosynthesis and dark matter/energy can be viewed as the messenger for new physics, which governed the Universe origin, evolution and structure. To specify the physics beyond…

High Energy Physics - Phenomenology · Physics 2021-02-03 Maxim Yu. Khlopov

We show that warm inflation can be realized within a minimal extension of the Standard Model with three right-handed neutrinos, three complex scalars and a gauged lepton/B-L U(1) symmetry. This simple model can address all the shortcomings…

High Energy Physics - Phenomenology · Physics 2022-01-05 Miguel Levy , João G. Rosa , Luis B. Ventura

We propose that the baryon asymmetry of the Universe may originate from the amplification of quantum fluctuations of a light complex scalar field during inflation. CP-violation is sourced by complex mass terms, which are smaller than the…

Astrophysics · Physics 2008-12-18 Bjorn Garbrecht , Tomislav Prokopec

We apply non-invertible selection rules coming from a fusion algebra to radiative neutrino mass models where fields are labeled by the elements in the algebra. Since non-invertible selection rules only hold at tree level, radiative…

High Energy Physics - Phenomenology · Physics 2025-12-17 Tatsuo Kobayashi , Hiroshi Okada , Hajime Otsuka

We show that spontaneous breaking of global $B-L$ symmetry responsible for small neutrino masses via the seesaw mechanism provides a unified picture of hybrid inflation and dark matter if the scale of $B-L$ breaking is close to the GUT…

High Energy Physics - Phenomenology · Physics 2009-11-10 D. Kazanas , R. N. Mohapatra , S. Nasri , V. L. Teplitz