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We propose a novel framework where baryon asymmetry can arise due to forbidden decay of dark matter (DM) enabled by finite temperature effects in the early universe. In order to implement it in a realistic setup, we consider the DM to be a…

High Energy Physics - Phenomenology · Physics 2023-09-06 Debasish Borah , Suruj Jyoti Das , Rishav Roshan

The big bang model and the history of the early universe according to the grand unified theories are introduced. The shortcomings of big bang are discussed together with their resolution by inflationary cosmology. Inflation, the subsequent…

High Energy Physics - Phenomenology · Physics 2008-11-26 G. Lazarides

Light scalar fields called moduli arise from a variety of different models involving supersymmetry and/or string theory; thus their existence is a generic prediction of leading theories for physics beyond the standard model. They also…

High Energy Physics - Phenomenology · Physics 2013-05-07 Alexander Kusenko , Michael Loewenstein , Tsutomu T. Yanagida

A variation of Affleck-Dine mechanism was proposed to generate the observed baryon asymmetry in [1], in which the inflaton was assumed to be a complex scalar field with a weakly broken $U(1)$ symmetry, and the baryon asymmetry generation…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-22 Nan Li , Ding-fang Zeng

We propose a consistent scenario of the evolution of the universe based on the large cutoff supergravity (LCSUGRA) hypothesis of supersymmetry breaking, where the gravitino and sfermion become as heavy a $\sim O(1-10 {\rm TeV})$. With such…

High Energy Physics - Phenomenology · Physics 2009-11-11 M. Ibe , Takeo Moroi , T. Yanagida

We claim that the Higgsino-like and wino-like neutralinos can be good dark matter candidates if they are produced by the late time decay of Q-ball, which is generally formed in Affleck-Dine baryogenesis. The late time decays of the Q-balls…

High Energy Physics - Phenomenology · Physics 2008-11-26 Masaaki Fujii , K. Hamaguchi

The abelian Higgs model on the noncommutative plane admits both BPS vortices and non-BPS fluxons. After reviewing the properties of these solitons, we discuss several new aspects of the former. We solve the Bogomoln'yi equations…

High Energy Physics - Theory · Physics 2009-11-07 David Tong

We formulate within Supergravity a model of induced-gravity inflation, excellently consistent with ACT DR6, inspired by the Palatini gravity. The inflaton belongs in the decomposition of a conjugate pair of Higgs superfields which lead to…

High Energy Physics - Phenomenology · Physics 2026-05-26 C. Pallis

We show that a class of Affleck--Dine baryogenesis directly relates the observed mass density of baryons, \Omega_{B}, to that of dark matter, \Omega_{DM}. In this scenario, the ratio of baryon to dark matter mass density is solely…

High Energy Physics - Phenomenology · Physics 2015-06-25 Masaaki Fujii , T. Yanagida

After the Higgs boson discovery, it is established that the Higgs mechanism explains electroweak symmetry breaking and generates the masses of all particles in the Standard Model, with the possible exception of neutrino masses. The…

High Energy Physics - Phenomenology · Physics 2017-01-04 Martin Bauer , Marcela Carena , Katrin Gemmler

We review the notion of the Higgs effect in the context of string theory. We find that by including this effect in time dependent backgrounds, one is led to a natural mechanism for stabilizing moduli at points of enhanced gauge symmetry. We…

High Energy Physics - Theory · Physics 2009-11-10 Scott Watson

We describe a Higgs mechanism for the partially massless graviton. In order to do so, we first construct a covariant fracton-like effective field theory on de Sitter space that linearly realizes a dipolar shift symmetry. The global symmetry…

High Energy Physics - Theory · Physics 2025-07-30 Kurt Hinterbichler , Austin Joyce

Affleck-Dine inflation is a recently proposed model in which a single complex scalar field, nonminimally coupled to gravity, drives inflation and simultaneously generates the baryon asymmetry of universe via Affleck-Dine mechanism. In this…

High Energy Physics - Phenomenology · Physics 2021-04-28 Masahiro Kawasaki , Shusuke Ueda

We revisit the gravitational leptogenesis scenario in which the inflaton is coupled to gravity by the Chern-Simons term and the lepton asymmetry is generated through the gravitational anomaly in the lepton number current during inflation.…

High Energy Physics - Phenomenology · Physics 2020-02-05 Kohei Kamada , Jun'ya Kume , Yusuke Yamada , Jun'ichi Yokoyama

We revisit inflationary cosmology of axion models in the light of recent developments on the inflaton decay in supergravity. We find that all the cosmological difficulties, including gravitino, axino overproduction and axionic isocurvature…

High Energy Physics - Phenomenology · Physics 2008-11-26 Masahiro Kawasaki , Kazunori Nakayama

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 present an inflationary scenario based on a phenomenologically viable model with direct gauge mediation of low-scale supersymmetry breaking. Inflation can occur in the supersymmetry-breaking hidden sector. Although the reheating…

High Energy Physics - Phenomenology · Physics 2011-06-06 Kohei Kamada , Yuichiro Nakai , Manabu Sakai

The Polonyi field is a necessary ingredient in any viable scenario of gravity mediated supersymmetry breaking. However, it is known that the presence of the Polonyi field leads to several serious cosmological problems, which are…

High Energy Physics - Phenomenology · Physics 2015-06-12 Keisuke Harigaya , Masahiro Ibe , Kai Schmitz , Tsutomu T. Yanagida

Axion rotations can simultaneously explain the dark matter abundance and the baryon asymmetry of the Universe by kinetic misalignment and axiogenesis. We consider a scenario in which the Peccei-Quinn symmetry breaking field is as large as…

High Energy Physics - Phenomenology · Physics 2024-09-25 Raymond T. Co , Masaki Yamada

We note that the maximum temperature during reheating can be much greater than the reheating temperature $T_r$ at which the Universe becomes radiation dominated. We show that the Standard Model anomalous $(B+L)$-violating processes can…

High Energy Physics - Phenomenology · Physics 2009-10-31 Sacha Davidson , Marta Losada , Antonio Riotto