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We propose a new baryogenesis scenario based on coherent production and mixing of different fermionic species. The mechanism is operative during phase transitions, at which the fermions acquire masses via Yukawa couplings to scalar fields.…

High Energy Physics - Phenomenology · Physics 2009-11-10 Bjorn Garbrecht , Tomislav Prokopec , Michael G. Schmidt

We investigate the baryon asymmetry in the supersymmetry Dine-Fischler-Srednicki-Zhitnitsky axion model without R-parity. It turns out that the R-parity violating terms economically explain the atmospheric mass-squared difference of…

High Energy Physics - Phenomenology · Physics 2019-04-03 Kensuke Akita , Hajime Otsuka

Radiation domination at the electroweak epoch is a simplifying assumption, but one for which there is no observational basis. Treating the expansion rate as a variable, I re-examine electroweak baryogenesis in various scenarios. At a first…

High Energy Physics - Phenomenology · Physics 2007-05-23 Michael Joyce

We study the conditions for successful Affleck-Dine baryogenesis and the origin of gravitino dark matter in GMSB models. AD baryogenesis in GMSB models is ruled out by neutron star stability unless Q-balls are unstable and decay before…

High Energy Physics - Phenomenology · Physics 2011-06-09 Francesca Doddato , John McDonald

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 perform a detailed analysis on Affleck-Dine leptogenesis taking into account the thermal effects on the dynamics of the flat direction field $\phi$. We find that an extremely small mass for the lightest neutrino $\nu_1$, ${m_\nu}_1\lsim…

High Energy Physics - Phenomenology · Physics 2009-10-31 T. Asaka , Masaaki Fujii , K. Hamaguchi , T. Yanagida

We present a non-supersymmetric mechanism for baryogenesis driven by the nonlinear dynamics of a complex scalar field with generalized self-interaction potentials that explicitly break the global $U(1)$ symmetry. Specifically, three…

General Relativity and Quantum Cosmology · Physics 2026-05-04 Surendra Kumar Gour , Malay K. Nandy

Modulated reheating scenario is one of the most attractive models that predict possible detections of not only the primordial non-Gaussianity but also the tensor fluctuation through future CMB observations such as the Planck satellite, the…

Cosmology and Nongalactic Astrophysics · Physics 2011-02-03 Kohei Kamada , Kazunori Kohri , Shuichiro Yokoyama

We study the impact of possible high density baryonic bubbles on the early formed QSO, IGM, and metal poor stars. Such bubbles could be created, under certain conditions, in Affleck-Dine model of baryogenesis and may occupy a relatively…

Astrophysics · Physics 2009-11-10 Shunji Matsuura , Alexander. D. Dolgov , Shigehiro Nagataki , Katsuhiko Sato

In this letter we explore the possibility of creating the baryon asymmetry of the universe during inflation and reheating due to the decay of a field associated with the inflaton. CP violation is attained by assuming that this field is…

High Energy Physics - Phenomenology · Physics 2014-11-17 D. V. Nanopoulos , Raghavan Rangarajan

We investigate the backreaction of the Affleck-Dine leptogenesis to inflaton dynamics in the F-term hybrid and chaotic inflation models in supergravity. We determine the lightest neutrino mass in both models so that the predictions of…

High Energy Physics - Phenomenology · Physics 2016-02-17 Masaki Yamada

Light fields get large scale fluctuations during inflation. If some of them are electrically charged, then large scale fluctuations of the electric charge will be generated. As a consequence, any finite portion of the Universe, including…

High Energy Physics - Phenomenology · Physics 2016-01-07 Cody Goolsby-Cole , Lorenzo Sorbo

It is shown that late-time decay of domain walls can dilute unwanted relics such as moduli, if the universe was dominated by frustrated domain walls with tension $\sigma = (1 - 100 TeV)^3$. Since energy density of the frustrated domain…

High Energy Physics - Phenomenology · Physics 2009-11-10 Masahiro Kawasaki , Fuminobu Takahashi

We propose a mechanism for baryogenesis in which the baryon asymmetry is generated as an equilibrium response of weak sphalerons in a region where electroweak sphaleron transitions remain unsuppressed, $h/T\lesssim 1$. A nonzero equilibrium…

High Energy Physics - Phenomenology · Physics 2026-05-18 Jacopo Azzola , Oleksii Matsedonskyi , Andreas Weiler

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 preheating after the inflation, which can be interpreted as particle creation in the oscillating inflaton background, provides a state far from thermal equilibrium. We extend the field theoretical treatment of the preheating by Linde et…

High Energy Physics - Phenomenology · Physics 2009-10-31 K. Funakubo , A. Kakuto , S. Otsuki , F. Toyoda

Pangenesis is the mechanism for jointly producing the visible and dark matter asymmetries via Affleck-Dine dynamics in a baryon-symmetric universe. The baryon-symmetric feature means that the dark asymmetry cancels the visible baryon…

High Energy Physics - Phenomenology · Physics 2012-05-21 Benedict von Harling , Kalliopi Petraki , Raymond R. Volkas

A baryogenesis scenario in supersymmetric standard models with Dirac neutrinos proposed by Abel and Page is reconsidered with introducing intermediate scale physics to stabilize the runaway potential along a right-handed sneutrino…

High Energy Physics - Phenomenology · Physics 2008-11-26 Masato Senami , Tsutomu Takayama

The Affleck-Dine leptogenesis scenario along the LHu flat direction is reconsidered. It is known that successful Affleck-Dine leptogenesis requires that the lightest neutrino mass is extremely small. This situation can be significantly…

High Energy Physics - Phenomenology · Physics 2017-03-08 Kyu Jung Bae , Howard Baer , Koichi Hamaguchi , Kazunori Nakayama

Affleck-Dine leptogenesis after thermal inflation along the $LH_u$ direction requires $m_L^2+m_{H_u}^2 < 0$ up to the AD scale ($|L|\simeq |H_u|\sim 10^9$ GeV). We renormalised this condition from the AD scale to the soft supersymmetry…

High Energy Physics - Phenomenology · Physics 2020-09-30 Seolhwa Kim , Ewan D. Stewart