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Related papers: Affleck-Dine Baryogenesis after Thermal Inflation

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We present a minimal framework that realises successful Dirac Leptogenesis through the Affleck-Dine mechanism. A single right-handed neutrino and a neutrinophillic Higgs doublet are introduced to the Standard Model, which couple via a…

High Energy Physics - Phenomenology · Physics 2024-03-12 Neil D. Barrie , Chengcheng Han

The minimal supersymmetric standard model (MSSM) has a truly supersymmetric way to explain both the baryon asymmetry and cold dark matter in the present Universe, that is, ``Affleck-Dine baryo/DM-genesis.'' The associated late-time decay of…

High Energy Physics - Phenomenology · Physics 2009-11-10 Masaaki Fujii , Masahiro Ibe

We discuss the non-thermal leptogenesis in the scheme of 5D orbifold SO(10) GUT with the smooth hybrid inflation. With an unambiguously determined Dirac Yukawa couplings and an assumption for the neutrino mixing matrix of the tri-bimaximal…

High Energy Physics - Phenomenology · Physics 2015-03-13 Takeshi Fukuyama , Nobuchika Okada

We examine the viability of the Affleck-Dine mechanism for baryogenesis under radiatively induced running of soft breaking $({\rm mass})^2$ of the flat directions stemming from non-zero energy density of the inflaton during inflation. A…

High Energy Physics - Phenomenology · Physics 2009-11-07 Rouzbeh Allahverdi , Manuel Drees , Anupam Mazumdar

In this work, we classify all the effective $U(1)$ symmetries and their associated Noether charges in the Standard Model (SM) and its minimal supersymmetric extension (MSSM) from the highest scale after inflation down to the weak scale. We…

High Energy Physics - Phenomenology · Physics 2021-08-26 Chee Sheng Fong

We propose that the observed baryon asymmetry of the Universe can naturally arise from a net asymmetry generated in the sleptonic sector at fairly low reheat temperatures. The best candidate is indeed the right-handed sneutrino. The initial…

High Energy Physics - Phenomenology · Physics 2009-11-10 Rouzbeh Allahverdi , Bhaskar Dutta , Anupam mazumdar

In this letter, we quantify the challenge of explaining the baryon asymmetry using initial conditions in a universe that undergoes inflation. Contrary to lore, we find that such an explanation is possible if net $B-L$ number is stored in a…

High Energy Physics - Phenomenology · Physics 2017-09-06 Gordan Krnjaic

We present a unified model where the same scalar field can drive inflation and account for the present dark matter abundance. This scenario is based on the incomplete decay of the inflaton field into right-handed neutrino pairs, which is…

High Energy Physics - Phenomenology · Physics 2025-02-14 Antonio Torres Manso , Joao G. Rosa

We study a minimal scenario to realize non-thermal leptogenesis and UV freeze-in of a Standard Model (SM) gauge singlet fermionic dark matter (DM) simultaneously, with inflaton field playing a non-trivial role in their yields. The…

High Energy Physics - Phenomenology · Physics 2021-09-01 Basabendu Barman , Debasish Borah , Rishav Roshan

The Minimal Supersymmetry Standard Model contains several hundreds of D- and F-flat directions that are lifted by soft susy breaking terms as well as by non-renormalizable terms. In a recent paper we find that only two of these directions,…

High Energy Physics - Phenomenology · Physics 2010-11-11 Juan Garcia-Bellido

We introduce an axion-inflation model embedded in the Left-Right symmetric extension of the SM in which $W_R$ is coupled to the axion. This model merges three milestones of modern cosmology, i.e., inflation, cold dark matter, and baryon…

High Energy Physics - Phenomenology · Physics 2021-10-13 Azadeh Maleknejad

We review the status of thermal leptogenesis in the minimal $SU(5)\times U(1)$ and $SO(10)$ unified models under the assumption that the leptonic asymmetry generated in the out-of-equilibrium decays of heavy Majorana neutrinos (and its…

High Energy Physics - Phenomenology · Physics 2025-07-01 Michal Malinský

Thermal inflation driven by a scalar field called "flaton" is a possible scenario to solve the cosmological moduli problem. We study a model of thermal inflation with a flaton chemical potential. In the presence of the chemical potential, a…

High Energy Physics - Phenomenology · Physics 2017-05-03 Masato Arai , Yoshishige Kobayashi , Nobuchika Okada , Shin Sasaki

Low-scale supersymmetry breaking in string motivated theories implies the presence of O(100) TeV scale moduli, which generically lead to a significant modification of the history of the universe prior to Big Bang Nucleosynthesis. Such an…

High Energy Physics - Phenomenology · Physics 2015-05-30 Gordon Kane , Jing Shao , Scott Watson , Hai-Bo Yu

We show that both the baryon asymmetry of the Universe and the dark matter abundance can be explained within a single framework that makes use of maximally helical hypermagnetic fields produced during pseudoscalar inflation and the chiral…

High Energy Physics - Phenomenology · Physics 2019-10-10 Yann Cado , Eray Sabancilar

For Affleck-Dine baryogenesis to proceed, there must have been two types of phase transitions. One is the destabilized-stabilized phase transition of the flat direction, which is in general induced by the Hubble parameter. The other is the…

High Energy Physics - Phenomenology · Physics 2016-09-06 Tomohiro Matsuda

We study F-term hybrid inflation in a novel supersymmetric extension of the SM with a subdominant Fayet-Iliopoulos D-term. We call this particular form of inflation, in short, F_D-term hybrid inflation. The proposed model ties the…

High Energy Physics - Phenomenology · Physics 2010-04-05 Bjorn Garbrecht , Apostolos Pilaftsis

We study a $D$-term inflation scenario in a model extended from the minimal supersymmetric standard model (MSSM) by two additional abelian factor groups focussing on its particle physics aspects. Condensates of the fields related to the…

High Energy Physics - Phenomenology · Physics 2014-11-17 Daijiro Suematsu

The Affleck-Dine mechanism creates the baryon asymmetry of the universe from an angular motion of a complex scalar field. The mechanism is efficient and allows for a low reheating temperature of the universe if the scalar field has a flat…

High Energy Physics - Phenomenology · Physics 2019-09-04 Keisuke Harigaya

The ultra-slow-roll (USR) inflation represents a class of single-field models with sharp deceleration of the rolling dynamics on small scales, leading to a significantly enhanced power spectrum of the curvature perturbations and primordial…

High Energy Physics - Phenomenology · Physics 2023-03-27 Yi-Peng Wu , Elena Pinetti , Kalliopi Petraki , Joseph Silk
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