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相关论文: Peccei-Quinn Genesis

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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…

高能物理 - 唯象学 · 物理学 2024-09-25 Raymond T. Co , Masaki Yamada

We propose a generic axion--driven cogenesis scenario in which both the baryon asymmetry and dark matter abundance originate from the kinetic misalignment. The framework unifies the Peccei--Quinn (PQ) mechanism with a Type--I seesaw sector,…

高能物理 - 唯象学 · 物理学 2026-01-15 Eung Jin Chun

The Peccei-Quinn symmetry is an automatic symmetry of the 3-3-1 gauge models which, consequently are not plagued with the strong CP problem. Nevertheless, the axion that emerges from spontaneous breaking of Peccei-Quinn symmetry cannot be…

高能物理 - 唯象学 · 物理学 2017-06-07 J. G. Ferreira , C. A de S. Pires , J. G. Rodrigues , P. S. Rodrigues da Silva

A minimal extension of the Standard Model (SM) with a single new mass scale and providing a complete and consistent picture of particle physics and cosmology up to the Planck scale is presented. We add to the SM three right-handed…

高能物理 - 唯象学 · 物理学 2017-02-22 Guillermo Ballesteros , Javier Redondo , Andreas Ringwald , Carlos Tamarit

We propose a consistent framework with the $U(1)$ Peccei-Quinn (PQ) symmetry for obtaining the initial condition for axion kinetic misalignment from inflation. We introduce a PQ complex scalar field and an extra Higgs doublet, which are…

高能物理 - 唯象学 · 物理学 2024-11-27 Hyun Min Lee , Adriana G. Menkara , Myeong-Jung Seong , Jun-Ho Song

If the Peccei-Quinn field containing the QCD axion undergoes rotations in the early universe, the dimension-five operator responsible for neutrino masses can generate a lepton asymmetry that ultimately gives rise to the observed baryon…

高能物理 - 唯象学 · 物理学 2023-05-24 Patrick Barnes , Raymond T. Co , Keisuke Harigaya , Aaron Pierce

We propose a simple extension of the minimal supersymmetric standard model by introducing a gauge singlet in addition to right-handed neutrinos. The model resolves the strong CP problem by Pecci-Quinn symmetry, explains the origin of…

高能物理 - 唯象学 · 物理学 2010-08-02 Wan-Il Park

We consider a phenomenological extension of the minimal supersymmetric standard model (MSSM) which incorporates non-minimal chaotic inflation, driven by a quadratic potential in conjunction with a linear term in the frame function.…

高能物理 - 唯象学 · 物理学 2012-07-27 C. Pallis , Q. Shafi

We study the lepto-axiogenesis scenario in the minimal supersymmetric KSVZ axion model. Only one Peccei-Quinn (PQ) field and vector-like fields are introduced besides the MSSM with the type-I see-saw mechanism. The PQ field is stabilized by…

高能物理 - 唯象学 · 物理学 2022-04-26 Junichiro Kawamura , Stuart Raby

We show that the hybrid inflation is naturally realized in the framework of a supersymmetric axion model, which is consistent with the WMAP observation if the Peccei-Quinn symmetry breaking scale is around 10^{15}GeV. By solving the post…

高能物理 - 唯象学 · 物理学 2015-03-19 Masahiro Kawasaki , Naoya Kitajima , Kazunori Nakayama

We propose a novel minimal scenario which simultaneously addresses the following theoretical/cosmological/phenomenological puzzles: (i) the origin of scales, (ii) primordial inflation, (iii) matter-antimatter asymmetry, (iv) tiny neutrino…

高能物理 - 唯象学 · 物理学 2025-07-24 Gabriela Barenboim , P. Ko , Wan-il Park

Axions in the Peccei-Quinn (PQ) mechanism provide a promising solution to the strong CP problem in the standard model of particle physics. Coherently generated PQ scalar fields could dominate the energy density in the early Universe and…

高能物理 - 唯象学 · 物理学 2015-08-12 Hironori Hattori , Tatsuo Kobayashi , Naoya Omoto , Osamu Seto

We propose a mechanism called axiogenesis where the cosmological excess of baryons over antibaryons is generated from the rotation of the QCD axion. The Peccei-Quinn (PQ) symmetry may be explicitly broken in the early universe, inducing the…

高能物理 - 唯象学 · 物理学 2020-04-01 Raymond T. Co , Keisuke Harigaya

Axion scenarios in which the spontaneous breaking of the Peccei-Quinn symmetry takes place before or during inflation, and in which axion dark matter arises from the misalignment mechanism, can be constrained by Cosmic Microwave Background…

高能物理 - 唯象学 · 物理学 2021-10-05 Guillermo Ballesteros , Andreas Ringwald , Carlos Tamarit , Yvette Welling

We propose a baryogenenesis mechanism that uses a rotating condensate of a Peccei-Quinn (PQ) symmetry breaking field and the dimension-five operator that gives Majorana neutrino masses. The rotation induces charge asymmetries for the Higgs…

高能物理 - 唯象学 · 物理学 2021-06-25 Raymond T. Co , Nicolas Fernandez , Akshay Ghalsasi , Lawrence J. Hall , Keisuke Harigaya

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,…

高能物理 - 唯象学 · 物理学 2019-04-03 P. V. Dong , D. T. Huong , Daniel A. Camargo , Farinaldo S. Queiroz , José W. F. Valle

We study in detail a supersymmetric Peccei-Quinn model, which has a DFSZ and a KSVZ version. The fields breaking the Peccei-Quinn (PQ) symmetry correspond to flat directions (flaton fields) and have unsuppressed couplings when PQ symmetry…

高能物理 - 唯象学 · 物理学 2007-05-23 E. J. Chun , D. Comelli , David H. Lyth

We propose a model which is a simple extension of the KSVZ invisible axion model with an inert doublet scalar. Peccei-Quinn symmetry forbids tree-level neutrino mass generation and its remnant $Z_2$ symmetry guarantees dark matter…

高能物理 - 唯象学 · 物理学 2018-02-14 Daijiro Suematsu

We show that a supersymmetric axion model naturally induces a hybrid inflation with the waterfall field identified as a Peccei-Quinn scalar. The Peccei-Quinn scale is predicted to be around 10^{15}GeV for reproducing the large-scale density…

高能物理 - 唯象学 · 物理学 2011-02-02 Masahiro Kawasaki , Naoya Kitajima , Kazunori Nakayama

In order to accommodate the QCD axion as the dark matter (DM) in a model in which the Peccei-Quinn (PQ) symmetry is broken before the end of inflation, a relatively low scale of inflation has to be invoked in order to avoid bounds from DM…

宇宙学与河外天体物理 · 物理学 2019-09-16 Tommi Tenkanen , Luca Visinelli
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