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We show that both the baryon asymmetry of the universe and dark matter (DM) can be accounted for by the dynamics of a single axion-like field. In this scenario, the observed baryon asymmetry is produced through spontaneous…

高能物理 - 唯象学 · 物理学 2019-02-13 Kyu Jung Bae , Jeff Kost , Chang Sub Shin

We argue that coherent oscillations of the axion field excited by the misalignment mechanism and non-thermal leptogenesis by the saxion decay can naturally explain the observed abundance of dark matter and baryon asymmetry, thus providing a…

高能物理 - 唯象学 · 物理学 2015-06-12 Kwang Sik Jeong , Fuminobu Takahashi

The QCD axion may offer a unified origin for the baryon asymmetry and dark matter through axiogenesis. However, in the minimal QCD axion scenario, axiogenesis either underproduces baryons or overproduces dark matter, and the required…

高能物理 - 唯象学 · 物理学 2025-11-21 Pouya Asadi , David Cyncynates , Stefania Gori

We introduce and study a model designed to simultaneously shed light on the mysteries connected with Baryogenesis, Dark Matter and Dark Energy. The model describes a self-interacting complex axion field whose imaginary part, a pseudo-scalar…

高能物理 - 理论 · 物理学 2021-04-21 Robert Brandenberger , Jürg Fröhlich

We propose late-time moduli decay as the common origin of baryons and dark matter. The baryon asymmetry is produced from the decay of new TeV scale particles, while dark matter is created from the (chain) decay of R-parity odd particles…

高能物理 - 唯象学 · 物理学 2011-04-22 Rouzbeh Allahverdi , Bhaskar Dutta , Kuver Sinha

We present a new mechanism of Baryogenesis and dark matter production in which both the dark matter relic abundance and the baryon asymmetry arise from neutral $B$ meson oscillations and subsequent decays. This set-up is testable at hadron…

高能物理 - 唯象学 · 物理学 2019-02-22 Gilly Elor , Miguel Escudero , Ann E. Nelson

We present a new mechanism to deplete the energy density of the QCD axion, making decay constants as high as $f_a \simeq 10^{17}\,\rm{GeV}$ viable for generic initial conditions. In our setup, the axion couples to a massless dark photon…

高能物理 - 唯象学 · 物理学 2018-04-04 Prateek Agrawal , Gustavo Marques-Tavares , Wei Xue

We show that the rotation of the QCD axion field, aided by $B-L$ violation from supersymmetric $R$-parity violating couplings, can yield the observed baryon abundance. Strong sphaleron processes transfer the angular momentum of the axion…

高能物理 - 唯象学 · 物理学 2021-12-22 Raymond T. Co , Keisuke Harigaya , Zachary Johnson , Aaron Pierce

In standard models of baryogenesis and of dark matter, the mechanisms which generate the densities in both sectors are unrelated to each other. In this paper we explore models which generate the baryon asymmetry through the dark matter…

高能物理 - 唯象学 · 物理学 2010-12-24 Jessie Shelton , Kathryn M. Zurek

A new mechanism for producing axion dark matter is proposed. By invoking low-scale inflation and a kinetic mixing between the axion and the inflaton, it is shown that the axion is driven to a field point slightly displaced from the…

高能物理 - 唯象学 · 物理学 2019-08-30 Takeshi Kobayashi , Lorenzo Ubaldi

Generating axion dark matter through the kinetic misalignment mechanism implies the generation of large asymmetries for Standard Model fermions in the early universe. Even if these asymmetries are washed out at later times, they can trigger…

高能物理 - 唯象学 · 物理学 2023-08-09 Raymond T. Co , Valerie Domcke , Keisuke Harigaya

Despite growing interest and extensive effort to search for ultralight dark matter in the form of a hypothetical dark photon, how it fits into a consistent cosmology is unclear. Several dark photon dark matter production mechanisms proposed…

高能物理 - 唯象学 · 物理学 2019-05-03 Raymond T. Co , Aaron Pierce , Zhengkang Zhang , Yue Zhao

The baryon asymmetry of the universe may be explained by rotations of the QCD axion in field space and baryon number violating processes. We consider the minimal extension of the Standard Model by a non-Abelian gauge interaction, $SU(2)_R$,…

高能物理 - 唯象学 · 物理学 2021-12-24 Keisuke Harigaya , Isaac R. Wang

We propose a scenario where the saxion dominates the energy density of the Universe and reheats the standard model sector via the dilatonic coupling, while its axionic partner contributes to dark matter decaying into photons via the same…

高能物理 - 唯象学 · 物理学 2014-04-29 Tetsutaro Higaki , Kwang Sik Jeong , Fuminobu Takahashi

Axion-like particles are a well-motivated dark matter candidate that can form a condensate with low momentum and high occupation number. In the presence of dark radiation, this condensate loses energy, naturally increasing the energy…

高能物理 - 唯象学 · 物理学 2024-09-24 Daniel Aloni , Hengameh Bagherian , Rashmish K. Mishra

We study a scenario in which the baryon asymmetry is created through Hawking radiation from primordial black holes via a dynamically-generated chemical potential. This mechanism can also be used to generate the observed dark matter…

高能物理 - 唯象学 · 物理学 2022-03-14 Nolan Smyth , Lillian Santos-Olmsted , Stefano Profumo

We demonstrate that the co-genesis of baryon asymmetry and dark matter can be achieved through the rotation of an axion-like particle, driven by a flip in the vacuum manifold's direction at the end of inflation. This can occur if the axion…

高能物理 - 唯象学 · 物理学 2025-09-03 Chao Chen , Suruj Jyoti Das , Konstantinos Dimopoulos , Anish Ghoshal

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 discuss relaxation solutions to the dark matter - baryon coincidence problem in the context of QCD axion dark matter. In relaxation solutions, a moduli dynamically adjusts the mass of dark matter and baryons until their energy densities…

高能物理 - 唯象学 · 物理学 2024-10-31 Abhishek Banerjee , Dawid Brzeminski , Anson Hook

We consider axino dark matter in large R-parity violation (RPV). In moduli-dominated universe, axino is produced thermally or non-thermally via saxion decay, then late-decaying moduli dilute axino density, which results in the right…

高能物理 - 唯象学 · 物理学 2015-06-22 Koji Ishiwata
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