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相关论文: New Perspectives on Axion Misalignment Mechanism

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In the conventional misalignment mechanism, the axion field has a constant initial field value in the early universe and later begins to oscillate. We present an alternative scenario where the axion field has a nonzero initial velocity,…

高能物理 - 唯象学 · 物理学 2020-07-21 Raymond T. Co , Lawrence J. Hall , Keisuke Harigaya

The axion field, the angular direction of the complex scalar field associated with the spontaneous symmetry breaking of the Peccei-Quinn (PQ) symmetry, could have originated with initial non-zero velocity. The presence of a non-zero angular…

高能物理 - 唯象学 · 物理学 2022-11-30 Basabendu Barman , Nicolás Bernal , Nicklas Ramberg , Luca Visinelli

Understanding axion production in the early Universe remains a pivotal challenge, given the axion as a compelling cold dark matter candidate. Conventional misalignment scenarios often overlook the possibility that a large initial axion…

高能物理 - 唯象学 · 物理学 2026-04-03 Wei Chao , Chang-Jie Dai

We consider the production of axion dark matter through the misalignment mechanism in the context of a nonstandard cosmological history involving early matter domination by a scalar field with a time-dependent decay rate. In cases where the…

高能物理 - 唯象学 · 物理学 2023-05-24 Paola Arias , Nicolás Bernal , Jacek K. Osiński , Leszek Roszkowski

We propose an alternative scenario for the axion misalignment mechanism based on the nontrivial interplay between the axion and a light dilaton in the early universe. Dark matter abundance is still sourced by the initial misalignment of the…

高能物理 - 唯象学 · 物理学 2023-05-31 Ling-Xiao Xu , Seokhoon Yun

We investigate the phenomenology induced by generic PQ-breaking operators within the axion kinetic misalignment framework. We analyze their impact on the relic density of axion dark matter (DM), the PQ quality problem, axion-mediated…

高能物理 - 唯象学 · 物理学 2026-03-12 Xiangwei Yin , Ligong Bian

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

The QCD axion is one of the best motivated dark matter candidates. The misalignment mechanism is well known to produce an abundance of the QCD axion consistent with dark matter for an axion decay constant of order $10^{12}$ GeV. For a…

高能物理 - 唯象学 · 物理学 2020-11-02 Junwu Huang , Amalia Madden , Davide Racco , Mario Reig

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 study axion dark matter production from a misalignment mechanism in scenarios featuring a general nonstandard cosmology. Before the onset of Big Bang nucleosynthesis, the energy density of the universe is dominated by a particle field…

高能物理 - 唯象学 · 物理学 2021-12-13 Paola Arias , Nicolás Bernal , Dimitrios Karamitros , Carlos Maldonado , Leszek Roszkowski , Moira Venegas

We propose a relaxation mechanism for the initial misalignment angle of the pre-inflationary QCD axion with a large decay constant. The proposal addresses the challenges posed to the axion dark matter scenario by an overabundance of axions…

高能物理 - 唯象学 · 物理学 2024-10-30 Abhishek Banerjee , Manuel A. Buen-Abad

The axion arises in well-motivated extensions of the Standard Model of particle physics and is regarded as an alternative to the weakly interacting massive particle paradigm to explain the nature of dark matter. In this contribution, we…

高能物理 - 唯象学 · 物理学 2018-01-30 Ken'ichi Saikawa

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

Axion cold dark matter from standard misalignment typically requires a decay constant $f_a~\gtrsim~10^{11}$ GeV. Kinetic misalignment and parametric resonance easily allow lower values of $f_a$ when the radial Peccei-Quinn (PQ) symmetry…

高能物理 - 唯象学 · 物理学 2020-09-02 Raymond T. Co , Lawrence J. Hall , Keisuke Harigaya , Keith A. Olive , Sarunas Verner

The conventional misalignment mechanism for scalar dark matter depends on the initial field value, which governs the oscillation amplitude and present-day abundance. We present a mechanism by which a feeble (Planck-suppressed) coupling of…

高能物理 - 唯象学 · 物理学 2021-09-13 Brian Batell , Akshay Ghalsasi

We build a model in which the relic abundance of axions is altered from the standard misalignment mechanism, either increased or decreased, due to the presence of a new light scalar that couples to the radial part of the Peccei-Quinn (PQ)…

高能物理 - 唯象学 · 物理学 2022-06-20 Itamar J. Allali , Mark P. Hertzberg , Yi Lyu

The main mechanism responsible for Axion-Like-Particle (ALP) production in the early universe is the so-called misalignment mechanism. Three regimes have been investigated in this context: standard misalignment, large misalignment and…

高能物理 - 唯象学 · 物理学 2025-04-02 Cem Eröncel , Ryosuke Sato , Geraldine Servant , Philip Sørensen

We investigate the possibility that the dark matter abundance is sourced by the baryon/lepton asymmetry of the early Universe. It turns out that a Goldstone field of a local classically preserved symmetry in the Standard Model experiences a…

高能物理 - 唯象学 · 物理学 2021-07-21 Rodrigo Alonso , Jakub Scholtz

We study for what specific values of the theoretical parameters the axion can form the totality of cold dark matter. We examine the allowed axion parameter region in the light of recent data collected by the WMAP5 mission plus baryon…

宇宙学与河外天体物理 · 物理学 2021-12-14 Luca Visinelli , Paolo Gondolo

We study for what specific values of the theoretical parameters the axion can form the totality of cold dark matter. We examine the allowed axion parameter region in the light of recent data collected by the WMAP5 mission plus baryon…

宇宙学与河外天体物理 · 物理学 2021-12-14 Luca Visinelli , Paolo Gondolo
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