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We show that very compact axion mini-clusters can form in models where axion-like-particle (ALP) dark matter is produced via the kinetic misalignment mechanism, which is well-motivated in pre-inflationary $U(1)$ symmetry breaking scenarios.…

高能物理 - 唯象学 · 物理学 2024-05-06 Cem Eröncel , Géraldine Servant

Axions and axion-like particles (ALPs) are among the most popular candidates that explain the origin of the mysterious dark matter. The most popular ALP production mechanism studied in the literature is the misalignment mechanism, where an…

高能物理 - 唯象学 · 物理学 2025-01-22 Cem Eröncel

The misalignment mechanism for axion-like particles (ALPs) is a leading explanation for dark matter. In this work we investigate ALPs with non-periodic potentials, which allow for large misalignment of the field from the minimum and make it…

高能物理 - 唯象学 · 物理学 2024-02-19 Aleksandr Chatrchyan , Cem Eröncel , Matthias Koschnitzke , Géraldine Servant

Axion-like particles (ALPs) are leading candidates to explain the dark matter in the universe. Their production via the misalignment mechanism has been extensively studied for cosine potentials characteristic of pseudo-Nambu-Goldstone…

高能物理 - 唯象学 · 物理学 2023-10-30 Aleksandr Chatrchyan , Cem Eröncel , Matthias Koschnitzke , Géraldine Servant

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

Adding an axion-like particle (ALP) to the Standard Model, with a field velocity in the early universe, simultaneously explains the observed baryon and dark matter densities. This requires one or more couplings between the ALP and photons,…

高能物理 - 唯象学 · 物理学 2021-02-24 Raymond T. Co , Lawrence J. Hall , Keisuke Harigaya

We investigate the production of dark radiation (DR) from axions and axion-like particles (ALPs) as potential origins of dark matter. Focusing on the dark matter misalignment mechanism, we examine non-thermal, pre-inflationary scenarios…

宇宙学与河外天体物理 · 物理学 2024-11-12 José María Pérez-Poyatos , Veronica Sanz

In this work, we extend the standard pre-inflationary misalignment mechanism for axion-like particles (ALPs) by introducing a pre-oscillatory phase with constant equation of state $\omega_\phi\in[-1,1]$, generated by a tracking potential.…

宇宙学与河外天体物理 · 物理学 2026-05-08 José María Pérez-Poyatos

We study the impact of sphaleron-induced thermal friction on the axion dark-matter abundance due to the interaction of an axion-like particle (ALP) with a dark non-abelian gauge sector in a secluded thermal bath. Thermal friction can either…

高能物理 - 唯象学 · 物理学 2023-02-16 Alexandros Papageorgiou , Pablo Quílez , Kai Schmitz

We study an axion-like particle (ALP) that experiences the first-order phase transition with respect to its mass or potential minimum. This can be realized if the ALP obtains a potential from non-perturbative effects of SU($N$) gauge theory…

高能物理 - 唯象学 · 物理学 2023-04-05 Shota Nakagawa , Fuminobu Takahashi , Masaki Yamada , Wen Yin

The axion kinetic misalignment mechanism (KMM) opens the possibility of explaining dark matter for almost any axion mass and decay constant that are not accessible by the standard misalignment mechanism, in particular at low values of the…

高能物理 - 唯象学 · 物理学 2024-08-19 Cem Eröncel , Ryosuke Sato , Géraldine Servant , Philip Sørensen

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 explore the phenomenology of QCD axion and axion-like particle (ALP) dark matter production via misalignment during inflationary reheating. We investigate scenarios involving inflaton oscillating in a generic potential $\sim \phi^n$,…

高能物理 - 唯象学 · 物理学 2023-10-13 Yong Xu

We investigate the non-perturbatively generated axion-like particle (ALP) potential, involving fermions in the dark sector that couple to the ALP, in an early cosmological inflationary stage with the ALP being a spectator field. The…

高能物理 - 唯象学 · 物理学 2023-02-02 Anish Ghoshal , Abhishek Naskar

Many existing and proposed experiments targeting QCD axion dark matter (DM) can also search for a broad class of axion-like particles (ALPs). We analyze the experimental sensitivities to electromagnetically-coupled ALP DM in different…

高能物理 - 唯象学 · 物理学 2019-08-07 Nikita Blinov , Matthew J. Dolan , Patrick Draper , Jonathan Kozaczuk

Production of axionlike particles (ALPs) by primordial magnetic fields may have significant impacts on cosmology. We discuss the production of ALPs in the presence of the primordial magnetic fields. We find a region of the ALP mass and…

高能物理 - 唯象学 · 物理学 2017-08-09 Kohei Kamada , Yuichiro Nakai

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-like particles (ALPs) can provide a portal to new states of a dark sector. We study the phenomenology of this portal when the ALP mainly decays invisibly, while its interaction with the standard model sector proceeds essentially via…

高能物理 - 唯象学 · 物理学 2021-06-16 Luc Darmé , Federica Giacchino , Enrico Nardi , Mauro Raggi

Despite considerable experimental progress large parts of the axion-like particle (ALP) parameter space remain difficult to probe in terrestrial experiments. In some cases, however, small-scale structure of the ALP dark matter (DM)…

宇宙学与河外天体物理 · 物理学 2020-02-18 Nikita Blinov , Matthew J. Dolan , Patrick Draper

Axions are some of the best motivated particles beyond the Standard Model. We show how the attractive self-interactions of dark matter (DM) axions over a broad range of masses, from $10^{-22}$ eV to $10^7$ GeV, can lead to nongravitational…

宇宙学与河外天体物理 · 物理学 2020-04-15 Asimina Arvanitaki , Savas Dimopoulos , Marios Galanis , Luis Lehner , Jedidiah O. Thompson , Ken Van Tilburg
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