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相关论文: Axion-like Dark Matter Mediators

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The axion is a pseudo-Nambu-Goldstone boson. It appears after the spontaneous breaking of the Peccei-Quinn symmetry, which was proposed to solve the strong-CP problem. Other pseudo-Nambu-Goldstone bosons, postulated in some extensions of…

高能物理 - 唯象学 · 物理学 2012-10-12 Davide Cadamuro

The recent detection of the cosmic microwave background polarimeter experiment BICEP2 of tensor fluctuations in the B-mode power spectrum basically excludes all plausible axion models where its decay constant is above $10^{13}$ GeV.…

高能物理 - 唯象学 · 物理学 2015-06-19 A. G. Dias , A. C. B. Machado , C. C. Nishi , A. Ringwald , P. Vaudrevange

Axion-like particles (ALPs) are promising dark matter candidates. They are typically described by a classical field, motivated by large phase space occupation numbers. Here we show that such a description is accompanied by a quantum effect:…

宇宙学与河外天体物理 · 物理学 2022-08-12 Michael Kopp , Vasileios Fragkos , Igor Pikovski

Light pseudoscalar resonances that couple to the Standard Model via non-renormalizable operators, such as axions and axion-like particles (ALPs), generate contributions to the renormalization group evolution equations of couplings of…

高能物理 - 唯象学 · 物理学 2025-06-10 Anne Mareike Galda , Matthias Neubert

Axion like particles (ALPs) are quite generic in many scenarios for physics beyond the Standard Model, they are pseudoscalar Nambu-Goldstone bosons, and appear once any global $U(1)$ symmetry is broken spontaneously. The ALPs can gain mass…

高能物理 - 唯象学 · 物理学 2016-03-23 Anupam Mazumdar , Saleh Qutub

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

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

One kind of particularly interesting pseudoscalar particles, called axion-like particles (ALPs), have rich physical phenomenology at high- and low-energy collider experiments. After discussing most of single production channels of ALP at…

高能物理 - 唯象学 · 物理学 2022-01-25 Chong-Xing Yue , Hua-Ying Zhang , Han Wang

We revisit the ALP miracle scenario where the inflaton and dark matter are unified by a single axion-like particle (ALP). We first extend our previous analysis on the inflaton dynamics to identify the whole viable parameter space consistent…

高能物理 - 唯象学 · 物理学 2020-06-24 Ryuji Daido , Fuminobu Takahashi , Wen Yin

Axionlike particles (ALPs) can be produced in the Sun, and are considered viable candidates for the cosmological dark matter (DM). It can decay into two photons or interact with matter. We identify new inelastic channels of inverse…

高能物理 - 唯象学 · 物理学 2023-08-29 C. -P. Wu , C. -P. Liu , Greeshma C. , L. Singh , J. -W. Chen , H. -C. Chi , M. K. Pandey , H. T. Wong

We show that an axionlike particle (ALP) can simultaneously generate the baryon asymmetry and constitute dark matter through dynamics triggered by a first-order electroweak phase transition (EWPT). In our proposal, the transition briefly…

高能物理 - 唯象学 · 物理学 2025-12-11 Dipendu Bhandari , Soumen Kumar Manna , Arunansu Sil

Axion-like particles (ALPs), a class of pseudoscalars common to many extensions of the Standard Model, have the capacity to drain energy from the interiors of stars. Consequently, stellar evolution can be used to derive many constraints on…

高能物理 - 唯象学 · 物理学 2021-09-16 Matthew J. Dolan , Frederick J. Hiskens , Raymond R. Volkas

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

Axion-like particles (ALPs) interacting with the Standard Model can be abundantly produced in proton beam fixed-target experiments. Looking for their displaced decays is therefore an effective search strategy for ALPs with a mass in the MeV…

高能物理 - 唯象学 · 物理学 2022-02-08 Nikita Blinov , Elizabeth Kowalczyk , Margaret Wynne

Dark matter could be a thermal relic comprised of strongly interacting massive particles (SIMPs), where $3 \rightarrow 2$ interactions set the relic abundance. Such interactions generically arise in theories of chiral symmetry breaking via…

高能物理 - 唯象学 · 物理学 2019-01-08 Yonit Hochberg , Eric Kuflik , Robert McGehee , Hitoshi Murayama , Katelin Schutz

We report on a search for dark matter axion-like particles (ALPs) using a Ramsey-type apparatus for cold neutrons. A hypothetical ALP-gluon-coupling would manifest in a neutron electric dipole moment signal oscillating in time. Twenty-four…

Axion-like particles (ALPs) are hypothetical pseudoscalar bosons that arise in many extensions of the Standard Model and are well-motivated dark matter candidates. Nearby massive stars in the late stages of stellar evolution provide a…

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

We show that an axionlike particle (ALP) naturally implements spontaneous electroweak baryogenesis through a cosmic evolution strongly tied to the electroweak phase transition (EWPT) if it feebly couples to the Higgs field while giving a…

高能物理 - 唯象学 · 物理学 2022-03-14 Sang Hui Im , Kwang Sik Jeong , Yeseong Lee

Asymmetric Dark Matter (ADM) models invoke a particle-antiparticle asymmetry, similar to the one observed in the Baryon sector, to account for the Dark Matter (DM) abundance. Both asymmetries are usually generated by the same mechanism and…

高能物理 - 唯象学 · 物理学 2015-06-04 Mattias Blennow , Enrique Fernandez-Martinez , Olga Mena , Javier Redondo , Paolo Serra