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Axions and axion-like particles (ALPs) are a prominent dark matter candidate, drawing motivation in part from the axiverse of string theory. Axion-like particles can also arise as composite degrees of freedom of a dark sector, for example,…

高能物理 - 唯象学 · 物理学 2023-12-19 Stephon Alexander , Humberto Gilmer , Tucker Manton , Evan McDonough

Axion and axion-like particles (ALPs) are a prominent candidate for physics beyond the Standard Model, and can play an important role in cosmology, serving as dark matter or dark energy, or both, drawing motivation in part from the string…

高能物理 - 唯象学 · 物理学 2024-04-19 Stephon Alexander , Tucker Manton , Evan McDonough

A light hidden photon or axion-like particle is a good dark matter candidate and they are often associated with the spontaneous breaking of dark global or gauged U(1) symmetry. We consider the dark Higgs dynamics around the phase transition…

高能物理 - 唯象学 · 物理学 2021-10-27 Kazunori Nakayama , Wen Yin

A well-motivated class of dark matter candidates, including axions and dark photons, takes the form of coherent oscillations of a light bosonic field. If the dark matter couples to Standard Model states, it may be possible to detect it via…

高能物理 - 唯象学 · 物理学 2018-08-08 Masha Baryakhtar , Junwu Huang , Robert Lasenby

Four decades after its prediction, the axion remains the most compelling solution to the Strong-CP problem and a well-motivated dark matter candidate, inspiring a host of elegant and ultrasensitive experiments based on axion-photon mixing.…

高能物理 - 实验 · 物理学 2016-02-02 Peter W. Graham , Igor G. Irastorza , Steven K. Lamoreaux , Axel Lindner , Karl A. van Bibber

The string axiverse predicts a unique connection between the high scales approachable only through theory and the low energies within reach of experimental verification: a multitude of light, feebly interacting axions. In order to capture…

高能物理 - 唯象学 · 物理学 2026-03-03 Masha Baryakhtar , David Cyncynates , Ella Henry

A generic low-energy prediction of string theory is the existence of a large collection of axions, commonly known as a string axiverse. Axions also have a natural cosmological production mechanism, vacuum misalignment, making them…

高能物理 - 唯象学 · 物理学 2022-03-22 David Cyncynates , Tudor Giurgica-Tiron , Olivier Simon , Jedidiah O. Thompson

The majoron is a well-motivated light (pseudo-Nambu-Goldstone) boson associated with the spontaneous breaking of a global lepton-number symmetry. In this {\it letter}, we relate the spontaneous breaking scale and its soft-breaking mass by…

高能物理 - 唯象学 · 物理学 2024-06-28 Qiuyue Liang , Xavier Ponce Díaz , Tsutomu T. Yanagida

Cosmologically long-lived, composite states arise as natural dark matter candidates in theories with a strongly interacting hidden sector at a scale of 10 - 100 TeV. Light axion-like states, with masses in the 1 MeV - 10 GeV range, are also…

高能物理 - 唯象学 · 物理学 2010-05-28 Jeremy Mardon , Yasunori Nomura , Jesse Thaler

An analysis is given of interacting dark energy and dark matter where the dark energy is assumed to be an ultralight axionic field with a pseudo-Nambu-Goldstone Boson potential which is in general a superposition of $N$ number of cosine…

宇宙学与河外天体物理 · 物理学 2025-12-01 Amin Aboubrahim , Andrew H. Giman , Pran Nath

It is widely believed that axions are ubiquitous in string theory and could be the dark matter. The peculiar features of the axion dark matter are coherent oscillations and a coupling to the electromagnetic field through the Chern-Simons…

高能物理 - 理论 · 物理学 2018-04-24 Daiske Yoshida , Jiro Soda

Light axion-like particles occur in many theories of beyond-Standard-Model physics, and may make up some or all of the universe's dark matter. One of the ways they can couple to the Standard Model is through the electromagnetic $F_{\mu\nu}…

高能物理 - 唯象学 · 物理学 2021-04-14 Robert Lasenby

We demonstrate that nuclear magnetic resonance based searches for dark matter (DM) have intrinsic and powerful sensitivity to dark photons and the axion-photon coupling. The reason is conceptually straightforward. An instrument such as…

高能物理 - 唯象学 · 物理学 2025-05-23 Carl Beadle , Sebastian A. R. Ellis , Jacob M. Leedom , Nicholas L. Rodd

The axion is a light pseudoscalar particle which suppresses CP-violating effects in strong interactions and also happens to be an excellent dark matter candidate. Axions constituting the dark matter halo of our galaxy may be detected by…

The particle nature of dark matter (DM) remains one of the most significant enigmas in modern cosmology. Axion-like particles (ALPs), as well-motivated candidates for cold dark matter, can undergo radiative decay into photon pairs, a…

宇宙学与河外天体物理 · 物理学 2026-05-08 Wen-Qing Guo

We propose new signals for the direct detection of ultralight dark matter such as the axion. Axion or axion like particle (ALP) dark matter may be thought of as a background, classical field. We consider couplings for this field which give…

高能物理 - 唯象学 · 物理学 2013-09-11 Peter W. Graham , Surjeet Rajendran

Dark matter (DM) refers to a new type of matter that may explain observed rotation curves of galaxies and the composite structure of the Universe. It may couple to the Standard Model particles via portals, which include the possibility of…

高能物理 - 实验 · 物理学 2023-11-30 Vindhyawasini Prasad

The dark matter and existence of new particles are now a possible explanation of several physics phenomena which evade the predictions of the Standard Model. In this context Axion-Like-Particles (ALP) with masses in the MeV to GeV range…

高能物理 - 实验 · 物理学 2026-01-23 M. Zielinski , K. Proscinski , P. Salabura

Axions are well motivated particles that could make up most or all of the dark matter if they have masses below 100 $\mu$eV. Microwave cavity techniques comprised of closed resonant structures immersed in solenoid magnets are sensitive to…

仪器与探测器 · 物理学 2015-02-24 Gray Rybka , Andrew Wagner , Aryeh Brill , Kunal Patel , Robert Percival , Katleiah Ramos

We discuss axion dark matter detection via two mechanisms: spontaneous decays and resonant conversion in neutron star magnetospheres. For decays, we show that the brightness temperature signal, rather than flux, is a less ambiguous measure…

宇宙学与河外天体物理 · 物理学 2020-07-15 Richard A. Battye , Bjoern Garbrecht , Jamie I. McDonald , Francesco Pace , Sankarshana Srinivasan
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