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The natural environment of the Earth can act as a sensitive detector for dark matter in ultralight axions. When axions with masses between $1\times10^{-15}\,{\rm eV}$ and $1\times10^{-13}\,{\rm eV}$ pass through the Earth, they interact…

High Energy Physics - Phenomenology · Physics 2025-04-23 Atsushi Nishizawa , Atsushi Taruya , Yoshiaki Himemoto

We point out that photon regeneration-experiments that search for the axion, or axion-like particles, may be resonantly enhanced by employing matched Fabry-Perot optical cavities encompassing both the axion production and conversion…

High Energy Physics - Phenomenology · Physics 2008-11-26 P. Sikivie , D. B. Tanner , Karl van Bibber

Axions with masses of order keV can be produced in great abundance within the Solar core. The majority of Sun-produced axions escape to infinity, but a small fraction of the flux is produced with speeds below the escape velocity. Over time,…

High Energy Physics - Phenomenology · Physics 2022-09-07 William DeRocco , Shalma Wegsman , Brian Grefenstette , Junwu Huang , Ken Van Tilburg

Advanced LIGO may be the first experiment to detect gravitational waves. Through superradiance of stellar black holes, it may also be the first experiment to discover the QCD axion with decay constant above the GUT scale. When an axion's…

High Energy Physics - Phenomenology · Physics 2015-04-16 Asimina Arvanitaki , Masha Baryakhtar , Xinlu Huang

The purpose of this paper is to assess the feasibility of axion detection by X-ray spectroscopy of the sun. We review the theory of axion-photon mode conversion with special attention to axions emitted in the 14.4 keV M1 decay of 57Fe at…

Solar and Stellar Astrophysics · Physics 2015-06-15 J. Martin Laming

A brief review of particle physics motivations for axion existence is followed by a discussion of optical observables that can be used for axion detection. It is emphasised that the resonant photon - axion transition can occur in the…

High Energy Physics - Phenomenology · Physics 2009-09-25 Ryszard Stroynowski , Ariel R. Zhitnitsky

We consider axion production during the formation of a quark-gluon plasma in relativistic heavy-ion collisions and discuss a possible detection scheme.

High Energy Physics - Phenomenology · Physics 2009-10-31 A. C. Melissinos

Conventional approaches to probing axions and axion-like particles (ALPs) typically rely on a coupling to photons. However, if this coupling is extremely weak, ALPs become invisible and are effectively decoupled from the Standard Model.…

High Energy Physics - Phenomenology · Physics 2019-01-30 Camila S. Machado , Wolfram Ratzinger , Pedro Schwaller , Ben A. Stefanek

A finite axion-nucleon coupling, nearly unavoidable for QCD axions, leads to the production of axions via the thermal excitation and subsequent de-excitation of Fe-57 isotopes in the sun. We revise the solar bound on this flux adopting the…

We study the coupling of axions to gauge bosons in heterotic string theory. The axion-gauge boson couplings in the low energy 4d theory are derived by matching mixed anomalies between higher-form global symmetries and the zero-form gauge…

High Energy Physics - Phenomenology · Physics 2024-10-08 Prateek Agrawal , Michael Nee , Mario Reig

We present first results and future plans for the Oscillating Resonant Group AxioN (ORGAN) experiment, a microwave cavity axion haloscope situated in Perth, Western Australia designed to probe for high mass axions motivated by several…

Instrumentation and Detectors · Physics 2022-05-11 Ben T. McAllister , Graeme Flower , Justin Kruger , Eugene N. Ivanov , Maxim Goryachev , Jeremy Bourhill , Michael E. Tobar

The QCD axion, originally proposed to solve the strong CP problem in QCD, is a prominent candidate for dark matter (DM). In the presence of strong magnetic fields, such as those around neutron stars, axions can theoretically convert into…

Cosmology and Nongalactic Astrophysics · Physics 2025-02-19 Luca Visinelli , Bradley Johnson , Bradley J. Kavanagh , David J. E. Marsh , Jordan E. Shroyer , Liam Walters

Axions are hypothetical particles proposed to solve the strong CP problem in QCD and may constitute a significant fraction of the dark matter in the Universe. Axions are expected to be produced in neutron stars and subsequently decay,…

High Energy Astrophysical Phenomena · Physics 2022-07-15 Bijan Berenji

We propose a method for remotely detecting backward reflection via induced decay of cold dark matter such as axion in the background of a propagating coherent photon field. This method can be particularly useful for probing concentrated…

High Energy Physics - Phenomenology · Physics 2024-08-21 Kensuke Homma

We discuss an improved detection scheme for a light-shining-through-wall (LSW) experiment for axion-like particle searches. We propose to use: gyrotrons or klystrons, which can provide extremely intense photon fluxes at frequencies around…

High Energy Physics - Phenomenology · Physics 2016-09-19 J. Ferretti

We describe a method based on precision magnetometry that can extend the search for axion-mediated spin-dependent forces by several orders of magnitude. By combining techniques used in nuclear magnetic resonance and short-distance tests of…

High Energy Physics - Phenomenology · Physics 2014-10-22 Asimina Arvanitaki , Andrew A. Geraci

Axions are hypothetical pseudoscalar particles that have been regarded as promising dark matter (DM) candidates. On the other hand, extended compact objects such as axion stars, which are supported by gravity and axion self interactions,…

High Energy Physics - Phenomenology · Physics 2025-05-09 Jan Tristram Acuña , Kuan-Yen Chou , Po-Yan Tseng

We consider a scenario with axions/axion-like particles Chern-Simons gravity coupling, such that gravitational waves can be produced directly from axion wave parametric resonance in the early universe after inflation. This axion gravity…

High Energy Physics - Phenomenology · Physics 2024-04-09 Mingqiu Li , Sichun Sun , Qi-Shu Yan , Zhijie Zhao

The search for solar axions produced by Compton ($\gamma+e^-\rightarrow e^-+A$) and bremsstrahlung-like ($e^-+Z \rightarrow Z+e^-+A$) processes has been performed. The axion flux in the both cases depends on the axion-electron coupling…

High Energy Physics - Experiment · Physics 2011-02-25 A. V. Derbin , A. S. Kayunov , V. N. Muratova , D. A. Semenov , E. V. Unzhakov