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An experiment is described to detect dark matter axions trapped in the halo of our galaxy. Galactic axions are converted into microwave photons via the Primakoff effect in a static background field provided by a superconducting magnet. The…

Electromagnetic fields surrounding pulsars may source coherent ultralight axion signals at the known rotational frequencies of the neutron stars, which can be detected by laboratory experiments (e.g., pulsarscopes). As a promising case…

High Energy Physics - Phenomenology · Physics 2025-03-25 Mariia Khelashvili , Mariangela Lisanti , Anirudh Prabhu , Benjamin R. Safdi

Axions are a well-motivated dark matter candidate. They may be detectable from radio line emission due to resonant conversion in neutron star magnetospheres. While radio data collection for this signal has begun, further efforts are…

High Energy Astrophysical Phenomena · Physics 2025-03-19 Jesse Satherley , Chris Gordon , Chris Stevens

When axion stars fly through an astrophysical magnetic background, the axion-to-photon conversion may generate a large electromagnetic radiation power. After including the interference effects of the spacially-extended axion-star source and…

High Energy Astrophysical Phenomena · Physics 2018-04-11 Yang Bai , Yuta Hamada

The status of the solar axion search with the CERN Axion Solar Telescope (CAST) will be discussed. Results from the first part of CAST phase II where the magnet bores were filled with \hefour gas at variable pressure in order to scan \ma up…

High Energy Physics - Experiment · Physics 2019-08-13 Esther Ferrer Ribas

Due to their high magnetic fields and plasma densities, pulsars provide excellent laboratories for tests of beyond Standard Model (BSM) physics. When axions or axion-like particles (ALPs) approach closely enough to pulsars, they can be…

Cosmology and Nongalactic Astrophysics · Physics 2020-10-29 Anirudh Prabhu , Nicholas M. Rapidis

Hypothetical axion-like particles with a two-photon interaction would be produced in the Sun by the Primakoff process. In a laboratory magnetic field (``axion helioscope'') they would be transformed into X-rays with energies of a few keV.…

High Energy Physics - Experiment · Physics 2012-08-27 CAST Collaboration

In the presence of a magnetic field, axions can convert into photons and vice versa. The phenomenology of the conversion is captured by a system of two coupled Klein-Gordon equations, which, assuming that the axion is relativistic, is…

High Energy Physics - Phenomenology · Physics 2025-03-24 Clemente Smarra , Pierluca Carenza

We investigate axion-photon conversion in stochastic magnetic fields, focusing on the evolution of the photon intensity and polarizations induced by conversion into axions. Assuming Gaussian magnetic fields characterized by the power…

High Energy Physics - Phenomenology · Physics 2025-12-25 Wataru Chiba , Ryusuke Jinno , Kimihiro Nomura

An x-ray detector for a solar axion search was developed. The detector is operated at 60K in a cryostat of a superconducting magnet. Special care was paid to microphonic noise immunity and mechanical structure against thermal contraction.…

Astrophysics · Physics 2009-11-07 T. Namba , Y. Inoue , S. Moriyama , M. Minowa

We show existence of strong negative correlation between the temporal variations of magnetic field toroidal component of the solar tachocline (the bottom of convective zone) and the Earth magnetic field (Y-component). The possibility that…

Earth and Planetary Astrophysics · Physics 2010-08-17 V. D. Rusov , E. P. Linnik , K. Kudela , S. Cht. Mavrodiev , T. N. Zelentsova , V. P. Smolyar , K. K. Merkotan

We investigate a search for the oscillating current induced by axion dark matter in an external magnetic field using optically pumped magnetometers (OPMs). This experiment is based upon the LC circuit axion detection concept of Sikivie,…

Instrumentation and Detectors · Physics 2018-04-24 P. -H. Chu , L. D. Duffy , Y. J. Kim , I. M. Savukov

We report details on the axion dark matter search experiment that uses the innovative technologies of a High-Temperature Superconducting (HTS) magnet and a Josephson Parametric Converter (JPC). An 18 T HTS solenoid magnet is developed for…

High Energy Physics - Experiment · Physics 2022-12-14 Hojin Yoon , Moohyun Ahn , Byeongsu Yang , Youngjae Lee , DongLak Kim , Heejun Park , Byeonghun Min , Jonghee Yoo

The coherent Bragg scattering of photons converted from solar axions inside crystals would boost the signal for axion-photon coupling enhancing experimental sensitivity for these hypothetical particles. Knowledge of the scattering angle of…

High Energy Physics - Experiment · Physics 2017-02-07 Wenqin Xu , Steven R. Elliott

We discuss the physics case for and the concept of a medium-scale axion helioscope with sensitivities in the axion-photon coupling a few times better than CERN Axion Solar Telescope (CAST). Search for an axion-like particle with these…

The XENON1T collaboration has observed an excess in electronic recoil events below $5~\mathrm{keV}$ over the known background, which could originate from beyond-the-Standard-Model physics. The solar axion is a well-motivated model that has…

High Energy Physics - Phenomenology · Physics 2020-12-25 Christina Gao , Jia Liu , Lian-Tao Wang , Xiao-Ping Wang , Wei Xue , Yi-Ming Zhong

In the near future BabyIAXO will be the most powerful axion helioscope, relying on a custom-made magnet of two bores of 70 cm diameter and 10 m long, with a total available magnetic volume of more than 7 m$^3$. In this document, we propose…

The Cern Axion Solar Telescope (CAST) is in operation and taking data since 2003. The main objective of the CAST experiment is to search for a hypothetical pseudoscalar boson, the axion, which might be produced in the core of the sun. The…

A search for the axioelectric absorption of 5.5-MeV solar axions produced in the $p+d\rightarrow \rm{^3He}+\gamma(5.5 \rm{MeV})$ reaction was performed with two BGO detectors placed inside a low-background setup. A model independent limit…

High Energy Physics - Experiment · Physics 2014-11-21 A. V. Derbin , A. S. Kayunov , V. N. Muratova