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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 4He gas at variable pressure in order to scan axion…

High Energy Physics - Experiment · Physics 2014-09-05 F. J. Iguaz

We investigate solar X-ray observations as a probe of axions and axion-like particles. These particles can be produced in the interior of the Sun via the conversion of thermal photons, as well as through processes involving axion-electron…

Cosmology and Nongalactic Astrophysics · Physics 2026-05-27 Tiziano Zanzarella , Francisco R. Candón , Maurizio Giannotti , Marco Regis , Jaime Ruz , Marco Taoso , Elisa Todarello , Julia K. Vogel

Recently the EDGES experiment reported an enhanced 21cm absorption signal in the radio wave observation, which may be interpreted as either anomalous cooling of baryons or heating of cosmic microwave background photons. In this paper, we…

High Energy Physics - Phenomenology · Physics 2018-07-10 Takeo Moroi , Kazunori Nakayama , Yong Tang

The Sun is replete with magnetic fields, with sunspots, pores and plage regions being their most prominent representatives on the solar surface. But even far away from these active regions, magnetic fields are ubiquitous. To a large extent,…

Solar and Stellar Astrophysics · Physics 2015-11-05 Andreas Lagg , Bruce Lites , Jack Harvey , Sanjay Gosain , Rebecca Centeno

We made a search for hadronic axions which could be emitted from the Sun in M1 transitions between the first 14.4 keV thermally excited and the ground state in Fe-57, and absorbed in the HPGe detector by axioelectric effect. An upper limit…

High Energy Physics - Experiment · Physics 2008-11-26 A. Ljubicic , D. Kekez , Z. Krecak , T. Ljubicic

In theories with the large extra dimensions beyond the standard 4-dimensional spacetime, axions could propagate in such extra dimensions, and acquire Kaluza-Klein (KK) excitations. These KK axions are produced in the Sun and could solve…

We compute the photon-axion conversion probability in an external magnetic field with a strong transverse gradient in the eikonal approximation for plane waves. We find it typically smaller than a comparable uniform case. Some insights into…

High Energy Physics - Phenomenology · Physics 2010-03-02 Javier Redondo

Axions seem ubiquitous in string theories and some of them may be produced non-thermally by heavy scalar decays, contributing to dark radiation. We study various cosmological effects of photons produced from the axionic dark radiation…

High Energy Physics - Phenomenology · Physics 2015-06-16 Tetsutaro Higaki , Kazunori Nakayama , Fuminobu Takahashi

The search for resonant absorption of Compton and bremsstrahlung solar axions by $^{169}$Tm nuclei have been performed. Such an absorption should lead to the excitation of low-lying nuclear energy level: $A+^{169}$Tm $\rightarrow…

High Energy Physics - Experiment · Physics 2013-12-03 A. V. Derbin , I. S. Dratchnev , A. S. Kayunov , V. N. Muratova , D. A. Semenov , E. V. Unzhakov

This work provides additional evidence on the involvement of exotic particles like axions and/or other WISPs, following recent measurements during the quietest Sun and flaring Sun. Thus, SPHINX mission observed a minimum basal soft X-rays…

Solar and Stellar Astrophysics · Physics 2011-12-20 K. Zioutas , M. Tsagri , Y. Semertzidis , T. Papaevangelou , E. Georgiopoulou , A. Gardikiotis , T. Dafni

In solar physics, it is a big challenge to measure the magnetic fields directly from observations in the upper solar atmosphere, including the chromosphere and corona. Radio observations are regarded as the most feasible approach to…

Solar and Stellar Astrophysics · Physics 2022-06-22 Baolin Tan

It is shown that dark matter axions cause an oscillating electric current to flow along magnetic field lines. The oscillating current induced in a strong magnetic field $\vec{B}_0$ produces a small magnetic field $\vec{B}_a$. We propose to…

High Energy Physics - Phenomenology · Physics 2015-06-17 P. Sikivie , N. Sullivan , D. B. Tanner

Strong solar magnetic fields are the energy source of intense flares and energetic coronal mass ejections of space weather importance. The key issue is the difficulty in predicting the occurrence time and location of strong solar eruptions,…

Solar and Stellar Astrophysics · Physics 2023-07-04 P. K. Manoharan , C. J. Salter , S. M. White , P. Perillat , F. Fernandez , B. Perera , A. Venkataraman , C. Brum

Ultralight dark matter candidates, such as axions and dark photons, are leading dark matter candidates. They may couple feebly to photons, sourcing oscillating electromagnetic signals in the Earth's conducting cavity formed between the…

High Energy Physics - Phenomenology · Physics 2025-12-08 Ariel Arza , Yuanlin Gong , Jun Guo , Xiaofei Huang , Jing Shu , Hongliang Tian , Wenyu Wang , Kai Wei , Lei Wu , Mingming Xia , Jin Min Yang , Qiang Yuan , Yang Zhang , Yi Zhang , Bin Zhu

We reconsider the conversion of the photon into axion in the external electromagnetic fields, namely in the static fields and in a periodic field of the wave guide. The total cross-sections for the conversion are evaluated in detail. The…

High Energy Physics - Phenomenology · Physics 2014-02-21 D. V. Soa , H. N. Long , T. D. Tham

The magnetospheres of neutron stars in the Galactic Center provide an exceptional environment to search for dark matter axions through their resonant conversion into photons. The combination of extreme magnetic fields and high dark matter…

Instrumentation and Methods for Astrophysics · Physics 2025-12-17 J. De Miguel , E. Hatziminaoglou , J. Prieto-Polo , J. D. Marrero-Falcón , Abaz Kryemadhi

A mass-shift of the axion propagating in an external constant homogenious magnetic field is calculated. The contributions via an electron loop and a virtual photon are examined. It is shown that the virtual photon contribution dominates…

High Energy Physics - Phenomenology · Physics 2016-11-03 N. V. Mikheev , A. Ya. Parkhomenko , L. A. Vassilevskaya

Northern auroral regions of Earth were imaged with energetic photons in the 0.1-10 keV range using the High-Resolution Camera (HRC-I) aboard the Chandra X-ray Observatory at 10 epochs (each ~20 min duration) between mid-December 2003 and…

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