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Axion dark matter (DM) may convert to radio-frequency electromagnetic radiation in the strong magnetic fields around neutron stars. The radio signature of such a process would be an ultra-narrow spectral peak at a frequency determined by…

Axion dark matter can resonantly convert to photons in the magnetosphere of neutron stars, possibly giving rise to radio signals observable on Earth. This method for the indirect detection of axion dark matter has recently received…

高能物理 - 唯象学 · 物理学 2021-11-11 Alexander J. Millar , Sebastian Baum , Matthew Lawson , M. C. David Marsh

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

We propose a new method to detect observational appearance of Dark Matter axions. The method utilizes observations of neutron stars (NSs) in radio. It is based on the conversion of axions to photons in strong magnetic fields of NSs…

天体物理学 · 物理学 2014-11-18 M. S. Pshirkov , S. B. Popov

A model is constructed to predict the emission originating from axion-to-photon conversion in the strongly magnetized ultrarelativistic plasma of neutron stars. The acceleration and multiplicity of the charges are observed to shift the…

高能物理 - 唯象学 · 物理学 2025-02-20 Javier De Miguel

Axion as one of the promising dark matter candidates can be detected through narrow radio lines emitted from the magnetic white dwarf stars. Due to the existence of the strong magnetic field, the axion may resonantly convert into the radio…

高能物理 - 唯象学 · 物理学 2021-06-23 Jin-Wei Wang , Xiao-Jun Bi , Run-Min Yao , Peng-Fei Yin

Axions are well-motivated candidates for dark matter. Recently, much interest has focused on the detection of photons produced by the resonant conversion of axion dark matter in neutron star magnetospheres. Various groups have begun to…

高能物理 - 唯象学 · 物理学 2021-10-04 R. A. Battye , B. Garbrecht , J. I. McDonald , S. Srinivasan

Axion dark matter can resonantly convert into photons in the magnetospheres of neutron stars (NSs). It has recently been shown that radio observations of nearby NSs can therefore provide a highly sensitive probe of the axion parameter…

高能物理 - 唯象学 · 物理学 2020-06-03 Mikaël Leroy , Marco Chianese , Thomas D. P. Edwards , Christoph Weniger

It has been suggested that radio telescopes may be sensitive to axion dark matter that resonantly converts to radio photons in the magnetospheres surrounding neutron stars (NSs). In this work, we closely examine this possibility by…

宇宙学与河外天体物理 · 物理学 2019-07-03 Benjamin R. Safdi , Zhiquan Sun , Alexander Y. Chen

The potential to detect axion dark matter through astrophysical processes has shown high promise in recent years. We therefore expand on previous work studying the axion-to-photon conversion efficacy of neutron stars and the interstellar…

高能天体物理现象 · 物理学 2026-05-15 Felix Weber , Vikram Ravi

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…

高能天体物理现象 · 物理学 2025-03-19 Jesse Satherley , Chris Gordon , Chris Stevens

Axion dark matter (DM) is predicted to convert into radio waves in neutron star magnetospheres. We assess the detectability of this signal using a 5 m radio telescope to be installed at the Fan Mountain Observatory, operating in the UHF, L-…

Axion dark matter (DM) may efficiently convert to photons in the magnetospheres of neutron stars (NSs), producing nearly monochromatic radio emission. This process is resonantly triggered when the plasma frequency induced by the underlying…

宇宙学与河外天体物理 · 物理学 2022-12-28 Joshua W. Foster , Samuel J. Witte , Matthew Lawson , Tim Linden , Vishal Gajjar , Christoph Weniger , Benjamin R. Safdi

We study the radio signals generated when an axion star enters the magnetosphere of a neutron star. As the axion star moves through the resonant region where the plasma-induced photon mass becomes equal to the axion mass, the axions can…

高能天体物理现象 · 物理学 2021-02-25 James H. Buckley , P. S. Bhupal Dev , Francesc Ferrer , Fa Peng Huang

Axion dark matter passing through the magnetospheres of magnetars can undergo hyper-efficient resonant mixing with low-energy photons, leading to the production of narrow spectral lines that could be detectable on Earth. Since this is a…

高能物理 - 唯象学 · 物理学 2025-05-28 Sandip Roy , Anirudh Prabhu , Christopher Thompson , Samuel J. Witte , Carlos Blanco , Jonathan Zhang

Dark photon dark matter that has a kinetic mixing with the Standard Model photon can resonantly convert in environments where its mass $m_{A'}$ coincides with the plasma frequency. We show that such conversion in neutron stars or accreting…

高能物理 - 唯象学 · 物理学 2023-09-14 Edward Hardy , Ningqiang Song

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…

高能天体物理现象 · 物理学 2018-04-11 Yang Bai , Yuta Hamada

One of the promising new proposals to search for axions in astrophysical environments is to look for narrow radio lines produced from the resonant conversion of axion dark matter falling through the magnetospheres of neutron stars. For…

高能物理 - 唯象学 · 物理学 2024-01-05 Jonas Tjemsland , Jamie McDonald , Samuel J. Witte

Axion dark matter can be converted into photons in the magnetospheres of neutron stars leading to a spectral line centred on the Compton wavelength of the axion. Due to the rotation of the star and the plasma effects in the magnetosphere…

宇宙学与河外天体物理 · 物理学 2023-11-29 R. A. Battye , M. J. Keith , J. I. McDonald , S. Srinivasan , B. W. Stappers , P. Weltevrede

Axions provide a natural and well-motivated dark matter candidate, with the capability to convert directly to photons in the presence of an electromagnetic field. A particularly compelling observational target is the conversion of dark…

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