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Axion-photon conversion is a prime mechanism to detect axion-like particles that share a coupling to the photon. We point out that in the vicinity of neutron stars with strong magnetic fields, magnetars, the effective photon mass receives…

高能物理 - 唯象学 · 物理学 2023-10-10 Kyrylo Bondarenko , Alexey Boyarsky , Josef Pradler , Anastasia Sokolenko

Recent experiments suggest that polarized photons may couple significantly to pseudoscalar particles such as axions. We study the possible observational signatures of axion-photon coupling for radiation from magnetic stars, with particular…

天体物理学 · 物理学 2008-11-26 Dong Lai , Jeremy Heyl

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

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

Neutron stars provide ideal astrophysical laboratories for probing new physics beyond the Standard Model. If axions exist, photons can develop linear polarization during photon-axion conversion in the magnetic field of a neutron star. We…

高能物理 - 唯象学 · 物理学 2025-02-12 Ningqiang Song , Liangliang Su , Lei Wu

We show that axion dark matter (DM) may be detectable through narrow radio lines emitted from neutron stars. The neutron star magnetosphere hosts a strong magnetic field and a plasma frequency that increases towards the neutron star…

高能物理 - 唯象学 · 物理学 2018-12-19 Anson Hook , Yonatan Kahn , Benjamin R. Safdi , Zhiquan Sun

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

Axion-like particles can be abundantly produced through scattering processes in the cores of neutron stars (NSs). If they are ultralight ($m_a \lesssim 10^{-4}$ eV), then they can efficiently convert to detectable photons in the external NS…

高能物理 - 唯象学 · 物理学 2025-12-19 Orion Ning , Kailash Raman , Benjamin R. Safdi

Gravitationally bound clumps of dark matter axions in the form of 'miniclusters' or even denser 'axion stars' can generate strong radio signals through axion-photon conversion when encountering highly magnetised neutron star magnetospheres.…

高能物理 - 唯象学 · 物理学 2023-03-29 Samuel J. Witte , Sebastian Baum , Matthew Lawson , M. C. David Marsh , Alexander J. Millar , Gustavo Salinas

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

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

We investigate the form of the radiation emitted by an axion star-neutron star binary using a $f(r)=\text{sech(r/R)}$ profile for the axion star. Our analysis takes into account the co-rotating plasma of the neutron star. We find that that…

高能物理 - 唯象学 · 物理学 2022-11-16 A. Kyriazis

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

Axions may make a significant contribution to the dark matter of the universe. It has been suggested that these dark matter axions may condense into localized clumps, called "axion stars." In this paper we argue that collisions of dilute…

高能物理 - 唯象学 · 物理学 2016-12-09 Stuart Raby

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

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

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

Axions are increasingly favoured as a candidate particle for the dark matter in galaxies, since they satisfy the observational requirements for cold dark matter and are theoretically well motivated. Fluctuations in the axion field give rise…

高能天体物理现象 · 物理学 2018-11-28 Tim Dietrich , Francesca Day , Katy Clough , Michael Coughlin , Jens Niemeyer

Black holes in binaries with other compact objects can provide natural venues for indirect detection of axions or other ultralight fields. The superradiant instability associated with a rapidly spinning black hole leads to the creation of…

高能天体物理现象 · 物理学 2020-08-10 Michael Kavic , Steven L. Liebling , Matthew Lippert , John H. Simonetti

We describe the possible electromagnetic signals expected from the magnetospheric interactions of a neutron star binary prior to merger. We find that both radio and X-ray signals of detectable strength are possible. We discuss possible…

天体物理学 · 物理学 2009-10-31 Brad M. S. Hansen , Maxim Lyutikov
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