Axion search with telescope for radio astronomy (ASTRA): forecast for observations between 0.5 and 4~GHz
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| Main Authors: | , , , , , , , , , , |
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| Format: | Preprint |
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2026
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| _version_ | 1866911512924258304 |
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| author | Bhura, Utkarsh Marsh, David J. E. Johnson, Bradley R. van Bibber, Karl Helfenbein, Mallory Kavanagh, Bradley J. Nelson, Matthew O'Hare, Ciaran A. J. Pierobon, Giovanni Rybka, Gray Visinelli, Luca |
| author_facet | Bhura, Utkarsh Marsh, David J. E. Johnson, Bradley R. van Bibber, Karl Helfenbein, Mallory Kavanagh, Bradley J. Nelson, Matthew O'Hare, Ciaran A. J. Pierobon, Giovanni Rybka, Gray Visinelli, Luca |
| contents | 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- and S-bands from 0.5 to 4~GHz. We demonstrate that such a telescope can search new parameter space for axion-like particles over a broad range from $2\,μ\text{eV}<m_a<17\,μ\text{eV}$ for axion-photon couplings $g_{aγγ} \gtrsim 2\times 10^{-12}\text{ GeV}^{-1}$ with a three year observing period assuming the standard halo model -- improving neutron star observations by more than an order of magnitude. The search is broadband and is thus complementary to other techniques in the same frequency range. We describe in detail our neutron star population model, noise model, and proposed observing strategy. Most constraining power comes from neutron stars at the Galactic centre, where the smooth DM halo is densest. If a DM spike exists at the Galactic centre, the search is sensitive in the QCD axion model band. UHF and L-band observations (0.5 to 2~GHz) represent the pathfinder phase of a wider program we call ``Axion Search with Telescope for Radio Astronomy'' (ASTRA). Future higher mass searches aimed at discovery potential for the post-inflation axion require further hardware development to cover S, C, X and Ku bands (2 to 18~GHz). |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2603_13194 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Axion search with telescope for radio astronomy (ASTRA): forecast for observations between 0.5 and 4~GHz Bhura, Utkarsh Marsh, David J. E. Johnson, Bradley R. van Bibber, Karl Helfenbein, Mallory Kavanagh, Bradley J. Nelson, Matthew O'Hare, Ciaran A. J. Pierobon, Giovanni Rybka, Gray Visinelli, Luca High Energy Physics - Phenomenology Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies High Energy Physics - Experiment 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- and S-bands from 0.5 to 4~GHz. We demonstrate that such a telescope can search new parameter space for axion-like particles over a broad range from $2\,μ\text{eV}<m_a<17\,μ\text{eV}$ for axion-photon couplings $g_{aγγ} \gtrsim 2\times 10^{-12}\text{ GeV}^{-1}$ with a three year observing period assuming the standard halo model -- improving neutron star observations by more than an order of magnitude. The search is broadband and is thus complementary to other techniques in the same frequency range. We describe in detail our neutron star population model, noise model, and proposed observing strategy. Most constraining power comes from neutron stars at the Galactic centre, where the smooth DM halo is densest. If a DM spike exists at the Galactic centre, the search is sensitive in the QCD axion model band. UHF and L-band observations (0.5 to 2~GHz) represent the pathfinder phase of a wider program we call ``Axion Search with Telescope for Radio Astronomy'' (ASTRA). Future higher mass searches aimed at discovery potential for the post-inflation axion require further hardware development to cover S, C, X and Ku bands (2 to 18~GHz). |
| title | Axion search with telescope for radio astronomy (ASTRA): forecast for observations between 0.5 and 4~GHz |
| topic | High Energy Physics - Phenomenology Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies High Energy Physics - Experiment |
| url | https://arxiv.org/abs/2603.13194 |