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In this paper by executing both analytical and numerical methods, we discuss about the resulting changes in polarization with photon path-length provide critical insights into the properties of the magnetic field B and the axion-photon coupling strength \(g_{\phi ^{\prime }\gamma \gamma }\) . We explore the impact of various parameters, such as magnetic field B, photon energy \(\omega \) and plasma frequency \(\omega _{p}\) on the polarization angle. Following the methods of [1] our findings suggest that measuring the polarization angle in this context can serve as a powerful tool for probing the nature of axions and the magnetic environments of compact stars, contributing to the broader understanding of dark matter and fundamental physics.

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Polarimetric Investigation of High Energy Photons Carrying Imprints of Axions

  • 会议论文

  • 发表日期：

    2025年

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  • Ankur Chaubey,
  • Avijit K. Ganguly

摘要

In this paper by executing both analytical and numerical methods, we discuss about the resulting changes in polarization with photon path-length provide critical insights into the properties of the magnetic field B and the axion-photon coupling strength \(g_{\phi ^{\prime }\gamma \gamma }\) . We explore the impact of various parameters, such as magnetic field B, photon energy \(\omega \) and plasma frequency \(\omega _{p}\) on the polarization angle. Following the methods of [1] our findings suggest that measuring the polarization angle in this context can serve as a powerful tool for probing the nature of axions and the magnetic environments of compact stars, contributing to the broader understanding of dark matter and fundamental physics.