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    Relativistic Maxwell-Bloch equations with applications to astrophysics

    Ningyan Fang

    Victor Botez

    Fereshteh Rajabi

    Martin Houde*

    • Department of Physics and Astronomy, McMaster University, 1280 Main Street West, Hamilton, Ontario, Canada L8S 4L8

    • *Contact author: mhoude2@uwo.ca

    Phys. Rev. A 113, 043711 – Published 6 April, 2026

    DOI: https://doi.org/10.1103/3dqj-hrht

    Abstract

    We derive relativistic Maxwell-Bloch equations for potential applications in astronomical environments, where various radiative processes are known to occur, including the maser action and Dicke's superradiance. We show that for both phenomena a radiating system's response is preserved at different relative velocities between the system's rest frame and the observer, while the relevant timescales and the radiation intensity transform as expected from relativistic considerations. We verify that the level of coherence between groups of emitters traveling at different speeds is unchanged in all reference frames. We also derive relativistic versions of the maser equations applicable in the steady-state regime.

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