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Relativistic damping of laser-beam-driven light sails

Rhys Mackintosh, Jadon Y. Lin, Michael S. Wheatland, and Boris T. Kuhlmey
Phys. Rev. Applied 21, 064032 – Published 13 June 2024
This article was published on 13 June 2024. Please update your links.

Abstract

Light sails using Earth-based lasers for propulsion require passive stabilization to stay within the beam. This can be achieved through the scattering properties of the sail, creating optical restoring forces and torques. Undamped restoring forces produce uncontrolled oscillations, which could jeopardize the mission, but it is not obvious how to achieve damping in the vacuum of space. Using a simple two-dimensional model, we show that the Doppler effect and relativistic aberration of the propelling laser beam create damping terms in the optical forces and torques. The effect is similar to the Poynting-Robertson effect causing loss of orbital momentum of dust particles around stars but can be enhanced by design of the geometry of the sail.

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  • Received 30 January 2024
  • Accepted 17 May 2024

DOI:https://doi.org/10.1103/PhysRevApplied.21.064032

© 2024 American Physical Society

Physics Subject Headings (PhySH)

Atomic, Molecular & OpticalGravitation, Cosmology & Astrophysics

Authors & Affiliations

Rhys Mackintosh, Jadon Y. Lin, and Michael S. Wheatland

Boris T. Kuhlmey*

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Issue

Vol. 21, Iss. 6 — June 2024

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