Direct Measurement of Radiation Pressure Forces on Membrane Lightsails
ORAL
Abstract
Ultrathin lightsails, propelled to relativistic speeds by laser radiation pressure, are being actively explored as a new generation of interstellar spacecraft probes, spearheaded by the Breakthrough Starshot Initiative. Realizing laser-driven lightsails necessitates precise characterization of the optical forces on a material platform capable of exhibiting mechanical, beam-riding, and thermal stability.
We performed sensitive force measurements that rely on three key components: a noise-robust common-path interferometer with picometer resolution, rational design of the tethered lightsail for enhanced mechanical susceptibility, and an off-resonant driving scheme for quasi-static, linear dynamics. For a laser power density of 200 W/cm2 at 514 nm, we measure displacements of ~10 pm, resulting from optical forces of ~30 fN. Contrary to optical trapping of microscopic objects, motion is induced by a collimated laser beam filling substantial part of the lightsail, mimicking the initial acceleration stage of interstellar lightsails. Furthermore, to predict the tilt-dependent dynamics of subwavelength thick lightsails, we characterize the nonintuitive trend of the optical force versus incidence angle in the range of ±20° for TE and TM polarization. Our study represents a critical milestone in realizing an experimental testbed for lightsail characterization, thus advancing the development of laser-driven spacecraft, and opening the door for manipulation of macroscopic objects through optical forces.
L.M. and R.G. contributed equally to this work.
We performed sensitive force measurements that rely on three key components: a noise-robust common-path interferometer with picometer resolution, rational design of the tethered lightsail for enhanced mechanical susceptibility, and an off-resonant driving scheme for quasi-static, linear dynamics. For a laser power density of 200 W/cm2 at 514 nm, we measure displacements of ~10 pm, resulting from optical forces of ~30 fN. Contrary to optical trapping of microscopic objects, motion is induced by a collimated laser beam filling substantial part of the lightsail, mimicking the initial acceleration stage of interstellar lightsails. Furthermore, to predict the tilt-dependent dynamics of subwavelength thick lightsails, we characterize the nonintuitive trend of the optical force versus incidence angle in the range of ±20° for TE and TM polarization. Our study represents a critical milestone in realizing an experimental testbed for lightsail characterization, thus advancing the development of laser-driven spacecraft, and opening the door for manipulation of macroscopic objects through optical forces.
L.M. and R.G. contributed equally to this work.
* This work was supported by the Air Force Office of Scientific Research under grant FA2386-18-1-4095 and the Breakthrough Initiatives, a division of the Breakthrough Prize Foundation. L.M. acknowledges support of the Fulbright Israel Postdoctoral Fellowship.
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Presenters
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Ramon Gao
Caltech
Authors
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Lior Michaeli
Caltech
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Ramon Gao
Caltech
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Michael D Kelzenberg
Caltech
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Claudio U Hail
Caltech
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John E Sader
Caltech
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Harry A Atwater
Caltech