Interferometric Measurement of Acceleration at Relativistic Speeds
Pierre Christian, Abraham Loeb

TL;DR
This paper proposes a relativistic interferometric accelerometer that is highly sensitive, robust, and capable of measuring planetary and galactic masses during interstellar missions.
Contribution
It introduces a novel interferometric accelerometer design that operates at relativistic speeds without moving parts, enhancing robustness and measurement capabilities.
Findings
Sensitive detection of acceleration at relativistic speeds
Potential for interstellar planetary mass measurements
Robust design with no moving parts
Abstract
We show that an interferometer moving at a relativistic speed relative to a point source of light offers a sensitive probe of acceleration. Such an accelerometer contains no moving parts, and is thus more robust than conventional "mass-on-a-spring" accelerometers. In an interstellar mission to Alpha-Centauri, such an accelerometer could be used to measure the masses of planets around other stars as well as the mass distribution of the Milky Way Galaxy.
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