Testing the Weak Equivalence Principle using Optical and Near-Infrared Crab Pulses
Calvin Leung, Beili Hu, Sophia Harris, Amy Brown, Hien Nguyen, and, Jason Gallicchio

TL;DR
This study tests the Weak Equivalence Principle by measuring pulse arrival times from the Crab Pulsar in optical and near-infrared wavelengths, setting a new upper limit on potential violations with high precision.
Contribution
It provides the first upper limit on the differential post-Newtonian parameter at optical and near-infrared wavelengths, using pulsar timing to constrain equivalence principle violations.
Findings
Infrared pulses arrive slightly before visible pulses.
Statistical errors in delay measurements are below microsecond level.
The upper limit on the differential post-Newtonian parameter is Δγ < 1.07×10⁻¹⁰ (3σ).
Abstract
The Weak Equivalence Principle states that the geodesics of a test particle in a gravitational field are independent of the particle's constitution. To constrain violations of the Weak Equivalence Principle, we use the one-meter telescope at Table Mountain Observatory near Los Angeles to monitor the relative arrival times of pulses from the Crab Pulsar in the optical ( nm) and near-infrared ( nm) using an instrument which detects single photons with nanosecond-timing resolution in those two bands. The infrared pulse arrives slightly before the visible pulse. Our three analysis methods give delays with statistical errors of , , and microseconds (at most 1/4000 of the pulsar period). We attribute this discrepancy to systematic error from the fact that the visible and infrared pulses have…
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