Radio pulsars: testing gravity and detecting gravitational waves
Delphine Perrodin, Alberto Sesana

TL;DR
Pulsar timing leverages the extreme regularity of pulsar signals to test gravity theories and detect gravitational waves, offering insights into fundamental physics and the universe's structure.
Contribution
This paper provides a comprehensive review of pulsar timing applications in testing gravity and detecting gravitational waves, including current results and future prospects.
Findings
Pulsar timing confirms predictions of general relativity in strong fields.
Ensemble pulsar observations can detect low-frequency gravitational waves.
Pulsar timing constrains alternative theories of gravity.
Abstract
Pulsars are the most stable macroscopic clocks found in nature. Spinning with periods as short as a few milliseconds, their stability can supersede that of the best atomic clocks on Earth over timescales of a few years. Stable clocks are synonymous with precise measurements, which is why pulsars play a role of paramount importance in testing fundamental physics. As a pulsar rotates, the radio beam emitted along its magnetic axis appears to us as pulses because of the lighthouse effect. Thanks to the extreme regularity of the emitted pulses, minuscule disturbances leave particular fingerprints in the times-of-arrival (TOAs) measured on Earth with the technique of pulsar timing. Tiny deviations from the expected TOAs, predicted according to a theoretical timing model based on known physics, can therefore reveal a plethora of interesting new physical effects. Pulsar timing can be used to…
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