CORDIS Project
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This project explores the time variability of pulsar radio emissions and the evolution of pulsar magnetic fields. By leveraging large datasets and machine learning, it aims to enhance our understanding of neutron star physics and improve gravitational wave detection methods.
Why is pulsar radio emission time-variable?
How does the pulsar magnetic field evolve over its lifetime?
The answers will change the landscape of fundamental physics, advancing our understanding of the universe’s most extreme environments and transforming the search for gravitational waves with pulsar timing arrays.
Pulsars are spinning magnetized neutron stars emitting a beam of radio waves, and this radio beam is our direct observational link to an environment with some of the highest densitie…
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