CORDIS Project
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The AEONS project investigates the extreme conditions within neutron star cores to understand their composition and behavior. By utilizing advanced pulse profile modeling techniques, it aims to refine measurements of neutron star mass and radius, enhancing our knowledge of dense matter physics.
Densities in neutron star (NS) cores can reach up to ten times the density of a normal atomic nucleus, and the stabilising effect of gravitational confinement permits long-timescale weak interactions.
This generates nucleonic matter that is extremely neutron-rich, and the exciting possibility of stable states of strange matter (hyperons or deconfined quarks).
Our uncertainty about the nature of cold ultradense matter is encoded in the Equation of State (EOS), which can be mapped via the stellar…
UNIVERSITEIT VAN AMSTERDAM
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