ERC Consolidator Grant · 2019
Advancing the Equation of state of Neutron Stars
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 structure equations to quantities like mass M and radius R that determine the exterior space-time. One very promising technique for measuring the EOS exploits hotspots that form on the NS surface due…
From the public funding record at EU CORDIS. Describes the funded project, not the reviews below.