CORDIS Project
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MAGNESIA aims to create a comprehensive model of neutron stars, particularly magnetars, to better understand their population and flaring rates. By integrating multi-band observations and advanced modeling techniques, the project seeks to clarify the role of these stars in cosmic events.
The gravitational wave window is now open.
It is then imperative to build quantitative models of neutron stars that use all the available tracers to constrain fundamental physics at the highest densities and magnetic fields.
The most magnetic neutron stars, the magnetars, have been recently suggested to be powering a large variety of explosive and transient events.
The enormous rotational power at birth, and the magnetic energy they can release via large flares, put the magnetars in the (yet) ha…
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