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The DIANA project aims to study the structure and evolution of accretion disks around neutron stars using advanced observational techniques. By combining X-ray polarization measurements with optical-infrared observations, it seeks to understand the instabilities in these disks and their implications for astrophysics.
Astrophusical accretion disks are the main engine of most of high energy sources.
Although they have been studies for decades, we still do not know their exact structure and their evolution with luminosity. A clear example is at high luminosity, for which our best theory predicts the presence in all sources of an instability which leads to the cyclic disruption/rebuilding of the disk.
However, from the observational point of view, we have observed only a handful of accreting black holes.
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ISTITUTO NAZIONALE DI ASTROFISICA
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