Special Session SS26
26 June 2019
Understanding the interior composition of neutron stars is an important goal of astrophysics and fundamental physics. By mid-2019, the promising results of the Neutron Star Interior Composition ExploreR mission (NICER) on the dense matter equation of state will be available. Around that time, run O3 of the LIGO/Virgo collaboration will be in progress (or completed) with several expected new NS-NS mergers discoveries.
We would like to cover EOS Constraints from:
Sebastien Guillot (IRAP), Fiorella Burgio (INFN Catania), Alessandro Drago (U Ferrara), Mark Alford (U Wash. St. Louis), Luciano Rezzolla (ITP Frankfurt), Jérôme Margueron (IPNL), Laura Tolos (ICE), Sebastiano Bernuzzi (TPI Jena), Veronica Dexheimer (Kent U.), Adrianna Raduta (NIPNE), Pierre Pizzochero (INFN Milano), Morgane Fortin (CAMK), Dipankar Bhattacharya (IUCAA), Nanda Rea (ICE), Tanja Hinderer (UvA), Anna Watts (UvA).
Updated on Mon Apr 15 13:49:52 CEST 2019
European Week of Astronomy and Space Science / The annual meeting of the EAS