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    • Chiral symmetry restoration and deconfinement in neutron stars 

      Dexheimer, Verônica Antocheviz (Univ. Frankfurt (Main), 2009)
      Neutron stars are very dense objects. One teaspoon of their material would have a mass of five billion tons. Their gravitational force is so strong that if an object were to fall from just one meter high it would hit the ...
    • Multi-telescope studies of neutron stars 

      Lazaridis, Kosmas (Univ. Köln, 2009)
      Neutron stars are unique stellar remnants with extreme properties, as their density and magnetic field. Their study can be the key to a number of unanswered problems in fundamental physics and astronomy, ranging from stellar ...