EAS Publications Series
Volume 30, 2008Spanish Relativity Meeting - Encuentros Relativistas Españoles , ERE2007: Relativistic Astrophysics and Cosmology
|Page(s)||137 - 140|
|Published online||30 September 2008|
A. Oscoz, E. Mediavilla and M. Serra-Ricart (eds)
EAS Publications Series, 30 (2008) 137-140
Properties of double neutron stars
Institute of Astronomy, University of Zielona Góra, Lubuska 2, 65-265 Zielona Góra,
Poland; e-mail: firstname.lastname@example.org
2 LUTH, Observatoire de Paris, Université Paris 7, Place Jules Janssen, 92195 Meudon Cedex, France
3 Astronomical Observatory, The University of Warsaw Al Ujazdowskie 4, 00-478 Warsaw, Poland
4 CAMK,PAN, Bartycka 18, Warsaw, Poland
5 MPI Garching, Germany
6 Los Alamos National Laboratory, New Mexico, USA
We summarize our studies on properties of double neutron stars observable in gravitational waves and in the radio. Binary population synthesis is used to calculate expected masses of neutron stars in binary systems taking into account the selection efects specific to each method of detection. We discuss recent relativistic results on final phase of inspiral of neutron star binaries showing how we can impose constraints on the equation of state of dense nuclear matter with gravitational wave observations.
© EAS, EDP Sciences, 2008
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