Physics of Neutron Stars as Gravitational Wave SourcesRome, January 25, 2010 Department of Physics, University of Rome "Sapienza", Italy
Neutron stars are among the most promising sources of gravitational waves.
In this workshop, preliminary to the GWDAW-14, we would like to bring together experts
in neutron star modelling and astrophysicists with the gravitational wave data analysis community.
The meeting will be held in in Rome, Italy. It will take place at the Department of Physics of the "Sapienza"
University of Rome, one day prior to the start of the 14th Gravitational Wave Data Analysis Workshop (GWDAW).
This webpage provides information on this meeting.
Credit: NASA/CXC/SAO/F.Seward et al.
Nils Andersson (Southampton University, U.K.)
Omar Benhar (Sapienza University, Rome, Italy)
Marta Burgay (Astronomic Observatory of Cagliari, Italy)
Leonardo Gualtieri (Sapienza University, Rome, Italy)
Kostas Kokkotas (University of Tubingen, Germany)
Luigi Stella (Monte Porzio Observatory, Rome, Italy)