Physics of Neutron Stars as Gravitational Wave Sources

Rome, 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).
 T
his webpage provides information on this meeting.

Credit: NASA/CXC/SAO/F.Seward et al.
Scientific committee:

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)