Numerical relativity with LORENE: the study of gravitational wave sources

Details Numerical relativity with LORENE: the study of gravitational wave sources Numerical relativity with LORENE: the study of gravitational wave sources

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005sf2a.conf..739n&link_type=abstract

SF2A-2005: Semaine de l'Astrophysique Francaise, meeting held in Strasbourg, France, June 27 - July 1, 2005, Edited by F. Casoli

Astronomy and Astrophysics

Astrophysics

Scientific paper

The data coming now from interferometric detectors of gravitational waves (VIRGO or LIGO) must be analysed using the best possible knowledge of the astrophysical sources. This is the goal of our group of numerical relativity which aims at a precise modelling of astrophysical sources containing compact objects (neutron stars or black holes). After a brief description of these aspects, we present numerical methods used in our group and, in particular, our numerical library LORENE. Finally, some recent results about the solution of dynamical 3D Einstein equations are given.

Affiliated with

Also associated with

No associations

Rating

Numerical relativity with LORENE: the study of gravitational wave sources does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Numerical relativity with LORENE: the study of gravitational wave sources, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Numerical relativity with LORENE: the study of gravitational wave sources will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1460881