Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010iaus..261..124p&link_type=abstract
Relativity in Fundamental Astronomy: Dynamics, Reference Frames, and Data Analysis, Proceedings of the International Astronomica
Astronomy and Astrophysics
Astronomy
Gravitation, Relativity, Methods: Analytical, Numericical
Scientific paper
The LISA mission is an interferometer, formed by three spacecraft, that aims at the detection of gravitational waves in the [10-4, 10-1] Hz frequency band. Present LISA TDI simulators, aimed at validating the novel Time Delay Interferometry method, use a classical Keplerian orbit model at first order in eccentricity in the gravitational field of a spherical non-rotating Sun, without planets. We propose to use the same model but described in the framework of relativistic gravity, and we focus here on quantifying the differences between classical and relativistic orbits for the LISA spacecraft, under the same assumptions.
Chauvineau Bertrand
Pireaux Sophie
No associations
LandOfFree
A relativistic orbit model for the LISA mission to be used in LISA TDI simulators 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 A relativistic orbit model for the LISA mission to be used in LISA TDI simulators, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A relativistic orbit model for the LISA mission to be used in LISA TDI simulators will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1447037