Data Analysis Challenges for the Einstein Telescope

Details Data Analysis Challenges for the Einstein Telescope Data Analysis Challenges for the Einstein Telescope

2009-10-02

arxiv.org/abs/0910.0380v1

Gen.Rel.Grav.43:519-535,2011

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

18 pages, Invited review for Einstein Telescope special edition of GRG

Scientific paper

10.1007/s10714-010-1084-3

The Einstein Telescope is a proposed third generation gravitational wave detector that will operate in the region of 1 Hz to a few kHz. As well as the inspiral of compact binaries composed of neutron stars or black holes, the lower frequency cut-off of the detector will open the window to a number of new sources. These will include the end stage of inspirals, plus merger and ringdown of intermediate mass black holes, where the masses of the component bodies are on the order of a few hundred solar masses. There is also the possibility of observing intermediate mass ratio inspirals, where a stellar mass compact object inspirals into a black hole which is a few hundred to a few thousand times more massive. In this article, we investigate some of the data analysis challenges for the Einstein Telescope such as the effects of increased source number, the need for more accurate waveform models and the some of the computational issues that a data analysis strategy might face.

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