Skip to Main content Skip to Navigation
Journal articles

Data analysis challenges for the Einstein Telescope

L. Bosi E.K. Porter 1
1 APC-Gravitation - APC - Gravitation
APC (UMR_7164) - AstroParticule et Cosmologie, AEI - Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut )
Abstract : 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.
Complete list of metadatas
Contributor : Edward K Porter <>
Submitted on : Monday, June 11, 2012 - 7:01:45 PM
Last modification on : Wednesday, October 21, 2020 - 4:32:14 PM

Links full text



L. Bosi, E.K. Porter. Data analysis challenges for the Einstein Telescope. General Relativity and Gravitation, Springer Verlag, 2011, 43, pp.519-535. ⟨10.1007/S10714-010-1084-3⟩. ⟨in2p3-00707017⟩



Record views