Satellite Meetings

Stabilisation of Parametric Instabilities in Advanced Gravitational Wave Detectors
Perth, 16-18 July 2007
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BARMODE INSTABILITY IN A NEUTRON STAR
Credit: Rezzolla (AEI) / Giacomazzo (SISSA)

Main banner captions:

image 1: 'Distribution of detached white-dwarf–white-dwarf binaries in our galaxy as a function of the gravitational wave frequency and chirp mass.' from Simulation of the white dwarf–white dwarf galactic background in the LISA data Jeffrey A Edlund, Massimo Tinto, Andrzej Królak, and Gijs Nelemans 2005 Class. Quantum Grav. 22 S913-S926

image 2: 'A three-dimensional visualization of the mesh including the excised region and the refinement around the particle.', from A toy model for testing finite element methods to simulate extreme-mass-ratio binary systems Carlos F Sopuerta, Pengtao Sun Pablo Laguna and Jinchao Xu 2006 Class. Quantum Grav. 23 251-285

image 3: 'Scalar gravitational field > at time t = 140M (n = 30 000).', from A toy model for testing finite element methods to simulate extreme-mass-ratio binary systems Carlos F Sopuerta, Pengtao Sun Pablo Laguna and Jinchao Xu 2006 Class. Quantum Grav. 23 251-285