Amaldi7 Program

Click here for the Program at a Glance.

Amaldi7 Workshops

	Monday 9 July	Tuesday 10 July	Wednesday 11 July	Thursday 12 July	Friday 13 July	Saturday 14 July
08.30 - 10.30						Data Analysis for Ground Based GW Detectors: Methods and Issues
10.30 - 11.00
11.00 - 13.00						R&D for Advanced Ground Based GW Detectors - Bars, Spheres, Other
14.00 - 18.30	Status of Current GW Detectors	GW Sources		LISA	Data Analysis for Ground Based GW Detectors: Methods and Searches	R&D for Advanced Ground Based GW Detectors - Laser Interferometers
19.00 - 21.00				Future GW Detectors

Amaldi7 Workshop Chairs

M1 Status of Current GW Detectors – David Blair
M2 R&D for Advanced Ground Based GW Detectors

a) Laser Interferometers – Raffaele Flaminio
b) Bars, Spheres, Other – Giorgio Frossati

M3 Future GW Detectors - Seiji Kawamura
M4 GW Sources – Graham Woan
M5 Data Analysis for Ground Based GW Detectors: Methods and Searches – Frederique Marion
M6 Data Analysis for Ground Based GW Detectors: Methods and Issues – Peter Saulson
M7 LISA – Stefan Vitale

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