Scientific Program

Click here for the Program at a Glance.

Click here to view the full concurrent program (subject to change)

Poster Presentation Information

• Your poster should be completely prepared before you arrive at the Conferences.
• The maximum size your poster can be is 1m x 1.2m
• You will be provided with a ‘poster number’ and information regarding where your poster is to be displayed upon registering at the Conferences.
• The posters are to be mounted on poster boards using velcro dots. You may supply these yourself or purchase them at the registration desk for 0.20 cents per dot.
• The posters will be displayed all week in various locations throughout the Conference venue.
• The poster session will be held on Wednesday 11 July from 12.30pm – 2.00pm where you will have the opportunity to discuss your poster findings.

If you require further information regarding your poster presentation please contact the Conference Secretariat on program@grg18.com

VISUALISATION OF A GRAVITATIONAL WAVE HAVING TEUKOLSKY'S SOLUTION AS INITIAL DATA
Credit: Seidel (AEI) / Benger (ZIB)

ROLLER COASTER DISTORTED BY SPECIAL RELATIVISTIC EFFECTS
Credit: Michael Hush, Department of Physics, The Australian National University

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