Programme


News: A number of presentations (but unfortunately not all) are now available on the web: click on individual titles to see if the presentation is available.


Click here for the conference booklet (PDF, 253kB)

Click here for a list of participants.


THURSDAY 26 August

8:30 - 9:20 Registration (Foyer, basement level, Maths building)
9:20 - 9:30 Opening remarks (David Wiltshire)
9:30 - 9:40 Official welcome (Roy Sharp, Vice-Chancellor)
PLENARY TALKS:
9:40 - 10:30 Brandon Carter [CNRS, Paris-Meudon, France]
Global and local problems with Kerr's solution
10:30 - 11:10 Coffee
11:10 - 12:00 Maurice van Putten [LIGO / MIT, USA]
The endpoint of binary evolution: Singlets, doublets? Triplets!
12:00- 1:30 Lunch
PLENARY TALK:
1:30 - 2:20 Gary Horowitz [U California, Santa Barbara, USA]
Higher dimensional generalizations of the Kerr black hole
CONTRIBUTED TALKS:
2:20 - 2:45 Ishwaree Neupane [U Canterbury, New Zealand]
Anti-de Sitter/de Sitter correspondence and twisting S-branes
2:45 - 3:10 Michael Kuchiev [UNSW, Australia]
Reflection from the horizon of black holes
3:10 - 3:35 Victor Flambaum [UNSW, Australia]
Reflection on the horizon and absorption of scalar particles by black holes
3:35 - 4:05 Coffee
4:05 - 4:30 Gabriela Slezakova [U Waikato, New Zealand]
Geodesics of Kerr black holes
4:30 - 4:55 Stephen Fletcher [Monash U, Australia]
Novikov coordinates for the Kerr spacetime
5:15 - 6:15 Welcome Reception (Physics and Astronomy, Room 701)
8:00 - 9:?? Public Lecture (Lecture Theatre C1)
Fulvio Melia [U Arizona, USA]
The supermassive black hole at the centre of our galaxy


FRIDAY 27 August

PLENARY TALKS:
9:00 - 9:50 Josh Goldberg [Syracuse U, USA]
Gravity and general relativity
9:50 - 10:40 Susan Scott [ANU, Australia]
Can the Milky Way be weighed using Earth-based interferometry?
10:40 - 11:10 Coffee
11:10 - 12:00 Andy Fabian [IOA, U Cambridge, UK]
Effects of strong gravity on X-ray spectra: observational evidence for Kerr black holes
12:00 - 1:30 Lunch
PLENARY TALK:
1:30 - 2:20 Steve Carlip [U California, Davis, USA]
Horizon constraints and black hole entropy
CONTRIBUTED TALKS:
2:20 - 2:45 Joey Medved [VUW, New Zealand]
The quantum Kerr black hole
2:45 - 3:10 Stuart Wyithe [U Melbourne, Australia]
Formation and evolution of early super-massive black holes
3:10 - 3:35 Andrew Melatos [U Melbourne, Australia]
Gravitational waves from X-ray millisecond pulsars with a polar magnetic mountain
3:35 - 3:45 Group photo (assemble steps at MCSC main door)
3:45 - 4:15 Coffee
4:15 - 4:40 Andrew Moylan [ANU, Australia]
Visualisation in the Kerr space-time using GRworkbench
4:40 - 5:05 Sung-Won Kim [Ewha Women's University, Korea]
The Kerr metric and rotating wormhole
5:05 - 5:30 Anthony Lun [Monash U, Australia]
On continued contraction of a rotating dust cloud to form a Kerr black hole
SPECIAL TALK:
5:30 - 6:00 Roy Kerr [U Canterbury, New Zealand]
Reminiscences: a personal spin on black holes
7:00-? Banquet: University Staff Club, Ilam Homestead.


SATURDAY 28 August

PLENARY TALKS:
9:00 - 9:50 David Robinson [Kings College, London, UK]
Four decades of black hole uniqueness theorems
9:50 - 10:40 Remo Ruffini [ICRA, U Rome, Italy]
The ergosphere and dyadosphere of black holes
10:40 - 11:10 Coffee
11:10 - 12:00 Zoltan Perjés [KFKI, RMKI, Budapest, Hungary]
The behaviour of principal null directions of a black hole under perturbations
12:00 - 12:50 Matt Visser [VUW, New Zealand]
Near horizon geometry for generic rotating black holes
12:50 - 1:00 Closing remarks

Afternoon: Ring Laser Visit

Join us for a visit to the world's largest Sagnac interferometer, in the Cashmere Cavern under the Christchurch Port Hills. The Canterbury Ring Laser routinely measures variations in the earth's rotation (earthquakes, movement of the rotation axis induced by tidal torques etc) with a sensitivity of 5-10 billionths of the Earth's rotation rate. The effect of Lense-Thirring frame dragging by the Earth - which of course reaches its greatest manifestation in the Kerr black hole - is one to two orders of magnitude smaller than our present sensitivity, at 0.5 billionths of the basic rotation rate of the Earth.

Depending on numbers and interest, we will make this a mini-excursion, with a scenic drive along the Port Hills crater rim, and lunch en route (costs not included in registration fee). Further details will be provided at the time of registering and those wishing to participate can sign up once you are here.