Here are the abstracts for the conference talks:
http://www.perimeterinstitute.ca/Events/Conformal_Nature_of_the_Universe/Abstracts/
I really like Joao Magueijo's title. I think it's funny:
Is Nothing Sacred? The Cosmological Pay Off from Breaking Lorentz and Diffeormorphism Invariance
Shape dynamics is an example where you give up diffeo invariance, you agree to be tied down to a fixed foliation into simultaneous time-slices (thus sacrificing diffeo invariance.) And in exchange you get CONFORMAL invariance. Is that good? Some people think so. With conformal invariance things have no definite size they are just in a definite angular relation to each other. Other theories are exploring conformal invariance as well--hence the conference.
So here we have these sacrosanct principles of Lorentz and Diffeo invariance and suddenly it is fashionable to devise and study theories which break them.
Julian Barbour is giving the COLLOQUIUM talk connected with the conference. Colloquia are generally aimed at a wider audience and held in a larger auditorium.
http://pirsa.org/12050050
One of the other speakers, Edward Anderson, just posted a paper called Relationalism on the arxiv, and will be giving a talk by the same title at the conference. Here's the talk's abstract.
==quote==
Edward Anderson, Université Paris Diderot
Relationalism
I shall describe Relationalism, especially in the Leibniz-Mach-Barbour sense of the word and my variations on that theme. My presentation shall give five extensions to Barbour's work: (more or less) phase space, categorization, subsystems analysis, quantization, and physics as a propositional logic (`questions about physical systems'). I shall also briefly explain how some of Crane and Rovelli's ideas do fit within this scheme, whilst others are at odds with the LMB scheme, leaving one choosing options rather thanjust considering unions. I shall also present how scale-invariant and scaled relational particle models (the latter originally discovered by Barbour and Bertotti in 1982) can, in dimension 1 and 2, which suffice to toy-model many midisuperspace aspects of GR, be very generally solved at the following levels. 1) configuration space geometry following my fortuitous connection with Kendall's work in the statistical theory of shape involving the self-same space of shapes, and then the cone over this in the scaled case. 2) Conserved quantities and classical equations of motion. 3) Quantum equations of motion and their solutions. 4) Parallels of many Problem of Time strategies. I view this second paragraph as relevant not only by 4) but more widely by how it is a model of quantum background independence (BI), with BI being argued to be the other half to 'relativistic gravitation' in that gestalt entity known as General Relativity.
==endquote==
Here's the arxiv paper's abstract:
http://arxiv.org/abs/1205.1256