PIRSA:12050070 Conference

DOI10.48660/12050070

Conference/School: Conformal Nature of the Universe - 2012

Anderson, E. (2012). Relationalism. Perimeter Institute. https://pirsa.org/12050070

Anderson, Edward. Relationalism. Perimeter Institute, May. 10, 2012, https://pirsa.org/12050070 

@misc{ pirsa_PIRSA:12050070,
  doi = {10.48660/12050070},
  url = {https://pirsa.org/12050070},
  author = {Anderson, Edward},
  keywords = {},
  language = {en},
  title = {Relationalism},
  publisher = {Perimeter Institute},
  year = {2012},
  month = {may},
  note = {PIRSA:12050070 see, \url{https://pirsa.org}}
}

Abstract

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.

Resources

Next talk