English

Shape Space Methods for Quantum Cosmological Triangleland

General Relativity and Quantum Cosmology 2011-04-22 v2

Abstract

With toy modelling of conceptual aspects of quantum cosmology and the problem of time in quantum gravity in mind, I study the classical and quantum dynamics of the pure-shape (i.e. scale-free) triangle formed by 3 particles in 2-d. I do so by importing techniques to the triangle model from the corresponding 4 particles in 1-d model, using the fact that both have 2-spheres for shape spaces, though the latter has a trivial realization whilst the former has a more involved Hopf (or Dragt) type realization. I furthermore interpret the ensuing Dragt-type coordinates as shape quantities: a measure of anisoscelesness, the ellipticity of the base and apex's moments of inertia, and a quantity proportional to the area of the triangle. I promote these quantities at the quantum level to operators whose expectation and spread are then useful in understanding the quantum states of the system. Additionally, I tessellate the 2-sphere by its physical interpretation as the shape space of triangles, and then use this as a back-cloth from which to read off the interpretation of dynamical trajectories, potentials and wavefunctions. I include applications to timeless approaches to the problem of time and to the role of uniform states in quantum cosmological modelling.

Keywords

Cite

@article{arxiv.0909.2439,
  title  = {Shape Space Methods for Quantum Cosmological Triangleland},
  author = {Edward Anderson},
  journal= {arXiv preprint arXiv:0909.2439},
  year   = {2011}
}

Comments

A shorter version, as per the first stage in the refereeing process, and containing some new references

R2 v1 2026-06-21T13:45:54.696Z