English

The Geometry of Small Causal Diamonds

High Energy Physics - Theory 2015-08-13 v3 General Relativity and Quantum Cosmology Differential Geometry

Abstract

The geometry of causal diamonds or Alexandrov open sets whose initial and final events pp and qq respectively have a proper-time separation τ\tau small compared with the curvature scale is a universal. The corrections from flat space are given as a power series in τ\tau whose coefficients involve the curvature at the centre of the diamond. We give formulae for the total 4-volume VV of the diamond, the area AA of the intersection the future light cone of pp with the past light cone of qq and the 3-volume of the hyper-surface of largest 3-volume bounded by this intersection valid to O(τ4){\cal O} (\tau ^4) . The formula for the 4-volume agrees with a previous result of Myrheim. Remarkably, the iso-perimetric ratio 3V34π/(A4π)32{3V_3 \over 4 \pi} / ({A \over 4 \pi}) ^{3 \over 2} depends only on the energy density at the centre and is bigger than unity if the energy density is positive. These results are also shown to hold in all spacetime dimensions. Formulae are also given, valid to next non-trivial order, for causal domains in two spacetime dimensions. We suggest a number of applications, for instance, the directional dependence of the volume allows one to regard the volumes of causal diamonds as an observable providing a measurement of the Ricci tensor.

Keywords

Cite

@article{arxiv.hep-th/0703098,
  title  = {The Geometry of Small Causal Diamonds},
  author = {G. W. Gibbons and S. N. Solodukhin},
  journal= {arXiv preprint arXiv:hep-th/0703098},
  year   = {2015}
}

Comments

17 pages, no figures; Misprints in eqs.(62), (65), (66) and (81) corrected; a new note on page 13 (with 2 new equations) added