A Closeness Function on Coarse Grained Lorentzian Geometries
Sumati Surya
TL;DR
The paper addresses quantifying how close Lorentzian geometries are within causal set theory by exploiting interval abundances in random causal sets. It introduces the $n$-interval spectrum $\mathcal{S}_n(M,g)$ and a family of $L^r$ closeness functions $\mathcal{D}^{(r)}_n$ based on the abundances $N_m^{(n)}$, offering a computable, scale-aware metric for large $n$ and a weak convergence notion on the quotient space $\tilde{\mathcal{L}}$. Although $\mathcal{D}^{(r)}_n$ is weaker than a full Lorentzian Gromov-Hausdorff distance due to interval isospectral degeneracies, it yields practical discrimination between spacetimes and supports a notion of interval convergence, demonstrated via simulations across Minkowski diamonds, thickened diamonds, hypercubes, and FRW regions. The work also analyzes degeneracies and discusses incorporating additional invariants to lift them, outlining a path toward stronger convergence criteria and broader applicability to non-flat cosmological spacetimes.
Abstract
We construct a family of closeness functions on the space of finite volume Lorentzian geometries using the abundance of discrete intervals in the underlying random causal sets. Although strictly weaker than a Lorentzian Gromov-Hausdorff distance function, it has the advantage of being numerically calculable for large causal sets. It thus provides a concrete and quantitative measure of continuumlike behaviour in causal set theory and can be used to define a weak convergence condition for Lorentzian geometries.
