Synge's World function and the quantum spacetime

TL;DR

This paper emphasizes the importance of non-local bi-tensors like Synge's World function and the van Vleck determinant in characterizing quantum spacetime, especially when incorporating a minimal length scale, and explores their implications for gravity and singularities.

Contribution

It introduces a non-local bi-tensor framework for spacetime geometry that captures quantum and small-scale effects, offering new insights into gravitational dynamics and cosmological phenomena.

Findings

Suggests a new description of gravity different from Einstein-Hilbert

Indicates dimensional reduction to 2 at small scales

Links cosmological constant to non-local spacetime structure

Abstract

All our observations that characterise space and time are expressed in terms of non-local, bi-tensorial objects such as geodesic intervals between events and two-point (Green) functions. In this contribution, I highlight the importance of characterising spacetime geometry in terms of such non-local objects, focusing particularly on two important bi-tensors that play a particular fundamental role -- Synge's World function and the van Vleck determinant. I will first discuss how these bi-tensors help capture information about spacetime geometry, and then describe their role in characterising quantum spacetime endowed with a lower bound, say $\ell_0$, on spacetime intervals. Incorporating such a length scale in a Lorentz covariant manner necessitates a description of spacetime geometry in terms of above bi-tensors, and naturally replaces the conventional description based on the metric tensor $g_{ab}(x)$ with a description in terms of a non-local bi-tensor $q_{ab}(x, y)$. The non-analytic structure of $q_{ab}(x, y)$ which renders a perturbative expansion in $\ell_0$ meaningless, also generically leaves a non-trivial ``relic" in the limit $\ell_0 \to 0$. I present some results where such a relic term is manifest; specifically, I will discuss how this: (i) suggests a description of gravitational dynamics different from the one based on Einstein-Hilbert lagrangian, (ii) implies dimensional reduction to $2$ at small scales, (iii) connects with the notion of cosmological constant itself being a non-local vestige of the small scale structure of spacetime, (iv) helps address the issues of spacetime singularities. I will conclude by discussing the ramifications of these ideas for quantum gravity.