Small scale structure of spacetime: van Vleck determinant and equi-geodesic surfaces
arXiv:1503.03793 · doi:10.1103/PhysRevD.92.024046
Abstract
It has recently been argued that if spacetime possesses non-trivial structure at small scales, an appropriate semi-classical description of it should be based on non-local bi-tensors instead of local tensors such as the metric . Two most relevant bi-tensors in this context are Synge's World function and the van Vleck determinant (VVD) , as they encode the metric properties of spacetime and (de)focussing behaviour of geodesics. They also characterize the leading short distance behavior of two point functions of the d'Alembartian . We begin by discussing the intrinsic and extrinsic geometry of equi-geodesic surfaces defined by in a geodesically convex neighbourhood of an event , and highlight some elementary identities relating the VVD with geometry of these surfaces. As an aside, we also comment on the contribution of to the surface term in the Einstein-Hilbert (EH) action and show that it can be written as a volume integral of . We then study the small scale structure of spacetime in presence of a Lorentz invariant short distance cut-off using and , based on some recently developed ideas. We derive a 2nd rank bi-tensor which naturally yields geodesic intervals bounded from below, and present a general and mathematically rigorous analysis of short distance structure of spacetime based on (a) geometry of , (b) structure of the non local d'Alembartian associated with , and (c) properties of the VVD. In particular, we show that the Ricci bi-scalar of is completely determined by , the tidal tensor, and first two derivatives of the van Vleck determinant, and has a non-trivial "classical" limit given by (constant) (see text).
v1: 12 pages, 1 figure; abstract formatted (see PDF file for the complete abstract). v2: minor typos corrected, references added
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