Minimum-length Ricci scalar for null separated events
Alessandro Pesci

TL;DR
This paper derives a zero-point length modified Ricci scalar for null separated events, revealing that in the limit of vanishing quantum effects, it converges to a quantity central in horizon thermodynamics and gravitational field equations.
Contribution
It introduces a novel expression for the Ricci scalar in a quantum-inspired zero-point length spacetime for null events, linking quantum spacetime structure to classical gravitational quantities.
Findings
The zero-point length modifies the Ricci scalar for null events.
In the limit, the expression reduces to (D-1) R_{ab} l^a l^b, not R.
This supports the idea that R_{ab} l^a l^b} encodes quantum spacetime remnants.
Abstract
We consider spacetime endowed with a zero-point length, i.e. with an effective metric structure which allows for a (quantum-mechanically arising) finite distance between events in the limit of their coincidence. Restricting attention to null separated events, we find an expression for the Ricci (bi)scalar in this zero-point-length metric; this is done for when geometric circumstances are such that the collection of all null geodesics emerging from a point has all the information needed to fix the value of scalar curvature at . Taking then the coincidence and further limits, we find that this expression does not reduce to the Ricci scalar of the ordinary metric but to in -dimensional spacetime (), where and are the ordinary Ricci tensor and tangent vector to the null geodesics. This adds nicely to the existing…
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