RRI Banner

Closeness function on coarse grained Lorentzian geometries

dc.contributor.authorSurya, Sumati
dc.date.accessioned2026-09-08T10:25:08Z
dc.date.available2026-09-08T10:25:08Z
dc.date.issued2026-01-16
dc.descriptionRestricted Access. An open-access version is available at arXiv.org (one of the alternative locations)en_US
dc.description.abstractWe 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 behavior in causal set theory and can be used to define a weak convergence condition for Lorentzian geometries.en_US
dc.identifier.citationPhysical Review D, 2026, Vol. 113 (2), AR No. 024034en_US
dc.identifier.issn2470-0029
dc.identifier.urihttp://hdl.handle.net/2289/8833
dc.language.isoenen_US
dc.publisherAmerican Physical Societyen_US
dc.relation.urihttps://doi.org/10.48550/arXiv.2510.19403en_US
dc.relation.urihttps://doi.org/10.1103/txbf-hvz3en_US
dc.rights© 2026 American Physical Societyen_US
dc.subjectQuantum cosmologyen_US
dc.subjectQuantum gravityen_US
dc.subjectSpacetime topology & causal structureen_US
dc.titleCloseness function on coarse grained Lorentzian geometriesen_US
dc.typeArticleen_US

Files