Tensor Networks from Kinematic Space
Bartlomiej Czech, Lampros Lamprou, Samuel McCandlish, James Sully

TL;DR
This paper reveals that MERA tensor networks for 1+1D CFT ground states structurally resemble kinematic space, suggesting MERA discretizes bulk geodesics in holographic theories, with tests on BTZ geometries supporting this view.
Contribution
It proposes viewing MERA as a discretization of bulk geodesic space rather than bulk geometry, extending the kinematic space concept to tensor networks.
Findings
MERA matches the structure of kinematic space in holographic CFTs.
Comparison with BTZ geometry shows detailed agreement including entwinement.
Extension of MERA to excited states via generalized compression networks.
Abstract
We point out that the MERA network for the ground state of a 1+1-dimensional conformal field theory has the same structural features as kinematic space---the geometry of CFT intervals. In holographic theories kinematic space becomes identified with the space of bulk geodesics studied in integral geometry. We argue that in these settings MERA is best viewed as a discretization of the space of bulk geodesics rather than of the bulk geometry itself. As a test of this kinematic proposal, we compare the MERA representation of the thermofield-double state with the space of geodesics in the two-sided BTZ geometry, obtaining a detailed agreement which includes the entwinement sector. We discuss how the kinematic proposal can be extended to excited states by generalizing MERA to a broader class of compression networks.
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