Finite-resolution Gaussian regularization of (2+1)D flat spacetime induces a curved metric with integrated Gaussian curvature of -2 pi and an effective negative energy source of -1/(4G) independent of resolution scale.
and Traschen, Jennie H
2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2verdicts
UNVERDICTED 2representative citing papers
Adapts Sbierski's proof to establish future C^0-inextendibility for warped-product black hole spacetimes with closed, connected, homogeneous, orientable fibres, including nonvacuum cases and multiple horizons.
citing papers explorer
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Finite-resolution measurement induces topological curvature defects in spacetime
Finite-resolution Gaussian regularization of (2+1)D flat spacetime induces a curved metric with integrated Gaussian curvature of -2 pi and an effective negative energy source of -1/(4G) independent of resolution scale.
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$C^0$-inextendibility of a class of warped-product black hole spacetimes
Adapts Sbierski's proof to establish future C^0-inextendibility for warped-product black hole spacetimes with closed, connected, homogeneous, orientable fibres, including nonvacuum cases and multiple horizons.