19 problems
Let a spacetime be a constant scalar invariant (CSI) spacetime, meaning that all scalar polynomial curvature invariants are constant. A VSI spacetime is one for which all scalar po…
Let a spacetime be a constant scalar invariant (CSI) spacetime, meaning that all scalar polynomial curvature invariants are constant. The higher-dimensional Kundt CSI class consist…
Let a spacetime have a Riemann tensor and all of its covariant derivatives. A null frame is a frame adapted to the Lorentzian structure, and the boost order and boost weight re…
Let a Lorentzian spacetime be a constant scalar invariant (CSI) spacetime, with curvature invariants . A spacetime is CSI when all scalar polynomial curv…
Positive surface curvature implies no nonpositive-Euler-characteristic surface subgroups. If then no subgroup of is isomorphic to .
Negative surface curvature implies hyperbolicity. If then is word-hyperbolic.
Non-positive surface curvature implies solvable word problem. If then the word problem is solvable in .
Non-positive surface curvature implies asphericity. If then is aspherical.
Negative irreducible curvature implies locally quasiconvex. If then is a locally quasiconvex hyperbolic group.
Non-positive irreducible curvature implies coherence. If then is coherent.
Graphs of free groups with cyclic edge groups. Then . Furthermore, unless has a Baumslag--Solitar subgroup.
Surface curvatures of mapping tori of free group endomorphisms. Then unless has a Baumslag--Solitar subgroup.
Irreducible curvatures of mapping tori of free group endomorphisms. Then .
Negative curvature for geometric complexes. If then either has a toroidal boundary component or has a subgroup.
Non-positive curvature for geometric complexes. If then either has a spherical component or splits freely.
Surface curvature of random complexes in the density model. The probability that tends to as .
Irreducible curvature bounds of few-relator complexes. The probability that tends to as . In particular, with high probability, …
Let be a natural pseudohermitian scalar invariant whose total integral is a secondary CR invariant. Here, a secondary CR invariant is a total integral invariant under changes o…
Characterization conjecture. If a spacetime is characterised by its invariants, weakly or strongly, then it is either -non-degenerate or of type D to all orders; that…