Magnitude homology of geodesic space
Kiyonori Gomi
TL;DR
This work connects magnitude homology to the geometry of geodesic spaces by giving concrete, geometrically meaningful descriptions of low-degree magnitude homology. It shows that H^_2 can be read from simplicial complexes A(a,b) and B^(a,b), while H^_3 in geodesic spaces is governed by H_1(A(a,b)); a non-branching assumption yields a complete diagonal description of all H^_n(X) in terms of sequences of geodesics and reveals a torsion-free structure. The authors introduce an invariant ν_f for third-magnitude classes that captures intersection properties of geodesic-driven edge paths, and demonstrate nontrivial examples. The results include explicit characterizations for classic spaces like S^1 and S^d, establish degeneracy in the higher spectral sequence under non-branching, and lay groundwork for further links between magnitude homology and geodesic geometry.
Abstract
This paper studies the magnitude homology groups of geodesic metric spaces. We start with a description of the second magnitude homology of a general metric space in terms of the zeroth homology groups of certain simplicial complexes. Then, on a geodesic metric space, we interpret the description by means of geodesics. The third magnitude homology of a geodesic metric space also admits a description in terms of a simplicial complex. Under an assumption on a metric space, the simplicial description allows us to introduce an invariant of third magnitude homology classes as an intersection number. Finally, we provide a complete description of all the magnitude homology groups of a geodesic metric space which fulfils a certain non-branching assumption.
