📝 SummarXiv

Abstract

Gravitational helicity flux density represents the angular distribution of helicity flux in general relativity. In this work, we explore its relationship to the reduction of topological invariants at future null infinity. Contrary to initial expectations, the Pontryagin term, which contributes to the gravitational chiral anomaly, is not related to the gravitational helicity flux density. Instead, the Nieh-Yan term, another topological invariant within the teleparallel equivalent of general relativity (TEGR), can reproduce this flux density. We also reduce these two topological invariants to null hypersurfaces describing near-horizon geometry. In this near-horizon context, the Pontryagin term yields a non-trivial quantity that may characterize a Carrollian fluid helicity relevant to near-horizon physics.