English

Exact d'Alembertian for Lorentz distance functions

Differential Geometry 2025-04-03 v2 General Relativity and Quantum Cosmology Mathematical Physics Metric Geometry math.MP

Abstract

We refine a recent distributional notion of d'Alembertian of a signed Lorentz distance function to an achronal set in a metric measure spacetime obeying the timelike measure contraction property. We show precise representation formulas and comparison estimates (both upper and lower bounds). Under a condition we call "infinitesimally strict concavity" (known for infinitesimally Minkowskian structures and established here for Finsler spacetimes), we prove the associated distribution is a signed measure certifying the integration by parts formula. This treatment of the d'Alembertian using techniques from metric geometry expands upon its recent nonlinear yet elliptic interpretation; even in the smooth case, our formulas seem to pioneer its exact shape across the timelike cut locus. Two central ingredients our contribution unifies are the localization paradigm of Cavalletti-Mondino and the Sobolev calculus of Beran-Braun-Calisti-Gigli-McCann-Ohanyan-Rott-S\"amann. In the second part of our work, we present several applications of these insights. First, we show the equivalence of the timelike curvature-dimension condition with a Bochner-type inequality. Second, we set up synthetic mean curvature (as well as barriers for CMC sets) exactly. Third, we prove synthetic volume and area estimates of Heintze-Karcher-type, which enable us to show several synthetic volume singularity theorems.

Keywords

Cite

@article{arxiv.2408.16525,
  title  = {Exact d'Alembertian for Lorentz distance functions},
  author = {Mathias Braun},
  journal= {arXiv preprint arXiv:2408.16525},
  year   = {2025}
}

Comments

83 pages. Title slightly changed. Orientation of the transport rays reversed for enhanced presentation. Minor changes. Comments welcome

R2 v1 2026-06-28T18:27:40.271Z