English

Geometric Obstructions on Gravity

Mathematical Physics 2019-12-25 v1 General Relativity and Quantum Cosmology Differential Geometry math.MP

Abstract

These are notes for a short course and some talks gave at Departament of Mathematics and at Departament of Physics of Federal University of Minas Gerais, based on the author's paper arXiv:1808.09249. Some new information and results are also presented. Unlike the original work, here we try to give a more physical emphasis. In this sense, we present obstructions to realize gravity, modeled by the tetradic Einstein-Hilbert-Palatini (EHP) action functional, in a general geometric setting. In particular, we show that if spacetime has dimension n4n\geq4, then the cosmological constant plays no role in any "concrete geometries" other than Lorentzian. If n6n\geq6, then the entire EHP theory is trivial, meaning that Lorentzian geometry is (essentially) the only "concrete geometry" in which gravity (i.e, the EHP action functional) makes sense. Examples of "concrete geometries" include those locally modeled by group reductions HO(k;A)H\hookrightarrow O(k;A) for some kk and some algebra AA, so that Riemannian geometry, Hermitian geometry, K\"ahler geometry and symplectic geometry, as well as Type II geometry, Hitchin's generalized complex geometry and G2G_{2}-geometry are included. We also study EHP theory in "abstract geometries", such as graded geometry (and hence supergeometry), and we show how the obstruction results extend to this context. We construct two theories naturally associated to EHP, which we call the geometric/algebraic dual of EHP, and we analyze the effect of the obstructions in these new theories. Finally, we speculate (and provide evidence for) the existence of a "universal obstruction condition".

Keywords

Cite

@article{arxiv.1912.11198,
  title  = {Geometric Obstructions on Gravity},
  author = {Yuri Ximenes Martins and Rodney Josué Biezuner},
  journal= {arXiv preprint arXiv:1912.11198},
  year   = {2019}
}

Comments

Essentially a reader-friendly version of arXiv:1808.09249 endowed with further results and discussion

R2 v1 2026-06-23T12:55:22.932Z