Emergence of Dark Energy from topology and chiral spinors
J. Lorca Espiro, Yerko Vásquez, M. Le Delliou
TL;DR
The paper introduces a torsionful Einstein–Cartan gravity on a Lorentzian 4-manifold with internal boundaries and shows that a harmonic 1-form $\\theta$ detected by the topology (captured by $H^1(\\mathcal{M})$ and related to π_3) acts as a source of contortion, generating a dynamical dark-energy–like term. By decomposing the connection into a Levi-Civita part and a contortion generated by $\\theta$, and imposing an Ehresmann parallel spinor hypothesis, the authors derive a chain of relations linking a topological current $J$ to the boundary data via a Dirichlet-to-Neumann operator $\\Lambda$, ultimately leading to a generalized Einstein equation with a positive term $|\\theta|^2_g$ that acts as dynamical dark energy. The framework ties the dark energy density to topology and boundary conditions (through $\\Lambda$ and boundary values $\\xi$) and provides a holographic flavor by showing the boundary data controls bulk cosmological dynamics. This topological mechanism offers a falsifiable route to explain dark energy without introducing new fundamental fields, and it invites cosmological applications and observational tests. The key mathematical objects are the harmonic form $\\theta$, the Dirac current $J$, the Nieh–Yan structure, and the boundary-to-bulk coupling mediated by $\\Lambda$.
Abstract
Under the existence of a massless spinor with respect to the total connection in a spacetime modeled as a Lorentzian manifold with internal boundaries, such as finite volume semi-classical Black Holes, we show that a topological mechanism naturally induces terms in the Einstein-Cartan gravitational action that can be interpreted as General Relativity with dark energy. This may alleviate the problems of dark energy. The topological information is carried by a harmonic 1-form associated to the first co-holomology group of the spacetime, which induces a spacetime contortion acting on the horizontal bundle.
