Toward Singularity Theorems with Torsion
arXiv:2407.21107 · doi:10.1103/PhysRevD.110.064082
Abstract
This study examines the formulation of a singularity theorem for timelike curves including torsion, and establishes the foundational framework necessary for its derivation. We begin by deriving the relative acceleration for an arbitrary congruence of timelike curves. The resulting ``deviation equation'' offers an alternative pathway to the well-known Raychaudhuri equation with torsion. Conjugate points are then introduced and analyzed in relation to the behavior of the scalar expansion. Together with the sensible requirement of hypersurface orthogonality, the Raychaudhuri equation is examined for several specific cases of torsion that are prominent in the literature. Our findings indicate that a totally antisymmetric torsion tensor does not influence the behavior of the congruence of timelike curves. Finally, we formulate a singularity theorem for timelike curves and highlight the critical requirement of non-autoparallel curves.
arXiv comment13 pages, 3 figures; Updated to published version
References in corpus (16)
- Physical Aspects of the Space-Time Torsion
- Friedmann-like universes with torsion
- Classical big-bounce cosmology: dynamical analysis of a homogeneous and irrotational Weyssenhoff fluid
- The Raychaudhuri equation in spacetimes with torsion and non-metricity
- Kinematics of Einstein-Cartan universes
- Raychaudhuri equation in spacetimes with torsion
- Weyssenhoff fluid dynamics in general relativity using a 1+3 covariant approach
- The dark side of the torsion: Dark Energy from propagating torsion
- Cosmological model with macroscopic spin fluid
- Torsional dark energy in quadratic gauge gravity
- Static compact objects in Einstein-Cartan theory
- Mathematical Structures of Space-Time
- Torsion driving cosmic expansion
- Singularity theorems and the inclusion of torsion in affine theories of gravity
- Does space-time torsion determine the minimum mass of gravitating particles?
- On the cosmological constant in the deformed Einstein-Cartan gauge gravity in De Donder-Weyl Hamiltonian formulation