Birkhoff's theorem for stable torsion theories
arXiv:1811.11021 · doi:10.1088/1475-7516/2019/03/002
Abstract
We present a novel approach to establish the Birkhoff's theorem validity in the so-called quadratic Poincaré Gauge theories of gravity. By obtaining the field equations via the Palatini formalism, we find paradigmatic scenarios where the theorem applies neatly. For more general and physically relevant situations, a suitable decomposition of the torsion tensor also allows us to establish the validity of the theorem. Our analysis shows rigorously how for all stable cases under consideration, the only solution of the vacuum field equations is a torsionless Schwarzschild spacetime, although it is possible to find non-Schwarzschild metrics in the realm of unstable Lagrangians. Finally, we study the weakened formulation of the Birkhoff's theorem where an asymptotically flat metric is assumed, showing that the theorem also holds.
39 pages, 5 figures, minor corrections, conclusions unchanged. It matches the version published in JCAP
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Cited by in corpus (8)
- Large and Ultra-compact Gauss-Bonnet Black Holes with a Self-interacting Scalar Field
- On the Existence of Solutions with a Horizon in Pure Scalar-Gauss-Bonnet Theories
- Revisiting the Stability of Quadratic Poincaré Gauge Gravity
- Carroll limit of four-dimensional gravity theories in the first order formalism
- Generalized Birkhoff theorem in the Poincaré gauge gravity theory
- Non-singular and ghost-free infinite derivative gravity with torsion
- Non-geodesic incompleteness in Poincaré gauge gravity
- New effective theories of gravitation and their phenomenological consequences