Algebraically independent nth derivatives of the Riemannian curvature spinor in a general spacetime
From MaRDI portal
Publication:3739835
DOI10.1088/0264-9381/3/6/013zbMath0603.53036OpenAlexW1994884783WikidataQ30054149 ScholiaQ30054149MaRDI QIDQ3739835
Jan E. Åman, Malcolm A. H. MacCallum
Publication date: 1986
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1088/0264-9381/3/6/013
Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Applications of local differential geometry to the sciences (53B50) Local differential geometry of Lorentz metrics, indefinite metrics (53B30)
Related Items (19)
On scalar curvature invariants in three dimensional spacetimes ⋮ Invariant classification and the generalised invariant formalism: Conformally flat pure radiation metrics ⋮ The parameters of the Lewis metric for the Weyl class ⋮ Cartan invariants and event horizon detection ⋮ Exact sets of test uncharged massive spin 3/2 fields in general relativity ⋮ Characterizing the curvature and its first derivative for imperfect fluids ⋮ Topological constraints on Maxwell fields in Robertson-Walker space-times ⋮ On local equivalence problem of space-times with two orthogonally transitive commuting Killing fields ⋮ Symmetry analysis of radiative spacetimes with a null isotropy using GHP formalism ⋮ Observer-based invariants for cosmological models ⋮ Totally symmetrized spinors and null rotation invariance ⋮ The equivalence problem ⋮ THE CURVATURE HOMOGENEITY BOUND FOR LORENTZIAN FOUR-MANIFOLDS ⋮ On a class of Riemann-Cartan space-times of Gödel type. ⋮ Spacetimes with continuous linear isotropies. I: Spatial rotations ⋮ Spacetimes with continuous linear isotropies. II: Boosts ⋮ Spacetimes with continuous linear isotropies. III: Null rotations ⋮ Computer-aided study of a class of Riemannian space-times ⋮ Algebraic computing in torsion theories of gravitation.
Uses Software
This page was built for publication: Algebraically independent nth derivatives of the Riemannian curvature spinor in a general spacetime