A spacetime for which the Karlhede invariant classification requires the fourth covariant derivative of the Riemann tensor
From MaRDI portal
Publication:4033851
DOI10.1088/0264-9381/9/10/003zbMath0773.53049OpenAlexW2080798912MaRDI QIDQ4033851
Publication date: 16 May 1993
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1088/0264-9381/9/10/003
Applications of differential geometry to physics (53Z05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20)
Related Items (10)
Coherent planar symmetric spacetimes generated by progressive waves of Nambu-Goldstone bosons ⋮ Invariant classification and the generalised invariant formalism: Conformally flat pure radiation metrics ⋮ Obtaining a class of type \(O\) pure radiation metrics with a negative cosmological constant, using invariant operators ⋮ Applications of SHEEP in general relativity ⋮ Integration in the GHP formalism. III: Finding conformally flat radiation metrics as an example of an `optimal situation' ⋮ Type 0 pure radiation metrics with a cosmological constant ⋮ Computer algebra: from the visible to the invisible ⋮ The equivalence problem ⋮ Spacetimes with continuous linear isotropies. I: Spatial rotations ⋮ Integration in the GHP formalism. IV: A new Lie derivative operator leading to an efficient treatment of Killing vectors
This page was built for publication: A spacetime for which the Karlhede invariant classification requires the fourth covariant derivative of the Riemann tensor
