Relativity : an introduction to special and general relativity

By H. Stephani. 2004

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Two-component spinor techniques and Feynman rules for quantum field theory and supersymmetry (2008, background): “[22,23,38,43,44,47,53,61,63,65]), the more common convention for the epsilon symbol (also adopted in refs.”
Cosmological perturbations (2008, background): “[39]) φ;μ = φ,μ, Vμ;ν = Vμ,ν − 0 μνVα, tμν;λ = tμν,λ − 0 μλtαν − 0 β νλtβμ.”
Rotating neutron stars: an invariant comparison of approximate and numerical space-time models (2004, methodology): “In a nutshell, the Petrov classification of a space–time depends on which of the Weyl scalars can be set to zero by suitable tetrad rotations (Chandrasekhar 1983; Stephani et al. 2003; Stephani 2004).”