Truesdell transport in general relativity

Physics

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Scientific paper

The Truesdell transport of a contravariant tensor fieldX ab is defined with respect to a time-like vector fieldu a analogous to the classical definition in continuum mechanics. Truesdell stress rate of the shear tensor (σ ab) and the metric tensor (g ab ) is Truesdell transported alongl a if and only if the medium is rigid. In case of two-dimensional projection operatorsγ ab andγ *ab are Truesdell transported along timelike vector fieldu a if and only if they are expansion free (alongu a ) withtau = λ - bar σ + μ - ρ = 0. A collapsing perfect fluid is Truesdell transported with respect tou a if and only if it is expansion free (alongu a ), energy density (D), pressure (P), and density of neutrino radiation (q) are conserved alongu a withσt=λ,α + bar β = tau = 0. In all the above cases, analogous results are found alongl a ,n a , andm a using freedom conditions (k=ɛ=π=γ+γ -=0) as null rays are always restricted to be geodesic (Carter [1]).

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