In Riemannian geometry and general relativity, the trace-free Ricci tensor of a pseudo-Riemannian manifold is the tensor defined by
where is the Ricci tensor, is the scalar curvature, is the metric tensor, and is the dimension of . The name of this object reflects the fact that its trace automatically vanishes:
If n 3, the trace-free Ricci tensor vanishes identically if and only if
for some constant . In mathematics, this is the condition for to be an Einstein manifold. In physics, this equation states that is a solution of Einstein's vacuum field equations with cosmological constant.
Read more about this topic: Ricci Curvature
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