A1.15 B1.24

General Relativity | Part II, 2002

(i) Given a covariant vector field VaV_{a}, define the curvature tensor RbcdaR_{b c d}^{a} by

Va;bcVa;cb=VeRabceV_{a ; b c}-V_{a ; c b}=V_{e} R_{a b c}^{e}

Express RabceR_{a b c}^{e} in terms of the Christoffel symbols and their derivatives. Show that

Rabce=RacbeR_{a b c}^{e}=-R_{a c b}^{e}

Further, by setting Va=ϕ/xaV_{a}=\partial \phi / \partial x^{a}, deduce that

Rabce+Rcabe+Rbcae=0.R_{a b c}^{e}+R_{c a b}^{e}+R_{b c a}^{e}=0 .

(ii) Write down an expression similar to (*) given in Part (i) for the quantity

gab;cdgab;dcg_{a b ; c d}-g_{a b ; d c}

and hence show that

Reabc=Raebc.R_{e a b c}=-R_{a e b c} .

Define the Ricci tensor, show that it is symmetric and write down the contracted Bianchi identities.

In certain spacetimes of dimension n2,Rabcdn \geq 2, R_{a b c d} takes the form

Rabcd=K(xe)[gacgbdgadgbc]R_{a b c d}=K\left(x^{e}\right)\left[g_{a c} g_{b d}-g_{a d} g_{b c}\right]

Obtain the Ricci tensor and Ricci scalar. Deduce that KK is a constant in such spacetimes if the dimension nn is greater than 2 .

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