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Curvature, Ricci, scalar and Einstein tensors of a metric with a round two-sphere factor

Example

Let S2:={(X,Y,Z)∈R3:X2+Y2+Z2=1} with the round metric induced by the Euclidean inner product, and let M:=R2×S2 with the product Lorentzian metric whose first factor has line element −(dx0)2+(dx3)2. Use the sphere chart σ:(0,π)×(0,2π)→S2 given by σ(θ,φ)=(sin⁡θcos⁡φ,sin⁡θsin⁡φ,cos⁡θ), and put U:=R2×σ((0,π)×(0,2π))⊂M. In the product chart with coordinate order x=(x0,x1,x2,x3)=(x0,θ,φ,x3), the metric is g:=−(dx0)2+(dx1)2+sin⁡2(x1) (dx2)2+(dx3)2,N:=∂0. This chart contains the equatorial geodesic segment used in An equator geodesic of the round-sphere factor: conjugate instant at distance pi with multiplicity one; the underlying manifold has an actual S2 factor, not an unwrapped angular cover. The metric is smooth and Lorentzian on M with time orientation N (Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model). Let ∇ be its metric-selected connection and R, Rabcd, Ric⁡ab, S and Gab its curvature data (Metric compatibility, torsion freedom and the metric-selected connection class, Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields, The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors). Then:

  1. The only nonzero Christoffel symbols in this chart are Γ122=−sin⁡x1cos⁡x1,Γ212=Γ221=cot⁡x1.
  2. The curvature has exactly one independent nonzero lowered component up to the algebraic symmetries, namely R1212=sin⁡2(x1); equivalently R(∂1,∂2)∂2=sin⁡2(x1)∂1 and R(∂1,∂2)∂1=−∂2, and every component containing an index 0 or 3 vanishes.
  3. The Ricci tensor, scalar curvature and Einstein tensor are Ric⁡11=1,Ric⁡22=sin⁡2(x1),S=2,G=diag⁡(1,0,0,−1).
  4. The contracted second Bianchi identity ∇aGab=0 holds. In the displayed chart U, ∇eGab=0 identically, so the divergence vanishes term by term there.

Facts & Assumptions

Given: The product M=R2×S2 with its product metric and time orientation N, and its local chart U with 0<x1<π and 0<x2<2π as specified above. Let ∇ be the metric-selected connection and R, Rabcd, Ric⁡, S, and G its curvature data.

[L1]

The product metric is smooth Lorentzian of signature (−,+,+,+) on M with time orientation N=∂0; its components on U are diag⁡(−1,1,sin⁡2(x1),1). The metric-selected connection exists and is unique, and on U its Christoffel symbols are Γabc=12gad(∂bgdc+∂cgbd−∂dgbc), with gad the matrix inverse of gab (Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model, Metric compatibility, torsion freedom and the metric-selected connection class, Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields clause (a), Christoffel symbols of an affine connection, The inverse metric, musical isomorphisms and index raising).

[L2]

The curvature components in a chart are Rabcd=∂cΓadb−∂dΓacb+∑e(ΓaceΓedb−ΓadeΓecb), and R is a tensor: its components transform between charts, while tensor identities and vanishing are chart-independent; the displayed nonzero component values below refer to the specified product chart (Tensoriality of the curvature, its coordinate formula and its point-normal metric formula clauses (a)-(b), The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors clause (b)).

[L3]

The lowered curvature satisfies Rabcd=−Rbacd=−Rabdc=Rcdab and Rabcd+Racdb+Radbc=0; equivalently R(X,Y)Z=−R(Y,X)Z and g(R(X,Y)Z,W)=−g(R(X,Y)W,Z) (The algebraic symmetries of the curvature tensor and the symmetry of the Ricci and Einstein tensors clauses (a)-(c)).

[L4]

The Ricci tensor, scalar curvature and Einstein tensor are Ric⁡bd=gacRabcd, S=gbdRic⁡bd and Gab=Ric⁡ab−12Sgab (The Riemann curvature operator and the derived Ricci, scalar and Einstein tensors clause (c)).

[L5]

The contracted second Bianchi identity reads ∇aGab=0, where ∇aGab=gae∇eGab and ∇ acts on tensor components by the metric-compatible derivative (The second Bianchi identity and the vanishing divergence of the Einstein tensor clause (b), Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields clause (c)).

Verification

technique · direct
1.1L1algebra

(Christoffel symbols.) Only g22=sin⁡2(x1) is nonconstant, with ∂1g22=2sin⁡x1cos⁡x1 and g22=sin⁡−2(x1); by [L1] the only possible nonzero symbols are Γ122=12g11(−∂1g22)=−sin⁡x1cos⁡x1 and Γ212=Γ221=12g22∂1g22=cot⁡x1, every other symbol vanishing because it contains ∂agbc with a≠1 or a constant component.

2.1L2step 1.1L3algebra

(Candidate components.) In the coordinate formula of [L2] every term contains a factor Γa⋅⋅ or a derivative of one; by step 1.1 a term can be nonzero only if all its symbol indices lie in {1,2}. Hence Rabcd=0 whenever one of a,b,c,d equals 0 or 3: the derivative terms contain Γadb or Γacb with a forbidden index in the lower pair, or are annihilated by ∂0,∂3, and each product term contains a symbol with a forbidden index. Of the four remaining candidates R1112, R1212, R2112, R2212, the first and the last have a repeated index in the first lower pair, so their lowered components vanish by the skew-symmetry of [L3], and R2112 is the negative of R2121; it therefore suffices to check R1212 and R2121, which are equal up to lowering and sign.

2.2step 1.1L2L3L4algebra

(The curvature component.) By [L2] and step 1.1, the products in R1212 contribute only through −∑eΓ12eΓe12=−Γ122Γ212, because Γ11e=0 for every e kills the first product and the only nonzero term of the second has e=2; hence R1212=∂1Γ122−∂2Γ112−Γ122Γ212=−∂1(sin⁡x1cos⁡x1)+sin⁡x1cos⁡x1cot⁡x1. Substituting and using cos⁡x1cot⁡x1=cos⁡2x1/sin⁡x1, R1212=−(cos⁡2x1−sin⁡2x1)+cos⁡2x1=sin⁡2(x1). Lowering with g11=1 gives R1212=sin⁡2(x1); by [L3], R2121=R1212 and the skew-symmetry gives R2121=sin⁡−2(x1)R2121=1, and the vector-valued forms follow from R(∂c,∂d)∂b=Rabcd∂a.

3.1step 2.1step 2.2L4algebra

(Ricci tensor.) By [L4] and step 2.1, the only components of Rabcd that can contribute to a contraction are those with all indices in {1,2}: Ric⁡11=g22R2121=sin⁡−2(x1)sin⁡2(x1)=1 and Ric⁡22=g11R1212=sin⁡2(x1), while Ric⁡bd=0 whenever b or d is 0 or 3, because every term of the sum gacRabcd then contains a component with a forbidden index.

4.1step 3.1L4algebra

(Scalar curvature and Einstein tensor.) By [L4] and step 3.1, S=g11Ric⁡11+g22Ric⁡22=1+sin⁡−2(x1)sin⁡2(x1)=2. Hence G11=1−12⋅2⋅1=0, G22=sin⁡2(x1)−12⋅2⋅sin⁡2(x1)=0, G00=0−12⋅2⋅(−1)=1, G33=0−12⋅2⋅1=−1, and all off-diagonal components vanish: G=diag⁡(1,0,0,−1).

5.1step 4.1L5algebra∎

(Divergence of the Einstein tensor in the chart.) By [L5] and the formula for the covariant derivative of a tensor, ∇eGab=∂eGab−∑d(ΓdeaGdb+ΓdebGad) on U. Step 4.1 gives ∂eGab=0; and each product vanishes because a nonzero Γdea has all three indices in {1,2}, while Gdb or Gad is nonzero only when both its indices are 0 or both are 3, so no index value is available for d. Hence ∇eGab=0 throughout U, and the contracted divergence vanishes term by term there, in accordance with the globally valid identity [L5].

Remarks

  • What the example checks. The computation verifies on an explicit curved metric the definitions of the Ricci, scalar and Einstein tensors, the algebraic symmetries in the form R1212=R2121 and R1212+R1122+R1221=0, and the contracted second Bianchi identity. The metric is not Ricci flat and is not flat: R1212=sin⁡2(x1) is nonzero throughout the chart U, so Ric⁡≠0 by step 3.1.
  • Relation to the tidal page. On the equator x1=π/2, the geodesic and field of An equator geodesic of the round-sphere factor: conjugate instant at distance pi with multiplicity one have T=∂2 and J(s)=sin⁡(s)∂1. The component R(∂1,∂2)∂2=sin⁡2(x1)∂1 computed above, together with skew-symmetry, gives the curvature term R(T,J)T=−sin⁡(s)∂1. That item verifies the Jacobi equation and the conjugate instant it entails.

Depends on

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