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General Relativity Homework 2

Chasse_neige

Problem 1

Suppose Tμρσ is a tensor under the general coordinate transformation. Please show that

Tμρσ;νTμρσ,ν+ΓμντTτρσΓκρνTμκσΓκσνTμρκ

is also a tensor under general coordinate transformation.

Transformation Rule for Christoffel Symbol

Given that the Christoffel Symbol’s transformation rule is

Γλρσ=xλξα2ξαxρxσ=xλxκxκξαxρ(ξαxνxνxσ)=xλxκxκξα(ξαxν2xνxρxσ+xμxρxνxσ2ξαxμxν)=xλxκxμxρxνxσΓκμν+xλxκ2xκxρxσ

Tensor after Transformation

After transformation, the tensor will give out 4 parts.

Tλαβ;γTλαβ,γPart 1+ΓλγκTκαβPart 2ΓηαγTληβPart 3ΓϵγβTλαϵPart 4

To deal with this complex tensor, we’ll analyse it one part after another.

The first part

Tλαβ,γ=xγ(xλxμxρxαxσxβTμρσ)=2xλxηxτxηxγxρxαxσxβTτρσ(Term 1)+2xρxγxαxλxμxσxβTμρσ(Term 2)+2xσxλxβxλxμxρxαTμρσ(Term 3)+xνxγxλxμxρxαxσxβTμρσ,ν(Term 4)

gives out 4 terms, and I’ll show in detail how the first three cancel with the Γ parts’ extra terms.

The second part

ΓλγκTκαβ=(xλxμxνxγxτxκΓμντ+2xζxγxκxλxζ)xκxτxρxαxσxβTτρσ=xλxμxνxγxτxκxκxτxρxαxσxβΓμντTτρσ+2xζxγxκxλxζxκxτxρxαxσxβTτρσ

To let the extra term of the second part cancel with the Term 1 of the first part, we’ll have to prove that

(1)2xλxηxτxηxγ+2xζxγxκxλxζxκxτ=0

Consider

xτδλγ=xτ(xλxηxηxγ)=0xτ(xλxηxηxγ)=2xλxτxηxηxγ+2xηxγxκxκxτxλxη=0

So equation (1) is right. We can see that the second part’s extra term cancels with the first part’s Term 1.

The third part

ΓηαγTληβ=xηxκxρxαxνxβxλxμxκxηxσxβΓκρνTμκσ+2xζxαxγxηxζxλxμxρxηxσxβTμρσ

To let the extra term of the third part cancel with the Term 2 of the first part, we’ll have to prove that

(2)2xρxγxα=2xζxαxγxηxζxρxη

Consider

xηxζxρxη=δρζ

Therefore

2xζxαxγxηxζxρxη=2xζxαxγδρζ=2xρxγxα

So this part’s extra term cancels with the first part’s Term 2.

The fourth part

ΓϵγβTλαϵ=xϵxκxσxγxβxνxλxμxρxαxκxϵΓκσνTμρκ+2xζxγxβxϵxζxλxμxρxαxσxϵTμρσ

To let the extra term of the fourth part cancel with the Term 3 of the first part, we’ll have to prove that

(3)2xσxλxβ=2xζxγxβxϵxζxσxϵ

Consider

xϵxζxσxϵ=δσζ

So

2xζxγxβxϵxζxσxϵ=2xζxγxβδσζ=2xσxλxβ

So this part’s extra term cancels with the first part’s Term 3.

In conclusion, the transformation for this tensor could be written as

Tλαβ;γTλαβ,γPart 1+ΓλγκTκαβPart 2ΓηαγTληβPart 3ΓϵγβTλαϵPart 4=xνxγxλxμxρxαxσxβTμρσ,ν+xλxμxνxγxτxκxκxτxρxαxσxβΓμντTτρσxϵxκxσxγxβxνxλxμxρxαxκxϵΓκσνTμρκxϵxκxσxγxβxνxλxμxρxαxκxϵΓκσνTμρκ

is a tensor under general coordinate transformation.

Problem 2

Please show that

Rρσμν=μΓρνσνΓρμσ+ΓρμλΓλνσΓρνλΓλμσ

is a tensor under general coordinate transformation.

Computing the Derivative Term

Define Aμν=μΓρνσ+ΓρμλΓλνσ. We can see that Rρσμν=AμνAνμ. Therefore, any term in Aμν that is symmetric under the exchange of μν will automatically cancel out. Using the product rule, the chain rule μ=xδxμδ, and μxβxν=2xβxμxν, we differentiate Γρνσ

μΓρνσ=μ(xρxαxβxνxγxσΓαβγ)+μ(xρxα2xαxνxσ)

Expanding this gives 6 terms

μΓρνσ=xδxμ2xρxδxαxβxνxγxσΓαβγ(Term 1)+xρxα2xβxμxνxγxσΓαβγ(Term 2)+xρxαxβxν2xγxμxσΓαβγ(Term 3)+xρxαxβxνxγxσxδxμδΓαβγ(Term 4)+xδxμ2xρxδxα2xαxνxσ(Term 5)+xρxα3xαxμxνxσ(Term 6)

Computing the Product Term

Next, we compute ΓρμλΓλνσ

Γρμλ=xρxϵxζxμxηxλΓϵζη+xρxϵ2xϵxμxλΓλνσ=xλxαxβxνxγxσΓαβγ+xλxα2xαxνxσ

Multiplying these gives 4 terms. Note that we can collapse xηxλxλxα=δαη

ΓρμλΓλνσ=xρxϵxζxμxβxνxγxσΓϵζαΓαβγ(Term A)+xρxϵxζxμ2xαxνxσΓϵζα(Term B)+(xρxϵ2xϵxμxλxλxα)xβxνxγxσΓαβγ(Term C)+(xρxϵ2xϵxμxλxλxα)2xαxνxσ(Term D)

Now, substitute the Lemma into Terms C and D. They become

Term C=xδxμ2xρxδxαxβxνxγxσΓαβγTerm D=xδxμ2xρxδxα2xαxνxσ

Cancellation of Extra Terms

When we sum Aμν=μΓρνσ+ΓρμλΓλνσ, Term 1 cancels perfectly with Term C and Term 5 cancels perfectly with Term D.

The remaining components of Aμν are the pure tensor terms (Term 4 and Term A) and the leftover "extra" non-tensor terms (Term 2, Term 6, Term 3 and Term B). Group the non-tensor terms remaining in Aμν

Sμν=xρxα2xβxμxνxγxσΓαβγTerm 2+xρxα3xαxμxνxσTerm 6+xρxαxβxν2xγxμxσΓαβγTerm 3+xρxϵxζxμ2xαxνxσΓϵζαTerm B

Relabel dummy indices in Term B (ϵα,ζβ,αγ) to make it directly comparable to Term 3. The sum of Term 3 and Term B is

Term 3+Term B=xρxαΓαβγ(xβxν2xγxμxσ+xβxμ2xγxνxσ)

Look at the expression for Sμν. Because mixed partial derivatives commute, 2xβxμxν and 3xαxμxνxσ are symmetric under μν. In our combined (Term 3 + Term B), swapping μν simply swaps the two pieces inside the parenthesis. Therefore, Sμν is completely symmetric.

Antisymmetrizing to obtain the Tensor

Recall that the Riemann tensor is Rρσμν=AμνAνμ. When we subtract the μν terms, SμνSνμ=0. All extra terms vanish and the only survivors are the pure tensor terms (Term 4 and Term A)

Rρσμν=(Term 4(μ,ν)Term 4(ν,μ))+(Term A(μ,ν)Term A(ν,μ))

Plugging in Term 4

xρxαxδxμxβxνxγxσδΓαβγxρxαxδxνxβxμxγxσδΓαβγ

Swap dummy indices δβ in the subtracted term

xρxαxδxμxβxνxγxσ(δΓαβγβΓαδγ)

Plugging in Term A

xρxϵxζxμxβxνxγxσΓϵζλΓλβγxρxϵxζxνxβxμxγxσΓϵζλΓλβγ

Swap dummy indices ζβ in the subtracted term

xρxϵxζxμxβxνxγxσ(ΓϵζλΓλβγΓϵβλΓλζγ)

Finally, renaming the global dummy indices to (ϵτ,ζα,ββ,γω) to match the right side conventions

Rρσμν=xρxτxωxσxαxμxβxν(αΓτβωβΓταω+ΓταλΓλβωΓτβλΓλαω)Rτωαβ

Thus, we are left strictly with the required transformation law

Rρσμν=xρxτxωxσxαxμxβxνRτωαβ

which shows that the Riemann tensor is a tensor.

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