This article delves into the intricacies of pseudotensor analysis, focusing on the derivation of Synge and Fock pseudotensors and their comparison with the Landau-Lifshitz pseudotensor. It underscores the differences in the derivation approaches between Synge and Landau-Lifshitz, particularly highlighting the use of covariant derivatives and the simplification of the Riemann tensor. The author further explores the symmetries of the tensors involved and the implications these have on the derived pseudotensors. The article concludes with a comparative analysis of the canonical forms of the Synge and Landau-Lifshitz pseudotensors, noting the differences in terms and signs.
In a previous post, I showed a detailed derivation of the Landau-Lifshitz pseudotensor in all its forms: metric (canonical), Christoffel, and metric densities. Here, I'll widen the scope of analysis by deriving the closely related Synge and Fock pseudotensors and compare them to the Landau-Lifshitz pseudotensor.
Synge’s stress-energy (pseudo)tensor of the gravitational field
In space and time, a force we see,
A pseudotensor, wild and free.
Synge's creation, a work of art,
It twists and turns, it plays its part.
In gravity's dance, it holds a key,
A mathematical symmetry.
It tells us how, with great precision,
Matter moves on its own decision.
A hidden force, it may appear,
But in the equations, it is clear.
It guides the stars, and bends the light,
In the universe, it holds a might.
So let us honor Synge's mind,
For the pseudotensor, we shall find,
Is a part of our cosmic tale,
A story yet to be unveiled.
Anonymous
Reading the literature about the Landau-Lifshitz (LL) pseudotensor one cannot help but observe that authors, having encountered the difficulty in deriving the LL pseudotensor, refer to John Lighton Synge's book [2] as a place to get another, simpler derivation of the pseudotensor. This implies that the Synge's pseudotensor in [2] is the same as that of LL in [1]. Some authors, when they talk about the LL pseudotensor, give reference [2] together with [1]. [3][4] Chandrasekhar [6] derives Synge's pseudotensor by the way given in [2] and calls it the Landau-Lifshitz pseudotensor. Synge himself, in footnote on page 252 in [2] writes
We follow here a different approach [than Einstein] presented by Landau and Lifshitz ...This statement speaks about the same approach but it doesn't mean that the pseudotensors obtained by this approach are the same. On the other hand, Fock writes [5]
A different, but also symmetric set of quantities is used in the book by Landau and Lifshitz, The Classical Theory of Fieldsthereby implying that his approach (which is the same as Synge's) derives a pseudotensor that is somewhat different from the Landau-Lifshitz one.
Moreover, Synge's statement about a same approach
is fundamentally incorrect because the approaches of Synge and LL are quite different: Synge uses the properties of covariant derivatives to derive his pseudotensor composed of Christoffels coming from the covariant derivatives themselves while LL first eliminate all Christoffels from the the Einstein tensor (transformed down to Riemann tensor), taking only the second metric derivatives and composing from them an antisymmetric tensor whose divergence is identically zero in the locality. Then LL supplement this local pseudotensor with Christoffels (first metric derivatives) taken from the Riemann tensor to make it valid (zero divergence) for the global spacetime. Note that LL do not use covariant derivatives anywhere in their approach.
Synge defines Ricci tensor in a different manner that LL. The latter simplify the Riemann tensor by the first and third indices while Synge simplifies by the second and fourth indices. The Synge's definition differs by sign from LL as mentioned in LL [1] (footnote to formula 92,6) and in Singe [2] (footnote to formula I-(104)). Here, we will recheck Synge's proof, using the Ricci tensor as defined in Synge. Let's define Riemann by Christoffels as in LL91,4:
RiemannLL =
MakeRule[{RiemannCD[i, -k, -l, -m],
PD[-l][ChristoffelCD[i, -k, -m]] -
PD[-m][ChristoffelCD[i, -k, -l]] +
ChristoffelCD[i, -n, -l] ChristoffelCD[n, -k, -m] -
ChristoffelCD[i, -n, -m] ChristoffelCD[n, -k, -l]}]; (*LL91,4*)
Equal[RiemannCD[i, -k, -l, -m], RiemannCD[i, -k, -l, -m] /. RiemannLL]
We transfer the terms containing the second derivatives on the LHS and the Riemann tensor on the RHS
Equal[%[[2, 3]] + %[[2, 4]], -%[[2, 1]] - %[[2, 2]] + %[[1]]]
For the Ricci tensor we make a rule exactly as in LL92,7
RicciLL =
MakeRule[{RicciCD[-i, -k],
PD[-l][ChristoffelCD[l, -i, -k]] -
PD[-k][ChristoffelCD[l, -i, -l]] +
ChristoffelCD[l, -i, -k] ChristoffelCD[m, -l, -m] -
ChristoffelCD[m, -i, -l] ChristoffelCD[l, -k, -m]}]; (*LL92,7*)
Equal[RicciCD[-i, -k], RicciCD[-i, -k] /. RicciLL];
Equal[%[[2, 3]] + %[[2, 4]], -%[[2, 1]] - %[[2, 2]] + %[[1]]]
Compare these with the Synge's formulae VI-(151) on page 254:
It is easy to see several differences in indices, some of which are sign changes, and others are due to reshuffling of the antisymmetric indices l and m which amounts to the same.
Let’s reiterate the formula for
The expression in the brackets can be replaced with a tensor
The order of indexes in
DefTensor[U[i, k, l, m], M4, RiemannSymmetric[{1, 2, 3, 4}]];
U1 = MakeRule[{U[i, k, l, m], Detmetricg[] (metricg[i, k] metricg[l, m] - metricg[i, l] metricg[k,m])}];
** DefTensor: Defining tensor U[i,k,l,m].
Next, Synge observes that if
ToCanonical[PD[-k][PD[-l][PD[-m][U[i, l, k, m]/.U1]]]] == 0
true
and the covariant derivative of
ToCanonical[CD[-n][U[i, k, l, m]./U1]] == 0
true
Let's develop the CD by an arbitrary index n to Christoffels as is its usual definition, not forgetting that this whole expression is zero. We will put the metric determinant on hold so that the expression will not be processed so as to nullify the covariant derivative of the determinant
SetOptions[ToCanonical, UseMetricOnVBundle -> None];
CDbyN = CD[-n][1/Hold[Detmetricg[]] U[i, k, l, m]] //
CovDToChristoffel
Since the LHS is zero, we can multiply this expression by g to get rid of the denominator
Uiklmn = Hold[Detmetricg[]] CDbyN // Expand
According to LL86,5
Uiklmn /. {PD[-n][Hold[Detmetricg[]]]/Hold[Detmetricg[]] -> 2 ChristoffelCD[p, -n, -p]}
Uiklmn = -(%[[1]] + %[[2]] + %[[3]] + %[[4]] + %[[5]])
To get the covariant derivative by k, simply substitute n by k
Uiklmn /. {n -> k}
Uiklmk = %/.{p -> n}
Canonicalization reduces the terms from 5 to 3
UiklmkCan = Uiklmk // ToCanonical
Since canonicalization is not transparent, let me explain what is going on. In the fourth term, we exchange the dummy indices k and n. This does not change sign because k and n are symmetric in
Then the fourth term cancels with the first term to give
Symmetrize[ChristoffelCD[i, -k, -n] U[n, k, l, m], {n, k}]
But
ToCanonical[Symmetrize[ChristoffelCD[i, -k, -n] U[n, k, l, m], {n, k}]] == 0
true
It remains to do some cosmetic changes to the canonicalized Uiklmk: exchange k and n in the last term which does not change sign
and exchange m and n in the second term, which changes sign
The expression for Uiklmk becomes
the same as Singe's VI-(154).
An ordinary differentiation of the above by m gives
Uiklmkm = PD[-m][UiklmkCan]
Note that the second derivatives of the metric are contained in the first three terms, while terms 4,5,6 contain only first derivatives. We will separate second and first derivatives in the tensors Ail and Bil, respectively. As we will not use Ail and Bil for tensor operations, it suffice to treat them just as ordinary variables. We will also do a simplification of Ail, which factors common multipliers
Ail = Uiklmkm[[1 ;; 3]] // Simplification
Bil = Uiklmkm[[4 ;; 6]]
Here, Synge's idea is to substitute the expression in parentheses in Ail, containing second metric derivatives with the RHS of the equation containing the Ricci tensor plus first metric derivatives. Let's exchange the dummy indices:
The third term in Ail is transformed in
and antisymmetrized by the lower n and m
Antisymmetrize[ U[i, k, n, m] PD[-n][ChristoffelCD[l, -k, -m]], {-n, -m}]
Thus, for Ail we arrive to Singe's VI-(157)
Now substitute the terms in the first parentheses with the RHS of the expression for the Ricci tensor as defined by Synge:
The terms in the second parentheses are substituted with the RHS of the expression for the Riemann tensor as defined by Synge:
or, by changing the indices n and m in the second term
$Substituting
U[i, k, l, m] RicciCD[-k, -m] /. U1 // ToCanonical // ContractMetric
- U[i, k, n, m] RiemannCD[l, -k, -n, -m] /. U1 //
ToCanonical // ContractMetric
Summing these terms in Ail, we obtain
So, for
where
It remains to substitute Bil, expressed in terms of
rule1 = MakeRule[{PD[-n][U[i, k, l, m]], 2*ChristoffelCD[p, -n, -p]*U[i, k, l, m] - ChristoffelCD[m, -n, -p]*U[i, k, l, p] - ChristoffelCD[l, -n, -p]*U[i, k, p, m] - ChristoffelCD[k, -n, -p]*U[i, p, l, m] - ChristoffelCD[i, -n, -p]*U[p, k, l, m]}];
Bik /. rule1 // ToCanonical
To these terms we should add the additional
% + U[i, k, l, m] (ChristoffelCD[n, -m, -k]*ChristoffelCD[p, -n, -p] - ChristoffelCD[n, -m, -p]*ChristoffelCD[p, -k, -n]) + U[i, k, n, m]*ChristoffelCD[p, -k, -n]*ChristoffelCD[l, -p, -m]
SyngeAutomatic = % // ToCanonical
This is the Synge VI-(162) in an expanded form. We have to check it to be sure by manual entering and comparing.
U[i, k, l, m] (ChristoffelCD[n, -n, -k] ChristoffelCD[p, -p, -m] + ChristoffelCD[n, -p, -k] ChristoffelCD[p, -n, -m] - 2 ChristoffelCD[n, -k, -m] ChristoffelCD[p, -n, -p]) + U[i, k, m, n] (-ChristoffelCD[l, -k, -m] ChristoffelCD[p, -p, -n] - ChristoffelCD[p, -k, -m] ChristoffelCD[l, -p, -n]) + U[l, k, m, n] (-ChristoffelCD[i, -k, -m] ChristoffelCD[p, -p, -n] - ChristoffelCD[p, -k, -m] ChristoffelCD[i, -p, -n]) + U[k, m, n, p] ChristoffelCD[i, -k, -p] ChristoffelCD[l, -m, -n]
SyngeManual = % // ToCanonical
SyngeAutomatic - SyngeManual == 0
true
The final result from our calculation is exactly the same as in Synge's book. Let's develop the
SyngeAutomatic /. U1 // ToCanonical;
SyngeInMetrics = %/Detmetricg[] // ToCanonical
Not a good sign in terms of comparison. From 16 potential terms in Synge's pseudotensor, canonicalization leaves only 12. Canonicalization of the LL pseudotensor leaves all 16 terms. There is no point in futher direct comparison. Let's try to see where the difference lies. It was said above that Synge's
Let us try to derive the Synge's tensor with differentiations by the third and fourth indices.
Uiklmn /. {n -> l};
Uiklml = % /. {p -> n}
UiklmlCan = Uiklml // ToCanonical
Uiklmlm = PD[-m][UiklmlCan]
Here, the terms with the second derivatives constituting the Aik tensor can no longer be arranged in Ricci tensor. This makes impossible to continue derivation of the Synge's pseudotensor.
As another check, let us see if the canonical pseudotensor derived from Synge's pseudotensor is the same as the LL canonical pseudotensor.
SyngeInMetrics/2 // ChristoffelToGradMetric // ToCanonical
Surprise, the canonical Synge pseudotensor has 16 terms, the same as the canonical LL pseudotensor. Now if we immediately try to subtract the above from the canonical LL pseudotensor and canonicalize, we will be thrown an error in validation because of inhomogeneous indices. Indeed, the free indices of the above expression are i, l while in LL canonical they are i, k. Therefore, we must first make the free indices in the two expressions the same (i, k) and then compare by subtracting.
ChangeFreeIndices[%, {i, k}];
(LLCanonical - %) // ToCanonical
We see that subtracting the 2 pseudotensors tends to increase their numerical coefficients. This means that on the whole they are with somewhat opposite sign. So let's add them.
(LLCanonical + %) // ToCanonical
We can conclude from here that the Synge pseudotensor has a sign opposite to that of LL pseudotensor and the sum of the two pseudotensors leaves a small 4-terms residue.
Finally, let's see if the Synge pseudotensor is symmetric for the free indices i and l which is equivalent to antisymmetrizing it and equating it to 0.
ToCanonical[Antisymmetrize[SyngeAutomatic, {i, l}]] == 0
true
This shows that Synge's pseudotensor is symmetric.
Fascinating and immensely relevant since the LL and other similar nonlocal pseudotensors show the affinity of general relativity and quantum mechanics, e.g., EPR=ER. This affinity for all quantum objects is considered in the KTOC theory under development (Levich, E. 2014, 2015, 2017, 2019, 2020, 2022).
ReplyDeleteThank you for the kind comment. I'll read your papers with pleasure.
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