A Mathematical Comparison of the Schwarzschild and Kerr Metrics ()
1. Introduction
In order to explain the type of problems we want to solve, let us start adding a constant parameter to the example provided by Macaulay in 1916 that we have presented in a previous paper for other reasons [1]. However, before doing so, we first recall the following key definition and formal theorem before sketching the main results obtained in this paper:
DEFINITION 1.1: A system of order q on E is an open vector subbundle
with prolongations
and symbols
only depending on
. For
, we denote by
the projection of
on
, which is thus defined by more equations in general. The system
is said to be formally integrable (FI) if we have
, that is if all the equations of order
can be obtained by means of only r prolongations. The system
is said to be involutive if it is FI with an involutive symbol
. We shall simply denote by
the “set” of (formal) solutions. It is finally easy to prove that the Spencer operator
restricts to
.
The most difficult but also the most important theorem has been discovered by M. Janet in 1920 [2] and presented by H. Goldschmidt in a modern setting in 1968 [3]. However, the first proof with examples is not intrinsic while the second, using the Spencer operator, is very technical and we have given a quite simpler different proof in 1978 ( [2], also [4] [5] ) that we shall use later on for studying the Killing equations for the Schwarzschild and Kerr metrics:
THEOREM 1.2: If
is a system of order q on E such that its first prolongation
is a vector bundle while its symbol
is also a vector bundle, then, if
is 2-acyclic, we have
.
COROLLARY 1.3: (PP procedure) If a system
is defined over a differential field K, then one can find integers
such that
is formally integrable or even involutive.
The paper will be organized as follows:
· First of all, starting with an arbitrary system
, the purpose of the next motivating examples is to prove that the generating CC of the operator:
![]()
though they are of course fully determined by the first order CC of the final involutive system
produced by the prolongation/projection (PP) procedure, are in general of order
like the Riemann or Weyl operators, but may be of strictly lower order.
· The same procedure will be applied to the two first order systems of infinitesimal Lie equations allowing to define the Killing operator for the S-metric and the K-metric while comparing the respective results obtained. We may say that the case of the S-metric has already been treated in the publication quoted in the abstract but that it took us two years just for daring to engage in dealing similarly with the K-metric as anybody can understand by looking at the components of the Riemann tensor in the literature. It has been a surprising “miracle” to discover in the proof of Theorem 4.2 that there was a unique but tricky way to bring this problem to a purely mathematical and relatively simple computation on Lie equations and their prolongations.
· In the case of the S-metric, starting with the system
, we shall obtain
but
with a strict inclusion both with
again with a strict inclusion but in such a way that
is FI though not involutive because only its first prolongation is involutive. From this result we shall exhibit 15 (generating) second order CC and 4 (generating) unexpected third order CC without having to refer to any specific technical relativistic tool.
· Then, the case of the K-metric seems to be similar as it is also leading to the strict inclusions
of systems but the new systems are quite different and in particular
is now involutive, a result providing 14 (generating) second order CC and 4 (generating) third order CC. As in the motivating examples, it does not seem that the total numbers
or
have any intrinsic mathematical meaning. In both cases, using the Spencer operator, we explain why the important object is the group of invariance of the metric but not the metric itself.
· Finally, we are able to relate these results to the computation of certain extension modules in differential homological algebra, showing why the mathematical foundations of conformal geometry in arbitrary dimension and general relativity must be entirely revisited in the light of these results.
MOTIVATING EXAMPLE 1.4: With
, let us consider the second order linear system
with
and parametric jets
, defined by the two inhomogeneous PD equations where a is a constant parameter:
![]()
First of all we have to look for the symbol
defined by the two linear equations
. The coordinate system is not
-regular and exchanging
with
, we get the Janet board:
![]()
is involutive, thus 2-acyclic and we obtain from the main theorem
. However,
with a strict inclusion because
is now defined by adding the equations
. We may start afresh with
and study its symbol
with Janet tabular:
![]()
Since that moment, we have to consider the two possibilities:
·
: The initial system becomes
,
and has an involutive symbol. It is thus involutive because it is trivially FI as the left members are homogeneous with only one generating first order CC, namely
. We have
and the following commutative and exact diagrams:
![]()
![]()
We have thus the Janet sequence:
![]()
or, equivalently, the exact sequence of differential modules over
:
![]()
where p is the canonical projection onto the residual differential module.
·
: When the coefficients are in a differential field of constants, for example if
is invertible, we may choose
like Macaulay [1]. It follows that
is still involutive but we have the strict inclusion
and thus the strict inclusion
because
. We may thus continue the PP procedure and obtain the new strict inclusion
because
as
is defined by the 4 equations with Janet tabular:
![]()
As
is easily seen to be involutive, we achieve the PP procedure, obtaining the strict intrinsic inclusions and corresponding fiber dimensions:
![]()
Finally, we have
.
It remains to find out the CC for
in the initial inhomogeneous system. As we have used two prolongations in order to exhibit
, we have second order formal derivatives of u and v in the right members. Now, as we have an involutive system, we have first order CC for the new right members and could hope therefore for third order generating CC. However, we have the 4 CC:
![]()
It follows that we have only one second order and one third order CC:
![]()
but, surprisingly, we are left with the only generating second order CC
which is coming from the fact that the operator P commutes with the operator Q.
We let the reader prove as an exercise (see [1] [6] for details) that
,
and thus
,
in the following commutative and exact diagrams where E is the trivial vector bundle with
and
:
![]()
We have thus the formally exact sequence:
![]()
or, equivalently, the exact sequence of differential modules over D as before:
![]()
which is nevertheless not a Janet sequence because R2 is not involutive.
MOTIVATING EXAMPLE 1.5: We now prove that the case of variable coefficients can lead to strikingly different results, even if we choose them in the differential field
of rational functions in the coordinates that we shall meet in the study of the S and K metrics. We denote by
the ring of differential operators with coefficients in K. For this, let us consider the simplest situation met with the second order system
:
![]()
We may consider successively the following systems of decreasing dimensions
:
![]()
![]()
![]()
The last system is involutive with the following Janet tabular:
![]()
The generic solution is of the form
and it is rather striking that such a system has constant coefficients (This will be exactly the case of the S and K metrics but similar examples can be found in [5] ). We could hope for 9 generating CC up to order 4 but tedious computations, left to the reader as a tricky exercise, prove that we have in fact, as before, only 2 generating third order CC described by the following involutive system, namely:
![]()
![]()
satisfying the only first order CC:
.
We obtain the sequence of D-modules:
![]()
where the order of an operator is written under its arrow. This example proves that even a slight modification of the parameter can change the corresponding differential resolution.
MOTIVATING EXAMPLE 1.6: We comment a tricky example first provided by M. Janet in 1920, that we have studied with details in [4] [7]. With
,
,
,
and using jet notations, let us consider the inhomogeneous second order system:
![]()
We let the reader prove that the space of solutions has dimension 12 over
and that we have
in such a way that
is involutive and even finite type with a zero symbol. Accordingly, we have
. Passing to the differential module point of view, it follows that
and
. According to the general results presented, we have thus to use 5 prolongations and could therefore wait for CC up to order … 6!!!. In fact, and we repeat that there is no hint at all for predicting this result in any intrinsic way, we have only two generating CC, one of order 3 and … one of order 6 indeed, namely:
![]()
![]()
satisfying the only fourth order CC
![]()
It follows that we have the unexpected differential resolution:
![]()
with, from left to right,
,
,
,
and Euler-Poincaré characteristic
as expected. In addition, if we introduce a constant parameter a by replacing the coefficient
by
, we obtain
and obtain the same conclusions as before. We point out the fact that, when
, the system
, which is trivially FI because it is homogeneous, has a symbol
which is neither involutive (otherwise it should admit a first order CC), nor even 2-acyclic because we have the parametric jets:
![]()
and the long δ-sequence:
![]()
![]()
in which
,![]()
.
However,
is involutive with the following Janet tabular for the vertical jets
:
![]()
Accordingly, R3 is thus involutive and the only CC
is of order 2 because we need one prolongation only to reach involution and thus 2-acyclicity.
MOTIVATING EXAMPLE 1.7: With
, let us consider the inhomogeneous second order system:
![]()
We obtain at once through crossed derivatives
and, by substituting, two fourth order CC for
, namely:
![]()
satisfying
. However, we may also obtain a single CC for
, namely
and we check at once
,
while
. We let the reader prove that
,
. Hence, if
is a section of
while C is a section of
, the jet prolongation sequence:
![]()
![]()
is not formally exact because
, while the corresponding long sequence:
![]()
![]()
is indeed formally exact because
![]()
but not strictly exact because
is quite far from being FI as we have even
.
It follows from these examples and the many others presented in [6] that we cannot agree with [8] [9] [10] [11]. Indeed, it is clear that one can use successive prolongations in order to look for CC of order
and so on, selecting each time the new generating ones and knowing that Noetherian arguments will stop such a procedure … after a while!
However, as long as the numbers r and s are not known, it is not effectively possible to decide in advance about the maximum order that must be reached. Therefore, it becomes clear that exactly the same procedure MUST be applied when looking for the CC of the Killing operators we want to study, the problem becoming only a “mathematical” one but surely not a “physical” one.
IMPORTANT REMARK 1.8: The intrinsic properties of a system with constant coefficients may drastically depend on these coefficients, even if the systems do not appear to be quite different at first sight. Using jet notations, let us consider the second order system
depending on a constant parameter a and defining a differential module M by residue. When
we have the differential sequence:
![]()
and the adjoint sequence:
![]()
though the CC sequence that must be used with
is:
![]()
On the contrary, if
say
, we have the differential sequence:
![]()
and the CC sequence does coincide with the adjoint sequence:
![]()
It is thus essential to notice that
generates the CC of
when
, a result leading to
but this is not true when
, a result leading to
[5] [12] [13] [14].
Comparing the sequences obtained in the previous examples, we may state:
DEFINITION 1.9: A differential sequence is said to be formally exact if it is exact on the jet level composition of the prolongations involved. A formally exact sequence is said to be strictly exact if all the operators/systems involved are FI (see [1] for more details). A strictly exact sequence is called canonical if all the operators/systems are involutive. The only known canonical sequences are the Janet and Spencer sequences that can be defined independently from each other.
With canonical projection
, the various prolongations are described by the following commutative and exact introductory diagram:
![]()
Applying the standard “snake” lemma, we obtain the useful long exact connecting sequence:
![]()
which is thus connecting in a tricky way FI (lower left) with CC (upper right).
We finally recall the Fundamental Diagram I that we have presented in many books and papers, relating the (upper) canonical Spencer sequence to the (lower) canonical Janet sequence, that only depends on the left commutative square
with
when one has an involutive system
over E with
and
is the derivative operator up to order q:
![]()
We shall use this result, first found exactly 40 years ago [2] but never acknowledged, in order to provide a critical study of the comparison between the S and K metrics.
EXAMPLE 1.10: The Janet tabular in Example 1.4 with
provides the fiber dimensions:
![]()
We notice that 6 − 16 + 14 − 4 = 0, 1 − 10 + 20 − 15 + 4 = 0 and 1 − 4 + 4 − 1 = 0. In this diagram, the Janet sequence seems simpler than the Spencer sequence but, sometimes as we shall see, it is the contrary and there is no rule. We invite the reader to treat similarly the cases
and
.
2. Schwarzschild versus Kerr
2.1. Schwarzschild Metric
In the Boyer-Lindquist (BL) coordinates
, the Schwarzschild metric is
and
, let us introduce
with the 4 formal derivatives
,
. With speed of light
and
where m is a constant, the metric can be written in the diagonal form:
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with a surprisingly simple determinant
.
Using the notations of differential modules or jet theory, we may consider the infinitesimal Killing equations:
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where we have introduced the Christoffel symbols
through the standard Levi-Civita isomorphism
while setting
in the differential field K of coefficients [15]. As in the Macaulay example just considered and in order to avoid any further confusion between sections and derivatives, we shall use the sectional point of view and rewrite the previous 10 equations in the symbolic form
where L is the formal Lie derivative:
![]()
Though this system
has 4 equations of class 3, 3 equations of class 2, 2 equations of class 1 and 1 equation of class 0, it is far from being involutive because it is finite type with second symbol
defined by the 40 equations
in the initial coordinates. From the symmetry, it is clear that such a system has at least 4 solutions, namely the time translation
and, using cartesian coordinates
, the 3 space rotations
.
We obtain in particular, modulo
:
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We may also write the Schwarzschild metric in cartesian coordinates as:
![]()
and notice that the
matrix of components of the three rotations has rank equal to 2, a result leading surely, before doing any computation, to the existence of one and only one zero order Killing equation
. Such a result also amounts to say that the spatial projection of any Killing vector on the radial spatial unit vector
vanishes beause r must stay invariant.
However, as we are dealing with sections,
implies
,
,
… but NOT (care)
, these later condition being only brought by one additional prolongation and we have the strict inclusions
that we rename as
. Hence, it remains to determine the dimensions of these subsystems and their symbols, exactly like in the Macaulay example. We shall prove in the next section that two prolongations bring the five new equations:
![]()
and a new prolongation only brings the single equation
.
Knowing that
,
,
, we have thus obtained the 15 equations defining
with
and let the reader draw the corresponding Janet tabular for the 4 equations of class 3, the 4 equations of class 1, the 3 equations of class 0 and the 3 equations of class 2. The symbol
has the two parametric jets
and is not 2-acyclic. Adding
, we finally achieve the PP procedure with the 16 equations defining the system
with
, namely:
![]()
and we have replaced by “×” the only “dot” (non-multiplicative variable) that cannot provide vanishing crossed derivatives and thus involution of the symbol
with the only parametric jets
. It is easy to check that
, having minimum dimension equal to 4, is formally integrable, though not involutive as it is finite type with
with parametric jet
and to exhibit 4 solutions linearly independent over the constants. We let the reader prove as an exercise that the dimension of the Spencer
-cohomology at
is
but we have proved in [15] that its restriction to
is of dimension 1 only. We obtain:
THIS SYSTEM IS NOT INVOLUTIVE BUT DOES NOT DEPEND ON m ANY LONGER
Denoting by
with
the prolongation of
, it is the involutive system provided by the prolongation/projection (PP) procedure. We are in position to construct the corresponding canonical/involutive (lower) Janet and (upper) Spencer sequences along the following fundamental diagram I that we recalled in the Introduction. In the present situation, the Spencer sequence is isomorphic to the tensor product of the Poincaré sequence by the underlying 4-dimensional Lie algebra G, namely:
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In this diagram, not depending any longer on m, we have now
and
is of order 2 like
while all the other operators are of order 1:
![]()
We notice the vanishing of the Euler-Poincaré characteristics:
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We point out that, whatever is the sequence used or the way to describe
, then
is parametrizing the Cauchy operator
for the S metric. However, such an approach does not tell us explicitly what are the second and third order CC involved in the initial situation.
In actual practice, all the preceding computations have been finally used to reduce the Poincaré group to its subgroup made with only one time translation and three space rotations! On the contrary, we have proved during almost fourty years that one must increase the Poincaré group (10 parameters), first to the Weyl group (11 parameters by adding 1 dilatation) and finally to the conformal group of space-time (15 parameters by adding 4 elations) while only dealing with he Spencer sequence in order to increase the dimensions of the Spencer bundles, thus the number
of potentials and the number
of fields (compare to [16] ).
2.2. Kerr Metric
We now write the Kerr metric in Boyer-Lindquist coordinates:
![]()
where we have set
as usual and we check that:
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as a well known way to recover the Schwarschild metric. We notice that t or
do not appear in the coefficients of the metric. As the maximum subgroup of invariance of the Kerr metric must be contained in the maximum subgroup of invariance of the Schwarzschild metric because of the above limit when
, we shall obtain the only two possible infinitesimal generators
. We shall prove that the new first order system
is involutive, contrary to the case of the S metric. Accordingly, we have the fundamental diagram I with fiber dimensions:
![]()
with Euler-Poincaré characteristic
. Comparing the surprisingly high dimensions of the Janet bundles with the surprisingly low dimensions of the Spencer bundles needs no comment on the physical usefulness of the Janet sequence, despite its purely mathematical importance. In addition, using the same notations as in the preceding section, we shall prove that we have now the additional zero order equations
,
produced by the non-zero components of the Weyl tensor and thus, at best,
as these zero order equations will be obtained after only two prolongations. They depend on
and we should obtain therefore eventually
CC of order 2 without any way to know about the desired third order CC.
Using now cartesian space coordinates
with
,
, we have only to study the following first order involutive system for
with coefficients no longer depending on
, providing the only generator
:
![]()
and the fundamental diagram
![]()
The involutive system produced by the PP procedure does not depend on
any longer. Accordingly, this final result definitively proves that, as far as differential sequences are concerned:
THE ONLY IMPORTANT OBJECT IS THE GROUP, NOT THE METRIC
2.3. Schwarzschild Metric Revisited
Let us now introduce the Riemann tensor
and use the metric in order to raise or lower the indices in order to obtain the purely covariant tensor
. Then, using r as an implicit summation index, we may consider the formal Lie derivative on sections:
![]()
that can be considered as an infinitesimal variation. As for the Ricci tensor
, we notice that
though we have only:
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The 6 non-zero components of the Riemann tensor are known to be:
![]()
First of all, we notice that:
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We obtain therefore:
![]()
![]()
Similarly, we also get:
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We also obtain for example, among the second order CC:
![]()
and thus, among the first prolongations, the third order CC that cannot be obtained by prolongation of the various second order CC while taking into account the Bianchi identities [15]. Using the Spencer operator and the fact that
, we first obtain the 3 third order CC:
![]()
However, introducing
in the right member as in the motivating examples, we have 3 PD equations for
, namely:
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Using two prolongations and eliminating the third order jets, we obtain successively:
![]()
![]()
![]()
![]()
![]()
![]()
Summing, we see that all terms in
and
disappear and that we are only left with terms in
, including in particular the second order jets
, namely:
![]()
Setting
,
,
,
,
with
, we obtain the additional strikingly unusual third order CC for
:
![]()
Nevertheless, in our opinion at least, we do not believe that such a purely “technical” relation could have any “physical” usefulness and let the reader compare it with the CC already found in ( [15], Lemma 3.B.3). Finally, we have:
![]()
![]()
a result showing that certain third order CC may be differential consequences of the Bianchi identities (see [15] for details). Finally, we notice that:
![]()
and, comparing to the previous computation for
, nothing can be said about the generating CC as long as the PP procedure has not been totally achieved with a FI or involutive system.
2.4. Kerr Metric Revisited
Though we shall provide explicitly all the details of the computations involved, we shall change the coordinate system in order to confirm these results by only using computer algebra as less as possible. The idea is to use the so-called “rational polynomial” coefficients while setting anew:
![]()
in order to obtain over the differential field
:
![]()
with now
and
. For a later use, it is also possible to set
.
As this result will be crucially used later on, we have:
LEMMA 4.1:
.
Proof: As an elementary result on matrices, we have:
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with
because
and
is thus equal to:
![]()
that is, after division by
and
:
![]()
Finally, after eliminating the last term, we get:
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that is (Compare to [ ] and [ ]):
![]()
in a coherent way with the result
obtained
for the S metric when
. For a later use, we have obtained
.
Q.E.D.
Contrary to the S-metric, the main “trick” for studying the K-metric is to take into account that the partition between the zero and nonzero terms will not change if we use convenient coordinates, even if the nonzero terms may change. Meanwhile, we notice that the most important property of the K-metric is the
existence of the off-diagonal term
, that is
the
coefficient of
in the metric
which is indeed
. We may obtain therefore successively the Killing equations for the Kerr type metric, using sections of jet bundles and writing simply
while framing the principal derivative
of
:
![]()
With
, multiplying
by
,
by
and adding, we notice that:
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Similarly, multiplying
by
(care to the factor 2), we get:
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Substracting, we obtain therefore the tricky formula (see the previous Lemma):
![]()
Substituting, we obtain:
![]()
a situation leading to modify
,
and
, similar to the one found in the Minkowski case with
,
,
when
. We also obtain with
and
:
![]()
and with
and
:
![]()
Finally, multiplying
by
,
by
and adding, we finally obtain (see the Lemma again)
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Using the rational coefficients belonging to the differential field
, the nonzero components of the corresponding Riemann tensor can be found in textbooks.
One has the classical orthonormal decomposition:
![]()
and defining:
![]()
in which the coefficient of
is
while the coefficient of
is
indeed. We have
and make thus the Minkowski metric appearing in a purely algebraic way. We now use the new coordinates
,
and it follows that the conditions
,
are invariant under such a change of basis because dX1 and dX2 are respectively proportional to
and
. Indeed, as
and thus
, the new symbol
of
while
as mixed tensors.
We may obtain simpler formulas in the corresponding basis, in particular the 6 components with only two different indices are proportional to
while the 3 components with all four different indices are proportional to
.
In the original rational coordinate system, the main nonzero components of the Riemann tensor can only be obtained by means of computer algebra. For helping the reader to handle the literature, for example the book “Computations in Riemann Geometry” written by Kenneth R. Koehler that can be found on the net with a free access, we refer to the seventh chapter on “Black Holes”. We notice that ω→−ω, that is to say changing the sign of the metric, does not change the Christoffel symbols (
) and the Riemann tensor (
) but changes the sign of (
). For this reason, we have adopted the sign convention of this reference for the explicit computation of these later components as the products and quotients used in the sequel will not be changed.
We have successively:
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It must be noticed that we have been able to factorize the six components with only two different indices by
and the three components with four different indices by
, a result not evident at first sight but coherent with the orthogonal decomposition.
After tedious computations, we obtain:
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which is indeed vanishing when
for the S metric, both with:
![]()
![]()
Introducing the formal Lie derivative
and using the fact that
is a tensor, the system
contains the new equations:
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Taking into account the original first order Killing equations, we obtain successively:
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and we must add:
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These linear equations are not linearly independent because:
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Also, linearizing while using the Kronecker symbol
, we get:
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Thus, introducing the Ricci tensor and linearizing, we get:
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It follows that
and we have in particular
:
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The first row proves that
is a linear combination of
and
. Then, if we want to solve the three other equations with respect to
,
and
, the corresponding determinant is, up to sign:
![]()
Accordingly, we only need to take into account
.
Similarly, we also obtain
:
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where we have to set
.
Hence, taking into account
, we just need to use
and
.
However, using the previous lemma, we obtain the formal Lie derivative:
![]()
and thus
with
.
In addition, we have
and thus
.
We have also:
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The following invariants are obtained successively in a coherent way:
![]()
![]()
However, as
, then
and
can be both divided by a and we get the new invariant:
![]()
These results are leading to
,
, thus to
,
and
after substitution. In the case of the S-metric, only the first invariant can be used in order to find
.
Taking into account the previous result, we obtain the two equations:
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Using the fact that we have now:
![]()
we may multiply the first equation by
, the second by
and sum in order to obtain:
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Using the previous identity for
, we obtain therefore:
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Taking into account the fact that
and substituting, we finally obtain:
![]()
A similar procedure could have been followed by using
and
.
Now, we must distinguish among the 20 components of the Riemann tensor along with the following tabular where we have to take into account the identity
:
![]()
In this tabular, the vanishing components obtained by computer algebra are put in a box, the nonzero components of the left column do not vanish when
and the other components vanish when
. Also, the 11 (care) lower components can be known from the 10 upper ones.
Keeping in mind the study of the S-metric and the fact that
,
,
,
while framing the leading terms not vanishing when
, we get:
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Then, taking into account the fact that
, we obtain similarly:
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The leading determinant does not vanish when
because, in this case, all terms are vanishing and we are left with the two linearly independent framed terms, a result amounting to
and
in the case of the S-metric in [15].
In the case of the K-metric, we may use the relations already framed in order to keep only the four parametric jets
on the right side. We may also rewrite them as follows:
![]()
if we use the fact that
in the inverse metric.
As a byproduct, we are now left with the two (complicated) equations
and
where the dots mean linear combinations of
with coefficients in K and the study of the Killing operator is quite more difficult in the case of the K-metric. Of course, it becomes clear that the use of the formal theory is absolutely necessary as an intrinsic approach could not be achieved if one uses solutions instead of sections. Indeed the strict inclusion
cannot be even imagined if one does believe that
,
brings
and
. The computation could have been done with
and
because
and
.
The next hard step will be to prove that the other linearized components of the Riemann tensor do not produce any new different first order equation. The main idea will be to revisit the new linearized tabular with:
![]()
Putting the leading terms into a box, we have the identity
that must be combined with the following formulas
:
![]()
![]()
![]()
and so on, allowing to compute the 11 (care) lower terms from the 2 + 4 + 4 = 10 upper ones.
We have thus the following successive eleven logical inter-relations:
![]()
![]()
![]()
![]()
![]()
![]()
![]()
Keeping in mind the four additional equations and their consequences that have been already framed, both with the vanishing components of the Riemann tensor, namely:
![]()
we get successively:
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As we have already exhibited an isomorphism
, we may use only the later right set of parametric jet components. Using the previous logical relations while framing the leading terms not vanishing a priori when
, there is only one possibility to choose four components of the linearized Riemann tensor, namely:
![]()
In order to understand the difficulty of the computations involved, we propose to the reader, as an exercise, to prove “directly” that the two following relations:
![]()
![]()
are only linear combinations of the previous ones
.
We are facing two technical problems “spoilting”, in our opinion, the use of the K metric:
· With
in place of
, we have
and the leading term of
becomes proportional to
with a wrong sign that cannot allow using
. A similar comment is valid for the four successive leading terms.
· We also discover the summation
in
with a wrong sign that cannot allow introducing
as one could hope. A similar comment is valid for the four successive summations.
Nevertheless, we obtain the following unexpected formal linearized result that will be used in a crucial intrinsic way for finding out the generating second order and third order CC:
THEOREM 4.2: The rank of the previous system with respect to the four jet coordinates
is equal to 2, for both the S and K-metrics. We obtain in particular the two striking identities:
Proof: In the case of the S-metric with
, only the framed terms may not vanish and, denoting by “~” a linear proportionality, we have already obtained
:
![]()
Hence, the rank of the system with respect to the 4 parametric jets
just drops to 2 and this fact confirms the existence of the 5 additional first order equations obtained, as we saw, after two prolongations.
In the case of the K-metric with
, the study is much more delicate.
With
, the coefficients of the
metric of the previous system on the basis of the above parametric jets are proportional to the symmetric matrix:
![]()
Indeed, we have successively for the common factor
:
![]()
![]()
![]()
![]()
and similarly for the common factor
:
![]()
![]()
![]()
![]()
We do not believe that such a purely computational mathematical result, though striking it may look like, could have any useful physical application and this comment will be strengthened by the next theorem provided at the end of this section.
Q.E.D.
COROLLARY 4.3: The Killing operator for the K metric has 14 generating second order CC.
Proof: According to the previous theorem, we have
as we can choose the 4 parametric jets
and
. Using the introductory diagram with
and thus
, we obtain at once
in a purely intrinsic way. We may thus start afresh with the new first order system
obtained from
after 2 prolongations. This result is thus obtained totally independently of any specific GR technical object like the Teukolski scalars, the Killing-Yano tensors or even the Penrose spinors introduced in [8] [9] [10] [11] [16].
Q.E.D.
Finally, we know from [2] [4] [12] [15] [17] [18] [19] that if
is a system of infinitesimal Lie equations, then we have the algebroid bracket
defined on sections by the following formula not depending on the lift
of
:
![]()
with the algebraic bracket bilinearly defined by
and such that:
![]()
It follows that
is such that
with
because we have obtained a total of 6 new different first order equations. We have on sections (care again) the 16 (linear) equations of
as follows:
![]()
and we may choose only the 2 parametric jets
among
to which we must add
in any case as they are not appearing in the Killing equations and their prolongations.
The system is not involutive because it is finite type with
and
cannot be thus involutive.
It remains to make one more prolongation in order to study
with strict inclusions in order to study the third order CC for
already described for the Schwarzschild metric in [15].
![]()
Surprisingly and contrary to the situation found for the S metric, we have now a trivially involutive first order system with only solutions
,
,
,
. However, the difficulty is to know what second members must be used along the procedure met for all the motivating examples. In particular, we have again identities to zero like
,
or, equivalently,
,
and thus 4 third order CC coming from the 4 following components of the Spencer operator:
![]()
a result that cannot be even imagined from [8] [9] [10] [11] [16]. Of course, proceeding like in the motivating examples, we must substitute in the right
members the values obtained from
and set for example ![]()
while replacing
and
by the corresponding linear combinations of the Riemann tensor already obtained for the right members of the two zero order equations.
Using one more prolongation, all the sections (care again) vanish but
and
, a result leading to
in a coherent way with the only nonzero Killing vectors
. We have indeed:
![]()
Like in the case of the S metric,
is not involutive but
is involutive. However, contrary to the S metric with
, now
for the K metric and
is trivially involutive with a full Janet tabular having 16 rows of first order jets and 2 rows of zero order jets.
REMARK 4.4: We have in general ( [2] [5] p 339, 345):
![]()
that is, in our case
. However, we have indeed the equality
even if the conditions of Theorem 1.1 are not satisfied because
is not 2-acyclic. Indeed, the Spencer map
is not injective and we let the reader check as an exercise that its kernel is generated by
and the Spencer δ-cohomology is such that
because the cocycles are defined by the equations
. Hence, contrary to what could be imagined, the major difference between the S and K-metrics is not at all the existence of off-diagonal terms but rather the fact that
is not involutive with
for the S-metric while
is involutive with
for the K-metric. This is the reason for which one among the four third order CC must be added with two prolongations for the S-metric while the four third order CC are obtained in the same way from the Spencer operator for the K-metric. Of course no classical approach can explain this fact which is lacking in [8] [9] [10] [11].
The following result even questions the usefulness of the whole previous approach:
THEOREM 4.5: The operator
admits a minimum parametrization by the operator
with 1 potential when
, found in 1863. It admits a canonical self-adjoint parametrization by the operator
with 6 potentials when
, found in 1892 and modified to a mimimum parametrization by the operator Maxwell with 3 potentials, found in 1870 or Morera found in 1892. More generally, it admits a canonical parametrization by the operator
with
potentials that can be modified to a relative parametrization by
with
potentials which is nevertheless not minimum when
, found in 2007. In all these cases, the corresponding potentials have nothing to do with the perturbation of the metric. Such a result is also valid for any Lie group of transformations, in particular for the conformal group in arbitrary dimension.
Proof: We provide successively the explicit corresponding parametrizations:
·
: Multiplying the linearized Riemann operator by a test function
and integrating by parts, we obtain (care to the factor 2 involved):
![]()
![]()
Cauchy operator ![]()
Airy operator ![]()
![]()
It is clear that the test function f has nothing to do with the metric ω ( [5], Introduction).
·
We now present the original Beltrami parametrization:
![]()
which does not seem to be self-adjoint but is such that
. Accordingly, the Beltrami parametrization of the Cauchy operator for the stress is nothing else than the formal adjoint of the Riemann operator. However, modifying slightly the rows, we get the new operator matrix:
![]()
which is indeed self-adjoint. Keeping
with
, we obtain the Maxwell parametrization:
![]()
which is minimum because
. However, the corresponding operator is FI because it is homogeneous but it is not evident at all to prove that it is also involutive as we must look for δ-regular coordinates (see [20] for the technical details).
·
This is far more complicated and we do believe that it is not possible to avoid using differential homological algebra, in particular extension modules. As we found it already in many books [4] [12] [17] [21] or papers [12] [13] [14] [15] [22], the linear Spencer sequence is (locally) isomorphic to the tensor product of the Poincaré sequence for the exterior derivative by a Lie algebra
with
equal to the dimension of the largest group of invariance of the metric involved. When
, this dimension is 10 for the M-metric, 4 for the S-metric and 2 for the K-metric. As a byproduct, the adjoint sequence roughly just exchanges the exterior derivatives up to sign and one has for example, when
, the relations
,
. It follows that, if D2 generates the CC of D1, then
is parametrizing
, a fact not evident at all, even when
for the Cosserat couple-stress equations exactly described by
[18]. Passing to the differential modules point of view with the ring (even an integral domain)
of differential operators with coefficients in a differential field K, this result amounts to say that
. As it is known that such a result does not depend on the differential resolution used or, equivalently, on the differential sequence used, if
generates the CC of
in the Janet sequence, then
is parametrizing
and this result is still true even if
is not involutive. In such a situation, which is the one considered in this paper, the Killing operators for the M-metric, the S-metric and the K-metric are such that, whatever are the generating CC
(second order for the M-metric, a mixture of second and third order for the S-metric and K-metric), then
is, in any case, parametrizing the Cauchy operator
for any
. Once more, the central object is the group, not the metric. The same results are also valid for any Lie group of transformations, in particular for the conformal group in arbitrary dimension, even if the operator
is of order 3 when
as we shall see below [6] [13] [14] [23].
Q.E.D.
REMARK 4.6: Accordingly, the situation met today in GR cannot evolve as long as people will not acknowledge the fact that the components of the Weyl tensor are the torsion elements (the so-called Lichnerowicz waves in [22] ) for the equations
because the Einstein equations cannot be parametrized and the extension modules are torsion modules [5] [7] [13] [19]. Such a result is only depending on the group structure of the conformal group of space-time that brings the canonical splitting
without any reference to a background metric as it is usually done [4] [15] [19] [22] [23]. It is an open problem to know why one may sometimes find a self-adjoint operator. It is such a confusion that led to introducing the so-called Einstein parametrizing operator [19] [22]. A minimum parametrization of the Cauchy operator when
with 6 potentials can be found by keeping only the Lagrange multipliers
with
used in [13] while setting
like Morera when
.
EXAMPLE 4.7: (Weyl tensor for
and euclidean metric) We proved in ( [21], p 156-158) and more recently in [14] [22] [23] that, for
, the natural “geometric object” corresponding to the Weyl tensor is no longer providing a second order differential operator but by a third order Weyl operator
with first order CC
in the differential sequence:
![]()
corresponding to the differential sequence of D-modules where p is the canonical residual projection:
![]()
The true reason is that the symbol
of
is finite type with second prolongation
while its first prolongation
is not 2-acyclic. It is important to notice that the operators are acting on the left on column vectors in the upper sequence but on the right on row vectors in the lower sequence though we have in any case the identities
and
.
Of course, these operators can be obtained by using computer algebra like in ([21], Appendix 2) but one may check at once that
and
are completely different operators while the operator
is far from being self-adjoint even though it is described by a
operator matrix. Our purpose is to prove that it can be nevertheless transformed in a very tricky way to a self-adjoint operator, exactly like the
curl operator in 3-dimensional classical geometry because
. It does not seem that these results are known today.
The starting point is the
first order operator matrix defining the conformal Killing operator
, namely:
![]()
Substracting the fourth row from the first row and multiplying the fourth row by
, we obtain the operator matrix:
![]()
Adding the fourth row to the first, we obtain the operator matrix:
![]()
Adding the first row to the fourth row and dividing by 2, we obtain the operator matrix:
![]()
Multiplying the second, fourth and fifth row by −1, then multiplying the central column of the matrix thus obtained by −1, we finally obtain the operator matrix
:
![]()
We now care about transforming
given in ( [21], p 158) by the
operator matrix:
![]()
Dividing the first column by 2 and the fourth column by −2, then using the central row as a new top row while using the former top row as new bottom row, we obtain the operator matrix
:
![]()
and check that
like in the Poincaré sequence for
where
. As the new corresponding operator
is homogeneous and of order 3 (care), we obtain locally
, a result not evident at first sight (compare to [21], p 157).
The combination of this example with the results announced in [14] [23] brings the need to revisit almost entirely the whole conformal geometry in arbitrary dimension and we notice the essential role performed by the Spencer δ-cohomology in this new framework.
3. Conclusion
First of all, comparing the M-metric, the S-metric and the K-metric by using the corresponding systems of first order infinitesimal Lie equations, we may summarize the results previously obtained by repeating that, when E = T, the smaller is the background Lie group, the smaller are the dimensions of the Spencer bundles and the higher are the dimensions of the Janet bundles. As a byproduct, we claim that the only solution for escaping is to increase the dimension of the Lie group involved, adding successively 1 dilatation and 4 elations in order to deal with the conformal group of space-time while using the Spencer sequence instead of the Janet sequence. In particular, the Ricci tensor only depends on the elations of the conformal group of space-time in the Spencer sequence where the perturbation of the metric tensor does not appear any longer contrary to the Janet sequence. It finally follows that Einstein equations are not mathematically coherent with group theory and formal integrability. In other papers and books, we have also proved that they were also not coherent with differential homological algebra which is providing intrinsic properties as the extension modules, which are torsion modules, do not depend on the sequence used for their definition, a quite beautiful but difficult theorem indeed. The main problem left is thus to find the best sequence and/or the best group that must be considered. Presently, we hope to have convinced the reader that only the Spencer sequence is clearly related to the group background and must be used, on the condition to change the group. As a byproduct, we may thus finally say that the situation will not evolve in GR as long as people will not acknowledge the existence of these new purely mathematical tools like Lie algebroids or differential extension modules and their purely mathematical consequences. Summarizing this paper in a few words, we do really believe that “God used group theory rather than computer algebra when He created the World”!