A NNALES DE L ’I. H. P., SECTION A
S. R. C ZAPOR
R. G. M C L ENAGHAN F. D. S ASSE
Complete solution of Hadamard’s problem for the scalar wave equation on Petrov type III space-times
Annales de l’I. H. P., section A, tome 71, n
o6 (1999), p. 595-620
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595
Complete solution of Hadamard’s problem for
the scalar
waveequation
onPetrov type III space-times
S.R. CZAPOR
R.G. McLENAGHAN
F.D. SASSEa Department of Mathematics and Computer Science, Laurentian University, Sudbury, Ontario, Canada P3E 2C6
b Department of Applied Mathematics, University of Waterloo, Waterloo, Ontario, Canada N2L 3G1
C Department of Mathematics, Centre for Technological Sciences-UDESC, Joinville 89223-100, Santa Catarina, Brazil
Article received 7 July 1998
Vol. 71, n° 6, 1999, Physique theorique
ABSTRACT. - We prove that there are no Petrov
type
IIIspace-times
on which the
conformally
invariant scalar waveequation
or the non-self-adjoint
scalar waveequation
satisfiesHuygens’ principle.
@Elsevier,
Paris
RESUME. - Nous prouvons
qu’ il
n’existe aucunespace-temps
detype
III de Petrov surlequel 1’ equation
invariante conforme des ondes scalairesou
F equation
des ondes scalairesnon-auto-adjoint
satisfait auprincipe
deHuygens.
@Elsevier,
ParisAnnales de l’Institut Henri Poincaré - Physique theorique - 0246-0211
Vol. 71/99/06/@ Elsevier, Paris
1. INTRODUCTION
This paper is devoted to the solution of Hadamard’s
problem
on Petrovtype
IIIspace-times,
for theconformally
invariant scalar waveequation
and the
non-self-adjoint
scalar waveequation
In the above
equations
D denotes theLaplace-Beltrami operator
corre-sponding
to the metric gab of thebackground space-time V4,
u the un-known
function, R
the Ricciscalar,
Aa thecomponents
of agiven
con-travariant vector field and C a
given
scalar function. Thebackground manifold,
metric tensor, vector field and scalar function are assumed to be All considerations of this paper areentirely
local.The
homogeneous equations ( 1 )
and(2) satisfy NMy’ principle
inthe sense of Hadamard
[ 15 ] if u(x) depends only
on theCauchy
data in anarbitrarily
smallneighborhood
of the intersection between the backward characteristic conoidC- (x)
with the vertex at x and the initial surfaceS,
for
arbitrary Cauchy
data onS, arbitrary S,
and for allpoints
x in thefuture of S.
problem
for( 1 )
and(2)
is that ofdetermining
all
space-times
for whichHuygens’ principle
is valid. We recall that twoequations (2)
are said to beequivalent
if andonly
if one may be transformed into the otherby
any combination of thefollowing
trivialtransformations:
(a)
ageneral
coordinatetransformation;
(b) multiplication
of theequation by
the function whichinduces a
conformal transformation
of the metric(c)
substitution of 03BBu for the unknown function u, where 03BB is a non-vanishing
function onV4.
We note that the
Huygens’
character of(2)
ispreserved by
any trivial transformation. In the case of( 1 )
the trivial transformations reduce to conformal transformations with À ==~.
Carminati and
McLenaghan [4]
have outlined a program for the solution of Hadamard’sproblem
for the scalar waveequation, Weyls’
neutrino
equation
and Maxwell’sequations
based on theconformally
Annales de l’ Institut Henri Poincaré - Physique theorique
invariant Petrov classification of the
Weyl
conformal curvature tensor.This involves the consideration of five
disjoint
cases which exhaustsall the
possibilities
fornon-conformally
flatspace-times.
Hadamard’sproblem
for( 1 )
and(2)
has beencompletely
solved for Petrovtype
Nspace-times by
Carminati andMcLenaghan [3,5]
andMcLenaghan
andWalton
[20].
Their results may be summarized as follows:Any non-self-adjoint eguation (2)
on any Petrov type Nbackground space-time satisfies Huygens’ principle af
andonly if
it isequivalent
to the wave
equation
~u = 0 on an exactplane
wavespace-time
withmetric
For Petrov
type
Dspace-times
thefollowing
result was obtainedby
Carminati and
McLenaghan [6], McLenaghan
and Williams[21 ]
andWunsch
[27] :
There exist no Petrov type D
space-times
on which theconformally
invariant scalar wave
eguation (1 ) satisfies Huygens’ principle.
In the
present
paper wecomplete
this program for theconformally
invariant scalar wave
equation ( 1 )
on Petrovtype
IIIspace-times by proving
thefollowing
theorem:THEOREM 1. - There exists no Petrov type III
space-times
on whichthe
conformally
invariant scalar waveequation ( 1 ) satisfies Huygens’
principle.
The results on
type
N andtype
Dspace-times
described above andTheorem 1 lend
weight
to theconjecture
which states that everyspace-
time on which the
conformally
invariant scalar waveequation
satisfiesHuygens’ principle
isconformally
related to theplane
wavespace-time (3)
or isconformally
flat[3,5].
Hadamard’s
problem
for thegeneral non-self-adjoint equation (2)
maynow be solved with the
help
of Theorem 1 and the results ofAnderson, McLenaghan
and Sasse[ 1 ]
where thefollowing
theorem isproved:
THEOREM 2. -
Any non-self-adjoint
scalar waveequation (2)
whichsatisfies Huygens’ principle
on any Petrov type IIIbackground space-time
is
equivalent
to theconformally
invariant scalar waveequation ( 1 ).
Combining
these two theorems we obtainVol. 71, n ° 6-1999.
THEOREM 3. - There exist no Petrov type III
space-times
on which thenon-selfadjoint
scalar waveequation satisfies Huygens’ principle.
The
corresponding problem
for theWeyl
neutrinoequation
andMaxwell’s
equations
is solved in[19].
The
starting point
of ourproof
of Theorem 1 is the paperby
Carminatiand
McLenaghan [7],
where thefollowing
results are obtained for Petrovtype
IIIspace-times:
THEOREM 4. - The
validity of Huygens’ principle for
theconformally
invariant scalar wave
equation (1),
on any Petrov type IIIspace-time implies
that thespace-time
isconformally
related to one in which everyrepeated principal spinor field oA, of
theWeyl spinor
is recurrerct, that iswhere
IBB
is a2-spinor;
andwhere
iA
is anyspinor field satisfying oAlA
= 1.THEOREM 5. -
If
anyoneof
thefollowing
three conditionsis
satisfied,
then there exist no Petrov type IIIspace-times on
whichthe
conformaLLy
invariant scalar waveequation (1) satisfies Huygens’
principle.
It is
important
to note that these earlier results solve Hadamard’sproblem
under what haveproved
to befairly strong assumptions (namely,
that one of
(7), (8)
or(9)
issatisfied).
The purpose of thepresent
paper is to make theanalysis completely general by removing
theseassumptions.
We follow the conventions of
[7],
and use the results established there to obtain(most of)
the basicequations
needed for theproof
of Theorem 1.In Section 2 we
give
the necessary conditions for thevalidity
ofHuygens’ principle
that will be used in this paper, andgive
a briefsummary of their
implications.
From these necessaryconditions,
wederive the further side relations needed for our
analysis
in terms of theAnnales de l’Institut Henri Poincaré - Physique theorique
Newman-Penrose scalars. The
key
to ourproof
is the six-index necessary condition obtainedby
Rinke and Wunsch[23]
which was not used in[7].
In Section 3 we examine these side relations in the case
(Pn
= 0 and show thatthey
lead to a contradiction. Theproof
of Theorem 1 iscompleted
inSection
4,
where the case~11 ~
0 is treated.It is worth
mentioning
that the tools ofcomputer algebra
are usedthroughout
this paper.Initially
weemploy
theMaple [22] package NPspinor [ 10,11 ]
to extractdyad
components ofspinor
versions of the necessaryconditions,
and then tomanipulate
theresulting expressions
inNewman-Penrose form. In the
case Ø11
= 0 we use the Grobner basispackage
of theMaple system
toexplicitly
determine solutions ofsystems
ofalgebraic equations. Finally,
for the case~11 ~
0 we use the GBpackage
ofFaugere [ 12]
to examine thesolvability
of a somewhatlarger system
ofalgebraic equations.
2. FORMALISM AND BASIC
EQUATIONS
The necessary conditions for the
validity
ofHuygens’ principle
for( 1 )
which we
employ
aregiven by
where
~bl.71,n°6-1999.
where
Here
Aa
:= denotes the Riemann tensor,Cabcd
theWeyl
tensor,
Rab
:= the Ricci tensor, and R :=gab Rab
the Ricciscalar associated to the metric gab. The conditions
(III), (V)
and(VII)
are
necessarily conformally
invariant.Spinor
versions of conditions(III)
and
(V),
and the conventions used for conversion from theoriginal
tensorform,
aregiven
in[7].
Mathisson
[ 17],
Hadamard[ 16],
andAsgeirson [2]
obtained condition(III)
for(2)
in the casegi~
constant. Condition(III)
was obtained in thegeneral
case for(2) by
Gunther[ 14] .
Condition V was obtainedby McLenagham [ 18]
in the caseRab
=0,
andby
Wunsch[26]
for thegeneral
case. Condition(VII)
was obtainedby
Rinke and Wunsch[23].
Petrov
type
IIIspace-times
are characterizedby
the existence of aspinor
fieldoA satisfying
Such a
spinor
field is called ’ arepeated principal spinor
of theWeyl spinor
and 0 is determined ’
by
the latter up to anarbitrary
variablecomplex
factor.Annales de l’ Institut Henri Poincare - Physique théorique
Let lA
be anyspinor
fieldsatisfying
The ordered set ~, called a
dyad,
defines a basis for the1-spinor
fields on
V4.
It was shown in
[7]
that the necessary conditions(III)
and(V) imply
that there exists a
dyad
and a conformaltransformation ~
suchthat
We notice that the
expressions (24)
determine the tetraduniquely.
On the other
hand,
conditions(23)
are invariant under any conformal transformationsatisfying
which
implies
that we still have some conformal freedom. Under aconformal transformation we have
[25] :
Thus,
we canchoose ~
such thatwhere c is a constant. The conditions
(28)
are satisfied in view of(27).
Let us now derive some side relations that follow from the
previously
obtained
Eqs. (23)-(30)
and the necessary conditions(10)-(12);
thesewill be
required
in theanalysis
of thefollowing
sections. We may assume that0,
since the case in which this is not true wasalready
considered in
[7]. By contracting
condition(III)
with weget
From the Bianchi
identities, using
the aboveconditions,
we obtainBbl.71,n° 6-1999.
From the Ricci identities we
get
thefollowing
relevant Pfaffians:We can obtain useful
integrability
conditions for the abovePfaffians, by using
Newman-Penrose(NP)
commutation relations.By substituting
them in the commutator
expression [~ , D]~22 2014 [ 0 , ~]~i2.
weget
By contracting
condition(V)
withlABCD-ABCD, we
findBy substituting (30)
into thisequation
weget
From
(40), (41 )
and(30)
we then obtain:By contracting
condition(V)
with we findUsing (36), (41 )
and thecomplex conjugate
of(42),
weget
Annales de l’Institut Henri Poincare - Physique theorique
On the other
hand, the
NP commutator[ ~ , 8 ] (a
+27r) = (a -
+27r)
+(- a
+~6) ~ (of + 27r), yields
thefollowing expression
Eliminating
between(47)
and(48),
andsolving
forD/~,
weget
where we have assumed that the denominator of the
expression above, given by
is non-zero. The case
dl
= 0 will be considered later.Substituting expression (49)
for into(47)
we obtainOne side relation can now be obtained
by subtracting
thecomplex conjugate
of(49)
from(51 ).
We obtain:Vol. 71, n° 6-1999.
We notice that
(49)
and(51 )
have the same denominator.Thus,
if wekeep
theseexpressions
forD/~
andD/Z,
the Pfaffians~,8 , ~a, ~~c,
given by (42), (38)
and(41 ), respectively,
and theircomplex conjugates,
also have the same denominator. This
procedure
is crucial tokeep
theexpressions
to be obtainedfrom
theintegrability conditions
within areasonable size.
Except for 03B403B1,
all Pfaffiansinvolving 8, 8, applied
toa,
,8, ~c
areexplicitly determined.
The
following expression
for canbe obtained
fromthe
NPcommutator
[Y, ~] ~ = (/7 - /~)D ~ + (a - ~)~ + (~6 - a) ~6 :
By substituting (49)
and(51 )
into thisequation
weget:
where,
for now, we assume that the denominator in theexpression
above:is non-zero.
Contracting
condition(VII)
withABCDEOF-BCDOAEF yields
Annales de l’Institut Henri Poincare - Physique theorique
Bbl.71,n° 6-1999.
The second-order terms
D( ~ y ), D( ~ y), D( ~ ,~c ), D(0_,8 ), D(A(Y),
D(A7r),
can beexpressed
in terms of known Pfaffians and 03B4 a,by using
the NP commutation relations
involving
eachpair
ofoperators.
After the substitutions we obtainSolving
£ thisequation
for 03B403B1 weget
Annales de Henri Poincare - Physique ~ theorique
where the denominator of
(58),
is assumed to be non-zero for now.
Vol. 71, n ° 6-1999.
Subtracting (54)
from(58)
andtaking
the numerator,Annales de Henri Poincaré - Physique theorique
3. THE
CASE (/)11 == 0
Carminati and
McLenaghan [7]
used the conditions(III)
and(V) given
in Section 2 to prove that
Huygens’ principle
is not satisfied if any of thespin
coefficients a,,8
or yr vanish. We now extend theproof
for thecase in which 0 and
(/)11 = 0; i.e.,
we shall prove thefollowing
theorem:
THEOREM 6. - Let
V4
be anyspace-time
which admits aspinor dyad
with the
properties
where
I BE is a 2-spinor,
andThen the
validity of Huygens’ principle for
theconformally
invariantequation (1) implies
thatProof. - When 03A611
= 0 thequantity given by (60),
factors in thefollowing
form:where
Let us
consider
first the case in which p2 = 0.Applying 8
to(67)
andsolving for 03B403B1,
we obtain:Vol. 71, n° 6-1999.
where the denominator of the
expression above, given by
is assumed to be non-zero, for now.
Here and all
equations
obtainedby comparing
different expres- sions for 03B4a ,
arepolynomials
in threecomplex
variables a,03B2
and 7r.One
complex
variable can be eliminatedby introducing
thefollowing
new variables:
In what follows we first prove that the necessary conditions
imply
thatboth Xl and x2 are constants.
Then, later,
we shall prove that this leads toa contradiction.
In the new variables defined
by (70),
theexpression (67)
assumes theform
Annales de l’Institut Henri Poincaré - Physique theorique
Subtracting (68)
from(58) (with
=0),
andtaking
the numerator,gives
Vol. 71, n° 6-1999.
We now wish to determine the solutions of the
system
ofalgebraic equations { p2
==0, N2
=0}.
This may beaccomplished
inprinciple using
the Grobner basis methodof Buchberger [ 13]
as follows.First,
wetreat the
quantities
x1, x2,x2
asindependent variables,
and viewthe
quantities
p2,N2
aspolynomials
in these indeterminates over the field of rational numbers.(In
thesubsequent analysis
we may use thefact that some variables are
complex conjugates
of eachother,
but thiswill not be necessary for our immediate
purpose.) Then, by computing
a Grobner basis for the set
{ p2, N2} (actually,
the ideal(~2~2))
withrespect
to apurely lexicographic ordering
of terms(see [ 13])
we obtain anew set of
polynomials
with the same solutions but in which the variables have beensuccessively
eliminated as far aspossible.
In order tospeed
the
computations,
we use aspecial
variant of thealgorithm [9]
whichcombines the nonlinear elimination with factorization of intermediate results.
(This algorithm
is available in theMaple system
as the functiongsolve.)
For thepolynomials {~2. ~2}.
thealgorithm produces
thefollowing components,
whichcollectively
contain all solutions:Annales de Poincaré - Physique theorique
Using
the fact that thepair (jci, ~2)
and(~1,~2)
arecomplex conjugates
of each
other,
we conclude that the setsGi
toGs provide
solutions whichare either
impossible
or in which xl and x2 are constant. In the case ofG6,
this is not
immediately
obvious. Its smallest term is:Subtracting (79)
from itscomplex conjugate
we obtain the conclusion that xl isreal,
whichimplies
that it must be constant. It follows that x2 must be constant as well.Let us consider now the case
We then use the side relation
Sl given by (52),
whose numerator takes theform:
Vol. 71,~6-1999.
Applying
our nonlinear eliminationalgorithm
as before to pi, p3 we obtain thefollowing equivalent system
ofequations:
Subtracting (82)
from itscomplex conjugate yields xl
==Subtracting (84)
from itscomplex conjugate
nowgives
x2 ==x2
=12x1
+ 22.Substituting
these relations back in(82)
and(83)
results in asystem
withno solution.
It thus follows that in either of the cases which arise from
Eq. (65),
xl and x2 mustnecessarily
be constant.However,
it may be shown(though
we
postpone
the details until thefollowing section)
that this too leads toa contradiction.
We must
finally
consider the case in which the denominator ofgiven by (49),
is zero. Here we shall suppose that(/)11
is notnecessarily
zero, so that the side relations derived in Section 2 will remain valid in the
following
section as well.According
to(50)
and(70),
From
(49)
we obtainwhere is defined as follows:
Applying 03B4
to/i, using (30), (38)
and(36),
andsolving
for 03B4 03B1, weget
Annales de l’ Institut Henri Poincare - Physique ~ theorique "
By applying 8
todl,
nowusing (40)-(42)
and(47)
andsolving
forwe
get
Subtracting
Dgiven by (47),
from thecomplex conjugate
of(89), gives
Applying 5
to(90) gives
Applying
nonlinear elimination toJi, f 1, E1, E2
andE3 ,
we findthat this
system
has no solution.The cases where each of the denominators
d2, d3
andd4,
thatappeared
in the
preceeding equations
are zero lead tocontradictions, according
to
[24].
The demonstration of this fact follows thesteps
described above and will not bepresented
here forbrevity.
Thus,
forHuygens’ principle
to be satisfied on Petrovtype
III space- times we musthave ~ 11 ~ 0,
and Theorem6,
which states this result in aconformally
invariant way, isproved.
4. THE
CASE ~ 11 ~ 0
We shall now examine the sole case which remains after the
analysis
ofthe
previous section, namely
that in which 0 and~11 ~
0.This,
inview of Theorem
6,
willcomplete
theproof
of Theorem 1. Ourapproach
is related to that of the
previous section,
in that we reduce theproblem
toan issue of
solvability
of apurely algebraic system
ofequations.
We first observe
that,
in addition to thealgebraic equations given by (52)
and(60),
an extraindependent equation
may be obtainedby applying
the NP
operator 8
to(52).
All of the Pfaffians which result are knownexplicitly,
and may bereplaced using
theexpressions
found in Section 2 to obtain a(very large) expression
in thecomplex
variables a,fJ,
and yrVol. 71, n° 6-1999.
and the real
quantity (/)11. Upon transforming
variablesaccording
to(70)
and
(87),
we obtain acomplex quantity
in the new variablesxl , .~2 ,
and~l 1. (This polynomial
contains 408 terms of maximum totaldegree 9.) Together
with theequations
whichsimilarly
follow from(52)
and
(60),
we have in effect asystem
of fiveequations
in five real variables.Let us denote the set of
polynomials
which arise in thissystem (i.e.,
whenthe
equations
are written with aright
hand side of0) by
F.It must be mentioned that the
approach
of theprevious section, namely computing
the solutionsby explicit elimination,
isimpossible
in thepresent
case due to the intrinsiccomputational complexity
of nonlinear elimination and thehigh degree
of ourpolynomials.
It ispossible
and willsuffice, however,
to bound the number of solutionsusing
thefollowing
result due to
Buchberger [ 13] :
THEOREM 7. - Let G be a Grobner
basis for (F) (the polynomial
ideal
generated by F)
with respect to agiven ordering
terms, and let H denote the setof leading
termsof the
elementsof G
with respect to the chosen termordering.
Then the systemof equations corresponding to
Fhas finitely
many solutionsif and only if for
every indeterminate x in F there is a natural number m such that xm E H.The
key
tousing
this result is that we may use anordering
of termsbased on total
degree (i.e.,
a non-eliminationordering)
for which thecomputational complexity
ofBuchberger’s algorithm
for Grobner bases is much lower.Unfortunately,
even in thissetting
a Grobner basis for F cannoteasily
becomputed
due to the extreme size of intermediate resultsproduced by
thealgorithm.
It would be
highly
desirable toapply
modularhomomorphisms
inthe manner used in
algorithms
for factorization(i.e.,
so-called Chineseremainder,
or Henselalgorithms [13])
in thepresent
situation. This is notcurrently possible
due to a number of unresolvedproblems
with theapproach. Nonetheless,
itprovides
a usefulprobabilistic experimental approach:
treat the elements of F aspolynomials
over aprime
fieldZp (rather
than therationals),
where p is of modestsize,
andcompute
the Grobner basis of F modulo p overZ p’
For asingle prime,
it ispossible
that the result so obtained may have no useful
relationship
with theGrobner basis of F over the rationals.
However,
if the basispolynomials computed using
alarge
number of differentprimes
all exhibit identical monomial structures, it isextremely likely
thatthey
eachrepresent
adistinct
homomorphic image
of the true Grobner basis of F. Thequestion
of
accurately computing
theprobability
of success for aspecific
series ofAnnales de l’ Institut Poincaré - Physique theorique
primes
remains an openproblem. However,
the individualprime
fieldcomputations
arecomparatively
easy since(unlike
the rationalcase)
nosingle
coefficient may belarger
than the chosenprime.
Thisprovides
an
experimental "sampling"
method whichgives
clues on how best tocompute
the trueresult,
and what that result willlikely
be.We must also consider that if we were able to
compute
a Grobner basis for F over therationals,
we would derive information on all solutions of thecorresponding system including
those which were examined in theprevious
section(i.e.,
for which(/)11
=0).
It ispossible
to exclude thosesolutions
entirely by adding
an additional constraint andvariable,
to our
equations
toproduce
theaugmented system
F.Still, only
an actualcomputation
reveals whether thisimproves
or worsens thetractability
ofthe
problem.
In our case, alarge
number(a
fewthousand) prime
field"sample" computations (done using
the GBpackage
ofFaugere [ 12],
which is far more efficient than the
general-purpose Maple system)
allsuggested
that the additionof Eq. (92)
made the Grobner basis calculation much more efficient. Moreimportantly,
once the solutions examined in theprevious
section were in effectdiscarded, only
afinite
numberremained when Theorem 7 is taken into account. With this in
mind, it
was
possible (and worthwhile)
tocompute
the true Grobner basis of Fover the rationals in the indeterminates xl, x2,
using
atotal
degree ordering
of terms. Since this basis containspolynomials
withleading
termswe may conclude that there are
only finitely
many solutions for whichY~11 ~
and hence~1 ~
aswell,
is nonzero.(For
this lastcomputation
thelatest and most efficient version of
Faugere’s
GBpackage,
known asFGB,
wasrequired.)
It follows that x2,~2
1 must be constants;it remains
only
to show that thisyields
a contradiction.Since must be constant
(including
the case in which~11 = 0)
it follows from
(70), (87)
that thequantities 03C003C0, 03B203B2
and areall constant as well. From the
equation 03B4(03B203B2)
= 0 weobtain,
in thevariables xl, x2,
given by (70), (87),
the side relationVol. 71, n° 6-1999.
Next, from ~(~2)
= 0 we obtain the PfaffianUsing this, along
with thepreviously
determinedPfaffians,
we thenobtain another side
relation;
onsubtracting
this result from(94) (and ignoring
thepossibility
that0,
which hasalready
been
considered)
we obtainFinally, from 03B4(03B1/03B2)
== 0 we obtainThe collection of
polynomials given by (94), (96), (97), (52)
and theircomplex conjugates
has a Grobner basis(computed easily using Maple) containing only
thepolynomial
1. This isequivalent
toshowing
that thereexists a combination of these
polynomials
whichequals 1,
and hence thatthey
cannot vanishsimultaneously (see [ 13]); i.e.,
the associatedsystem
ofequations
has no solutions. Thiscompletes
theproof.
5. CONCLUSION
In
completing
theproof
of Theorem1,
we havefully
solved Hada-mard’s
problem
for the scalar waveequation
in the case of Petrovtype
IIIspace-times.
Essential to ourproof
were use of the six-index necessary condition obtainedby
Rinke and Wunsch[23],
andseparate analyses (and
different ideal-theoretictools)
for the cases(/)11
= 0 and~11 ~
0.To
complete
theproof
of theconjecture
stated in the Introduction it remains to consider thespace-times
of Petrovtypes
I and II. Apartial
result for
type
II has been obtainedby Carminati, Czapor, McLenaghan
and Williams
[8]. However,
it is notyet
clear whether thecomplicated equations
which arise from conditions(III), (V),
and(VII)
can be solvedby
the method used in thepresent
paper.The authors would like to thank J.C.
Faugere
for his assistance with the FGBpackage.
This work wassupported
inpart by
the Natural Sciences andEngineering
Research Council of Canada in the form of individual Research Grants(S.R. Czapor
and R.G.McLenaghan).
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