A NNALES DE L ’I. H. P., SECTION A
R ICHARD K ERNER
Geometrical background for the unified field theories : the Einstein-Cartan theory over a principal fibre bundle
Annales de l’I. H. P., section A, tome 34, n
o4 (1981), p. 437-463
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437
Geometrical background
for the unified field theories:
the Einstein-Cartan theory
overa
principal fibre bundle
Richard KERNER
Departement de Mecanique, Universite Pierre-et-Marie Curie, 4, Place Jussieu, 75005 Paris, France
Ann. Inst. Poincare, Vol. XXXIV, n° 4, 1981,
Section A :
Physique ’ ’
ABSTRACT. The gauge and Lorentz invariant interactions of
spinors,
vectors, scalar
multiplets
and gauge fields are constructedusing
the Einstein- Cartantheory
with torsion over aprincipal
fibre bundle. Thisgeneraliza-
tion enables us to get rid of the un-renormalizable terms which are present in the
purely
Riemannian version of thistheory.
Thedecomposition
of thegeneralized spinors
over the fibre bundle into themultiplets
of Lorentzspinors
canprovide
thetheory
with the rich mass spectrum.RESUME. Nous construisons les interactions invariantes sous 1’action d’un groupe de
jauge
et du groupe deLorentz,
comprenant leschamps spinoriels, vectoriels, multiplets
scalaires et leschamps
dejauge.
La cons-truction se base sur 1’utilisation de la theorie d’Einstein-Cartan avec tor- sion au-dessus d’un fibre
principal.
Cettegeneralisation
nous permet desupprimer
des termes non-renormalisablesqui apparaissaient
dansla version Riemannienne de cette theorie.
La
decomposition
desspineurs generalises
au-dessus du fibre en desmultiplets
despineurs
lorentziens peut aboutir a l’obtention d’un spectre de masse interessant.Annales de l’Institut Poincaré-Section A-Vol. XXXIV, 0020-2339/1981/437/5 5,00/
(Q Gauthier-Villars 17
1. INTRODUCTION
One of the most
important problems
in theelementary particle physics
is to
identify
the knownparticles
or theirhypothetical
components(quarks)
with the irreducible
representations
of some Lie groupcontaining
boththe Lorentz group and what is called the internal symmetry group, or the gauge group. The
assignement
of well-definedparticle properties
to thetype of the
representation
of the Lorentz group is well understood : that is how wedistinguish
the scalarparticles, spin 1/2 particles,
vectorbosons,
etc. The situation is less clear when it comes to the
symmetries
betweenthe different
particles
of the samefamily.
First of all we are uncertain even as to the choice of the groupitself,
except that we know that it has to containat least a
U( 1) subgroup
for the conservation of the electriccharge,
anda
SU(2) subgroup
for theisospin conservation;
the conservation of thebaryonic
orleptonic
number may come fromSU(2)
or somelarger
group.Even when the group is
chosen,
theambiguity persists
in the way it mixes with the Lorentz group. The situation is similar to whathappens
with the
spectral
lines of thehydrogen
atom. We know that this spectrum is invariant under the group0(4)
=0(3)
x0(3),
but this does not meanat all that the
physical
system evolves in a 4-dimensional Euclidean space.It
just happens
that the kinematical anddynamical symmetries
of thesystem mix up in such a curious way. The same may be true with respect
to the
elementary particles
or their constituents.Now,
to describe the vectormultiplets
of bosons as well as the electro-magnetic field,
thetheory
of gaugefields,
i. e. the connections on a fibrebundle,
hasprovided
an ideal mathematical tool. However thespin or
fieldsare not
incorporated
into thistheory
onequal footing;
themultiplets
ofspinors
interact with the gauge field via the minimal interaction which is constructedby analogy
with theelectromagnetic
interaction.Moreover,
therepresentation
of the gauge group to which such amultiplet belongs
is
arbitrary.
Theonly leading principle
is to obtain the system ofequations
invariant both under the Lorentz group and the gauge group.
To obtain such an invariant system of
equations
twocomplementary approaches
arecurrently
in use :a)
the variational one, which consists infinding
out aLagrangian density
invariant under the symmetry group we have
chosen,
and thenderiving
the
equations
ofmotion,
which will be invariant under the aforementioned symmetry group.b)
To define some differential operators invariant under the chosen symmetry group, and thenapply
them to the local sections of the appro-priate
fibre bundles. In whatfollows,
we shall consideronly
two types of invariant operators : the Dirac operator and theLaplace-Beltrami
operator.Annales de l’Institut Henri Poincaré-Section A
GEOMETRICAL BACKGROUND FOR UNIFIED FIELD THEORIES 439
Both
approaches
have some inconvenience. E. g. in the first case theLagrangian density
is a 4-form over the Minkowskispace-time,
but wehave to know what are the
building
blocks it wassupposed
to be construc-ted with :
spinor fields,
vectorfields,
scalarmultiplets,
tensors, and allother
possible
cases. There are many ways( « interactions » )
in which such a4-form can be constructed.
In the second case the invariance is built in into the differential operator, but as a
rule,
the local section of the fibre bundlebelongs
to a represen- tation of somelarge
group,containing
both the Lorentz group and the internal symmetry group, and we have todecompose
it into themultiplets
of the irreducible
representations
of the Lorentz group in order togive
it an intrinsic
physical meaning.
What we propose here is to take the best out of these two
approaches
and try to construct the invariant models of interactions in a
synthetic
way. The most
important
feature of ourapproach
is that the choice of group determines also the choice of itsrepresentation,
and therefore the exactform of
spinor
and vectormultiplets permitted by
the model.2. GAUGE FIELDS ON A
PRINCIPAL
FIBRE BUNDLE Let us remind the fibre bundle formulation of the gauge fieldtheory.
LetM4
be the Minkowskianspace-time
with the metric form gM. Let G bea compact,
semi-simple
Lie group of dimension N. TheCartan-Killing
metric form on G will be
designed by
gG.We form a
principal
fibre bundleP(M4, G)
with the base spaceM4
andthe structural group G.
. The group G acts on the
right
onP(M4, G), generating
the left-invariantvector fields. The N-dimensional
subspace
of the tangent spaceG) spanned by
these fields is called verticalsubspace.
The connection on
P(M4, G)
is a distribution of 4-dimensionalsubspaces
which are invariant under the group action on
P(M4, G).
It isequivalent
with
defining
a left invariant 1-form onP(M4, G)
with values in the Liealgebra
of G.This form is called
A ;
a vector field at thepoint p E P(M4, G)
is calledhorizontal
if A(X)
= 0. The 1-form A isleft-invariant,
which means thatwhere ad means the
adjoint representation
of G in its Liealgebra
andph
isthe
image
of p EG)
under theright
action of h E G.Any
vector field onG)
can be nowdecomposed
into its horizontal and vertical parts relative to the connection A :This enables us to define the metric on
G)
as follows : for any two vectorsX,
Y we definewhere d~ is the differential of the canonical
projection
7t:P(M4, G)
-+M4.
The connection form A defines also the covariant
dinerentiation
of forms onP(M4, G).
Let M be such aform; then,
if itsdegree
is1,
thenWe define the curvature form of A :
where the bracket means the Lie
algebra
skewproduct.
Obviously :
Finally,
let 03C6 be atensorial 1-form
of type adG. Then we can define its covariant differentialThe metric forms on G and on
M4
define the scalarproduct
notonly
for vectors
belonging
to thehorizontal
or verticalsubspaces of P(M4, G),
but
also,
in a canonical way, the scalarproduct
of two forms of the samedegree.
Therefore we can define the scalarproduct
of F withitself, symbo- lically
F. F. Whenmultiplied by ae
itgives
an invariantLagrangian
density .
Whenintegrated
overP(M4, G)
with a measure which is the pro- duct of the invariant Haar measure on G and the usual volume elementon
M4,
it willgive
where
VG
is a constant(volume
ofG).
The
principal
bundleP(M4, G)
endowed with the canonical metricgpis
a
Riemannian
space. In a usual way we can introduce theChristoffel
connection,
which defines theparallel transport
and the covarlant diffe-rentiation of forms and vector fields over
P(M4, G).
Let us denote thisChristoffel
connectionby
It is a 1-form overP(M4, G)
with values in the Liealgebra
of theorthogonal group
in 4 + N dimensions preser-ving
the metric gp. This connection is torsionless.It can be calculated that the Riemann scalar of this new
connection,
which we note R, is
equal
to theLagrangian density
of the gauge field F FAnnales de Henri Poincaré-Section A
GEOMETRICAL BACKGROUND FOR UNIFIED FIELD THEORIES 441
plus
the scalar curvature K of the base spaceM4 (in
our case K =0) plus
a constant :
In the case when K =
0,
the Einsteinian variationalprinciple applied
to the Riemannian space
G) gives
once moreThe
equations resulting
from thisLagrangian density
are the well-known
Yang-Mills
fieldequations :
Here F* means the dual 2-form of F. The
duality
of forms is definedby
the usual
Hodge procedure,
i. e.by
the invarianttotally antisymmetric
4-form on
M4, numerically equal
to the .If K #-
0,
then thesupplementary
set ofequations gives
the definition of the energy-momentum tensor of theYang-Mills
field via Einsteinsequations
where x is the
gravitational
constant,i, j
=0, 1, 2, 3,
and means theenergy-momentum
tensor of the field F.3. SPINORS OVER THE BUNDLE
Our next task is to describe the interaction of the gauge field with other
fields, namely spin or,
scalar or vector fields.Following
thesuggestions
formulated in
(1), (2), (3)
we shall definespin or
fieldsdirectly
on the fibrebundle
G)
endowed with the connection form A. Let us remindbriefly
how thespinor
fields are constructed over the Minkowskian space- timeM4 (4), (5), (6).
Theisometry
group ofM4
isSO(3,1).
Construct nowthe
principal
fiber bundleSO(3, 1));
forsimplicity
we will assumethat it is
globally
trivial:S0(3,1)) ~ M4
xS0(3,1).
Let(:4
denotethe 4-dimensional linear
complex
space. The associatedspinor
bundle is defined as follows :In order to
give
anexplicit meaning
to thisformula,
we have to define theaction of the group
S0(3,1)
on the linearcomplex
space([4,
i. e. to definethe
representation.
Thespinor representation,
which is in fact a represen- tation notonly ofSO(3,1)
but of itscovering
groupSpin (3, 1),
is constructedas follows. For a
given
metric tensor gi~ we define the generators of the associated Cliffordalgebra
as follows :where M means the
identity
operator in therepresentation
space. The lowest lalt i’: . hf u Irepresentation
0 f thematrices ~
has the dimension ~ ==2[N_;~J
,where f ==
1, 2,
..., ~ and[~c]
means the entire part of ~. In the case of== 4 and m == 22 =
4;
that iswhy
we take(:4.
It is easy toverify
nowthat the matrices
generate the Lie
algebra
ofS0(3,1).
Let = 2014 be the generators ofan infinitesimal Lorentz rotation. Then a
spinor
which has its values inC4,
transforms under an infinitesimal Lorentz rotation as follows :Define a
matrix ~ by requiring
forany
i == 0, 1,2,
3The
Dirac-conjugate spinor 03C8
will be defined then as :and it transforms under the
conjugate
transformation law :Therefore,
the scalarproduct ~~
ismanifestly
invariant under Lorentz transformations.Let us define the collection of 1-forms
spanning
a basis at anypoint
of
M4 : { 6’},
i =0, 1, 2, 3. Usually,
in holonomiccoordinates,
one can choosesimply 8‘
=dxi.
Let the matricesEi
form the basis of the Liealgebra
of
orthogonal
transformations of frames. The connection in the bundle oforthogonal
frames is a left-invariant 1-form with values in the Liealgebra
of
orthogonal
transformations of frames :Defining
03C9kl = it is easy to see that for theorthogonal
frames onemust have
Annales de l’Institut Henri Poincaré-Section A
443
GEOMETRICAL BACKGROUND FOR UNIFIED FIELD THEORIES
With the connection on the bundle of frames thus
defined,
we can intro- duce the covariant derivative in the associatedspinor
bundle :Therefore if t
The covariant derivative of a
conjugate spinor
isgiven by
In a
general
case of a Riemannian spaceV4 replacing M4,
let us definethe
density
~ijkl, atotally antisymmetric
tensor such that 170123=
det112.
Next,
we define the associate formsWe can also introduce their dual forms :
Finally,
we define the Cliffordalgebra-valued
forms : the 1-form y = and its dual3-form ~
= Then the DiracLagrangian density
for thespinor
field can be written in thefollowing
concise form :which is
manifestly
hermitian and does notdepend
on the choice of coordi- nates.The
corresponding equations
can be written in the formwhich in the case of
D
=0, (what
weassume), explicitly
takes on the familiar formand coincides with the Dirac
equation
in curvedspace-time.
The conserved current is
given by j
= withdj
= 0by
virtue ofthe Dirac
equation.
-The
generalization
of the Diracequation
that we propose now means that we should repeat the same construction over the Riemannian manifoldG; g).
In thisnotation g
means the Riemannian metric(2-3).
Thusinstead of
working
with the directproduct
of the Lorentz group and the internal symmetry group we imbed the two in theisometry
group of themetric gp, and then try to
decompose
thecorresponding spinorial
repre-sentation.
The
spinors
will be constructed now as the sections of the associated fiber bundlewhere r
The
generalization
of the construction of Lorentzspinors
to thespinors
defined over x
G), SO(3
+N, 1))
is obvious.Any
Cliffordalgebra
can be
decomposed
into a tensorproduct
of the fourelementary
Cliffordalgebras :
C(0, 1 ) = ([1
= thecomplex
manifoldC(l, 0)
= R 3 R = sum of the two real linesC(0,2) = H! = quaternions
C(l, 1 )
=Mat2R
= 2 x 2 real matricesHere
C( p, q)
means the Cliffordalgebra corresponding
to thediagonal
metric with the
signature ( p +, q - ).
We have also the reduction formulae :
To
give
anexample,
if G =SU(2),
N = 3 and we have to construct :C(3
+N, 1) = C(6,1)
The lowest-dimensional faithful
representation
ofC(6, 1)
isgiven by
16 x 16
matrices;
it is easy to construct itexplicitly.
If we want to definethen
(up
to anequivalence)
one of thepossible
realizations is :Where
yi
are the usual 4 x 4 Diracmatrices,
Ta are the 2 x 2 Paulimatrices, and 12 or 14
means 2 x 2 or 4 x 4identity matrix;
if we omit the H matrixin the first
definition,
we would have arepresentation still,
but not a faithfulone-it will be realized in 8 dimensions :
In what follows we shall
always
suppose that the faithfulrepresentation
is taken. The
only thing left
now is togeneralize
’ thedensity
tensor 11 forAnnales de l’Institut Henri Poincaré-Section A
445
GEOMETRICAL BACKGROUND FOR UNIFIED FIELD THEORIES
our bundle. For the base space
M4
we take ~0123. for the group G we shall take the tensor for the directproduct M4
x G we shall take theproduct
tensor and for the fibre bundleG)
we willdefine
and other components
by antisymmetrization.
The new
Lagrangian
isanalogous
to the DiracLagrangian
onM4,
i. e.and the
corresponding generalized
Diracequation
can be written as :Now we shall
proceed
toexplicit
calculus of thisequation, expressed
inlocal coordinates. The easiest way to do it is
by introducing
the anholo- nomic coordinate systems.4. THE GENERALIZED DIRAC
EQUATION
Let us remind that in our notation the indices
i, j
take on the values0, 1, 2, 3 ;
theindices a,
b take on the values1, 2,
..., N = dimG,
and the Greek indices a,~3
take on the values1, 2,
..., N +4,
and we writesymbolically
a
= { ~ ~}, meaning
that the index a means both i and a. Let us take anopen subset of
G),
which isisomorphic
to aproduct
of the open subsets ofM4
and G :Without loss in
generality
we can assume that W is aneighborhood
ofunity
of G. We denote the local coordinates in Vby xt,
the local coordi-nates in W
by 03BEa
and the local coordinates in U= {pi,pa}.
Let us choose a basis in the Lie
algebra j~c
such that for any vector Y E Y = withThe structure constants
Cab satisfy Cab
= -Cba
and the Jacobiidentity
+ + = 0. The bracket above means the skew pro- duct in The action of the group on
G)
defines N left-invariantwector fields on the
bundle,
which span a Liealgebra isomorphic
tod G,
with the
operation being
the Lie bracket of vector fields. Let us denote these N vector fieldsisomorphic
toLa by Sa, a
=1, 2, ... , N.
In local coordinates we can write :Vol. 4-1981.
The
Sa
shouldsatisfy SJ =
thereforeWe call
Sa
the vertical vector fields.Let 7r be the canonical
projection
fromG)
ontoM4,
let d?c be its differential. Then in local coordinates we can write = X when Y EG)
and X ETM4.
If in local coordinates X = Y = thenWe get also the condition of
verticality
in local coordinates :Because any fibre is transformed into a
point
inM4 by
7r, any vertical vector will be transformed into 0by
With no less ingenerality
we canchoose such local coordinates in
U,
in which =~~, ~
= 0. Thisimplies
thatS~
= 0, andThe horizontal
subspaces
are definedby
the connection formThe
image
of a vertical vector field should be thecorresponding
elementin therefore
A(SJ
=La;
this means that in local coordinatesTherefore
A«Sa
=~Q.
IfS~
=0,
we have(the
matrixAd
is at everypoint
inverse ofS~).
The
components
are stillarbitrary.
It is easy to see that the matricesA~ satisfy
A vector Y E
G)
is horizontal ifA(Y)
= 0. In local coordinates it means that = 0 for any a =1,2,
..., N.a Let Y E
G),
Y =The vertical and horizontal parts of Y are
given by :
In local coordinates we have
Annales de l’Instilut Henri Poincaré-Section A
GEOMETRICAL BACKGROUND FOR UNIFIED FIELD THEORIES 447
In our
coordinates,
whereFinally,
let X = b e a vector from We define the horizontal lift of X as the vectorT-(X)
defined at anypoint
ofG) by
Therefore,
where
We have the
following
relations satisfied :The form A has a remarkable property of
being
left-invariant of type ad(2-1).
If we take a
1-parameter subgroup
ofG, h(t),
which generates a left- invariant vector fieldX,
the same property can be writteninfinitesimally :
where Ad is the
adjoint representation
ofj~ ~
is the Lie derivative withx
respect to the field X. The structure constants
Ca~
can beregarded
uponas N matrices which
provide
us with the Adrepresentation
of the Nleft-invariant vector fields :
Cb =
which isnothing
else thanJacobi
identity.
Therefore :or, in local coordinates and
finally :
Because of
S~
=0,
andAbSd
=~~
we can writeMultiplying
both sidesby A~
we getVol.
Now,
for oc = g we obtain the relation which we have gotalready
whereas for a = i we get
because we assume the coordinate system in which = 0.
The last two
formulae,
i. e.(4-25)
and(4-26)
can beinterpreted
in anotherway
by telling
that the curvature form of the connection A is horizontal:one of the two vectors is vertical.
In local coordinates we have :
and
If F has to vanish on vertical vectors, its
only non-vanishing components
will beThe formulae
(4-25)
and(4-26)
define the derivatives ofAa
with respectto the group
parameters.
The canonical metric on the
principal bundle,
introduced in§ . 2 by (2-3)
will
give
in local coordinates :which can be written in a matrix form :
The inverse matrix to
(4-31)
isgiven by :
With the
help
of the formulae of derivation(4-25)
and(4-26)
we canproceed
to compute the Christoffel
symbols corresponding
to our metric :de l’Institut Poincaré-Section A
449
The
non-vanishing
jcomponents
are " then:The calculus of the Riemann tensor is even more
complicated.
It is mucheasier to use the anholonomic coordinate system. As a matter of
fact,
we can
interpret
the metric tensor gaa as animage
of thediagonal
matrixunder a local
change
of basis in the tangent space : and-1
where the matrices
Up
andUp
aregiven by
thefollowing
formulae :and the inverse matrix :
It is useful to introduce a « non-holonomic » derivative
by :
of course,
Vol. XXXIV, n° 4-1981.
The connection transforms as
usually
and in new basis we getand all other components vanish.
In this local
basis,
the components of the Riemann tensor are thefollowing :
Here
The invariant scalar curvature is
equal
toIt is easy to write down
explicitly
thegeneralized
Diracequation :
in ourbasis it will be :
Annales de ’ l’Institut Henri Poincaré-Section A
GEOMETRICAL BACKGROUND FOR UNIFIED FIELD THEORIES 451
where
The
superscript
means that the Cliffordalgebra
generatorscorrespond
to the
diagonal
metric in whichTherefore
(4-45)
becomesThe
equation (4-46)
can not be used unless we know what meansIn other
words,
we have to fix thegeometrical properties of 03C8
with respectto the group transformations on
G).
The otherproblem
we face nowis the presence of a
Pauli-type term 1 203B3aFakl03C3kl
which makes ourtheory
unrenormalizable after
quantization.
5. METRIC THEORY WITH TORSION OVER THE BUNDLE
Let us return to
physics
for a while and remind that we aredescribing
an invariant interaction between the gauge field A and the
generalized spinor
We know how does theLie-algebra
valued 1-form A transform under the action of the structural group G on the bundle : if X is a left- invariant vector field onG) generated by
thecorresponding
elementin
~/G (which
we denoteby
the same letterX)
thenor, if we choose a basis of N left-invariant fields
Sm
we have in local coordi-nates
It seems
natural,
in order to makeeverything
invariant and in order togive
an intrinsicmeaning
to theequation (4-46),
topostulate
that thespinor 03C8
transforms in the same way as the form A. This meansthat 03C8
satisfies
Spinors satisfying
the relation(5-1 )
will be called left-invariantspinors
Vol. XXXI V, n° 4-1981.
of type Ad. We can also introduce another type of
spinors
onP(M G), namely
thespinors satisfying
the relationThe first
assumption (5-1 ),
makes ourtheory entirely covariant,
whereasthe condition
(5-2)
breaks the symmetry.The most
general
definition of the Lie derivative of aspinor
field has been elaboratedby
A. Lichnerowicz[S, 6 and
Y. Kosmann[4J.
If X is a vectorfield over a
manifold,
and if ~pt is a1-parameter
group of transformationsgenerating X,
thenOn a
manifold,
with a metric connection(non necessarily riemannian),
when
expressed
in localcoordinates,
thisgives
Finally,
if the linear connection form can be written in a coordinate system as and if we introduce the notationrays
= then wecan write
explicitly
Here we denote
by
Let us remind that the Ad
representation of AG
acts onspinors
aswhere
gcdCab
and istotally anti-symmetric
for any compact andsemi-simple
Lie group.What we are interested in
is,
infact,
the behaviourof 03C8
under an infini-tesimal Lie group
transformation,
i. e. when X is a left-invariant vectorfield on
G).
Then we can put XIX =
(Xa, 0)(X’ =E 0),
avertical,
left-invariantfield,
and take any of the fieldsSa-
In this case theonly thing
left in(5-5)
will be(in
non-holonomiccoordinates, using
theproperties
ofSb
and oA~
esta-blished 0 in
§ . 4).
The formula .(5-7)
is sosimple
" because " the fieldsS~
are " left-Annales de l’Institut Henri Poincaré-Section A
GEOMETRICAL BACKGROUND FOR UNIFIED FIELD THEORIES 453
invariant and transform into each other under the ~ action of the group.
It is easy to check
[£, JE =
Sa Sb Sc
Finally,
if =A~(+
it will meanand
whereas = 0 means
just
= 0 in our coordinate system. The equa-Sa
tion
(4-47)
becomes now :in the case when
£1/1
=Ad( +
andSa
in the case when =
0,
i. e. when thesymmetry
is broken.Let us remark
sa
that the Pauli
term - 1 Fkl03C3kl
will bepresent
also ln the2
abelian case when G = S 1 and the gauge field is identified with the electro-
magnetic field.
Now theequations (5-10)
and(5-11 )
areoperational,
butstill describe an unrenormalizable
theory
because of thePauli-type
termIt is obvious that in this
theory only
thechange
of the geometry of the fibre bundleG)
canmodify
the interaction and suppress the Pauli term. We propose toenlarge
ourtheory
and to include torsion. This meansthat now, in
general,
for any vector fields on thebundle,
sayX, Y,
thequantity
is not null.
The
(vector-valued)
2-form 8 is called the torsionform;
in local coordi-nates we use the notation :
Vol. XXXIV, n° 4-1981.
The new connection will be now
( { r1 } being the riemannian connec-
tion): ~-)
In
general,
this connection is notmetric;
but there exists aunique
connec-tion which has the same torsion
(the antisymmetric part)
and which ismetric. That is
precisely
the connection we want to have. The torsion will becompletely
definedby
thefollowing req-uirements :
because we want to get rid of the Pauli term in the
generalized
Dirac equa-tion ;
moreover we wantwhich will make the new connection metric. This is
important
if we wantto be able to define the
spinorial
connection and a covariant derivative of aspin or.
It is easy to see that the
only independent equations
in(5-15)
areand
Combining (5-15)
and(5-16)
we findeasily
and
The new
connection,
which has torsion but is metric angives
Dirac’sequation
withoutPauli-type
termis,
in the non-holonomic coordinate system introduced in§ . 4,
thefollowing
Annales de Henri Poincaré-Section A
GEOMETRICAL BACKGROUND FOR UNIFIED FIELD THEORIES 455
The new curvature scalar is
changed
veryslightly :
which amounts to a
change
of the scale in theLagrangian.
Thus we arenaturally
led to the Einstein-Cartantheory,
which can be found in a modernversion in the works
of Trautman,
Hehl andKopczynski [8 to [12 ].
Inthis
theory,
the energy-momentum tensor is the source of curvature, whereas thespin-density
tensor is the source of torsion : in properunits,
where
by
definitionIn our version
only
thespace-time
componentsSkl
are to bedetermined;
it is easy to see that
sik
=0,
thereforeother components of
S~y being
determinedby (5-20).
The Dirac
equation
for the left-invariantspinors
of Ad type reducesto a usual one
whereas the
spinors
constant under group action do not interact at all with the gauge field :6. INTERACTION WITH A VECTOR FIELD
To
complete
ourtheory,
which includesalready
thegeneralized spinors
and the gauge
fields,
we want to introduce theequivalent
of the Klein-Gordon
equation
for massive vector fields. The existence of the metricon the fibre bundle
G) gives
usimmediately
the natural operator, which is theLaplace-Beltrami
operator, and which is introduced as follows : Define first theHodge duality
operator, which for anyp-form
cc~ overan n-dimensional manifold
gives
ann - p-form
*cv which has the samevolume as the former one. It is easy to see that * is an
isomorphism
of thecorresponding
vector spaces. Then we define the derivation ~ _* -1 d* ;
itis easy to see that 03B4 :
p-forms
intop -1-forms. Finally,
as 03B403B4 = 0(because
dd =
0)
we can define aself-adjoint
operator of second order:acting
on anyp-form
andpreserving
its type.Vol. XXXIV, n° 4-1981.
The
generalized
Klein-Gordonequation
will be written asWe are interested in the
explicit expression
for a 1-form overG);
let us remind that the metric structure over our fibre bundle
gives
a one-to-one
correspondance
between the 1-forms and the vectors.A
1-form 03C6
isdecomposed
in a local frame e*03B1as 4> =
The ope- ratorA,
whenexpressed
in localcoordinates,
willgive
where
03B1
means the covariant derivative with respect to theChristoffel
defined in
(4-33).
The same formula can be written as
where
R03B103B303B403B2
is the Riemann tensor of the Christoffel connection. Remark that the existence of torsion does notmodify
the definition of theLaplace-
Beltrami operator, which is introduced in a
unique
wayby
the metricstructure
only.
In order to find out theexplicit expression
for(6-2)
we shallwork once more in our non-holonomic system of frames. Our 1-form can
be written
symbolically
aswhere
~a
is the vertical part ofWj
its horizontal part.Correspondingly,
we shall obtain two
independent
systems ofequations.
In order to make them
operational,
we have to define the behaviour ofour form under the action of the structural group G. We are interested in the form of ad type, such that
therefore
As for the horizontal part
Wj,
we assume thatAfter some
calculus,
we get thefollowing
two sets ofequations :
The first two terms in each of these ~
equations
describe an invariantinteraction of the scalar
multiplet 03C6c
with the gaugefield,
and 0 the Klein-Annales de , l’Institut Henri Poincare-Section A
457
GEOMETRICAL BACKGROUND FOR UNIFIED FIELD THEORIES
Gordon
equation
for the massive vector field.Moreover,
next terms describe a veryugly
non-minimalcouplings
which are unrenormalizable.Let us write down the
Lagrangian giving
rise to theseequations :
Remark that even if
Ø0153
had to bevertical,
i. e.0,
theequation (6-10)
would
give
a strange constraint. We shall see that the symmetry between~b
and
~Vk
can be restored and the non-minimalcouplings
can be removedonce more if we introduce an
appropriate terms
with torsionS~Y.
The Pauli-term
representing
the non-minimalcoupling
in the Diracequation
was removedby introducing
the torsion term into theLagrangian :
Let us try to add to the
Lagrangian
of the vector field on the bundlea similar term
including
the torsion. If we look closer at ourLagrangian
and the
corresponding Laplace-Beltrami equation,
we see that theLagran- gian
can be written as(The
tilda means thateverything
is taken with respect to the Christoffelconnection).
Let us prove that we can obtain a new
Lagrangian
with minimalcoupling
if we suppress the second term in
(6-13)
and add instead the term of thefollowing
form :As a matter of
fact,
we have:Vol. XXXIV, n° 4-1981.
whereas a
simple
calculusgives
usThe sum of these two
expressions gives
aLagrangian
with the minimalcoupling :
The last term,
being
a puredivergence,
does notmodify
theequations
of motion. We can write
therefore, together
with the mass term :In
physical applications
the structure constants are rescaled and multi-plied by
somecoupling
parameter,characterizing
the interaction force with the gauge field : We remind that5~
for any compact andsemi-simple
Lie group. We see then that the masses of the vector fieldWk
and the scalarmultiplet ~~
are different : if the vector fieldWk
/201420142014?
has the mass
M,
the scalarmultiplet
will have the mass + 2014 where 03BBis the
coupling
constant. The asymmetry in masses is due to the fact thatour operator is no
longer conformally
invariant with respect to theglobal
metric on the fibre bundle. Remark that even if M =
0,
the scalar field willAnnales de l’Institut Henri Poincaré-Section A