A NNALES DE L ’I. H. P., SECTION A
R OBERTO C ATENACCI A NNALISA M ARZUOLI
A note on a hermitian analog of Einstein spaces
Annales de l’I. H. P., section A, tome 40, n
o2 (1984), p. 151-157
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151
A note
on ahermitian analog
of Einstein spaces (*)
Roberto CATENACCI
Annalisa MARZUOLI
Dipartimento di Matematica, Universita di Pavia, Italy INFN, Sezione di Pavia
Dipartimento di Fisica Nucleare e Teorica Universita di Pavia, Italy
Vol. 40, n° 2, 1984. Physique ’ theorique ’
ABSTRACT. - It is shown that a Hermitian Einstein space, i. e. a her- mitian space such that the Ricci tensor of the hermitian connection is
proportional
to the hermitianmetric,
is Kahlerian.RESUME. - On montre
qu’un
espace d’Einsteinhermitien,
c’est-a-direun espace hermitien tel que Ie tenseur de Ricci de la connection hermitienne soit
proportionnel
a lametrique hermitienne,
est kahlerien.INTRODUCTION
An Einstein space is a manifold of dimension n endowed with a rieman- nian
metric g proportional
to the Ricci tensor of the Levi-Civita connec-tion of g. Besides their intrinsic interest from the mathematical
point
ofview,
Einstein spaces have been introduced also inphysics, mainly
in(*) Work partially supported by GNFM, CNR.
Annales de l’lnstitut Henri Poincaré- Physique theorique - Vol. 40, 0246-0211
84/02/151/7/$ 2,70 cg Gauthier-Villars
152 R. CATENACCI AND A. MARZUOLI
connection with the «
space-time
foam »approach
to thequantization
of the
gravitational
field(see
e. g.1)
for a review.It can be noticed that most of the work on this lasttopic
has been doneby assuming (just
formathematical convenience and not for any
physical reasons)
that themanifolds considered are Kahlerian. This
requirement simplifies,
in par-ticular,
thestudy
ofproblems
about existence and classification of Einstein’smetrics,
at least for 4-dimensional manifolds.However we can
observe,
atfirst,
that on acomplex
manifold thereare two different connections which have
geometrical meaning, namely
the Levi-Civita connection and the hermitian connection.
Therefore,
thecondition of
being
Einstein’s could be defined for both the Ricci tensors atdisposal,
and the two definitionscoincide a priori only
in the Kahleriancase. Moreover we recall that for the Levi-Civita connection the condition
(Ricci
= ~, .metric) implies
the constancy of ~,(for
manifold of dimension >3).
While from the
expression (Ricci=03BB.metric)
for the Ricci tensor of the hermitianconnection,
it follows ~, = constantonly
if the hermitian metric is also Kahler. In this paper we prove that an Einstein hermitian manifold(i.
e. a hermitian manifold such that its hermitian metric is Einstein with~, 5~ 0
constant)
isnecessarily
Kahler and hence it is Einstein also in the usual sense.Note that the converse is not true, i. e. there exist
complex
manifolds(e.
g. thecomplex projective
spaceCP2
with apoint
blownup)
with a rieman-nian metric which is Einstein but not Einstein-Kahler.
We shall recall in the first
paragraph
some definitions and results onthe
theory
of hermitianmanifolds ;
the reader may refer to2), 3), 4)
for amore extensive and
complete
survey of thesubject.
1. THE HERMITIAN CONNECTION
Let M be a
complex manifold, dime
M = n = 2dimR
M = 2m andthe space of all Coo
complex-valued
functions on M.Let us denote
by e TM
andcTM*
thecomplex tangent
and thecomplex
cotangent bundle of M
respectively.
We can form thecomplex
exteriorproduct
ArcTM*
which is called the bundle ofcomplex
r-forms on M.It is well known that
eTM splits
as a sum ofcomplex
vector bundles :where TM and TM are
respectively
theholomorphic
and the antiholo-morphic tangent
bundles of M.Similarly
we have :where TM *
[resp.TM*] ]
is theholomorphic [resp. antiholomorphic]
Annales de l’Institut Henri Poincaré - Physique - theorique .
cotangent
bundle of M. Thesplitting (lb)
induces thefollowing decompo-
sition of A’
cTM*:
where denotes the
image
of (8) in ArcTM*
andis called the bundle of
complex (p, q)-forms
on M.Before
dealing
withconnections,
wespend
a few words about sec-tions of the
complex
vector bundles which we introduced above. If E is anyone of thesebundles,
we shall denote its COO sectionsby (For example:
Coo(cTM)
are thecomplex
vector fields onM,
are the fields of
complex (p, q)-forms
onM,
and soon).
We shall also need C~-sections of bundles built upby
tensorproduct
of two other bundles(for example:
are the fields of vector-valued 1-formson
M,
(8)E)
= are the fields of E-valued( p, q)-
forms on
M,
and soon).
,A connection on
C TM
is acomplex
linear map :which satisfies the condition :
The connection V induces
(by using
the Leibnitzrule)
connections on all the tensor bundles onM ;
we shall denote themby
the samesymbol
V.In
particular,
for039BrCTM*
we have :Using
thesplittings (Ib)
and(2)
one can write V = V + V" where :A connection V is said of
type ( 1, 0) (or compatible
with the complexstructure of
M)
iffor any
holomorphic
section s of TM and for any W E A hermitian metric on M is apositive
definitequadratic
form h E Coo(TM*
(x)TM*)
such that
It is a well known result
( 1 )
that there exists aunique
connection D which is of type( 1, 0)
and such thatVol. 40, n° 2-1984
154 R. CATENACCI AND A. MARZUOLI
D is called the hermitian connection of M associated with the metric.
The torsion form of a
complex
connection is an element ofit can be shown
(2) that
thetorsion
form T of the hermitian connection Dspits
into : T = S +S,
where S is theconjugate
of Sand :Hence,
taking
into account thesplittings (3a, b)
we have :The curvature R of a
complex
connection is a 2-form with values in the space of linearcomplex
mapsc TM cTM,
that is :For a hermitian connection it can be
shown,
forexample by
direct compu- tation in local components andusing splittings b),
thatHowever,
since it is known(3) that,
for the hermitianconnection,
R isa form of type
( 1, 1),
we can write :R E (8) TM
(8).TM*
CA 1,l(M)
(8) TM (8)TM*) (7)
We shall need in the
following
the Blanches identitiesexpressed
in termsof
T,
R and their covariant derivatives(4).
For any
A, B,
C E Coo(cTM)
the first and the second identities are res-pectively :
denotes sum over the
cyclic permutation
of the argu-ments
A, B,
C.2. HERMITIAN EINSTEIN SPACES We recall
(5)
that the Ricci tensor isdefined,
for anyA, B,
C Eas:
(2) See ref. 2, p. 224.
(4) See ref. 4, vol. 1, p. 135.
(5) See ref. 4, vol. 1, p. 248.
Annules de l’lnstitut Henri Poincaré - Physique theorique
By
a hermitian Einstein space we mean acomplex
manifold with a her- mitian metric h such thatWe shall show that h is Kahler.
Proof
- IfZ, W,
condition( 10) implies
inparticular :
Furthermore, using
the form of Rgiven
in(7)
and condition(10),
one cansee
easily
that theonly non-vanishing
part of(9)
isLet us use Blanches first
identity (8a)
to transformR(V, Z)W. Taking
the
cyclic permutation
on(B’, Z, W)
we obtainexplicitly :
A lot
of
terms in the lastexpression
vanish. Infact, using (7)
we have thatR(W, V)Z
=0;
from(5,
a,b)
we see that all the terms which arequadra-
tic in T vanish too;
finally, (6 a, b) imply that
theonly
non-null derivative of T is obtained from the term(DzT)(W, V).
Summing
up theseresults,
we can rewrite( 12)
as :We are
going
to show now that Trace of[V
-+ vanishes.It turns out that the
computation
is easier when local components areused;
let(f==l,...~;oc,~=l,...,~)
be a local chart of coordinates. Then the components of T andR,
in terms of the local bases{ ~~zi }and {dzk}
of the tangent and cotangent spaces, are definedby:
where (,)
is the usualpairing
between 1-forms and vectors. If we write down the second Bianchi’sidentity (8b)
in local components, contract it twice and use condition(10),
we get(see Appendix A) :
Vol. 40, n° 2-1984
156 R. CATENACCI AND A. MARZUOLI
From
(7)
we have that = 0 and = 0Vi, k,
from(5 a, b)
we have= 0 and = 0~i and so the second term in
(14)
vanishes anyway.Then,
as À i=0,
we haveTiki
= 0 or, in thecoordinate-independent
form :That
implies
also :Expression (13)
with(15)
reads :By using equations ( 11
a,b)
and the condition(7)
we can extend the( 16)
Ric
(A, B) = -
Trace of[R(A, B) ] .
The
right
hand side of( 16), by
a directcomputation,
can be written as-
[Trace of R ](A, B).
Moreover, as it is known(e.
g. from Blanches iden-tities)
that the two form(Trace
ofR)
isclosed,
we see that the fundamental form of h is alsoclosed, namely h
is Kahler.Annales de l’Institut Henri Poincaré - Physique ’ theorique "
APPENDIX A
In this appendix we give the details of the derivation of the equation (14). From eq. 8 b
we have, in local components,
By contracting on ik we have :
Another contraction on jm gives:
and hence using the condition (10) we finally obtain the equation (14).
[1] R. CATENACCI and C. REINA, Einstein-Kähler Surfaces and Gravitational Instantons.
Gen. Rel. Grav., t. 14, 1982, p. 255-277.
[2] M. J. FIELD, Several Complex Variables in Complex Analysis and its Applications,
vol. 1, International Atomic Energy Agency, Vienna, 1976.
[3] P. GRIFFITHS and J. HARRIS, Principles of Algebraic Geometry, Wiley-Interscience,
New York, 1978.
[4] S. KOBAYASHI and K. NOMIZU, Foundations of Differential Geometry, vol. 1, vol. 2, Wiley-Interscience, New York, 1963, 1969.
(Manuscrit reçu Ie 16 Mars 1983) (Version revisee reçue ’ Ie 16 Mai 1983)
Vol. 40, n° 2-1984