Volume 2012, Article ID 356263,18pages doi:10.1155/2012/356263
Research Article
Characterization of Holomorphic Bisectional Curvature of GCR-Lightlike Submanifolds
Sangeet Kumar,
1Rakesh Kumar,
2and R. K. Nagaich
31Department of Applied Sciences, Rayat Institute of Engineering & Information Technology, Railmajra, SBS Nagar, Punjab 144533, India
2Department of Basic and Applied Sciences, University College of Engineering, Punjabi University, Patiala 147002, India
3Department of Mathematics, Punjabi University, Patiala 147002, India
Correspondence should be addressed to Rakesh Kumar,dr [email protected] Received 27 March 2012; Accepted 19 May 2012
Academic Editor: M. Lakshmanan
Copyrightq2012 Sangeet Kumar et al. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
We obtain the expressions for sectional curvature, holomorphic sectional curvature, and holomorphic bisectional curvature of a GCR-lightlike submanifold of an indefinite Kaehler manifold. We discuss the boundedness of holomorphic sectional curvature of GCR-lightlike submanifolds of an indefinite complex space form. We establish a condition for a GCR-lightlike submanifold of an indefinite complex space form to be null holomorphically flat. We also obtain some characterization theorems for holomorphic sectional and holomorphic bisectional curvature.
1. Introduction
The study of CR submanifolds of Kaehler manifolds was initiated by Bejancu 1, as a generalization of totally real and complex submanifolds and further developed by2–7. The CR structures on real hypresurfaces of complex manifolds have interesting applications to relativity. Penrose8discovered a correspondence, called Penrose correspondence, between points of a Minkowski space and projective lines of a certain real hypersurfaces in a complex projective space, which is an interesting means of passing from the geometry of a Minkowski space to the geometry of aCRmanifold. Duggal9,10studied the geometry of CR submanifolds with Lorentzian metric and obtained their interaction with relativity.
The theory of lightlike submanifolds has interaction with some results on Killing horizon, electromagnetic, and radition fields and asymptotically flat spacetimes for detail see
chapters 7, 8, and 9 of 11. Thus due to the significant applications of CR structures in relativity and growing importance of lightlike submanifolds in mathematical physics and relativity, Duggal and Bejancu 11 introduced the notion of CR-lightlike submanifolds of indefinite Kaehler manifolds which have direct relation with physically important asymptotically flat space time which further lead to Twistor theory of Penrose and Heaven theory of Newman. Moreover, they concluded that, contrary to the CR-non degenerate submanifolds, CR-lightlike submanifolds do not include invariant complex and totally real lightlike submanifolds. Therefore, Duggal and Sahin 12 introduced SCR-lightlike submanifolds of indefinite Kaehler manifold which contain complex and totally real subcases but there was no inclusion relation betweenCRandSCRcases. Later on, Duggal and Sahin 13introducedGCR-lightlike submanifolds of indefinite Kaehler manifolds, which behaves as an umbrella of invariantcomplex, screen real and CR-lightlike submanifolds and also studied the existenceor nonexistenceof this new class in an indefinite space form. R. Kumar et al.14studied geodesicGCR-lightlike submanifolds of indefinite Kaehler manifolds and obtained some characterization theorems for a GCR-lightlike submanifold to be a GCR- lightlike product.
Since sectional curvature offers a lot of information concerning the intrinsic geometry of Riemannian manifolds, therefore in this paper, we obtain the expressions for sectional curvature, holomorphic sectional curvature, and holomorphic bisectional curvature of a GCR-lightlike submanifold of an indefinite Kaehler manifold. In15, Kulkarni showed that the boundedness of the sectional curvature on a semi-Riemannian manifold implies the constancy of the sectional curvature. In16, Bonome et al. showed that the boundedness of the holomorphic sectional curvature on indefinite almost Hermitian manifolds leads to the space of pointwise constant holomorphic sectional curvature. Therefore inSection 4, we discuss the boundedness of holomorphic sectional curvature ofGCR-lightlike submanifolds of an indefinite complex space form. In Section 5, we established a condition for a GCR- lightlike submanifold of an indefinite complex space form to be null holomorphically flat.
We also obtain some characterization theorems on holomorphic sectional and holomorphic bisectional curvature.
2. Lightlike Submanifolds
Let M, g be a realmn-dimensional semi-Riemannian manifold of constant index q such that m, n ≥ 1, 1 ≤ q ≤ m n− 1, M, g an m-dimensional submanifold of M and g the induced metric ofg onM. Ifg is degenerate on the tangent bundleTM ofM, then M is called a lightlike submanifold of M see 11. For a degenerate metric g on M,TM⊥ is a degenerate n-dimensional subspace of TxM. Thus both TxM and TxM⊥ are degenerate orthogonal subspaces but no longer complementary. In this case, there exists a subspace RadTxMTxM∩TxM⊥which is known as radicalnullsubspace. If the mapping RadTM :x ∈ M → RadTxMdefines a smooth distribution onMof rankr > 0, then the submanifoldMofMis called anr-lightlike submanifold and RadTMis called the radical distribution onM.
Screen distribution STM is a semi-Riemannian complementary distribution of RadTMinTM, that is
TMRadTM⊥STM, 2.1
and STM⊥ is a complementary vector subbundle to RadTM in TM⊥. Let trTM and ltrTM be complementary but not orthogonal vector bundles to TM in TM|M and to RadTMinSTM⊥⊥, respectively. Then we have
trTM ltrTM⊥S TM⊥
, 2.2
TM|MTM⊕trTM RadTM⊕ltrTM⊥STM⊥S TM⊥
. 2.3
For a quasi-orthonormal fields of frames onTM, we have the following.
Theorem 2.1 see11. Let M, g, STM, STM⊥ be an r-lightlike submanifold of a semi- Riemannian manifoldM, g. Then there exists a complementary vector bundle ltrTMof RadTM inSTM⊥⊥and a basis ofΓltrTM|uconsisting of smooth section{Ni}ofSTM⊥⊥|u, whereu is a coordinate neighborhood ofMsuch that
g Ni, ξj
δij, g
Ni, Nj
0, for anyi, j ∈ {1,2, . . . , r}, 2.4 where{ξ1, . . . , ξr}is a lightlike basis ofΓRadTM.
Let∇be the Levi-Civita connection onM, then, according to the decomposition2.3, the Gauss and Weingarten formulas are given by the following:
∇XY ∇XY hX, Y, ∇XU−AUX∇⊥XU, 2.5
for anyX, Y ∈ΓTMandU ∈ΓtrTM, where{∇XY, AUX}and{hX, Y,∇⊥XU}belong toΓTMandΓtrTM, respectively. Here∇is a torsion-free linear connection onM,his a symmetric bilinear form onΓTMwhich is called second fundamental form, andAUis a linear a operator onMand known as shape operator.
According to 2.2 considering the projection morphisms L and S of trTM on ltrTMandSTM⊥, respectively, then Gauss and Weingarten formulas become
∇XY ∇XYhlX, Y hsX, Y, ∇XU−AUXDlXUDsXU, 2.6
where we put hlX, Y LhX, Y, hsX, Y ShX, Y, DXlU L∇⊥XU, DXsU S∇⊥XU. AshlandhsareΓltrTMvalued andΓSTM⊥valued, respectively, therefore they are called the lightlike second fundamental form and the screen second fundamental form onM. In particular,
∇XN−ANX∇lXNDsX, N, ∇XW−AWX∇sXWDlX, W, 2.7
whereX∈ΓTM, N∈ΓltrTM, andW ∈ΓSTM⊥. Using2.6and2.7, we obtain ghsX, Y, W g
Y, DlX, W
gAWX, Y, 2.8 gDsX, N, W gAWX, N, 2.9 for anyX∈ΓTM,W∈ΓSTM⊥, andN, N∈ΓltrTM.
LetP be the projection morphism ofTMonSTM, then, using2.1, we can induce some new geometric objects on the screen distributionSTMonMas follows:
∇XPY ∇∗XPYh∗X, PY, ∇Xξ−A∗ξX∇∗tXξ, 2.10
for anyX, Y ∈ΓTMandξ∈ΓRadTM, where{∇∗XPY, A∗ξX}and{h∗X, PY,∇∗tXξ}belong toΓSTMandΓRadTM, respectively. Using2.6and2.10, we obtain
g
hlX, PY, ξ g
A∗ξX, PY
, gh∗X, PY, N gANX, PY, 2.11
for anyX, Y ∈ΓTM, ξ∈ΓRadTMandN∈ΓltrTM.
Denote byRandRthe curvature tensors of∇and∇, respectively, then by straightfor- ward calculations11, we have
RX, YZRX, YZAhlX,ZY −AhlY,ZXAhsX,ZY
−AhsY,ZX
∇Xhl
Y, Z−
∇Yhl X, Z DlX, hsY, Z−DlY, hsX, Z ∇XhsY, Z
−∇YhsX, Z Ds
X, hlY, Z
−Ds
Y, hlX, Z ,
2.12
where
∇XhsY, Z ∇sXhsY, Z−hs∇XY, Z−hsY,∇XZ 2.13 ∇Xhl
Y, Z ∇lXhlY, Z−hl∇XY, Z−hlY,∇XZ. 2.14
Then Codazzi equation is given, respectively, by the following:
RX, YZ⊥
∇Xhl
Y, Z−
∇Yhl X, Z
DlX, hsY, Z−DlY, hsX, Z ∇XhsY, Z
−∇YhsX, Z Ds
X, hlY, Z
−Ds
Y, hlX, Z .
2.15
Barros and Romero17defined indefinite Kaehler manifolds as follows.
Definition 2.2. LetM, J, gbe an indefinite almost Hermitian manifold and∇the Levi-Civita connection on M, with respect to an indefinite metric g. Then M is called an indefinite Kaehler manifold ifJis parallel, with respect to∇, that is
J2 −I,
∇XJ
Y 0, gJX, JY gX, Y ∀X, Y ∈Γ TM
. 2.16
3. Generalized Cauchy-Riemann Lightlike Submanifolds
Definition 3.1. LetM, g, STMbe a real lightlike submanifold of an indefinite Kaehler man- ifoldM, g, J, thenMis called a generalized Cauchy-RiemannGCR-lightlike submanifold if the following conditions are satisfied.
AThere exist two subbundlesD1andD2of RadTMsuch that
RadTM D1⊕D2, JD1 D1, JD2⊂STM. 3.1
BThere exist two subbundlesD0andDofSTMsuch that
STM
JD2⊕D
⊥D0, JD0 D0, J D
L1⊥L2, 3.2
whereD0is a nondegenerate distribution onM,L1andL2are vector bundle of ltrTMand STM⊥, respectively.
Then the tangent bundle TM of M is decomposed as TM D ⊥ D, where D RadTM ⊕ D0 ⊕ JD2. M is called a proper GCR-lightlike submanifold if D1/{0}, D2/{0}, D0/{0}, andL2/{0}. LetQ, P1andP2be the projections onD,JL1 M1, andJL2 M2, respectively. Then, for anyX ∈ΓTM, we have
XQXP1XP2X, 3.3
applyingJto3.3, we obtain
JXTXwP1XwP2X, 3.4
and we can write3.4as follwos:
JXTXwX, 3.5
whereTX andwX are the tangential and transversal components ofJX, respectively. Simi- larly,
JV BVCV, 3.6
for anyV ∈ΓtrTM, whereBV andCV are the sections ofTMand trTM, respectively.
ApplyingJto3.5and3.6, we get
T2−I−Bω, C2−I−ωB. 3.7
Differentiating3.4and using2.6,2.7, and3.6, we have
DsX, wP1Y −∇sXwP2YwP2∇XY−hsX, TY ChsX, Y, 3.8 DlX, wP2Y −∇lXwP1YwP1∇XY−hlX, TY ChlX, Y. 3.9
Using Kaehlerian property of∇with2.7, we have the following lemmas.
Lemma 3.2. LetMbe aGCR-lightlike submanifold of an indefinite Kaehlerian manifoldM. Then one has
∇XTY AwYXBhX, Y,
∇tXw
Y ChX, Y−hX, TY, 3.10
whereX, Y ∈ΓTMand
∇XTY ∇XTY−T∇XY,
∇tXw
Y ∇tXwY−w∇XY. 3.11
Lemma 3.3. LetMbe aGCR-lightlike submanifold of an indefinite Kaehlerian manifoldM. Then one has
∇XBV ACVX−TAVX,
∇tXC
V −wAVX−hX, BV, 3.12
whereX∈ΓTM,V ∈ΓtrTM, and
∇XBV ∇XBV−B∇tXV,
∇tXC
V ∇tXCV −C∇tXV. 3.13
4. Holomorphic Sectional Curvature of a GCR-Lightlike Submanifold
Let Mbe a complex space form of constant holomorphic curvaturec. Then the curvature tensorRofMcis given by the following:
RX, YZ c 4
gY, ZX−gX, ZYgJY, ZJX
−gJX, ZJY2gX, JYJZ ,
4.1
forX, Y, Zvector fields onM. Using4.1and2.12, we obtain gRX, YZ, W c
4
gY, ZgX, W−gX, ZgY, W gJY, ZgJX, W
−gJX, ZgJY, W 2gX, JYgJZ, W
−g
AhlX,ZY, W g
AhlY,ZX, W
−g
AhsX,ZY, W g
AhsY,ZX, W
−g
∇Xhl
Y, Z, W g
∇Yhl
X, Z, W
−g
DlX, hsY, Z, W g
DlY, hsX, Z, W .
4.2
Using2.8in4.2, we obtain gRX, YZ, W c
4
gY, ZgX, W−gX, ZgY, W gJY, ZgJX, W
−gJX, ZgJY, W 2gX, JYgJZ, W
−g
AhlX,ZY, W g
AhlY,ZX, W
−ghsY, W, hsX, Z ghsX, W, hsY, Z
−g
∇Xhl
Y, Z, W g
∇Yhl
X, Z, W .
4.3
Then the sectional curvatureKMX, Y gRX, YY, XofMdetermined by orthonormal vectorsXandY ofΓD0⊕M2and given by the following:
KMX, Y c 4
13gX, JY2 −g
AhlX,YY, X g
AhlY,YX, X
−ghsY, X, hsX, Y ghsX, X, hsY, Y.
4.4
Corollary 4.1. LetMbe aGCR-lightlike submanifold of an indefinite Complex space formMc.
Then sectional curvature ofMis given byKMX, Y c/4{13gX, JY2}, if iM2defines a totally geodesic foliation inM,
iiD0defines a totally geodesic foliation inM, iiiMis totally geodesic inM.
Definition 4.2. The holomorphic sectional curvatureHX gRX, JXJX, XofMdeter- mined by a unit vectorX ∈ΓD0is the sectional curvature of a plane section{X, JX}.
Then using2.11and4.4, for a unit vector fieldX∈ΓD0, we get HX c−g
hlX, JX, h∗JX, X g
hlJX, JX, h∗X, X
−ghsJX, X, hsX, JX ghsX, X, hsJX, JX.
4.5
From3.8, for anyX, Y ∈ΓD0, we have
hsX, JY wP2∇XY ChsX, Y, 4.6
and further using3.7and4.6, we have
hsJX, JY wP2∇JXY−wBhsX, Y−hsX, Y. 4.7
Hence using 4.6 and 4.7 in 4.5, we obtain the expression for holomorphic sectional curvature as follows:
HX c−g
hlX, JX, h∗JX, X g
hlJX, JX, h∗X, X
− wP2∇XX2
− ChsX, X2g
hsX, X, wP2∇JXX
BhsX, X2− hsX, X2.
4.8
Theorem 4.3. LetMbe aGCR-lightlike submanifold of an indefinite complex space formMc. If Mis totally geodesic inMc, thenHX≤c, for any unit vector fieldX ∈ΓD0.
Proof. Using the hypothesis in4.8, we getHX c−wP2∇XX2. Hence the result follows.
Theorem 4.4see13. LetMbe aGCR-lightlike submanifold of an indefinite Kaehler manifold M, then the distributionDis integrable if and only ifhX, JY hY, JX, for anyX, Y ∈ΓD.
Theorem 4.5. LetMbe aGCR-lightlike submanifold of an indefinite complex space formMc, and D0is integrable, thenHX≤cfor any unit vector fieldX∈ΓD0.
Proof. SinceD0is integrable therefore usingTheorem 4.4, we havehJX, JY −hX, Y, for any unit vector fieldX∈ΓD0. Therefore, from4.5, we obtain
HX c−g
hlX, JX, h∗JX, X
−g
hlX, X, h∗X, X
− hsX, JX2− hsX, X2≤c.
4.9
Theorem 4.6. AGCR-lightlike submanifold of an indefinite complex space formMcisD0-totally geodesic if and only if
iD0is integrable,
iiHX c, for any unit vector fieldX ∈ΓD0. Proof. Proof follows from4.9.
Theorem 4.7see13. LetMbe aGCR-lightlike submanifold of an indefinite Kaehler manifold M. Then the distributionDdefines a totally geodesic foliation inMif and only ifBhX, Y 0, for anyX, Y ∈ΓD.
Theorem 4.8. LetMbe aGCR-lightlike submanifold of an indefinite complex space formMc, and D0defines a totally geodesic foliation inM, thenHX≤c, for any unit vector fieldX∈ΓD0. Proof. SinceD0defines a totally geodesic foliation inM, therefore by definition∇XX ∈ΓD0, this implies that h∗X, X 0. Also by usingTheorem 4.7, we haveBhX, X 0, for any X∈ΓD0; hence,4.8becomesHX c−2ChsX, X2and the result follows.
Definition 4.9. The horizontal distribution D is called parallel with respect to the induced connection∇onMif∇XY ∈Dfor anyX∈ΓTMandY ∈ΓD.
Theorem 4.10. LetMbe aGCR-lightlike submanifold of an indefinite complex space formMcand D0is parallel, with respect to∇, thenHX≤c, for any unit vector fieldX ∈ΓD0.
Proof. SinceD0is parallel, with respect to the induced connection∇onM, therefore∇∗XY ∈ ΓD0andh∗X, Y 0, for anyX ∈ ΓTMandY ∈ ΓD0. Hence, from 4.8, we obtain HX cBhsX, X2−hsX, X2−ChsX, X2, and then by using3.6, we getHX c−2ChsX, X2. Hence the result is complete.
Lemma 4.11. LetM be aGCR-lightlike submanifold of an indefinite Kaehler manifold M. If the distributionD0defines a totally geodesic foliation inM, thenMisD0-geodesic.
Proof. By the definition ofGCR-lightlike submanifold, MisD0-geodesic ifghlX, Y, ξ ghsX, Y, W 0, for anyX, Y ∈ ΓD0,ξ ∈ ΓRadTM, andW ∈ ΓSTM⊥. Since D0 defines a totally geodesic foliation in M, thereforeghlX, Y, ξ g∇XY, ξ 0 and ghsX, Y, W g∇XY, W 0. Hence, the assertion follows.
Theorem 4.12. LetMbe aGCR-lightlike submanifold of an indefinite complex space formMc. If D0defines a totally geodesic foliation inM, thenHX c, for any unit vector fieldX∈ΓD0.
Proof. The result follows directly usingLemma 4.11and4.8.
5. Null Holomorphically Flat GCR-Lightlike Submanifold
Letx∈MandUbe a null vector ofTxM. A planeπofTxMis called a null plane directed by Uif it containsU,gxU, V 0, for anyV ∈π, and there existsV0∈πsuch thatgxV0, V0/0.
Following Beem-Ehrlich18, the null sectional curvature ofπ, with respect toUand∇, as a real number, is defined as follows:
KUπ gx
RV, UU, V
gxV, V , 5.1
whereVis an arbitrary non null vector inπ. ClearlyKUπis independent ofV but depends in a quadratic fashion onU.
Consideru∈Mand a null planeπ ofTuMdirected byξu ∈RadTM, then the null sectional curvature ofπ, with respect toξuand∇, as a real number is defined as
Kξuπ guRVu, ξuξu, Vu
guVu, Vu , 5.2
whereVuis an arbitrary non-null vector inπ.
LetMbe aGCR-lightlike submanifold of an indefinite complex space formMcthen using4.3, the null sectional curvature ofπ, with respect toξ, is given by the following:
Kξπ 1 gV, V
g
Ahlξ,ξV, V
−g
AhlV,ξξ, V
ghsV, V, hsξ, ξ
−ghsξ, V, hsV, ξ−g
∇Vhl
ξ, ξ, V g
∇ξhl
V, ξ, V . 5.3
Then, using2.11, we obtain
Kξπ 1 gV, V
g
h∗V, V, hlξ, ξ
−g
h∗ξ, V, hlV, ξ
ghsV, V, hsξ, ξ
−ghsξ, V, hsV, ξ−g
∇Vhl
ξ, ξ, V g
∇ξhl
V, ξ, V . 5.4
We know that a planeπ is called holomorphic if it remains invariant under the action of the almost complex structureJ, that is, ifπ {Z, JZ}. The sectional curvature associated with the holomorphic plane is called the holomorphic sectional curvature, denoted byHπ and given by Hπ RZ, JZ, Z, JZ/gZ, Z2. The holomorphic plane π {Z, JZ} is called null or degenerate if and only ifZis a null vector. A manifoldM, g, Jis called null holomorphically flat if the curvature tensorRsatisfiessee19.
R
Z, JZ, Z, JZ
0, 5.5
for all null vectorsZ. PutgRX, YZ, W RX, Y, Z, W, then, from5.4, we obtain R
ξ, Jξ, ξ, Jξ g
h∗ξ, ξ, hl
Jξ, Jξ
−g h∗
Jξ, ξ , hl
ξ, Jξ g
hsξ, ξ, hs
Jξ, Jξ
−g hs
Jξ, ξ , hs
ξ, Jξ
−g
∇ξhl Jξ, Jξ
, ξ g
∇Jξhl ξ, Jξ
, ξ .
5.6
Definition 5.1 see 20. A lightlike submanifold M, g of a semi-Riemannian manifold M, g is said to be a totally umbilical in M if there is a smooth transversal vector field
H ∈ ΓtrTM on M, called the transversal curvature vector field of M, such that, for X, Y ∈ΓTM,
hX, Y HgX, Y. 5.7
Using 2.6, it is clear that M is a totally umbilical if and only if on each coordinate neighborhooduthere exist smooth vector fieldsHl∈ΓltrTMandHs∈ΓSTM⊥such that
hlX, Y HlgX, Y, hsX, Y HsgX, Y, DlX, W 0, 5.8
forX, Y∈ΓTMandW∈ΓSTM⊥. A lightlike submanifold is said to be totally geodesic ifhX, Y 0, for anyX, Y ∈ ΓTM. Therefore, in other words, a lightlike submanifold is totally geodesic ifHl0 andHs0.
LetMbe a totally umbilical lightlike submanifold, then, using above definition, we have hJξ, Jξ HgJξ, Jξ Hgξ, ξ 0 and hξ, Jξ Hgξ, Jξ 0, for any ξ∈ΓRadTM. Thus, from5.6, we have the following theorem.
Theorem 5.2. LetMbe aGCR-lightlike submanifold of an indefinite complex space formMc. If Mis totally umbilical lightlike submanifold inMc, thenMis null holomorphically flat.
Moreover, from 5.6, it is clear that the expression of Rξ, Jξ, ξ, Jξ is expressed in terms of screen second fundamental forms ofM, thusGCR-lightlike submanifoldMof an indefinite complex space formMcis null holomorphically flat ifMis totally geodesic.
6. Holomorphic Bisectional Curvature of a GCR-Lightlike Submanifold
Definition 6.1. The holomorphic bisectional for the pair of unit vector fields{X, Y}onMis given byHX, Y gRX, JXJY, Y.
Theorem 6.2. LetMbe a mixed totally geodesicGCR-lightlike submanifold of an indefinite Kaehler manifoldMwithD0 parallel distribution. ThenHX, Z 0, for any unit vector fieldsX ∈ΓD0 andZ∈ΓM2.
Proof. LetX, Y∈ΓD0andZ∈ΓM2then, by using that hypothesis that the distributionD0 is a parallel, with respect to∇onM, we havegT∇XZ, Y −g∇XZ, TY gZ,∇XTY 0.
Hence, the non degeneracy of the distributionD0implies that
∇XZ∈Γ D
, 6.1
for anyZ ∈ ΓM2. Now replacingY byJX, respectively, in 2.15and then taking inner product withJZ, for anyX∈ΓD0andZ∈ΓM2, we get
HX, Z ghs∇XJX, Z, JZ−g∇XhsJX, Z, JZ ghsJX,∇XZ, JZ g
∇JXhsX, Z, JZ
−g hs
∇JXX, Z , JZ
−g hs
X,∇JXZ , JZ
−g Ds
X, hlJX, Z , JZ
g Ds
JX, hlX, Z , JZ
.
6.2
Hence by using thatMis mixed totally geodesic with6.1, the assertion follows.
Theorem 6.3. In order that an indefinite complex space form Mc may admit a mixed totally geodesicGCR-lightlike submanifoldMwith parallel horizontal distributionD0, it is necessary that c0.
Proof. LetX ∈ΓD0andZ∈ΓM2be unit vector fields, then4.1implies thatHX, Z
−c/2gX, XgZ, Z, then the non degeneracy of the distributions D0 and M2 with the Theorem 6.2, we obtainc0. Hence, the result follows.
Lemma 6.4. LetMbe aGCR-lightlike submanifold of an indefinite Kaehler manifoldM. Then we have the following:
iifDdefines a totally geodesic foliation inMthenghsD, D0, JD 0,
iiif D0 is a parallel distribution, with respect to∇, then hZ, JX ChZ, X for any X∈ΓD0, Z∈ΓM2.
Proof. i Let D define a totally geodesic foliation in M this implies that∇XY ∇XY ∈ ΓDandhX, Y 0, for anyX, Y ∈ ΓD. Therefore by using3.10, we obtainAwYX
−BhX, Y 0. LetZ∈ΓD0, then by using2.8, we get 0gAwYX, Z ghsX, Z, wY. Thus we haveghsD, D0, JD 0.
iiLetD0is a parallel distribution with respect to the induced connection∇, therefore
∇XY ∈ ΓD0, for any Y ∈ ΓD0, X ∈ ΓTM. SinceMis Kaehler manifold, therefore for Z ∈ ΓM2andX ∈ ΓD0, we have∇ZJX J∇ZX. This implies that∇ZJXhZ, JX J∇ZXBhZ, X ChZ, X, then by equating transversal components on both sides, we get the result.
Theorem 6.5. LetMbe aGCR-lightlike submanifold of an indefinite Kaehler manifoldM. IfD0is parallel with respect to the induced connection∇, andM2 defines a totally geodesic foliation inM, then
HX, Z ghJX, Z, J∇XZ−g
hX, Z, J∇JXZ g
AJZJX,∇XZ
−g
AJZX,∇JXZ
2ChsX, Z2, 6.3
for any unit vector fieldsX ∈ΓD0andZ∈ΓM2.
Proof. LetX ∈ΓD0andZ∈ΓM2, then the equation of Codazzi2.15becomes g
RX, JXZ, JZ
g∇XhsJX, Z, JZ−g
∇JXhs
X, Z, JZ
g Ds
X, hlJX, Z , JZ
−g Ds
JX, hlX, Z , JZ
.
6.4
By using2.13and6.1with theLemma 6.4i, we obtain
HX, Z g
∇sJXhsX, Z, JZ
−g
∇sXhsJX, Z, JZ g
AJZJX,∇XZ
−g
AJZX,∇JXZ
−g Ds
X, hlJX, Z , JZ
g Ds
JX, hlX, Z , JZ
.
6.5
Now by using2.7with theLemma 6.4ii, we have
g
∇sXhsJX, Z, JZ g
∇XhsJX, Z, JZ
−ghsJX, Z, J∇XZ− ChsX, Z2,
6.6
and similarly
g
∇sJXhsX, Z, JZ −g
hsX, Z, J∇JXZ
ChsX, Z2. 6.7
By using2.7, we have
g Ds
X, hlJX, Z , JZ
−g
hlJX, Z, J∇XZ
, 6.8
g Ds
JX, hlX, Z , JZ
−g
hlX, Z, J∇JXZ
. 6.9
Hence by using6.6–6.9in6.5, the result follows.
Definition 6.6see13. AGCR-lightlike submanifoldMof an indefinite Kaehler manifold Mis called aGCR-lightlike product if both the distributionsDandDdefine totally geodesic foliations inM.
Theorem 6.7see14. LetMbe aGCR-lightlike submanifold of an indefinite Kaehler manifoldM.
Then,Mis aGCR-lightlike product if and only if∇XTY 0, for anyX, Y ∈ΓDorX, Y ∈ΓD.
Theorem 6.8. Let M be a GCR-lightlike submanifold of an indefinite Kaehler manifold M. If
∇XTY 0, for anyX, Y ∈ΓTM, then
HX, Z 2ghsJX, Z, JhsX, Z, 6.10
for any unit vector fieldsX ∈ΓD0andZ∈ΓM2. Proof. Let∇XTY 0, then3.10implies that
AwYXBhX, Y 0, 6.11
for anyX, Y ∈ΓTM. LetY ∈ΓD, X∈ΓTM, then6.11gives
BhX, Y 0. 6.12
LetZ∈ΓDandX ∈ΓD, then using6.11and6.12, we obtain
AwZX0. 6.13
Particularly choosingX ∈ΓD0andZ∈ΓM2in2.15, we get g
RX, JXZ, JZ
g∇XhsJX, Z, JZ−g
∇JXhs
X, Z, JZ g
Ds
X, hlJX, Z , JZ
−g Ds
JX, hlX, Z , JZ
. 6.14
Since∇XTY 0 therefore, by usingTheorem 6.7, the distributionsDandDdefine totally geodesic foliations inM. ThenDdefines totally geodesic foliation inMimplies that for any Z1, Z2 ∈ΓD, we have∇Z1Z2 ∈ΓD. Therefore, using3.10and3.11, we getAwZ2Z1 BhZ1, Z2 0. By taking inner product withX∈ΓD0and using2.8, we get
ghsZ1, X, wZ2 0. 6.15
Also,3.11implies thatT∇XZ0, that is,∇XZ∈ΓD. Therefore using2.8,2.13,6.13, and6.15in6.14, we obtain
g
RX, JXZ, JZ g
∇sXhsJX, Z, JZ
−g
∇sJXhsX, Z, JZ g
Ds
X, hlJX, Z , JZ
−g Ds
JX, hlX, Z , JZ
.
6.16
Now using2.6,2.7,2.8, and6.15, we have g
∇sXhsJX, Z, JZ
gJhsJX, Z, hsX, Z. 6.17
Similarly,
g
∇sJXhsX, Z, JZ
−gJhsJX, Z, hsX, Z. 6.18
Also using2.7, we have g
Ds
X, hlJX, Z , JZ
0, g Ds
JX, hlX, Z , JZ
0. 6.19
Hence, using6.17–6.19in6.16, the result follows.
Lemma 6.9. Let M be a GCR-lightlike submanifold of an indefinite Kaehler manifold such that
∇XBY 0. ThenhsJX, Z∈ΓL⊥2for anyX∈ΓD0,Z∈ΓM2.
Proof. Since∇XBY 0, therefore, from3.12we haveTAWX 0, for anyX ∈ΓTMand W∈ΓL2, this implies that
AWX ∈Γ D
, 6.20
for anyW ∈ ΓL2andX ∈ ΓTM. SincehsJX, Z ∈ΓSTM⊥, therefore, to prove that hsJX, Z ∈ ΓL⊥2, it is sufficient to prove that ghsJX, Z, W 0, for any W ∈ ΓL2. Let X ∈ ΓD0 and Z ∈ ΓM2 such that W wZ, we have g∇UZ, X g∇UZ, X g∇UJZ, JX −gAJZU, JX gJAJZU, X, then using2.8we obtain
ghsJX, Z, W −gJAWZ, X −g∇ZZ, X −gT∇ZZ, TX. 6.21
Since, from3.10, we haveT∇ZZ−AwZZ−BhZ, Z, then using6.20in6.21, the result follows.
Theorem 6.10. LetMbe aGCR-lightlike submanifold of an indefinite Kaehler manifold such that
∇XBY 0, then
HX, Z 2gJhsX, Z, hsJX, Z−g
AJZ∇JXX, Z g
AJZ∇XJX, Z
, 6.22
for any unit vector fieldsX ∈ΓD0andZ∈ΓM2.
Proof. LetX ∈ΓD0andZ∈ΓM2, then, from2.15and2.13, we obtain g
RX, JXZ, JZ g
∇sXhsJX, Z, JZ
−ghs∇XJX, Z, JZ
−ghsJX,∇XZ, JZ−g
∇sJXhsX, Z, JZ g
hs
∇JXX, Z , JZ
g hs
X,∇JXZ , JZ g
Ds
X, hlJX, Z , JZ
−g Ds
JX, hlX, Z , JZ
,
6.23
using6.20in2.9, we obtain g
Ds
X, hlJX, Z , JZ
0, g Ds
JX, hlX, Z , JZ
0. 6.24
Now consider g
∇sXhsJX, Z, JZ −g
hsJX, Z, J∇XZ
ghsX, Z, JhsJX, Z, 6.25
and similarly
g
∇sJXhsX, Z, JZ
−ghsX, Z, JhsJX, Z. 6.26
Also using2.8, we have
ghs∇XJX, Z, JZ g
AJZ∇XJX, Z , g
hs
∇JXX, Z , JZ
g
AJZ∇JXX, Z
. 6.27
Using6.20in2.8, we have
ghsJX,∇XZ, JZ 0, g hs
X,∇JXZ , JZ
0. 6.28
Thus using6.24–6.28in6.23, the result follows.
Theorem 6.11. LetMbe a mixed foliateGCR-lightlike submanifold of an indefinite Kaehler manifold M, andSTMis parallel distribution, with respect to the induced connection∇, then
HX, Z 2g
AJZJX, JAJZX
, 6.29
for any unit vector fieldsX ∈ΓD0andZ∈ΓM2.
Proof. SinceMis mixed foliate therefore for anyX∈ΓD0andZ∈ΓM2, Codazzi equation 2.15and2.13, imply that
HX, Z ghs∇XJX, Z, JZ ghsJX,∇XZ, JZ
−g hs
∇JXX, Z , JZ
−g hs
X,∇JXZ , JZ
. 6.30
Since using 2.8 and the hypothesis, we have gAJZX, JW 0 and gAJZX, Jξ ghsX, Jξ, JZ g∇XJξ, JZ −gξ,∇XZ 0. Therefore, by the definition of a GCR- lightlike submanifold, we have
AJZX ∈ΓD. 6.31
Thus, using2.7,2.8, and6.31with the hypothesis, we obtain ghsJX,∇XZ, JZ g
AJZJX,∇XZ g
JAJZJX, J∇XZ g
AJZJX, JAJZX
−g
AJZJX, JDlX, JZ g
AJZJX, JAJZX .
6.32
Similarly, we obtain
g hs
X,∇JXZ , JZ
g
AJZX, JAJZJX , g
hs
∇JXX, Z , JZ
g
AJZZ,∇JXX
−g
∇JXX, DlJZ, Z , ghs∇XJX, Z, JZ g
AJZZ,∇XJX
−g
∇XJX, DlJZ, Z .
6.33
Thus,6.30becomes HX, Z 2g
AJZJX, JAJZX
−g
AJZZ,∇JXX g
∇JXX, DlJZ, Z g
AJZZ,∇XJX
−g
∇XJX, DlJZ, Z .
6.34
Since the distributionDis integrable, therefore∇JXX− ∇XJX X, JX X ∈ΓD, then 6.34becomesHX, Z 2gAJZJX, JAJZX−gAJZZ, X gX, DlJZ, Z. Hence, using the hypothesis and2.8, the result follows.
Acknowledgment
The authors would like to thank the anonymous referee for his/her comments that helped us to improve this paper.
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