Abstract

We study the geometry of lightlike submanifolds (𝑀,𝑔,𝑆(𝑇𝑀),𝑆(𝑇𝑀)) of a semi-Riemannian manifold (𝑀,̃𝑔) of quasiconstant curvature subject to the following conditions: (1) the curvature vector field ζ of 𝑀 is tangent to 𝑀, (2) the screen distribution 𝑆(𝑇𝑀) of 𝑀 is totally geodesic in 𝑀, and (3) the coscreen distribution 𝑆(𝑇𝑀) of 𝑀 is a conformal Killing distribution.

1. Introduction

In the generalization from the theory of submanifolds in Riemannian to the theory of submanifolds in semi-Riemannian manifolds, the induced metric on submanifolds may be degenerate (lightlike). Therefore, there is a natural existence of lightlike submanifolds and for which the local and global geometry is completely different than nondegenerate case. In lightlike case, the standard text book definitions do not make sense, and one fails to use the theory of nondegenerate geometry in the usual way. The primary difference between the lightlike submanifolds and nondegenerate submanifolds is that in the first case, the normal vector bundle intersects with the tangent bundle. Thus, the study of lightlike submanifolds becomes more difficult and different from the study of nondegenerate submanifolds. Moreover, the geometry of lightlike submanifolds is used in mathematical physics, in particular, in general relativity since lightlike submanifolds produce models of different types of horizons (event horizons, Cauchy’s horizons, and Kruskal’s horizons). The universe can be represented as a four-dimensional submanifold embedded in a (4+𝑛)-dimensional spacetime manifold. Lightlike hypersurfaces are also studied in the theory of electromagnetism [1]. Thus, large number of applications but limited information available motivated us to do research on this subject matter. Kupeli [2] and Duggal and Bejancu [1] developed the general theory of degenerate (lightlike) submanifolds. They constructed a transversal vector bundle of lightlike submanifold and investigated various properties of these manifolds.

In the study of Riemannian geometry, Chen and Yano [3] introduced the notion of a Riemannian manifold of a quasiconstant curvature as a Riemannian manifold (𝑀,̃𝑔) with the curvature tensor 𝑅 satisfying the conditioñ𝑔𝑅(𝑋,𝑌)𝑍,𝑊=𝛼{̃𝑔(𝑌,𝑍)̃𝑔(𝑋,𝑊)̃𝑔(𝑋,𝑍)̃𝑔(𝑌,𝑊)}+𝛽{̃𝑔(𝑋,𝑊)𝜃(𝑌)𝜃(𝑍)̃𝑔(𝑋,𝑍)𝜃(𝑌)𝜃(𝑊)+̃𝑔(𝑌,𝑍)𝜃(𝑋)𝜃(𝑊)̃𝑔(𝑌,𝑊)𝜃(𝑋)𝜃(𝑍)},(1.1)for any vector fields 𝑋,𝑌,𝑍, and 𝑊 on 𝑀, where 𝛼,𝛽 are scalar functions and 𝜃 is a 1-form defined by𝜃(𝑋)=̃𝑔(𝑋,𝜁),(1.2) where 𝜁 is a unit vector field on 𝑀 which called the curvature vector field. It is well known that if the curvature tensor 𝑅 is of the form (1.1), then the manifold is conformally flat. If 𝛽=0, then the manifold reduces to a space of constant curvature.

A nonflat Riemannian manifold of dimension 𝑛(>2) is defined to be a quasi-Einstein manifold [4] if its Ricci tensor satisfies the conditionRic(𝑋,𝑌)=𝑎̃𝑔(𝑋,𝑌)+𝑏𝜙(𝑋)𝜙(𝑌),(1.3)

where 𝑎,𝑏 are scalar functions such that 𝑏0, and 𝜙 is a nonvanishing 1-form such that ̃𝑔(𝑋,𝑈)=𝜙(𝑋) for any vector field 𝑋, where 𝑈 is a unit vector field. If 𝑏=0, then the manifold reduces to an Einstein manifold. It can be easily seen that every Riemannian manifold of quasiconstant curvature is a quasi-Einstein manifold.

The subject of this paper is to study the geometry of lightlike submanifolds of a semi-Riemannian manifold (𝑀,̃𝑔) of quasiconstant curvature. We prove two characterization theorems for such a lightlike submanifold (𝑀,𝑔,𝑆(𝑇𝑀),𝑆(𝑇𝑀)) as follows.

Theorem 1.1. Let 𝑀 be an 𝑟-lightlike submanifold of a semi-Riemannian manifold (𝑀,̃𝑔) of quasiconstant curvature. If the curvature vector field 𝜁 of 𝑀 is tangent to 𝑀 and 𝑆(𝑇𝑀) is totally geodesic in 𝑀, then one has the following results: (1)if 𝑆(𝑇𝑀) is a Killing distribution, then the functions 𝛼 and 𝛽, defined by (1.1), vanish identically. Furthermore, 𝑀, 𝑀, and the leaf 𝑀 of 𝑆(𝑇𝑀) are flat manifolds;(2)if 𝑆(𝑇𝑀) is a conformal Killing distribution, then the function 𝛽 vanishes identically. Furthermore, 𝑀 and 𝑀 are space of constant curvatures, and 𝑀 is an Einstein manifold such that Ric=(𝑟/(𝑚𝑟))𝑔, where 𝑟 is the induced scalar curvature of 𝑀.

Theorem 1.2. Let 𝑀 be an irrotational 𝑟-lightlike submanifold of a semi-Riemannian manifold (𝑀,̃𝑔) of quasiconstant curvature. If 𝜁 is tangent to 𝑀, 𝑆(𝑇𝑀) is totally umbilical in 𝑀, and 𝑆(𝑇𝑀) is a conformal Killing distribution with a nonconstant conformal factor, then the function 𝛽 vanishes identically. Moreover, 𝑀 and 𝑀 are space of constant curvatures, and 𝑀 is a totally umbilical Einstein manifold such that Ric=(𝑐/(𝑚𝑟))𝑔, where 𝑐 is the scalar quantity of 𝑀.

2. Lightlike Submanifolds

Let (𝑀,𝑔) be an 𝑚-dimensional lightlike submanifold of an (𝑚+𝑛)-dimensional semi-Riemannian manifold (𝑀,̃𝑔). We follow Duggal and Bejancu [1] for notations and results used in this paper. The radical distribution Rad(𝑇𝑀)=𝑇𝑀𝑇𝑀 is a vector subbundle of the tangent bundle 𝑇𝑀 and the normal bundle 𝑇𝑀, of rank 𝑟(1𝑟min{𝑚,𝑛}). Then, in general, there exist two complementary nondegenerate distributions 𝑆(𝑇𝑀) and 𝑆(𝑇𝑀) of Rad(𝑇𝑀) in 𝑇𝑀 and 𝑇𝑀, respectively, called the screen and coscreen distribution on 𝑀, and we have the following decompositions:𝑇𝑀=Rad(𝑇𝑀)orth𝑆(𝑇𝑀);𝑇𝑀=Rad(𝑇𝑀)orth𝑆𝑇𝑀,(2.1) where the symbol orth denotes the orthogonal direct sum. We denote such a lightlike submanifold by 𝑀=(𝑀,𝑔,𝑆(𝑇𝑀),𝑆(𝑇𝑀)). Let tr(𝑇𝑀) and ltr(𝑇𝑀) be complementary (but not orthogonal) vector bundles to 𝑇𝑀 in 𝑇𝑀|𝑀 and 𝑇𝑀 in 𝑆(𝑇𝑀), respectively, and let {𝑁𝑖} be a lightlike basis of Γ(ltr(𝑇𝑀)|𝒰) consisting of smooth sections of 𝑆(𝑇𝑀)|𝒰, where 𝒰 is a coordinate neighborhood of 𝑀, such that𝑁̃𝑔𝑖,𝜉𝑗=𝛿𝑖𝑗𝑁,̃𝑔𝑖,𝑁𝑗=0,(2.2)

where {𝜉1,,𝜉𝑟} is a lightlike basis of Γ(Rad(𝑇𝑀)). Then,𝑇𝑀=𝑇𝑀tr(𝑇𝑀)={Rad(𝑇𝑀)tr(𝑇𝑀)}orth𝑆(𝑇𝑀)={Rad(𝑇𝑀)ltr(𝑇𝑀)}orth𝑆(𝑇𝑀)orth𝑆𝑇𝑀.(2.3) We say that a lightlike submanifold (𝑀,𝑔,𝑆(𝑇𝑀),𝑆(𝑇𝑀)) of 𝑀 is

(1) 𝑟-lightlike submanifold if 1𝑟<𝑚𝑖𝑛{𝑚,𝑛},

(2) coisotropic submanifold if 1𝑟=𝑛<𝑚,

(3) isotropic submanifold if 1𝑟=𝑚<𝑛,

(4) totally lightlike submanifold if 1𝑟=𝑚=𝑛.

The above three classes (2)~(4) are particular cases of the class (1) as follows: 𝑆(𝑇𝑀)={0},𝑆(𝑇𝑀)={0}, and 𝑆(𝑇𝑀)=𝑆(𝑇𝑀)={0}, respectively.

Example 2.1. Consider in 42 the 1-lightlike submanifold 𝑀 given by equations 𝑥3=12𝑥1+𝑥2,𝑥4=12𝑥log1+1𝑥22,(2.4) then we have 𝑇𝑀=span{𝑈1,𝑈2} and 𝑇𝑀={𝐻1,𝐻2}, where we set 𝑈1=2𝑥1+1𝑥22𝜕𝑥1+𝑥1+1𝑥22𝜕𝑥3+2𝑥1𝑥2𝜕𝑥4,𝑈2=2𝑥1+1𝑥22𝜕𝑥2+𝑥1+1𝑥22𝜕𝑥3+2𝑥1𝑥2𝜕𝑥4,𝐻1=𝜕𝑥1+𝜕𝑥2+2𝜕𝑥3,𝐻2𝑥=21+2𝑥12𝜕𝑥2+2𝑥1𝑥2𝜕𝑥3+𝑥1+1𝑥22𝜕𝑥4.(2.5) It follows that Rad(𝑇𝑀) is a distribution on 𝑀 of rank 1 spanned by 𝜉=𝐻1. Choose 𝑆(𝑇𝑀) and 𝑆(𝑇𝑀) spanned by 𝑈2 and 𝐻2 where are timelike and spacelike, respectively. Finally, the lightlike transversal vector bundle 1ltr(𝑇𝑀)=Span𝑁=2𝜕𝑥1+12𝜕𝑥2+12𝜕𝑥3(2.6) and the transversal vector bundle tr(𝑇𝑀)=Span𝑁,𝐻2(2.7) are obtained.
Let be the Levi-Civita connection of 𝑀 and 𝑃 the projection morphism of Γ(𝑇𝑀) on Γ(𝑆(𝑇𝑀)) with respect to the decomposition (2.1). For an 𝑟-lightlike submanifold, the local Gauss-Weingartan formulas are given by𝑋𝑌=𝑋𝑌+𝑟𝑖=1𝑖(𝑋,𝑌)𝑁𝑖+𝑛𝛼=𝑟+1𝑠𝛼(𝑋,𝑌)𝑊𝛼,(2.8)𝑋𝑁𝑖=𝐴𝑁𝑖𝑋+𝑟𝑗=1𝜏𝑖𝑗(𝑋)𝑁𝑗+𝑛𝛼=𝑟+1𝜌𝑖𝛼(𝑋)𝑊𝛼,(2.9)𝑋𝑊𝛼=𝐴𝑊𝛼𝑋+𝑟𝑖=1𝜙𝛼𝑖(𝑋)𝑁𝑖+𝑛𝛽=𝑟+1𝜃𝛼𝛽(𝑋)𝑊𝛽,(2.10)𝑋𝑃𝑌=𝑋𝑃𝑌+𝑟𝑖=1𝑖(𝑋,𝑃𝑌)𝜉𝑖,(2.11)𝑋𝜉𝑖=𝐴𝜉𝑖𝑋𝑟𝑗=1𝜏𝑗𝑖(𝑋)𝜉𝑗,(2.12) for any 𝑋,𝑌Γ(𝑇𝑀), where and are induced linear connections on 𝑇𝑀 and 𝑆(𝑇𝑀), respectively, the bilinear forms 𝑖 and 𝑠𝛼 on 𝑀 are called the local lightlike second fundamental form and local screen second fundamental form on 𝑇𝑀, respectively, and 𝑖 is called the local radical second fundamental form on 𝑆(𝑇𝑀). 𝐴𝑁𝑖,𝐴𝜉𝑖, and 𝐴𝑊𝛼 are linear operators on Γ(𝑇𝑀), and 𝜏𝑖𝑗,𝜌𝑖𝛼,𝜙𝛼𝑖, and 𝜃𝛼𝛽 are 1-forms on 𝑇𝑀.
Since is torsion-free, is also torsion-free and both 𝑖 and 𝑠𝛼 are symmetric. From the fact that 𝑖(𝑋,𝑌)=̃𝑔(𝑋𝑌,𝜉𝑖), we know that 𝑖 are independent of the choice of a screen distribution. Note that 𝑖,𝜏𝑖𝑗, and 𝜌𝑖𝛼 depend on the section 𝜉Γ(Rad(𝑇𝑀)|𝒰). Indeed, take 𝜉𝑖=𝑟𝑗=1𝑎𝑖𝑗𝜉𝑗, then we have 𝑑(tr(𝜏𝑖𝑗))=𝑑(tr(̃𝜏𝑖𝑗)) [5].
The induced connection on 𝑇𝑀 is not metric and satisfies 𝑋𝑔(𝑌,𝑍)=𝑟𝑖=1𝑖(𝑋,𝑌)𝜂𝑖(𝑍)+𝑖(𝑋,𝑍)𝜂𝑖,(𝑌)(2.13) where 𝜂𝑖 is the 1-form such that 𝜂𝑖(𝑋)=̃𝑔𝑋,𝑁𝑖,𝑋Γ(𝑇𝑀),𝑖{1,,𝑟}.(2.14) But the connection on 𝑆(𝑇𝑀) is metric. The above three local second fundamental forms of 𝑀 and 𝑆(𝑇𝑀) are related to their shape operators by 𝑖𝐴(𝑋,𝑌)=𝑔𝜉𝑖𝑋,𝑌𝑟𝑘=1𝑘𝑋,𝜉𝑖𝜂𝑘(𝑌),(2.15)𝑖𝐴(𝑋,𝑃𝑌)=𝑔𝜉𝑖𝐴𝑋,𝑃𝑌,̃𝑔𝜉𝑖𝑋,𝑁𝑗𝜖=0,(2.16)𝛼𝑠𝛼𝐴(𝑋,𝑌)=𝑔𝑊𝛼𝑋,𝑌𝑟𝑖=1𝜙𝛼𝑖(𝑋)𝜂𝑖𝜖(𝑌),(2.17)𝛼𝑠𝛼(𝐴𝑋,𝑃𝑌)=𝑔𝑊𝛼𝐴𝑋,𝑃𝑌,̃𝑔𝑊𝛼𝑋,𝑁𝑖=𝜖𝛼𝜌𝑖𝛼(𝑋),(2.18)𝑖𝐴(𝑋,𝑃𝑌)=𝑔𝑁𝑖𝑋,𝑃𝑌,𝜂𝑗𝐴𝑁𝑖𝑋+𝜂𝑖𝐴𝑁𝑗𝑋=0,(2.19) and 𝜖𝛽𝜃𝛼𝛽=𝜖𝛼𝜃𝛽𝛼, where 𝑋,𝑌Γ(𝑇𝑀). From (2.19), we know that the operators 𝐴𝑁𝑖 are shape operators related to 𝑖 for each 𝑖, called the radical shape operators on 𝑆(𝑇𝑀). From (2.16), we know that the operators 𝐴𝜉𝑖 are Γ(𝑆(𝑇𝑀)) valued. Replace 𝑌 by 𝜉𝑗 in (2.15), then we have 𝑖(𝑋,𝜉𝑗)+𝑗(𝑋,𝜉𝑖)=0 for all 𝑋Γ(𝑇𝑀). It follows that 𝑖𝑋,𝜉𝑖=0,𝑖𝜉𝑗,𝜉𝑘=0.(2.20) Also, replace 𝑋 by 𝜉𝑗 in (2.15) and use (2.20), then we have 𝑖𝑋,𝜉𝑗=𝑔𝑋,𝐴𝜉𝑖𝜉𝑗,𝐴𝜉𝑖𝜉𝑗+𝐴𝜉𝑗𝜉𝑖=0,𝐴𝜉𝑖𝜉𝑖=0.(2.21) Thus 𝜉𝑖 is an eigenvector field of 𝐴𝜉𝑖 corresponding to the eigenvalue 0. For an 𝑟-lightlike submanifold, replace 𝑌 by 𝜉𝑖 in (2.17), then we have 𝑠𝛼𝑋,𝜉𝑖=𝜖𝛼𝜙𝛼𝑖(𝑋).(2.22)
From (2.15)~(2.18), we show that the operators 𝐴𝜉𝑖 and 𝐴𝑊𝛼 are not self-adjoint on Γ(𝑇𝑀) but self-adjoint on Γ(𝑆(𝑇𝑀)).

Theorem 2.2. Let (𝑀,𝑔,𝑆(𝑇𝑀),𝑆(𝑇𝑀)) be an 𝑟-lightlike submanifold of a semi-Riemannian manifold (𝑀,̃𝑔), then the following assertions are equivalent: (i)𝐴𝜉𝑖 are self-adjoint on Γ(𝑇𝑀) with respect to 𝑔,  for all 𝑖,(ii)𝑖 satisfy 𝑖(𝑋,𝜉𝑗)=0 for all 𝑋Γ(𝑇𝑀),𝑖 and 𝑗,(iii)𝐴𝜉𝑖𝜉𝑗=0 for all 𝑖 and 𝑗, that is, the image of Rad(𝑇𝑀) with respect to 𝐴𝜉𝑖 for each 𝑖 is a trivial vector bundle,(iv)𝑖(𝑋,𝑌)=𝑔(𝐴𝜉𝑖𝑋,𝑌) for all 𝑋,𝑌Γ(𝑇𝑀) and 𝑖, that is, 𝐴𝜉𝑖 is a shape operator on 𝑀, related by the second fundamental form 𝑖.

Proof. From (2.15) and the fact that 𝑖 are symmetric, we have 𝑔𝐴𝜉𝑖𝑋,𝑌𝑔𝑋,𝐴𝜉𝑖𝑌=𝑟𝑗=1𝑘𝑋,𝜉𝑖𝜂𝑘(𝑌)𝑘𝑌,𝜉𝑖𝜂𝑘(𝑋).(2.23)
(i)(ii). If 𝑖(𝑋,𝜉𝑗)=0 for all 𝑋Γ(𝑇𝑀),𝑖 and 𝑗, then we have 𝑔(𝐴𝜉𝑖𝑋,𝑌)=𝑔(𝐴𝜉𝑖𝑌,𝑋) for all 𝑋,𝑌Γ(𝑇𝑀), that is, 𝐴𝜉𝑖 are self-adjoint on Γ(𝑇𝑀) with respect to 𝑔. Conversely, if 𝐴𝜉𝑖 are self-adjoint on Γ(𝑇𝑀) with respect to 𝑔, then we have 𝑘𝑋,𝜉𝑖𝜂𝑘(𝑌)=𝑘𝑌,𝜉𝑖𝜂𝑘(𝑋),(2.24) for all 𝑋,𝑌Γ(𝑇𝑀). Replace 𝑌 by 𝜉𝑗 in this equation and use the second equation of (2.20), then we have 𝑗(𝑋,𝜉𝑖)=0 for all 𝑋Γ(𝑇𝑀),𝑖 and 𝑗.
(ii)(iii). Since 𝑆(𝑇𝑀) is nondegenerate, from the first equation of (2.21), we have 𝑖(𝑋,𝜉𝑗)=0𝐴𝜉𝑖𝜉𝑗=0, for all 𝑖 and 𝑗.
(ii)(iv). From (2.16), we have 𝑖(𝑋,𝑌)=𝑔(𝐴𝜉𝑖𝑋,𝑌)𝑗(𝑋,𝜉𝑖)=0 for any 𝑋,𝑌Γ(𝑇𝑀) and for all 𝑖 and 𝑗.

Corollary 2.3. Let (𝑀,𝑔,𝑆(𝑇𝑀),𝑆(𝑇𝑀)) be a 1-lightlike submanifold of a semi-Riemannian manifold (𝑀,̃𝑔), then the operators 𝐴𝜉𝑖 are self-adjoint on Γ(𝑇𝑀) with respect to 𝑔.

Definition 2.4. An 𝑟-lightlike submanifold (𝑀,𝑔,𝑆(𝑇𝑀),𝑆(𝑇𝑀)) of a semi-Riemannian manifold (𝑀,̃𝑔) is said to be irrotational if 𝑋𝜉𝑖Γ(𝑇𝑀) for any 𝑋Γ(𝑇𝑀) and 𝑖.

For an 𝑟-lightlike submanifold 𝑀 of 𝑀, the above definition is equivalent to 𝑗(𝑋,𝜉𝑖)=0 and 𝑠𝛼(𝑋,𝜉𝑖)=0 for any 𝑋Γ(𝑇𝑀). In this case, 𝐴𝜉𝑖 are self-adjoint on Γ(𝑇𝑀) with respect to 𝑔, for all 𝑖.

We need the following Gauss-Codazzi equations (for a full set of these equations see [1, chapter 5]) for M and 𝑆(𝑇𝑀). Denote by 𝑅,𝑅, and 𝑅 the curvature tensors of the Levi-Civita connection of 𝑀, the induced connection of 𝑀, and the induced connection on 𝑆(𝑇𝑀), respectively:+̃𝑔𝑅(𝑋,𝑌)𝑍,𝑃𝑊=𝑔(𝑅(𝑋,𝑌)𝑍,𝑃𝑊)𝑟𝑖=1𝑖(𝑋,𝑍)𝑖(𝑌,𝑃𝑊)𝑖(𝑌,𝑍)𝑖(+𝑋,𝑃𝑊)𝑛𝛼=𝑟+1𝜖𝛼𝑠𝛼(𝑋,𝑍)𝑠𝛼(𝑌,𝑃𝑊)𝑠𝛼(𝑌,𝑍)𝑠𝛼,𝜖(𝑋,𝑃𝑊)(2.25)𝛼̃𝑔𝑅(𝑋,𝑌)𝑍,𝑊𝛼=𝑋𝑠𝛼(𝑌,𝑍)𝑌𝑠𝛼+(𝑋,𝑍)𝑟𝑖=1𝑖(𝑌,𝑍)𝜌𝑖𝛼(𝑋)𝑖(𝑋,𝑍)𝜌𝑖𝛼+(𝑌)𝑛𝛽=𝑟+1𝑠𝛽(𝑌,𝑍)𝜃𝛽𝛼(𝑋)𝑠𝛽(𝑋,𝑍)𝜃𝛽𝛼,(𝑌)(2.26)̃𝑔𝑅(𝑋,𝑌)𝑍,𝑁𝑖=̃𝑔𝑅(𝑋,𝑌)𝑍,𝑁𝑖+𝑟𝑗=1𝑗(𝑋,𝑍)𝜂𝑖𝐴𝑁𝑗𝑌𝑗(𝑌,𝑍)𝜂𝑖𝐴𝑁𝑗𝑋+𝑛𝛼=𝑟+1𝜖𝛼𝑠𝛼(𝑋,𝑍)𝜌𝑖𝛼(𝑌)𝑠𝛼(𝑌,𝑍)𝜌𝑖𝛼,(𝑋)(2.27)̃𝑔𝑅(𝑋,𝑌)𝜉𝑖,𝑁𝑗=̃𝑔𝑅(𝑋,𝑌)𝜉𝑖,𝑁𝑗+𝑟𝑘=1𝑘𝑋,𝜉𝑖𝜂𝑗𝐴𝑁𝑘𝑌𝑘𝑌,𝜉𝑖𝜂𝑗𝐴𝑁𝑘𝑋+𝑛𝛼=𝑟+1𝜌𝑗𝛼(𝑋)𝜙𝛼𝑖(𝑌)𝜌𝑗𝛼(𝑌)𝜙𝛼𝑖𝐴(𝑋)=𝑔𝜉𝑖𝑋,𝐴𝑁𝑗𝑌𝐴𝑔𝜉𝑖𝑌,𝐴𝑁𝑗𝑋2𝑑𝜏𝑗𝑖+(𝑋,𝑌)𝑟𝑘=1𝑘𝑋,𝜉𝑖𝜂𝑗𝐴𝑁𝑘𝑌𝑘𝑌,𝜉𝑖𝜂𝑗𝐴𝑁𝑘𝑋+𝑟𝑘=1𝜏𝑗𝑘(𝑋)𝜏𝑘𝑖(𝑌)𝜏𝑗𝑘(𝑌)𝜏𝑘𝑖+(𝑋)𝑛𝛼=𝑟+1𝜌𝑗𝛼(𝑋)𝜙𝛼𝑖(𝑌)𝜌𝑗𝛼(𝑌)𝜙𝛼𝑖(,𝑅𝑋)(2.28)̃𝑔(𝑅(𝑋,𝑌)𝑃𝑍,𝑃𝑊)=𝑔+(𝑋,𝑌)𝑃𝑍,𝑃𝑊𝑟𝑖=1𝑖(𝑋,𝑃𝑍)𝑖(𝑌,𝑃𝑊)𝑖(𝑌,𝑃𝑍)𝑖,𝑔(𝑋,𝑃𝑊)(2.29)𝑅(𝑋,𝑌)𝑃𝑍,𝑁𝑖=𝑋𝑖(𝑌,𝑃𝑍)𝑌𝑖+(𝑋,𝑃𝑍)𝑟𝑗=1𝑗(𝑋,𝑃𝑍)𝜏𝑖𝑗(𝑌)𝑗(𝑌,𝑃𝑍)𝜏𝑖𝑗.(𝑋)(2.30)

The Ricci tensor of 𝑀 is given by𝑇𝑀Ric(𝑋,𝑌)=trace𝑍𝑅(𝑍,𝑋)𝑌,𝑋,𝑌Γ,(2.31) for any 𝑋,𝑌Γ(𝑇𝑀). Let 𝑀dim = 𝑚+𝑛. Locally, Ric is given byRic(𝑋,𝑌)=𝑚+𝑛𝑖=1𝜖𝑖𝑅𝐸̃𝑔𝑖,𝑋𝑌,𝐸𝑖,(2.32) where {𝐸1,,𝐸𝑚+𝑛} is an orthonormal frame field of 𝑇𝑀. If dim(𝑀)>2 andRic=𝜅̃𝑔,𝜅isaconstant,(2.33) then 𝑀 is an Einstein manifold. If dim(𝑀)=2, any 𝑀 is Einstein, but 𝜅 in (2.33) is not necessarily constant. The scalar curvature ̃𝑟 is defined bỹ𝑟=𝑚+𝑛𝑖=1𝜖𝑖𝐸Ric𝑖,𝐸𝑖.(2.34) Putting (2.33) in (2.34) implies that 𝑀 is Einstein if and only ifRic=̃𝑟𝑚+𝑛̃𝑔.(2.35)

3. The Tangential Curvature Vector Field

Let 𝑅(0,2) denote the induced Ricci tensor of type (0,2) on 𝑀, given by𝑅(0,2)𝑇𝑀(𝑋,𝑌)=trace{𝑍𝑅(𝑍,𝑋)𝑌},𝑋,𝑌Γ.(3.1) Consider an induced quasiorthonormal frame field𝜉1,,𝜉𝑟;𝑁1,,𝑁𝑟;𝑋𝑟+1,,𝑋𝑚;𝑊𝑟+1,,𝑊𝑛,(3.2)

where {𝑁𝑖,𝑊𝛼} is a basis of Γ(tr(𝑇𝑀)|𝒰) on a coordinate neighborhood 𝒰 of 𝑀 such that 𝑁𝑖Γ(ltr(𝑇𝑀)|𝒰) and 𝑊𝛼Γ(𝑆(𝑇𝑀)|𝒰). By using (2.29) and (3.1), we obtain the following local expression for the Ricci tensor:Ric(𝑋,𝑌)=𝑛𝑎=𝑟+1𝜖𝑎𝑅𝑊̃𝑔𝑎,𝑋𝑌,𝑊𝑎+𝑟𝑖=1𝑅𝜉̃𝑔𝑖,𝑋𝑌,𝑁𝑖+𝑚𝑏=𝑟+1𝜖𝑏𝑅𝑋̃𝑔𝑏,𝑋𝑌,𝑋𝑏+𝑟𝑖=1𝑅𝑁̃𝑔𝑖,𝑋𝑌,𝜉𝑖,𝑅(3.3)(0,2)(𝑋,𝑌)=𝑚𝑎=𝑟+1𝜖𝑎𝑔𝑅𝑋𝑎,𝑋𝑌,𝑋𝑎+𝑟𝑖=1𝑅𝜉̃𝑔𝑖,𝑋𝑌,𝑁𝑖.(3.4) Substituting (2.25) and (2.27) in (3.3) and using (2.15)~(2.18) and (3.4), we obtain𝑅(0,2)(𝑋,𝑌)=Ric(𝑋,𝑌)+𝑟𝑖=1𝑖(𝑋,𝑌)tr𝐴𝑁𝑖+𝑛𝛼=𝑟+1𝑠𝛼(𝑋,𝑌)tr𝐴𝑊𝛼𝑟𝑖=1𝑔𝐴𝑁𝑖𝑋,𝐴𝜉𝑖𝑌𝑛𝛼=𝑟+1𝜖𝛼𝑔𝐴𝑊𝛼𝑋,𝐴𝑊𝛼𝑌𝑟𝑖,𝑗=1𝑗𝜉𝑖𝜂,𝑌𝑖𝐴𝑁𝑗𝑋+𝑟𝑛𝑖=1𝛼=𝑟+1𝜌𝑖𝛼(𝑋)𝜙𝛼𝑖(𝑌)𝑛𝛼=𝑟+1𝜖𝛼𝑅𝑊̃𝑔𝛼,𝑋𝑌,𝑊𝛼𝑟𝑖=1𝑅𝜉̃𝑔𝑖,𝑌𝑋,𝑁𝑖,(3.5)

for any 𝑋, 𝑌Γ(𝑇𝑀). This shows that 𝑅(0,2) is not symmetric. A tensor field 𝑅(0,2) of 𝑀, given by (3.1), is called its induced Ricci tensor if it is symmetric. From now and in the sequel, a symmetric 𝑅(0,2) tensor will be denoted by Ric.

Using (2.28), (3.5), and the first Bianchi identity, we obtain𝑅(0,2)(𝑋,𝑌)𝑅(0,2)(𝑌,𝑋)=𝑟𝑖=1𝑔𝐴𝜉𝑖𝑋,𝐴𝑁𝑖𝑌𝐴𝑔𝜉𝑖𝑌,𝐴𝑁𝑖𝑋s+𝑟𝑖,𝑗=1𝑗𝑋,𝜉𝑖𝜂𝑖𝐴𝑁𝑗𝑌𝑗𝑌,𝜉𝑖𝜂𝑖𝐴𝑁𝑗𝑌+𝑟𝑛𝑖=1𝛼=𝑟+1𝜌𝑖𝛼(𝑋)𝜙𝛼𝑖(𝑌)𝜌𝑖𝛼(𝑌)𝜙𝛼𝑖(𝑋)𝑟𝑖=1̃𝑔𝑅(𝑋,𝑌)𝜉𝑖,𝑁𝑖.(3.6)

From this equation and (2.28), we have𝑅(0,2)(𝑋,𝑌)𝑅(0,2)𝜏(𝑌,𝑋)=2𝑑tr𝑖𝑗(𝑋,𝑌).(3.7)

Theorem 3.1 (see[5]). Let 𝑀 be a lightlike submanifold of a semi-Riemannian manifold (𝑀,̃𝑔), then the tensor field 𝑅(0,2) is a symmetric Ricci tensor Ric if and only if each 1-form tr(𝜏𝑖𝑗) is closed, that is, 𝑑(tr(𝜏𝑖𝑗))=0, on any 𝒰𝑀.

Note 1. Suppose that the tensor 𝑅(0,2) is symmetric Ricci tensor Ric, then the 1-form tr(𝜏𝑖𝑗) is closed by Theorem 3.1. Thus, there exist a smooth function 𝑓 on 𝒰 such that tr(𝜏𝑖𝑗)=df. Consequently, we get tr(𝜏𝑖𝑗)(𝑋)=𝑋(𝑓). If we take ̃𝜉𝑖=𝑟𝑗=1𝛼𝑖𝑗𝜉𝑗, it follows that tr(𝜏𝑖𝑗)(𝑋)=tr(̃𝜏𝑖𝑗)(𝑋)+𝑋(lnΔ). Setting Δ=exp(𝑓) in this equation, we get tr(̃𝜏𝑖𝑗)(𝑋)=0 for any 𝑋Γ(𝑇𝑀|𝒰). We call the pair {𝜉𝑖,𝑁𝑖}𝑖 on 𝒰 such that the corresponding 1-form tr(𝜏𝑖𝑗) vanishes the canonical null pair of 𝑀.

For the rest of this paper, let 𝑀 be a lightlike submanifold of a semi-Riemannian manifold 𝑀 of quasiconstant curvature. We may assume that the curvature vector field 𝜁 of 𝑀 is a unit spacelike tangent vector field of 𝑀 and 𝑀dim>4,𝑅𝜉Ric(𝑋,𝑌)={(𝑛+𝑚1)𝛼+𝛽}𝑔(𝑋,𝑌)+(𝑛+𝑚2)𝛽𝜃(𝑋)𝜃(𝑌),(3.8)̃𝑔𝑖,𝑌𝑋,𝑁𝑖𝜖=𝛼𝑔(𝑋,𝑌)+𝛽𝜃(𝑋)𝜃(𝑌),(3.9)𝛼𝑅𝑊̃𝑔𝛼,𝑌𝑋,𝑊𝛼=𝛼𝑔(𝑋,𝑌)+𝛽𝜃(𝑋)𝜃(𝑌),(3.10) for all 𝑋,𝑌Γ(𝑇𝑀). Substituting (3.8)~(3.10) into (3.5), we have𝑅(0,2)+(𝑋,𝑌)={(𝑚1)𝛼+𝛽}𝑔(𝑋,𝑌)+(𝑚2)𝛽𝜃(𝑋)𝜃(𝑌)𝑟𝑖=1𝑖(𝑋,𝑌)tr𝐴𝑁𝑖+𝑛𝛼=𝑟+1𝑠𝛼(𝑋,𝑌)tr𝐴𝑊𝛼𝑟𝑖=1𝑔𝐴𝑁𝑖𝑋,𝐴𝜉𝑖𝑌𝑛𝛼=𝑟+1𝜖𝛼𝑔𝐴𝑊𝛼𝑋,𝐴𝑊𝛼𝑌𝑟𝑖,𝑗=1𝑗𝜉𝑖𝜂,𝑌𝑖𝐴𝑁𝑗𝑋+𝑟𝑛𝑖=1𝛼=𝑟+1𝜌𝑖𝛼(𝑋)𝜙𝛼𝑖(𝑌).(3.11)

Definition 3.2. We say that the screen distribution 𝑆(𝑇𝑀) of 𝑀 is totally umbilical [1] in 𝑀 if, on any coordinate neighborhood 𝒰𝑀, there is a smooth function 𝛾𝑖 such that 𝐴𝑁𝑖𝑋=𝛾𝑖𝑃X for any 𝑋Γ(𝑇𝑀), or equivalently,

𝑖(𝑋,𝑃𝑌)=𝛾𝑖𝑔(𝑋,𝑌),𝑋,𝑌Γ(𝑇𝑀).(3.12) In case 𝛾𝑖=0 on 𝒰, we say that 𝑆(𝑇𝑀) is totally geodesic in 𝑀.

A vector field 𝑋 on 𝑀 is said to be a conformal Killing vector field [6] if 𝑋̃𝑔=2𝛿̃𝑔 for any smooth function 𝛿, where 𝑋 denotes the Lie derivative with respect to 𝑋, that is,𝑋[][]𝑇𝑀̃𝑔(𝑌,𝑍)=𝑋(̃𝑔(𝑌,𝑍))̃𝑔(𝑋,𝑌,𝑍)̃𝑔(𝑌,𝑋,𝑍),𝑋,𝑌,𝑍Γ.(3.13)

In particular, if 𝛿=0, then 𝑋 is called a Killing vector field [7]. A distribution 𝒢 on 𝑀 is called a conformal Killing (resp., Killing) distribution on 𝑀 if each vector field belonging to 𝒢 is a conformal Killing (resp., Killing) vector field on 𝑀. If the coscreen distribution 𝑆(𝑇𝑀) is a Killing distribution, using (2.10) and (2.17), we havẽ𝑔𝑋𝑊𝛼𝐴,𝑌=𝑔𝑊𝛼+𝑋,𝑌𝑟𝑖=1𝜙𝛼𝑖(𝑋)𝜂𝑖(𝑌)=𝜖𝛼𝑠𝛼(𝑋,𝑌).(3.14)

Therefore, since 𝑠𝛼 are symmetric, we obtain𝑊𝛼̃𝑔(𝑌,𝑍)=2𝜖𝛼𝑠𝛼(𝑋,𝑌).(3.15)

Theorem 3.3. Let 𝑀 be an 𝑟-lightlike submanifold of a semi-Riemannian manifold (𝑀,̃𝑔), then the coscreen distribution 𝑆(𝑇𝑀) is a conformal Killing (resp., Killing) distribution if and only if there exists a smooth function 𝛿𝛼 such that 𝑠𝛼(𝑋,𝑌)=𝜖𝛼𝛿𝛼𝑔(𝑋,𝑌),resp.𝑠𝛼(𝑋,𝑌)=0,𝑋,𝑌Γ(𝑇𝑀).(3.16)

Theorem 3.4. Let 𝑀 be an irrotational 𝑟-lightlike submanifold of a semi-Riemannian manifold (𝑀,̃𝑔) of quasiconstant curvature. If the curvature vector field 𝜁 of 𝑀 is tangent to 𝑀, 𝑆(𝑇𝑀) is totally umbilical in 𝑀, and 𝑆(𝑇𝑀) is a conformal Killing distribution, then the tensor field 𝑅(0,2) is an induced symmetric Ricci tensor of 𝑀.

Proof. From (2.17)~(2.20), (2.22), (3.16), and (3.11), we have 𝑠𝛼(𝑋,𝑌)=𝜖𝛼𝛿𝛼𝑔(𝑋,𝑌),𝜙𝛼𝑖(𝑋)=0,𝐴𝑊𝛼𝑋=𝛿𝛼𝑃𝑋+𝑟𝑖=1𝜖𝛼𝜌𝑖𝛼(𝑋)𝜉𝑖,(3.17)𝑅(0,2)(𝑋,𝑌)=(𝑚1)𝛼+𝛽+(𝑚𝑟1)𝑛𝛼=𝑟+1𝜖𝛼𝛿2𝛼+𝑛𝑟𝛼=𝑟+1𝑖=1𝛿𝛼𝜌𝑖𝛼𝜉𝑖𝑔(𝑋,𝑌)+(𝑚2)𝛽𝜃(𝑋)𝜃(𝑌)+(𝑚𝑟1)𝑟𝑖=1𝛾𝑖𝑔𝐴𝜉𝑖𝑋,𝑌,𝑋,𝑌Γ(𝑇𝑀).(3.18) Using (3.17), we show that 𝑅(0,2) is symmetric.

4. Proof of Theorem 1.1

As 𝑖=0, we get ̃𝑔(𝑅(𝑋,𝑌)𝑃𝑍,𝑁𝑖)=0 by (2.30). From (2.27) and (3.16), we havẽ𝑔𝑅(𝑋,𝑌)𝑃𝑍,𝑁𝑖=𝑛𝛼=𝑟+1𝛿𝛼𝑔(𝑋,𝑃𝑍)𝜌𝑖𝛼(𝑌)𝑔(𝑌,𝑃𝑍)𝜌𝑖𝛼.(𝑋)(4.1)

By Theorems 3.1 and 3.4, we get 𝑑𝜏=0 on 𝑇𝑀. Thus, we have ̃𝑔(𝑅(𝑋,𝑌)𝜉𝑖,𝑁𝑖)=0 due to (2.28). From the above results, we deduce the following equation:̃𝑔𝑅(𝑋,𝑌)𝑍,𝑁𝑖=𝑛𝛼=𝑟+1𝛿𝛼𝑔(𝑋,𝑃𝑍)𝜌𝑖𝛼(𝑌)𝑔(𝑌,𝑃𝑍)𝜌𝑖𝛼.(𝑋)(4.2) Taking 𝑋=𝜉𝑖 and 𝑍=𝑋 to (4.2) and then comparing with (3.9), we have𝛽𝜃(𝑋)𝜃(𝑌)=𝛼+𝑛𝛼=𝑟+1𝛿𝛼𝜌𝑖𝛼𝜉𝑖𝑔(𝑋,𝑌),𝑋,𝑌Γ(𝑇𝑀).(4.3)

Case 1. If 𝑆(𝑇M) is a Killing distribution, that is, 𝛿𝛼=0, then we have 𝛽𝜃(𝑋)𝜃(𝑌)=𝛼𝑔(𝑋,𝑌),𝑋,𝑌Γ(𝑇𝑀).(4.4) Substituting (4.3) into (1.1) and using (2.25) and the facts ̃𝑔(𝑅(𝑋,𝑌)𝑍,𝜉𝑖)=0 and ̃𝑔(𝑅(𝑋,𝑌)𝑍,𝑁𝑖)=0 due to (1.1), we have 𝑅(𝑋,𝑌)𝑍=𝛼{𝑔(𝑌,𝑍)𝑋𝑔(𝑋,𝑍)𝑌},𝑋,𝑌,𝑍Γ(𝑇𝑀).(4.5) Thus, 𝑀 is a space of constant curvature 𝛼. Taking 𝑋=𝑌=𝜁 to (4.3), we have 𝛽=𝛼. Substituting (4.3) into (3.18) with 𝛿𝛼=𝛾𝑖=0, we have Ric(𝑋,𝑌)=0,𝑋,𝑌Γ(𝑇𝑀).(4.6) On the other hand, substituting (4.5) and 𝑔(𝑅(𝜉𝑖,𝑌)𝑋,𝑁𝑖)=0 into (3.4), we have Ric(𝑋,𝑌)=(𝑚1)𝛼𝑔(𝑋,𝑌),𝑋,𝑌Γ(𝑇𝑀).(4.7) From the last two equations, we get 𝛼=0 as 𝑚>1. Thus, 𝛽=0, and 𝑀 and 𝑀 are flat manifolds by (1.1) and (4.5). From this result and (2.29), we show that 𝑀 is also flat.

Case 2. If 𝑆(𝑇𝑀) is a conformal Killing distribution, assume that 𝛽0. Taking 𝑋=𝑌=𝜁 to (4.3), we have 𝛽={𝛼+𝑛𝛼=𝑟+1𝛿𝛼𝜌𝑖𝛼(𝜉𝑖)}. From this and (4.3), we show that 𝑔(𝑋,𝑌)=𝜃(𝑋)𝜃(𝑌),𝑋,𝑌Γ(𝑇𝑀).(4.8) Substituting (4.8) into (1.1) and using (2.25) with 𝑖=0 and (3.16), we have 𝑔(𝑅(𝑋,𝑌)𝑍,𝑊)=𝛼+2𝛽+𝑛𝛼=𝑟+1𝜖𝛼𝛿2𝛼{𝑔(𝑌,𝑍)𝑔(𝑋,𝑊)𝑔(𝑋,𝑍)𝑔(𝑌,𝑊)},(4.9) for all 𝑋,𝑌,𝑍,𝑊Γ(𝑇𝑀). Substituting (4.8) into (3.18) with 𝛾𝑖=0, we have Ric(𝑋,𝑌)=(𝑚𝑟1)𝛼+𝛽+𝑛𝛼=𝑟+1𝜖𝛼𝛿2𝛼𝑔(𝑋,𝑌),𝑋,𝑌Γ(𝑇𝑀),(4.10) by the fact that 𝑛𝛼=𝑟+1𝛿𝛼𝜌𝑖𝛼(𝜉𝑖)=(𝛼+𝛽). On the other hand, from (2.27), (3.9), and (4.3), we have 𝑔(𝑅(𝜉𝑖,𝑌)𝑋,𝑁𝑖)=0. Substituting this result and (4.9) into (3.4), we have Ric(𝑋,𝑌)=(𝑚𝑟1)𝛼+2𝛽+𝑛𝛼=𝑟+1𝜖𝛼𝛿2𝛼𝑔(𝑋,𝑌),𝑋,𝑌Γ(𝑇𝑀).(4.11) The last two equations imply 𝛽=0 as 𝑚𝑟>1. It is a contradiction. Thus, 𝛽=0 and 𝑀 is a space of constant curvature 𝛼. From (2.29) and (4.9), we show that 𝑀 is a space of constant curvature (𝛼+𝑛𝛼=𝑟+1𝜖𝛼𝛿2𝛼). But 𝑀 is not a space of constant curvature by (3.17)3. Let 𝜅=(𝑚𝑟1)(𝛼+𝑛𝛼=𝑟+1𝜖𝛼𝛿2𝛼), then the last two equations reduce to 𝑅(0,2)(𝑋,𝑌)=Ric(𝑋,𝑌)=𝜅𝑔(𝑋,𝑌),𝑋,𝑌Γ(𝑇𝑀).(4.12) Thus 𝑀 is an Einstein manifold. The scalar quantity 𝑟 of 𝑀 [8], obtained from 𝑅(0,2) by the method of (2.34), is given by 𝑟=𝑟𝑖=1𝑅(0,2)𝜉𝑖,𝜉𝑖+𝑚𝑎=𝑟+1𝜖𝑎𝑅(0,2)𝑋𝑎,𝑋𝑎.(4.13) Since 𝑀 is an Einstein manifold satisfying (4.12), we obtain 𝑟=𝜅𝑟𝑖=1𝑔𝜉𝑖,𝜉𝑖+𝜅𝑚𝑎=𝑟+1𝜖𝑎𝑔𝑋𝑎,𝑋𝑎=𝜅(𝑚𝑟).(4.14) Thus, we have 𝑟Ric(𝑋,𝑌)=𝑚𝑟𝑔(𝑋,𝑌),(4.15) which provides a geometric interpretation of half lightlike Einstein submanifold (the same as in Riemannian case) as we have shown that the constant 𝜅=𝑟/(𝑚𝑟).

5. Proof of Theorem 1.2

Assume that 𝜁 is tangent to 𝑀, 𝑆(𝑇𝑀) is totally umbilical, and 𝑆(𝑇𝑀) is a conformal Killing vector field. Using (1.1), (2.26) reduces to𝑋𝑠𝛼(𝑌,𝑍)𝑌𝑠𝛼(𝑋,𝑍)=𝑟𝑖=1𝑖(𝑋,𝑍)𝜌𝑖𝛼(𝑌)𝑖(𝑌,𝑍)𝜌𝑖𝛼+(𝑋)𝑛𝛽=𝑟+1𝑠𝛽(𝑋,𝑍)𝜃𝛽𝛼(𝑌)𝑠𝛽(𝑌,𝑍)𝜃𝛽𝛼,(𝑋)(5.1)

for all 𝑋,𝑌,𝑍Γ(𝑇𝑀). Replacing 𝑊 by 𝑁 to (1.1), we havẽ𝑔𝑅(𝑋,𝑌)𝑍,𝑁𝑖=𝛼𝜂𝑖(𝑋)+𝑒𝑖𝛽𝜃(𝑋)𝑔(𝑌,𝑍)𝛼𝜂𝑖(𝑌)+𝑒𝑖𝛽𝜃(𝑌)𝑔(𝑋,𝑍)+𝛽𝜃(𝑌)𝜂𝑖(𝑋)𝜃(𝑋)𝜂𝑖(𝑌)𝜃(𝑍),(5.2)

for all 𝑋,𝑌,𝑍Γ(𝑇𝑀) and where 𝑒𝑖=𝜃(𝑁𝑖). Applying 𝑋 to (3.12) and using (2.13), we have𝑋𝑖𝑋𝛾(𝑌,𝑃𝑍)=𝑖𝑔(𝑌,𝑃𝑍)+𝛾𝑖𝑟𝑗=1𝑗(𝑋,𝑃𝑍)𝜂𝑗(𝑌),(5.3)

for all 𝑋,𝑌,𝑍Γ(𝑇𝑀). Substituting this equation into (2.30), we obtaiñ𝑔𝑅(𝑋,𝑌)𝑃𝑍,𝑁𝑖=𝑋𝛾𝑖𝑟𝑗=1𝛾𝑗𝜏𝑖𝑗𝑌𝛾(𝑋)𝑔(𝑌,𝑃𝑍)𝑖𝑟𝑗=1𝛾𝑗𝜏𝑖𝑗(𝑌)𝑔(𝑋,𝑃𝑍)+𝛾𝑖𝑟𝑗=1𝑗(𝑋,𝑃𝑍)𝜂𝑗(𝑌)𝛾𝑖𝑟𝑗=1𝑗(𝑌,𝑃𝑍)𝜂𝑗(𝑋),𝑋,𝑌,𝑍Γ(𝑇𝑀).(5.4)

Substituting this equation and (5.2) into (2.27) and using 𝜃(𝜉𝑖)=0, we obtain𝑋𝛾𝑖𝑟𝑗=1𝛾𝑗𝜏𝑖𝑗(𝑋)𝛼𝜂𝑖(𝑋)𝑒𝑖𝛽𝜃(𝑋)𝑛𝛼=𝑟+1𝛿𝛼𝜌𝑖𝛼𝑌𝛾(𝑋)𝑔(𝑌,𝑍)𝑖𝑟𝑗=1𝛾𝑗𝜏𝑖𝑗(𝑌)𝛼𝜂𝑖(𝑌)𝑒𝑖𝛽𝜃(𝑌)𝑛𝛼=𝑟+1𝛿𝛼𝜌𝑖𝛼(𝑌)𝑔(𝑋,𝑍)=𝛾𝑖𝑟𝑗=1𝑗(𝑌,𝑃𝑍)𝜂𝑗(𝑋)𝑟𝑗=1𝑗(𝑋,𝑃𝑍)𝜂𝑗(𝑌)+𝛽𝜃(𝑌)𝜂𝑖(𝑋)𝜃(𝑋)𝜂𝑖(𝑌)𝜃(𝑍),𝑋,𝑌,𝑍Γ(𝑇𝑀).(5.5)

Replacing 𝑌 by 𝜉𝑖 to this and using (2.20)1 and the fact 𝜃(𝜉𝑖)=0, we have𝛾𝑖𝑖𝜉(𝑋,𝑌)=𝑖𝛾𝑖𝑟𝑗=1𝛾𝑗𝜏𝑖𝑗𝜉𝑖𝛼𝑛𝛼=𝑟+1𝛿𝛼𝜌𝑖𝛼𝜉𝑖𝑔(𝑋,𝑌)𝛽𝜃(𝑋)𝜃(𝑌),(5.6)for all 𝑋,𝑌Γ(𝑇𝑀). Differentiating (3.16) and using (5.1), we have𝑟𝑖=1𝛿𝛼𝜂𝑖(𝑋)𝜖𝛼𝜌𝑖𝛼(𝑋)𝑖(𝑌,𝑍)𝑟𝑖=1𝛿𝛼𝜂𝑖(𝑌)𝜖𝛼𝜌𝑖𝛼(𝑌)𝑖=𝑋𝛿(𝑋,𝑍)𝛼+𝜖𝛼𝑛𝛽=𝑟+1𝜖𝛽𝛿𝛽𝜃𝛽𝛼𝑌𝛿(𝑋)𝑔(𝑌,𝑍)𝛼+𝜖𝛼𝑛𝛽=𝑟+1𝜖𝛽𝛿𝛽𝜃𝛽𝛼(𝑌)𝑔(𝑋,𝑍).(5.7)

Replacing 𝑌 by 𝜉𝑖 in the last equation and using (2.20)1, we obtain𝛿𝛼𝜖𝛼𝜌𝑖𝛼𝜉𝑖𝑖𝜉(𝑋,𝑍)=𝑖𝛿𝛼+𝜖𝛼𝑛𝛽=𝑟+1𝜖𝛽𝛿𝛽𝜃𝛽𝛼𝜉𝑖𝑔(𝑋,𝑍).(5.8)

As the conformal factor 𝛿𝛼 is nonconstant, we show that 𝛿𝛼𝜖𝛼𝜌𝑖𝛼(𝜉𝑖)0. Thus, we have𝑖(𝑋,𝑌)=𝜎𝑖𝑔(𝑋,𝑌),𝑋,𝑌Γ(𝑇𝑀),(5.9) where 𝜎𝑖={𝜉𝑖[𝛿𝛼]+𝜖𝛼𝑛𝛽=𝑟+1𝜖𝛽𝛿𝛽𝜃𝛽𝛼(𝜉𝑖)}(𝛿𝛼𝜖𝛼𝜌𝑖𝛼(𝜉𝑖))1. From (3.17)1 and (5.9), we show that the second fundamental form tensor , given by (𝑋,𝑌)=𝑟𝑖=1𝑖(𝑋,𝑌)𝑁𝑖+𝑛𝛼=𝑟+1𝑠𝛼(𝑋,𝑌)𝑊𝛼, satisfies(𝑋,𝑌)=𝑔(𝑋,𝑌),𝑋,𝑌Γ(𝑇𝑀).(5.10)

Thus, 𝑀 is totally umbilical [5]. Substituting (5.9) into (5.6), we have𝜉𝑖𝛾𝑖𝑟𝑗=1𝛾𝑗𝜏𝑖𝑗𝜉𝑖𝛾𝑖𝜎𝑖𝛼𝑛𝛼=𝑟+1𝛿𝛼𝜌𝑖𝛼𝜉𝑖𝑔(𝑋,𝑌)=𝛽𝜃(𝑋)𝜃(𝑌),(5.11)

for all 𝑋,𝑌Γ(𝑇𝑀). Taking 𝑋=𝑌=𝜁 to this equation, we have𝛽=𝜉𝑖𝛾𝑖𝑟𝑗=1𝛾𝑗𝜏𝑖𝑗𝜉𝑖𝛾𝑖𝜎𝑖𝛼𝑛𝛼=𝑟+1𝛿𝛼𝜌𝑖𝛼𝜉𝑖.(5.12)

Assume that 𝛽0, then we have𝑔(𝑋,𝑌)=𝜃(𝑋)𝜃(𝑌),𝑋,𝑌Γ(𝑇𝑀).(5.13) Substituting (5.13) into (1.1) and using (2.25), (3.12), (3.17)1, and (5.9), we have=𝑔(𝑅(𝑋,𝑌)𝑍,𝑊)𝛼+2𝛽+𝑟𝑖=1𝜎𝑖𝛾𝑖+𝑛𝛼=𝑟+1𝜖𝛼𝛿2𝛼{𝑔(𝑌,𝑍)𝑔(𝑋,𝑊)𝑔(𝑋,𝑍)𝑔(𝑌,𝑊)},(5.14) for all 𝑋,𝑌,𝑍,𝑊Γ(𝑇𝑀). Substituting (5.9) and (5.13) into (3.18), we haveRic(𝑋,𝑌)=(𝑚1)(𝛼+𝛽)+(𝑚𝑟1)𝑟𝑖=1𝜎𝑖𝛾𝑖+𝑛𝛼=𝑟+1𝜖𝛼𝛿2𝛼+𝑛𝑟𝛼=𝑟+1𝑖=1𝛿𝛼𝜌𝑖𝛼𝜉𝑖𝑔(𝑋,𝑌).(5.15) On the other hand, substituting (5.14) and the fact that𝑅𝜉̃𝑔𝑖,𝑌𝑋,𝑁𝑖=𝛼+𝛽+𝑛𝛼=𝑟+1𝜖𝛼𝛿𝛼𝜌𝑖𝛼𝜉𝑖𝑔(𝑋,𝑌)(5.16)

into (3.4), we haveRic(𝑋,𝑌)=(𝑚1)𝛼+2(𝑚1)𝛽+(𝑚𝑟1)𝑟𝑖=1𝜎𝑖𝛾𝑖+𝑛𝛼=𝑟+1𝜖𝛼𝛿2𝛼+𝑛𝑟𝛼=𝑟+1𝑖=1𝛿𝛼𝜌𝑖𝛼𝜉𝑖𝑔(𝑋,𝑌).(5.17) Comparing (5.15) and (5.17), we obtain (𝑚1)𝛽=0. As 𝑚>1, we have 𝛽=0, which is a contradiction. Thus, we have 𝛽=0. Consequently, by (1.1), (2.29), and (5.14), we show that 𝑀 and 𝑀 are spaces of constant curvatures 𝛼 and (𝛼+2𝑟𝑖=1𝜎𝑖𝛾𝑖+𝑛𝛼=𝑟+1𝜖𝛼𝛿2𝛼), respectively. Let𝜅=(𝑚1)𝛼+(𝑚𝑟1)𝑟𝑖=1𝜎𝑖𝛾𝑖+𝑛𝛼=𝑟+1𝜖𝛼𝛿2𝛼+𝑛𝑟𝛼=𝑟+1𝑖=1𝛿𝛼𝜌𝑖𝛼𝜉𝑖,(5.18)

then (5.15) and (5.17) reduce to𝑅(0,2)(𝑋,𝑌)=Ric(𝑋,𝑌)=𝜅𝑔(𝑋,𝑌),𝑋,𝑌Γ(𝑇𝑀).(5.19)

Thus, 𝑀 is an Einstein manifold. The scalar quantity 𝑐 of 𝑀 is given by𝑐=𝑟𝑖=1𝑅(0,2)𝜉𝑖,𝜉𝑖+𝑚𝑎=𝑟+1𝜖𝑎𝑅(0,2)𝑋𝑎,𝑋𝑎=𝑟𝑖=1𝜉𝜅𝑔𝑖,𝜉𝑖+𝜅𝑚𝑎=𝑟+1𝜖𝑎𝑔𝑋𝑎,𝑋𝑎=𝜅(𝑚𝑟).(5.20)

Thus, we have𝑐Ric(𝑋,𝑌)=𝑔𝑚𝑟(𝑋,𝑌).(5.21)

Example 5.1. Let (𝑀,𝑔) be a lightlike hypersurface of an indefinite Kenmotsu manifold 𝑀 equipped with a screen distribution 𝑆(𝑇𝑀), then there exist an almost contact metric structure (𝐽,𝜁,𝜗,𝑔) on 𝑀, where 𝐽 is a (1,1)-type tensor field, 𝜁 is a vector field, 𝜗 is a 1-form, and 𝑔 is the semi-Riemannian metric on 𝑀 such that 𝐽2𝑋=𝑋+𝜗(𝑋)𝜁,𝐽𝜁=0,𝜗𝐽=0,𝜗(𝜁)=1,𝜗(𝑋)=𝑔(𝜁,𝑋),𝑔(𝐽𝑋,𝐽𝑌)=𝑔(𝑋,𝑌)𝜗(𝑋)𝜗(𝑌),𝑋𝜁=𝑋+𝜗(𝑋)𝜁,𝑋𝐽𝑌=𝑔(𝐽𝑋,𝑌)𝜁+𝜗(𝑌)𝐽𝑋,(5.22) for any vector fields 𝑋,𝑌 on 𝑀, where is the Levi-Civita connection of 𝑀. Using the local second fundamental forms 𝐵 and 𝐶 of 𝑀 and 𝑆(𝑇𝑀), respectively, and the projection morphism 𝑃 of 𝑀 on 𝑆(𝑇𝑀), the curvature tensors 𝑅,𝑅, and 𝑅 of the connections , , and on 𝑀,𝑀, and 𝑆(𝑇𝑀), respectively, are given by (see [9]) 𝑔𝑅𝑅(𝑋,𝑌)𝑍,𝑃𝑊=𝑔(𝑅(𝑋,𝑌)𝑍,𝑃𝑊)+𝐵(𝑋,𝑍)𝐶(𝑌,𝑃𝑊)𝐵(𝑌,𝑍)𝐶(𝑋,𝑃𝑊),𝑔(𝑅(𝑋,𝑌)𝑃𝑍,𝑃𝑊)=𝑔(𝑋,𝑌)𝑃𝑍,𝑃𝑊+𝐶(𝑋,𝑃𝑍)𝐵(𝑌,𝑃𝑊)𝐶(𝑌,𝑃𝑍)𝐵(𝑋,𝑃𝑊),(5.23) for any 𝑋,𝑌,𝑍,𝑊Γ(𝑇𝑀). In case the ambient manifold 𝑀 is a space form 𝑀(𝑐) of constant 𝐽-holomorphic sectional curvature 𝑐, 𝑅 is given by (see [10]) 𝑅(𝑋,𝑌)𝑍=𝑔(𝑋,𝑍)𝑌𝑔(𝑌,𝑍)𝑋.(5.24) Assume that 𝑀 is almost screen conformal, that is, 𝐶(𝑋,𝑃𝑌)=𝜑𝐵(𝑋,𝑃𝑌)+𝜂(𝑋)𝜗(𝑌),(5.25) where 𝜑 is a nonvanishing function on a neighborhood 𝒰 in 𝑀, and 𝜁 is tangent to 𝑀, then, by the method in Section 2 of [9], we have 𝐵(𝑋,𝑌)=𝜌{𝑔(𝑋,𝑌)𝜗(𝑋)𝜗(𝑌)},(5.26) where 𝜌 is a nonvanishing function on a neighborhood 𝒰. Then the leaf 𝑀 of 𝑆(𝑇𝑀) is a semi-Riemannian manifold of quasiconstant curvature such that 𝛼=1+2𝜑𝜌2, 𝛽=2𝜑𝜌2, and 𝜃=𝜗 in (1.1).

Acknowledgment

The authors are thankful to the referee for making various constructive suggestions and corrections towards improving the final version of this paper.