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Journal of Function Spaces and Applications
VolumeΒ 2012Β (2012), Article IDΒ 636242, 16 pages
doi:10.1155/2012/636242
Research Article

Special Half Lightlike Submanifolds of an Indefinite Cosymplectic Manifold

Department of Mathematics, Dongguk University, Gyeongju 780-714, Republic of Korea

Received 1 May 2012; Revised 17 August 2012; Accepted 25 August 2012

Academic Editor: DashanΒ Fan

Copyright Β© 2012 Dae Ho Jin. 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.

Abstract

We study the geometry of half lightlike submanifolds 𝑀 of an indefinite cosymplectic manifold 𝑀 . First, we construct two types of half lightlike submanifolds according to the form of the structure vector field of 𝑀 , named by tangential and ascreen half lightlike submanifolds. Next, we characterize the lightlike geometries of such two types of half lightlike submanifolds.

1. Introduction

The class of codimension 2 lightlike submanifolds of a semi-Riemannian manifold is composed entirely of two classes by virtue of the rank of its radical distribution, called half lightlike and coisotropic submanifolds [14]. Half lightlike submanifold is a special case of π‘Ÿ -lightlike submanifold [5, 6] such that π‘Ÿ = 1 and its geometry is more general than that of coisotropic submanifold. Moreover much of the works on half lightlike submanifolds will be immediately generalized in a formal way to arbitrary π‘Ÿ -lightlike submanifolds. Recently several authors studied the geometry of lightlike submanifolds of indefinite cosymplectic manifolds. Much of them have studied so-called CR-types (CR, SCR, GCR, QCR, etc) lightlike submanifolds of indefinite cosymplectic manifolds. Unfortunately, an intrinsic study of lightlike submanifolds of indefinite cosymplectic manifolds is slight as yet. Only there are some limited papers on particular subcases recently studied [79].

The objective of this paper is to study the geometry of half lightlike submanifolds 𝑀 of an indefinite cosymplectic manifold 𝑀 . There are many different types of half lightlike submanifolds of an indefinite cosymplectic manifold 𝑀 according to the form of the structure vector field of 𝑀 . We study two types of them here: tangential and ascreen half lightlike submanifolds. We provide several new results on each types by using the structure of 𝑀 induced by the contact metric structure of 𝑀 .

2. Half Lightlike Submanifolds

An odd dimensional smooth manifold ( 𝑀 , 𝑔 ) is called a contact metric manifold if there exists a contact metric structure ( 𝐽 , πœƒ , 𝜁 , 𝑔 ) , where 𝐽 is a ( 1 , 1 ) -type tensor field, 𝜁 a vector field which is called the structure vector field of 𝑀 and πœƒ a 1-form satisfying 𝐽 2 𝑋 = βˆ’ 𝑋 + πœƒ ( 𝑋 ) 𝜁 , 𝐽 𝜁 = 0 , πœƒ ∘ 𝐽 = 0 , πœƒ ( 𝜁 ) = 1 , 𝑔 ( 𝜁 , 𝜁 ) = 1 , 𝑔 ( 𝐽 𝑋 , 𝐽 π‘Œ ) = 𝑔 ( 𝑋 , π‘Œ ) βˆ’ πœƒ ( 𝑋 ) πœƒ ( π‘Œ ) , πœƒ ( 𝑋 ) = 𝑔 ( 𝜁 , 𝑋 ) , 𝑑 πœƒ ( 𝑋 , π‘Œ ) = 𝑔 ( 𝐽 𝑋 , π‘Œ ) , ( 2 . 1 ) for any vector fields 𝑋 , π‘Œ on 𝑀 . We say that 𝑀 has a normal contact structure if 𝑁 𝐽 + 𝑑 πœƒ βŠ— 𝜁 = 0 , where 𝑁 𝐽 is the Nijenhuis tensor field of 𝐽 . A normal contact metric manifold is called a cosymplectic [10, 11] for which we have βˆ‡ 𝑋 πœƒ = 0 , βˆ‡ 𝑋 𝐽 = 0 , ( 2 . 2 ) for any vector field 𝑋 on 𝑀 , where βˆ‡ is the Levi-Civita connection of 𝑀 . A cosymplectic manifold 𝑀 = ( 𝑀 , 𝐽 , 𝜁 , πœƒ , 𝑔 ) is called an indefinite cosymplectic manifold [79] if ( 𝑀 , 𝑔 ) is a semi-Riemannian manifold of index πœ‡ ( > 0 ) .

For any indefinite cosymplectic manifold 𝑀 , applying βˆ‡ 𝑋 to 𝐽 𝜁 = 0 and using (2.2), we have 𝐽 ( βˆ‡ 𝑋 𝜁 ) = 0 . Applying 𝐽 to this and using the fact πœƒ ( βˆ‡ 𝑋 𝜁 ) = 0 , we get βˆ‡ 𝑋 𝜁 = 0 . ( 2 . 3 )

A submanifold 𝑀 of a semi-Riemannian manifold 𝑀 of codimension 2 is called a half lightlike submanifold if the rank of the radical distribution R a d ( 𝑇 𝑀 ) = 𝑇 𝑀 ∩ 𝑇 𝑀 βŸ‚ is 1 , where 𝑇 𝑀 and 𝑇 𝑀 βŸ‚ are the tangent and normal bundles of 𝑀 , respectively. Then there exist complementary nondegenerate distributions 𝑆 ( 𝑇 𝑀 ) and 𝑆 ( 𝑇 𝑀 βŸ‚ ) of R a d ( 𝑇 𝑀 ) in 𝑇 𝑀 and 𝑇 𝑀 βŸ‚ , respectively, which are called the screen and coscreen distribution on 𝑀 : 𝑇 𝑀 = R a d ( 𝑇 𝑀 ) βŠ• o r t h 𝑆 ( 𝑇 𝑀 ) , 𝑇 𝑀 βŸ‚ = R a d ( 𝑇 𝑀 ) βŠ• o r t h 𝑆 ξ€· 𝑇 𝑀 βŸ‚ ξ€Έ , ( 2 . 4 ) where the symbol βŠ• o r t h denotes the orthogonal direct sum. We denote such a half lightlike submanifold by 𝑀 = ( 𝑀 , 𝑔 , 𝑆 ( 𝑇 𝑀 ) ) . Denote by 𝐹 ( 𝑀 ) the algebra of smooth functions on 𝑀 and by Ξ“ ( 𝐸 ) the 𝐹 ( 𝑀 ) module of smooth sections of a vector bundle 𝐸 over 𝑀 . Choose 𝐿 as a unit vector field of 𝑆 ( 𝑇 𝑀 βŸ‚ ) such that 𝑔 ( 𝐿 , 𝐿 ) = Β± 1 . In this paper we may assume that 𝑔 ( 𝐿 , 𝐿 ) = 1 without loss of generality. Consider the orthogonal complementary distribution 𝑆 ( 𝑇 𝑀 ) βŸ‚ to 𝑆 ( 𝑇 𝑀 ) in 𝑇 𝑀 . Certainly R a d ( 𝑇 𝑀 ) and 𝑆 ( 𝑇 𝑀 βŸ‚ ) are vector subbundles of 𝑆 ( 𝑇 𝑀 ) βŸ‚ . Thus we have the following orthogonal decomposition: 𝑆 ( 𝑇 𝑀 ) βŸ‚ ξ€· = 𝑆 𝑇 𝑀 βŸ‚ ξ€Έ βŠ• o r t h 𝑆 ξ€· 𝑇 𝑀 βŸ‚ ξ€Έ βŸ‚ , ( 2 . 5 ) where 𝑆 ( 𝑇 𝑀 βŸ‚ ) βŸ‚ is the orthogonal complementary to 𝑆 ( 𝑇 𝑀 βŸ‚ ) in 𝑆 ( 𝑇 𝑀 ) βŸ‚ . It is well-known [1, 2] that, for any null section πœ‰ of R a d ( 𝑇 𝑀 ) on a coordinate neighborhood 𝒰 βŠ‚ 𝑀 , there exists a uniquely defined null vector field 𝑁 ∈ Ξ“ ( l t r ( 𝑇 𝑀 ) ) satisfying 𝑔 ( πœ‰ , 𝑁 ) = 1 , 𝑔 ( 𝑁 , 𝑁 ) = 𝑔 ( 𝑁 , 𝑋 ) = 𝑔 ( 𝑁 , 𝐿 ) = 0 , βˆ€ 𝑋 ∈ Ξ“ ( 𝑆 ( 𝑇 𝑀 ) ) . ( 2 . 6 ) Let t r ( 𝑇 𝑀 ) = 𝑆 ( 𝑇 𝑀 βŸ‚ ) βŠ• o r t h l t r ( 𝑇 𝑀 ) . We say that 𝑁 , l t r ( 𝑇 𝑀 ) and t r ( 𝑇 𝑀 ) are the lightlike transversal vector field, lightlike transversal vector bundle and transversal vector bundle of 𝑀 with respect to 𝑆 ( 𝑇 𝑀 ) , respectively. Therefore 𝑇 𝑀 is decomposed as 𝑇 𝑀 = 𝑇 𝑀 βŠ• t r ( 𝑇 𝑀 ) = { R a d ( 𝑇 𝑀 ) βŠ• t r ( 𝑇 𝑀 ) } βŠ• o r t h 𝑆 ( 𝑇 𝑀 ) = { R a d ( 𝑇 𝑀 ) βŠ• l t r ( 𝑇 𝑀 ) } βŠ• o r t h 𝑆 ( 𝑇 𝑀 ) βŠ• o r t h 𝑆 ξ€· 𝑇 𝑀 βŸ‚ ξ€Έ . ( 2 . 7 )

Let 𝑃 be the projection morphism of 𝑇 𝑀 on 𝑆 ( 𝑇 𝑀 ) with respect to the decomposition (2.4). The local Gauss and Weingarten formulas for 𝑀 and 𝑆 ( 𝑇 𝑀 ) are given by βˆ‡ 𝑋 π‘Œ = βˆ‡ 𝑋 π‘Œ + 𝐡 ( 𝑋 , π‘Œ ) 𝑁 + 𝐷 ( 𝑋 , π‘Œ ) 𝐿 , ( 2 . 8 ) βˆ‡ 𝑋 𝑁 = βˆ’ 𝐴 𝑁 𝑋 + 𝜏 ( 𝑋 ) 𝑁 + 𝜌 ( 𝑋 ) 𝐿 , ( 2 . 9 ) βˆ‡ 𝑋 𝐿 = βˆ’ 𝐴 𝐿 βˆ‡ 𝑋 + πœ™ ( 𝑋 ) 𝑁 ; ( 2 . 1 0 ) 𝑋 𝑃 π‘Œ = βˆ‡ βˆ— 𝑋 βˆ‡ 𝑃 π‘Œ + 𝐢 ( 𝑋 , 𝑃 π‘Œ ) πœ‰ , ( 2 . 1 1 ) 𝑋 πœ‰ = βˆ’ 𝐴 βˆ— πœ‰ 𝑋 βˆ’ 𝜏 ( 𝑋 ) πœ‰ , ( 2 . 1 2 ) for all 𝑋 , π‘Œ ∈ Ξ“ ( 𝑇 𝑀 ) , where βˆ‡ and βˆ‡ βˆ— are induced linear connections on 𝑇 𝑀 and 𝑆 ( 𝑇 𝑀 ) , respectively, 𝐡 and 𝐷 are called the local second fundamental forms of 𝑀 , 𝐢 is called the local second fundamental form on 𝑆 ( 𝑇 𝑀 ) . 𝐴 𝑁 , 𝐴 βˆ— πœ‰ , and 𝐴 𝐿 are linear operators on 𝑇 𝑀 and 𝜏 ,   𝜌 , and πœ™ are 1-forms on 𝑇 𝑀 . Since βˆ‡ is torsion-free, βˆ‡ is also torsion-free, and 𝐡 and 𝐷 are symmetric. From the facts 𝐡 ( 𝑋 , π‘Œ ) = 𝑔 ( βˆ‡ 𝑋 π‘Œ , πœ‰ ) and 𝐷 ( 𝑋 , π‘Œ ) = 𝑔 ( βˆ‡ 𝑋 π‘Œ , 𝐿 ) , we know that 𝐡 and 𝐷 are independent of the choice of the screen distribution 𝑆 ( 𝑇 𝑀 ) and 𝐡 ( 𝑋 , πœ‰ ) = 0 , 𝐷 ( 𝑋 , πœ‰ ) = βˆ’ πœ™ ( 𝑋 ) , βˆ€ 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . ( 2 . 1 3 ) We say that β„Ž ( 𝑋 , π‘Œ ) = 𝐡 ( 𝑋 , π‘Œ ) 𝑁 + 𝐷 ( 𝑋 , π‘Œ ) 𝐿 is the second fundamental tensor of 𝑀 . The induced connection βˆ‡ of 𝑀 is not metric and satisfies ξ€· βˆ‡ 𝑋 𝑔 ξ€Έ ( π‘Œ , 𝑍 ) = 𝐡 ( 𝑋 , π‘Œ ) πœ‚ ( 𝑍 ) + 𝐡 ( 𝑋 , 𝑍 ) πœ‚ ( π‘Œ ) , ( 2 . 1 4 ) for all 𝑋 , π‘Œ , 𝑍 ∈ Ξ“ ( 𝑇 𝑀 ) , where πœ‚ is a 1-form on 𝑇 𝑀 such that πœ‚ ( 𝑋 ) = 𝑔 ( 𝑋 , 𝑁 ) , βˆ€ 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . ( 2 . 1 5 ) But the connection βˆ‡ βˆ— on 𝑆 ( 𝑇 𝑀 ) is metric. The above three local second fundamental forms of 𝑀 and 𝑆 ( 𝑇 𝑀 ) are related to their shape operators by ξ‚€ 𝐴 𝐡 ( 𝑋 , π‘Œ ) = 𝑔 βˆ— πœ‰  , 𝑋 , π‘Œ 𝑔 ξ‚€ 𝐴 βˆ— πœ‰  ξ€· 𝐴 𝑋 , 𝑁 = 0 , ( 2 . 1 6 ) 𝐢 ( 𝑋 , 𝑃 π‘Œ ) = 𝑔 𝑁 ξ€Έ , 𝑋 , 𝑃 π‘Œ 𝑔 ξ€· 𝐴 𝑁 ξ€Έ ξ€· 𝐴 𝑋 , 𝑁 = 0 , ( 2 . 1 7 ) 𝐷 ( 𝑋 , 𝑃 π‘Œ ) = 𝑔 𝐿 ξ€Έ , 𝑋 , 𝑃 π‘Œ 𝑔 ξ€· 𝐴 𝐿 ξ€Έ ξ€· 𝐴 𝑋 , 𝑁 = 𝜌 ( 𝑋 ) , ( 2 . 1 8 ) 𝐷 ( 𝑋 , π‘Œ ) = 𝑔 𝐿 ξ€Έ 𝑋 , π‘Œ βˆ’ πœ™ ( 𝑋 ) πœ‚ ( π‘Œ ) , βˆ€ 𝑋 , π‘Œ ∈ Ξ“ ( 𝑇 𝑀 ) . ( 2 . 1 9 ) By (2.16) and (2.17), we show that 𝐴 βˆ— πœ‰ and 𝐴 𝑁 are Ξ“ ( 𝑆 ( 𝑇 𝑀 ) ) -valued shape operators related to 𝐡 and 𝐢 , respectively, and 𝐴 βˆ— πœ‰ is self-adjoint on 𝑇 𝑀 and 𝐴 βˆ— πœ‰ πœ‰ = 0 . ( 2 . 2 0 ) Replacing π‘Œ by πœ‰ to (2.8) and using (2.12) and (2.13), we have βˆ‡ 𝑋 πœ‰ = βˆ’ 𝐴 βˆ— πœ‰ 𝑋 βˆ’ 𝜏 ( 𝑋 ) πœ‰ βˆ’ πœ™ ( 𝑋 ) 𝐿 , βˆ€ 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . ( 2 . 2 1 )

3. Tangential Half Lightlike Submanifolds

Let 𝑀 be a half lightlike submanifold of an indefinite cosymplectic manifold 𝑀 . In general the structure vector field 𝜁 of 𝑀 , defined by (2.1), belongs to 𝑇 𝑀 . Thus, from the decomposition (2.7) of 𝑇 𝑀 , the structure vector field 𝜁 is decomposed as follows: 𝜁 = πœ” + π‘Ž πœ‰ + 𝑏 𝑁 + 𝑒 𝐿 , ( 3 . 1 ) where πœ” is a smooth vector field on 𝑆 ( 𝑇 𝑀 ) , and π‘Ž = πœƒ ( 𝑁 ) , 𝑏 = πœƒ ( πœ‰ ) , and 𝑒 = πœƒ ( 𝐿 ) are smooth functions on 𝑀 . First of all, we introduce the following result.

Proposition 3.1 (see [3]). Let 𝑀 be a half lightlike submanifold of an indefinite almost contact metric manifold 𝑀 . Then there exists a screen distribution 𝑆 ( 𝑇 𝑀 ) such that 𝐽 ξ€· 𝑆 ( 𝑇 𝑀 ) βŸ‚ ξ€Έ βŠ‚ 𝑆 ( 𝑇 𝑀 ) . ( 3 . 2 )

Note 1. Although, in general, 𝑆 ( 𝑇 𝑀 ) is not unique, it is canonically isomorphic to the factor vector bundle 𝑆 ( 𝑇 𝑀 ) βˆ— = 𝑇 𝑀 / R a d ( 𝑇 𝑀 ) considered by Kupeli [12]. Thus all screen distributions are mutually isomorphic. For this reason, we consider only half lightlike submanifold 𝑀 equipped with a screen distribution 𝑆 ( 𝑇 𝑀 ) such that 𝐽 ( 𝑆 ( 𝑇 𝑀 ) βŸ‚ ) βŠ‚ 𝑆 ( 𝑇 𝑀 ) , such a screen distribution 𝑆 ( 𝑇 𝑀 ) is called a generic screen distribution [8] of 𝑀 .

Proposition 3.2. Let 𝑀 be a half lightlike submanifold of an indefinite cosymplectic manifold 𝑀 . Then the structure vector field 𝜁 does not belong to R a d ( 𝑇 𝑀 ) and l t r ( 𝑇 𝑀 ) .

Proof. Assume that 𝜁 belongs to R a d ( 𝑇 𝑀 ) (or l t r ( 𝑇 𝑀 ) ). Then (3.1) deduces to 𝜁 = π‘Ž πœ‰ and π‘Ž β‰  0 (or 𝜁 = 𝑏 𝑁 and 𝑏 β‰  0 ). From this, we have 1 = 𝑔 ( 𝜁 , 𝜁 ) = π‘Ž 2 𝑔 ξ€Ί ( πœ‰ , πœ‰ ) = 0 o r 1 = 𝑔 ( 𝜁 , 𝜁 ) = 𝑏 2 𝑔 ξ€» . ( 𝑁 , 𝑁 ) = 0 ( 3 . 3 ) It is a contradiction. Thus 𝜁 does not belong to R a d ( 𝑇 𝑀 ) and l t r ( 𝑇 𝑀 ) .

Note 2. If the structure vector field 𝜁 is tangent to 𝑀 , that is, 𝑏 = 𝑒 = 0 , then 𝜁 does not belong to R a d ( 𝑇 𝑀 ) by Proposition 3.2. This enables one to choose a screen distribution 𝑆 ( 𝑇 𝑀 ) which contains 𝜁 . This implies that if 𝜁 is tangent to 𝑀 , then it belongs to 𝑆 ( 𝑇 𝑀 ) . Călin [13] also proved this result which we assume in this section.

Definition 3.3. A half lightlike submanifold 𝑀 of an indefinite cosymplectic manifold 𝑀 is said to be a tangential half lightlike submanifold [4] of 𝑀 if 𝜁 is tangent to 𝑀 .

For any tangential half lightlike submanifold 𝑀 , we show that 𝜁 belongs to 𝑆 ( 𝑇 𝑀 ) , that is, π‘Ž = 𝑏 = 𝑒 = 0 by Note 2. Then there exists a nondegenerate almost complex distribution 𝐻 π‘œ on 𝑀 with respect to 𝐽 , that is, 𝐽 ( 𝐻 π‘œ ) = 𝐻 π‘œ , such that 𝑆 ( 𝑇 𝑀 ) = { 𝐽 ( R a d ( 𝑇 𝑀 ) ) βŠ• 𝐽 ( l t r ( 𝑇 𝑀 ) ) } βŠ• o r t h 𝐽 ξ€· 𝑆 ξ€· 𝑇 𝑀 βŸ‚ βŠ• ξ€Έ ξ€Έ o r t h 𝐻 π‘œ . ( 3 . 4 ) Thus the general decompositions (2.4) and (2.7) reduce, respectively, to 𝑇 𝑀 = 𝐻 βŠ• 𝐻 ξ…ž , 𝑇 𝑀 = 𝐻 βŠ• 𝐻 β€² βŠ• t r ( 𝑇 𝑀 ) , ( 3 . 5 ) where 𝐻 and 𝐻 β€² are 2- and 1-lightlike distributions on 𝑀 such that 𝐻 = R a d ( 𝑇 𝑀 ) βŠ• o r t h 𝐽 ( R a d ( 𝑇 𝑀 ) ) βŠ• o r t h 𝐻 π‘œ , 𝐻 β€² = 𝐽 ( l t r ( 𝑇 𝑀 ) ) βŠ• o r t h 𝐽 ξ€· 𝑆 ξ€· 𝑇 𝑀 βŸ‚ . ξ€Έ ξ€Έ ( 3 . 6 ) 𝐻 is an almost complex distribution of 𝑀 with respect to 𝐽 . Consider a pair of local null vector fields { π‘ˆ , 𝑉 } and a local nonnull vector field π‘Š on 𝑆 ( 𝑇 𝑀 ) defined by π‘ˆ = βˆ’ 𝐽 𝑁 , 𝑉 = βˆ’ 𝐽 πœ‰ , π‘Š = βˆ’ 𝐽 𝐿 . ( 3 . 7 ) Denote by 𝑆 the projection morphism of 𝑇 𝑀 on 𝐻 with respect to the decomposition (3.5). Then any vector field 𝑋 on 𝑀 and its action 𝐽 𝑋 by 𝐽 are expressed as follows: 𝑋 = 𝑆 𝑋 + 𝑒 ( 𝑋 ) π‘ˆ + 𝑀 ( 𝑋 ) π‘Š , 𝐽 𝑋 = 𝐹 𝑋 + 𝑒 ( 𝑋 ) 𝑁 + 𝑀 ( 𝑋 ) 𝐿 , ( 3 . 8 ) where 𝑒 , 𝑣 , and 𝑀 are 1-forms locally defined on 𝑀 by 𝑒 ( 𝑋 ) = 𝑔 ( 𝑋 , 𝑉 ) , 𝑣 ( 𝑋 ) = 𝑔 ( 𝑋 , π‘ˆ ) , 𝑀 ( 𝑋 ) = 𝑔 ( 𝑋 , π‘Š ) ( 3 . 9 ) and 𝐹 is a tensor field of type ( 1 , 1 ) globally defined on 𝑀 by 𝐹 = 𝐽 ∘ 𝑆 . Applying the operator βˆ‡ 𝑋 to (3.7) and the second equation of (3.8) (denote (3.8)2) and using (2.2), (2.8), (2.9), (2.10), (2.21), (3.7), (3.8) and (3.9), for all 𝑋 , π‘Œ ∈ Ξ“ ( 𝑇 𝑀 ) , we have βˆ‡ 𝐡 ( 𝑋 , π‘ˆ ) = 𝐢 ( 𝑋 , 𝑉 ) , 𝐡 ( 𝑋 , π‘Š ) = 𝐷 ( 𝑋 , 𝑉 ) , 𝐢 ( 𝑋 , π‘Š ) = 𝐷 ( 𝑋 , π‘ˆ ) , ( 3 . 1 0 ) 𝑋 ξ€· 𝐴 π‘ˆ = 𝐹 𝑁 𝑋 ξ€Έ βˆ‡ + 𝜏 ( 𝑋 ) π‘ˆ + 𝜌 ( 𝑋 ) π‘Š , ( 3 . 1 1 ) 𝑋 ξ‚€ 𝐴 𝑉 = 𝐹 βˆ— πœ‰ 𝑋  βˆ‡ βˆ’ 𝜏 ( 𝑋 ) 𝑉 βˆ’ πœ™ ( 𝑋 ) π‘Š , ( 3 . 1 2 ) 𝑋 ξ€· 𝐴 π‘Š = 𝐹 𝐿 𝑋 ξ€Έ ξ€· βˆ‡ + πœ™ ( 𝑋 ) π‘ˆ , ( 3 . 1 3 ) 𝑋 𝐹 ξ€Έ ( π‘Œ ) = 𝑒 ( π‘Œ ) 𝐴 𝑁 𝑋 + 𝑀 ( π‘Œ ) 𝐴 𝐿 𝑋 βˆ’ 𝐡 ( 𝑋 , π‘Œ ) π‘ˆ βˆ’ 𝐷 ( 𝑋 , π‘Œ ) π‘Š . ( 3 . 1 4 )

Note 3. From now on, 𝑀 = ( 𝑅 π‘ž 2 π‘š + 1 , 𝐽 , 𝜁 , πœƒ , 𝑔 ) will denote the semi-Euclidean manifold 𝑅 π‘ž 2 π‘š + 1 equipped with its usual cosymplectic structure given by πœƒ = 𝑑 𝑧 , 𝜁 = πœ• 𝑧 , 𝑔 = πœƒ βŠ— πœƒ βˆ’ π‘ž / 2  𝑖 = 1 ξ€· 𝑑 π‘₯ 𝑖 βŠ— 𝑑 π‘₯ 𝑖 + 𝑑 𝑦 𝑖 βŠ— 𝑑 𝑦 𝑖 ξ€Έ + π‘š  𝑖 = π‘ž + 1 ξ€· 𝑑 π‘₯ 𝑖 βŠ— 𝑑 π‘₯ 𝑖 + 𝑑 𝑦 𝑖 βŠ— 𝑑 𝑦 𝑖 ξ€Έ , 𝐽  π‘š  𝑖 = 1 ξ€· 𝑋 𝑖 πœ• π‘₯ 𝑖 + π‘Œ 𝑖 πœ• 𝑦 𝑖 ξ€Έ ξƒͺ = + 𝑍 πœ• 𝑧 π‘š  𝑖 = 1 ξ€· π‘Œ 𝑖 πœ• π‘₯ 𝑖 βˆ’ 𝑋 𝑖 πœ• 𝑦 𝑖 ξ€Έ , ( 3 . 1 5 ) where ( π‘₯ 𝑖 , 𝑦 𝑖 , 𝑧 ) are the Cartesian coordinates and 𝑔 is a semi-Euclidean metric of signature ( βˆ’ , + , … , + ; βˆ’ , + , … , + ; + ) with respect to the canonical basis ξ€½ πœ• π‘₯ 1 , πœ• π‘₯ 2 , … , πœ• π‘₯ π‘š ; πœ• 𝑦 1 , πœ• 𝑦 2 , … , πœ• 𝑦 π‘š ξ€Ύ ; πœ• 𝑧 . ( 3 . 1 6 ) This construction will help in understanding how the indefinite cosymplectic structure is recovered in examples of this paper.

Example 3.4. Consider a submanifold 𝑀 of 𝑀 = ( 𝑅 9 2 , 𝐽 , 𝜁 , πœƒ , 𝑔 ) given by the equations π‘₯ 1 = 𝑦 4 , π‘₯ 2 =  1 βˆ’ 𝑦 2 2 , 𝑦 2 β‰  Β± 1 . ( 3 . 1 7 ) Then a local frame fields of 𝑇 𝑀 are given by πœ‰ = πœ• π‘₯ 1 + πœ• 𝑦 4 , π‘ˆ 1 = πœ• π‘₯ 4 βˆ’ πœ• 𝑦 1 , π‘ˆ 2 = πœ• π‘₯ 3 , π‘ˆ 3 = πœ• 𝑦 3 , π‘ˆ 4 𝑦 = βˆ’ 2 π‘₯ 2 πœ• π‘₯ 2 + πœ• 𝑦 2 , π‘ˆ 5 = πœ• π‘₯ 4 + πœ• 𝑦 1 , π‘ˆ 6 = 𝜁 = πœ• 𝑧 . ( 3 . 1 8 ) This implies R a d ( 𝑇 𝑀 ) = S p a n { πœ‰ } , 𝐽 πœ‰ = π‘ˆ 1 , and R a d ( 𝑇 𝑀 ) ∩ 𝐽 ( R a d ( 𝑇 𝑀 ) ) = { 0 } . Next, 𝐽 π‘ˆ 2 = βˆ’ π‘ˆ 3 implies that 𝐻 π‘œ = { π‘ˆ 2 , π‘ˆ 3 } invariant with respect to the almost contact structure tensor 𝐽 . By direct calculations, we have 𝑆 ξ€· 𝑇 𝑀 βŸ‚ ξ€Έ ξ‚» = S p a n 𝐿 = πœ• π‘₯ 2 + 𝑦 2 π‘₯ 2 πœ• 𝑦 2 ξ‚Ό  1 , l t r ( 𝑇 𝑀 ) = S p a n 𝑁 = 2 ξ€· βˆ’ πœ• π‘₯ 1 + πœ• 𝑦 4 ξ€Έ  . ( 3 . 1 9 ) We show that 𝐽 𝐿 = βˆ’ π‘ˆ 4 , 𝐽 𝑁 = ( 1 / 2 ) π‘ˆ 5 , 𝐽 𝜁 = 0 and βˆ‡ 𝑋 𝜁 = 0 for all 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . Therefore 𝑀 is a tangential half-lightlike submanifold of an indefinite cosymplectic manifold 𝑀 .

Theorem 3.5. Let 𝑀 be a tangential half lightlike submanifold of an indefinite cosymplectic manifold 𝑀 . Then the structure vector field 𝜁 is parallel with respect to the connections βˆ‡ and βˆ‡ βˆ— . Furthermore, 𝜁 is conjugate to any vector field of 𝑀 with respect to β„Ž and 𝐢 .

Proof. Replacing π‘Œ by 𝜁 to (2.8) and using (2.3) and the fact 𝜁 ∈ Ξ“ ( 𝑇 𝑀 ) , we get βˆ‡ 𝑋 𝜁 + 𝐡 ( 𝑋 , 𝜁 ) 𝑁 + 𝐷 ( 𝑋 , 𝜁 ) 𝐿 = 0 , βˆ€ 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . ( 3 . 2 0 ) Taking the scalar product with πœ‰ and 𝐿 to this equation by turns, we have βˆ‡ 𝑋 𝜁 = 0 , 𝐡 ( 𝑋 , 𝜁 ) = 0 , 𝐷 ( 𝑋 , 𝜁 ) = 0 , βˆ€ 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . ( 3 . 2 1 ) From (3.21)1, we see that 𝜁 is parallel with respect to the induced connection βˆ‡ . (3.21)2,3 implies that 𝜁 is conjugate to any vector field on 𝑀 with respect to the second fundamental form β„Ž . Replacing 𝑃 π‘Œ by 𝜁 to (2.11) and using (3.21)1 and the fact 𝜁 ∈ Ξ“ ( 𝑆 ( 𝑇 𝑀 ) ) , we get βˆ‡ βˆ— 𝑋 𝜁 + 𝐢 ( 𝑋 , 𝜁 ) πœ‰ = 0 , βˆ€ 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . ( 3 . 2 2 ) Taking the scalar product with 𝑁 to this equation, we have βˆ‡ βˆ— 𝑋 𝜁 = 0 , 𝐢 ( 𝑋 , 𝜁 ) = 0 , βˆ€ 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . ( 3 . 2 3 ) Thus 𝜁 is also parallel with respect to the lieasr connection βˆ‡ βˆ— and conjugate to any vector field on 𝑀 with respect to 𝐢 . Thus we have our assertions.

Definition 3.6. A half lightlike submanifold 𝑀 of 𝑀 is totally umbilical [5] if there is a smooth vector field β„‹ on t r ( 𝑇 𝑀 ) on any coordinate neighborhood 𝒰 such that β„Ž ( 𝑋 , π‘Œ ) = β„‹ 𝑔 ( 𝑋 , π‘Œ ) , βˆ€ 𝑋 , π‘Œ ∈ Ξ“ ( 𝑇 𝑀 ) . ( 3 . 2 4 ) In case β„‹ = 0 , that is, β„Ž = 0 on 𝒰 , we say that 𝑀 is totally geodesic.

It is easy to see that 𝑀 is totally umbilical if and only if there exist smooth functions 𝛽 and 𝛿 on each coordinate neighborhood 𝒰 such that 𝐡 ( 𝑋 , π‘Œ ) = 𝛽 𝑔 ( 𝑋 , π‘Œ ) , 𝐷 ( 𝑋 , π‘Œ ) = 𝛿 𝑔 ( 𝑋 , π‘Œ ) , βˆ€ 𝑋 , π‘Œ ∈ Ξ“ ( 𝑇 𝑀 ) . ( 3 . 2 5 )

Theorem 3.7. Any totally umbilical tangential half lightlike submanifold 𝑀 of an indefinite cosymplectic manifold 𝑀 is totally geodesic.

Proof. Assume that 𝑀 is totally umbilical. From (3.21) and (3.25), we have 𝛽 𝑔 ( 𝑋 , 𝜁 ) = 0 , 𝛿 𝑔 ( 𝑋 , 𝜁 ) = 0 , βˆ€ 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . ( 3 . 2 6 ) Replacing 𝑋 by 𝜁 in this equations and using the fact 𝑔 ( 𝜁 , 𝜁 ) = 1 , we have 𝛽 = 𝛿 = 0 , that is, 𝐡 = 𝐷 = 0 . Thus we have β„Ž = 0 and 𝑀 is totally geodesic.

Definition 3.8. Ascreen distribution 𝑆 ( 𝑇 𝑀 ) is called totally umbilical [5] (in 𝑀 ) if there is a smooth function 𝛾 on any coordinate neighborhood 𝒰 in 𝑀 such that 𝐢 ( 𝑋 , 𝑃 π‘Œ ) = 𝛾 𝑔 ( 𝑋 , π‘Œ ) , βˆ€ 𝑋 , π‘Œ ∈ Ξ“ ( 𝑇 𝑀 ) . ( 3 . 2 7 ) In case 𝛾 = 0 on 𝒰 , we say that 𝑆 ( 𝑇 𝑀 ) is totally geodesic (in 𝑀 ).

Theorem 3.9. Let 𝑀 be a tangential half lightlike submanifold of an indefinite cosymplectic manifold 𝑀 such that 𝑆 ( 𝑇 𝑀 ) is totally umbilical. Then 𝑆 ( 𝑇 𝑀 ) is totally geodesic.

Proof. Assume that 𝑆 ( 𝑇 𝑀 ) is totally umbilical in 𝑀 . Replacing π‘Œ by 𝜁 to (3.27) and using (3.23), we have 𝛾 𝑔 ( 𝑋 , 𝜁 ) = 0 for all 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . Replacing 𝑋 by 𝜁 to this equation and using the fact 𝑔 ( 𝜁 , 𝜁 ) = 1 , we obtain 𝛾 = 0 . Thus 𝑆 ( 𝑇 𝑀 ) is totally geodesic in 𝑀 .

Theorem 3.10. Let 𝑀 be a tangential half lightlike submanifold of an indefinite cosymplectic manifold 𝑀 . Then 𝐻 is an integrable distribution on 𝑀 if and only if β„Ž ( 𝑋 , 𝐹 π‘Œ ) = β„Ž ( 𝐹 𝑋 , π‘Œ ) , βˆ€ 𝑋 , π‘Œ ∈ Ξ“ ( 𝐻 ) . ( 3 . 2 8 ) Moreover, if 𝑀 is totally umbilical, then 𝐻 is a parallel distribution on 𝑀 .

Proof. Taking π‘Œ ∈ Ξ“ ( 𝐻 ) , we show that 𝐹 π‘Œ = 𝐽 π‘Œ ∈ Ξ“ ( 𝐻 ) . Applying βˆ‡ 𝑋 to 𝐹 π‘Œ = 𝐽 π‘Œ and using (2.3), (2.8), (3.7), (3.8)2, and (3.9), we have 𝐡 ξ€· βˆ‡ ( 𝑋 , 𝐹 π‘Œ ) = 𝑔 𝑋 ξ€Έ ξ€· βˆ‡ π‘Œ , 𝑉 , 𝐷 ( 𝑋 , 𝐹 π‘Œ ) = 𝑔 𝑋 ξ€Έ ξ€· βˆ‡ π‘Œ , π‘Š , ( 3 . 2 9 ) 𝑋 𝐹 ξ€Έ ( π‘Œ ) = βˆ’ 𝐡 ( 𝑋 , π‘Œ ) π‘ˆ βˆ’ 𝐷 ( 𝑋 , π‘Œ ) π‘Š , βˆ€ 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . ( 3 . 3 0 ) By direct calculations from two equations of (3.29), we have [ ] [ ] β„Ž ( 𝑋 , 𝐹 π‘Œ ) βˆ’ β„Ž ( 𝐹 𝑋 , π‘Œ ) = 𝑔 ( 𝑋 , π‘Œ , 𝑉 ) 𝑁 + 𝑔 ( 𝑋 , π‘Œ , π‘Š ) 𝐿 . ( 3 . 3 1 ) If 𝐻 is integrable, then [ 𝑋 , π‘Œ ] ∈ Ξ“ ( 𝐻 ) for any 𝑋 , π‘Œ ∈ Ξ“ ( 𝐻 ) . This implies 𝑔 ( [ 𝑋 , π‘Œ ] , 𝑉 ) = 𝑔 ( [ 𝑋 , π‘Œ ] , π‘Š ) = 0 . Thus we get β„Ž ( 𝑋 , 𝐹 π‘Œ ) = β„Ž ( 𝐹 𝑋 , π‘Œ ) for all 𝑋 , π‘Œ ∈ Ξ“ ( 𝐻 ) . Conversely if β„Ž ( 𝑋 , 𝐹 π‘Œ ) = β„Ž ( 𝐹 𝑋 , π‘Œ ) for all 𝑋 , π‘Œ ∈ Ξ“ ( 𝐻 ) , then we have 𝑔 ( [ 𝑋 , π‘Œ ] , 𝑉 ) = 𝑔 ( [ 𝑋 , π‘Œ ] , π‘Š ) = 0 . This imply [ 𝑋 , π‘Œ ] ∈ Ξ“ ( 𝐻 ) for all 𝑋 , π‘Œ ∈ Ξ“ ( 𝐻 ) . Thus 𝐻 is an integrable distribution of 𝑀 .
If 𝑀 is totally umbilical, from Theorem 3.7 and (3.29), we have 𝑔 ξ€· βˆ‡ 𝑋 ξ€Έ ξ€· βˆ‡ π‘Œ , 𝑉 = 𝑔 𝑋 ξ€Έ π‘Œ , π‘Š = 0 , βˆ€ 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) , βˆ€ π‘Œ ∈ Ξ“ ( 𝐻 ) . ( 3 . 3 2 ) This imply βˆ‡ 𝑋 π‘Œ ∈ Ξ“ ( 𝐻 ) for all 𝑋 , π‘Œ ∈ Ξ“ ( 𝐻 ) , that is, 𝐻 is a parallel distribution on 𝑀 .

Theorem 3.11. Let 𝑀 be a tangential half lightlike submanifold of an indefinite cosymplectic manifold 𝑀 . Then 𝐹 is parallel on 𝐻 with respect to the connection βˆ‡ if and only if 𝐻 is a parallel distribution on 𝑀 .

Proof. Assume that 𝐹 is parallel on 𝐻 with respect to βˆ‡ . For any 𝑋 , π‘Œ ∈ Ξ“ ( 𝐻 ) , we have ( βˆ‡ 𝑋 𝐹 ) π‘Œ = 0 . Taking the scalar product with 𝑉 and π‘Š to (3.30) with ( βˆ‡ 𝑋 𝐹 ) π‘Œ = 0 , we have 𝐡 ( 𝑋 , π‘Œ ) = 0 and 𝐷 ( 𝑋 , π‘Œ ) = 0 for all 𝑋 , π‘Œ ∈ Ξ“ ( 𝐻 ) , respectively. From (3.29), we have 𝑔 ( βˆ‡ 𝑋 π‘Œ , 𝑉 ) = 0 and 𝑔 ( βˆ‡ 𝑋 π‘Œ , π‘Š ) = 0 . This imply βˆ‡ 𝑋 π‘Œ ∈ Ξ“ ( 𝐻 ) for all 𝑋 , π‘Œ ∈ Ξ“ ( 𝐻 ) . Thus 𝐻 is a parallel distribution on 𝑀 .
Conversely if 𝐻 is a parallel distribution on 𝑀 , from (3.29) we have 𝐡 ( 𝑋 , 𝐹 π‘Œ ) = 0 , 𝐷 ( 𝑋 , 𝐹 π‘Œ ) = 0 , βˆ€ 𝑋 , π‘Œ ∈ Ξ“ ( 𝐻 ) . ( 3 . 3 3 ) For any π‘Œ ∈ Ξ“ ( 𝐻 ) , we show that 𝐹 2 π‘Œ = 𝐽 2 π‘Œ = βˆ’ π‘Œ + πœƒ ( π‘Œ ) 𝜁 . Replacing π‘Œ by 𝐹 π‘Œ to (3.33) and using (3.21), we have 𝐡 ( 𝑋 , π‘Œ ) = 0 and 𝐷 ( 𝑋 , π‘Œ ) = 0 for any 𝑋 , π‘Œ ∈ Ξ“ ( 𝐻 ) . Thus 𝐹 is parallel on 𝐻 with respect to βˆ‡ by (3.30).

Theorem 3.12. Let 𝑀 be a tangential half lightlike submanifold of an indefinite cosymplectic manifold 𝑀 . If 𝐹 is parallel with respect to the induced connection βˆ‡ , then 𝐻 is a parallel distribution on 𝑀 and 𝑀 is locally a product manifold 𝐿 π‘ˆ Γ— 𝐿 π‘Š Γ— 𝑀 𝑇 , where 𝐿 π‘ˆ and 𝐿 π‘Š are null curves tangent to 𝐽 ( l t r ( 𝑇 𝑀 ) ) and 𝐽 ( 𝑆 ( 𝑇 𝑀 βŸ‚ ) ) , respectively, and 𝑀 𝑇 is a leaf of 𝐻 .

Proof. Assume that 𝐹 is parallel on 𝑇 𝑀 with respect to βˆ‡ . Then 𝐹 is parallel on 𝐻 with respect to βˆ‡ . By Theorem 3.11, 𝐻 is a parallel distribution on 𝑀 . Applying the operator 𝐹 to (3.14) with ( βˆ‡ 𝑋 𝐹 ) π‘Œ = 0 , we have 𝑒 ξ€· 𝐴 ( π‘Œ ) 𝐹 𝑁 𝑋 ξ€Έ ξ€· 𝐴 + 𝑀 ( π‘Œ ) 𝐹 𝐿 𝑋 ξ€Έ = 0 , βˆ€ 𝑋 , π‘Œ ∈ Ξ“ ( 𝑇 𝑀 ) , ( 3 . 3 4 ) due to 𝐹 π‘ˆ = 𝐹 π‘Š = 0 . Replacing π‘Œ by π‘ˆ and π‘Š to this equation by turns and using (3.9), we have 𝐹 ( 𝐴 𝑁 𝑋 ) = 0 and 𝐹 ( 𝐴 𝐿 𝑋 ) = 0 . Taking the scalar product with π‘Š and 𝑁 to (3.14) with ( βˆ‡ 𝑋 𝐹 ) π‘Œ = 0 by turns, we have 𝐷 ξ€· 𝐴 ( 𝑋 , π‘Œ ) = 𝑒 ( π‘Œ ) 𝑀 𝑁 𝑋 ξ€Έ ξ€· 𝐴 + 𝑀 ( π‘Œ ) 𝑀 𝐿 𝑋 ξ€Έ ξ€· 𝐴 , ( 3 . 3 5 ) 𝑀 ( π‘Œ ) 𝑔 𝐿 ξ€Έ 𝑋 , 𝑁 = 0 , βˆ€ 𝑋 , π‘Œ ∈ Ξ“ ( 𝑇 𝑀 ) . ( 3 . 3 6 ) Replacing π‘Œ by πœ‰ to (3.35), we get πœ™ = 0 due to (2.13)2. Also replacing π‘Œ by π‘Š to (3.36), we have 𝜌 = 0 due to (2.18)2. From thess results, (3.11) and (3.13), we get βˆ‡ 𝑋 π‘ˆ = 𝜏 ( 𝑋 ) π‘ˆ and βˆ‡ 𝑋 π‘Š = 0 for all 𝑋 ∈ Ξ“ ( 𝐻 β€² ) . Thus 𝐽 ( l t r ( 𝑇 𝑀 ) ) and 𝐽 ( 𝑆 ( 𝑇 𝑀 βŸ‚ ) ) are also parallel distributions on 𝑀 . By the decomposition theorem of de Rham [14], we show that 𝑀 = 𝐿 π‘ˆ Γ— 𝐿 π‘Š Γ— 𝑀 𝑇 , where 𝐿 π‘ˆ and 𝐿 π‘Š are null curves tangent to 𝐽 ( l t r ( 𝑇 𝑀 ) ) and 𝐽 ( 𝑆 ( 𝑇 𝑀 βŸ‚ ) ) , respectively, and 𝑀 𝑇 is a leaf of 𝐻 .

Definition 3.13. A half lightlike submanifold 𝑀 of a semi-Riemannian manifold 𝑀 is said to be irrotational [12] if βˆ‡ 𝑋 πœ‰ ∈ Ξ“ ( 𝑇 𝑀 ) for any 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) .

Note 4. From (2.21) we see that a necessary and sufficient condition for 𝑀 to be irrotational is 𝐷 ( 𝑋 , πœ‰ ) = 0 = πœ™ ( 𝑋 ) for all 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) .

Theorem 3.14. Let 𝑀 be a tangential half lightlike submanifold of an indefinite cosymplectic manifold 𝑀 . Then one has the following assertions.(i)If 𝑉 is parallel with respect to βˆ‡ , then 𝑀 is irrotational, 𝜏 = 0 and 𝐴 βˆ— πœ‰ ξ‚€ 𝐴 𝑋 = 𝑒 βˆ— πœ‰ 𝑋  ξ‚€ 𝐴 π‘ˆ + 𝑀 βˆ— πœ‰ 𝑋  π‘Š , βˆ€ 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . ( 3 . 3 7 ) (ii)If π‘ˆ is parallel with respect to βˆ‡ , then one has 𝜏 = 𝜌 = 0 and 𝐴 𝑁 ξ€· 𝐴 𝑋 = 𝑒 𝑁 𝑋 ξ€Έ ξ€· 𝐴 π‘ˆ + 𝑀 𝑁 𝑋 ξ€Έ π‘Š , βˆ€ 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . ( 3 . 3 8 ) (iii)If π‘Š is parallel with respect to βˆ‡ , then 𝑀 is irrotational and 𝐴 𝐿 ξ€· 𝐴 𝑋 = 𝑒 𝐿 𝑋 ξ€Έ ξ€· 𝐴 π‘ˆ + 𝑀 𝐿 𝑋 ξ€Έ π‘Š , βˆ€ 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . ( 3 . 3 9 ) Moreover, if all of 𝑉 , π‘ˆ , and π‘Š are parallel on 𝑇 𝑀 with respect to βˆ‡ , then 𝑆 ( 𝑇 𝑀 ) is totally geodesic in 𝑀 and 𝜏 = πœ™ = 𝜌 = 0 on Ξ“ ( 𝑇 𝑀 ) . In this case, the null transversal vector field 𝑁 of 𝑀 is a constant on 𝑀 .

Proof. If 𝑉 is parallel with respect to βˆ‡ , then, taking the scalar product with π‘ˆ and π‘Š to (3.12) by turns, we have 𝜏 = 0 and πœ™ = 0 ( 𝑀 is irrotational), respectively. Thus we have 𝐹 ( 𝐴 βˆ— πœ‰ 𝑋 ) = 0 for all 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . From this result and (3.8), we obtain 𝐽 ( 𝐴 βˆ— πœ‰ 𝑋 ) = 𝑒 ( 𝐴 βˆ— πœ‰ 𝑋 ) 𝑁 + 𝑀 ( 𝐴 βˆ— πœ‰ 𝑋 ) 𝐿 . Applying 𝐽 to this equation and using πœƒ ( 𝐴 βˆ— πœ‰ 𝑋 ) = 0 , we obtain (i). In a similar way, by using (3.11), (3.13), (3.21), and (3.23), we have (ii) and (iii).
Assume that all of 𝑉 , π‘ˆ , and π‘Š are parallel on 𝑇 𝑀 with respect to βˆ‡ . Substituting the equation of (i) into (3.10)-1, we have 𝑒 ξ€· 𝐴 𝑁 𝑋 ξ€Έ ξ‚€ 𝐴 = 𝑣 βˆ— πœ‰ 𝑋  ξ‚€ 𝐴 = 𝑔 βˆ— πœ‰  𝑋 , π‘ˆ = 0 , βˆ€ 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . ( 3 . 4 0 ) Also, substituting the equation of (iii) into (3.10)-3, we have 𝑀 ξ€· 𝐴 𝑁 𝑋 ξ€Έ ξ€· 𝐴 = 𝑣 𝐿 𝑋 ξ€Έ ξ€· 𝐴 = 𝑔 𝐿 ξ€Έ 𝑋 , π‘ˆ = 0 , βˆ€ 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . ( 3 . 4 1 ) From the last two equations and the equation of (ii), we see that 𝐴 𝑁 = 0 . Thus 𝑆 ( 𝑇 𝑀 ) is totally geodesic in 𝑀 and the 1-forms 𝜏 , πœ™ , and 𝜌 , defined by (2.9) and (2.10), satisfy 𝜏 = πœ™ = 𝜌 = 0 on Ξ“ ( 𝑇 𝑀 ) . Using this results, we see that 𝑁 is a constant on 𝑀 .

Theorem 3.15. Let 𝑀 be a totally umbilical tangential half lightlike submanifold of an indefinite cosymplectic manifold 𝑀 such that 𝑆 ( 𝑇 𝑀 ) is totally umbilical. Then 𝑀 is locally a product manifold 𝑀 = 𝑀 4 Γ— 𝑀 𝑇 π‘œ , where 𝑀 4 and 𝑀 𝑇 π‘œ are leaves of 𝐻 βŸ‚ π‘œ and 𝐻 π‘œ , respectively.

Proof. By Theorem 3.10, 𝐻 is a parallel distribution 𝑀 . Thus, for all 𝑋 , π‘Œ ∈ Ξ“ ( 𝐻 π‘œ ) , we have βˆ‡ 𝑋 π‘Œ ∈ Ξ“ ( 𝐻 ) . From (2.11) and (3.30), we have 𝐢 ξ€· βˆ‡ ( 𝑋 , 𝐹 π‘Œ ) = 𝑔 𝑋 ξ€Έ βˆ‡ 𝐹 π‘Œ , 𝑁 = 𝑔 ξ€· ξ€· 𝑋 𝐹 ξ€Έ ξ€· βˆ‡ π‘Œ + 𝐹 𝑋 π‘Œ ξ€Έ ξ€Έ ξ€· 𝐹 ξ€· βˆ‡ , 𝑁 = 𝑔 𝑋 π‘Œ ξ€Έ ξ€Έ ξ€· βˆ‡ , 𝑁 = βˆ’ 𝑔 𝑋 ξ€Έ ξ€· βˆ‡ π‘Œ , 𝐽 𝑁 = 𝑔 𝑋 ξ€Έ , π‘Œ , π‘ˆ ( 3 . 4 2 ) due to 𝐹 π‘Œ ∈ Ξ“ ( 𝐻 π‘œ ) . If 𝑆 ( 𝑇 𝑀 ) is totally umbilical in 𝑀 , then we have 𝐢 = 0 due to Theorem 3.7. By (2.11) and (3.42), we get 𝑔 ξ€· βˆ‡ 𝑋 ξ€Έ ξ€· βˆ‡ π‘Œ , 𝑁 = 0 , 𝑔 𝑋 ξ€Έ ξ€· 𝐻 π‘Œ , π‘ˆ = 0 , βˆ€ 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) , βˆ€ π‘Œ ∈ Ξ“ π‘œ ξ€Έ . ( 3 . 4 3 ) These results and (3.29) imply βˆ‡ 𝑋 π‘Œ ∈ Ξ“ ( 𝐻 π‘œ ) for all 𝑋 , π‘Œ ∈ Ξ“ ( 𝐻 π‘œ ) . Thus 𝐻 π‘œ is a parallel distribution on 𝑀 and 𝑇 𝑀 = 𝐻 π‘œ βŠ• o r t h 𝐻 βŸ‚ π‘œ , where 𝐻 βŸ‚ π‘œ = S p a n { πœ‰ , 𝑉 , π‘ˆ , π‘Š } . By Theorems 3.5 and 3.7, we have 𝐡 = 𝐷 = 𝐴 𝑁 = πœ™ = 0 and 𝐴 𝐿 𝑋 = 𝜌 ( 𝑋 ) πœ‰ . Thus (2.12) and (3.11) ∼ (3.13) deduce, respectively, to βˆ‡ 𝑋 πœ‰ = βˆ’ 𝜏 ( 𝑋 ) πœ‰ , βˆ‡ 𝑋 βˆ‡ π‘ˆ = 𝜏 ( 𝑋 ) π‘ˆ + 𝜌 ( 𝑋 ) π‘Š , 𝑋 𝑉 = βˆ’ 𝜏 ( 𝑋 ) 𝑉 , βˆ‡ 𝑋 ξ€· 𝐻 π‘Š = βˆ’ 𝜌 ( 𝑋 ) 𝑉 , βˆ€ 𝑋 ∈ Ξ“ βŸ‚ π‘œ ξ€Έ . ( 3 . 4 4 ) Thus 𝐻 βŸ‚ π‘œ is also a parallel distribution on 𝑀 . Thus we have 𝑀 = 𝑀 4 Γ— 𝑀 𝑇 π‘œ , where 𝑀 4 is a leaf of 𝐻 βŸ‚ π‘œ and 𝑀 𝑇 π‘œ is a leaf of 𝐻 π‘œ .

4. Ascreen Half Lightlike Submanifolds

Definition 4.1. A half lightlike submanifold 𝑀 of an indefinite cosymplectic manifold 𝑀 is said to be an ascreen half lightlike submanifold [4] of 𝑀 if the structure vector field 𝜁 of 𝑀 belongs to the distribution R a d ( 𝑇 𝑀 ) βŠ• l t r ( 𝑇 𝑀 ) .

For any ascreen half lightlike submanifold 𝑀 , the vector field 𝜁 is decomposed as 𝜁 = π‘Ž πœ‰ + 𝑏 𝑁 . ( 4 . 1 ) In this case, we show that π‘Ž β‰  0 and 𝑏 β‰  0 by Proposition 3.2.

Definition 4.2. A half lightlike submanifold 𝑀 is called screen conformal [2, 3] if there exists a nonvanishing smooth function πœ‘ such that 𝐴 𝑁 = πœ‘ 𝐴 βˆ— πœ‰ , or equivalently, 𝐢 ( 𝑋 , 𝑃 π‘Œ ) = πœ‘ 𝐡 ( 𝑋 , π‘Œ ) , βˆ€ 𝑋 , π‘Œ ∈ Ξ“ ( 𝑇 𝑀 ) . ( 4 . 2 )

Theorem 4.3. Let 𝑀 be an ascreen half lightlike submanifold of an indefinite cosymplectic manifold 𝑀 . Then 𝑀 is screen conformal.

Proof. Applying βˆ‡ 𝑋 to (4.1) and using (2.3), (2.9), and (2.21), we have π‘Ž 𝐴 βˆ— πœ‰ 𝑋 + 𝑏 𝐴 𝑁 𝑋 = { 𝑋 π‘Ž βˆ’ π‘Ž 𝜏 ( 𝑋 ) } πœ‰ + { 𝑋 𝑏 + 𝑏 𝜏 ( 𝑋 ) } 𝑁 + { 𝑏 𝜌 ( 𝑋 ) βˆ’ π‘Ž πœ™ ( 𝑋 ) } 𝐿 . ( 4 . 3 ) Taking the product with πœ‰ , 𝑁 , and 𝐿 by turns and using (2.16)2 and (2.17)2, we get 𝐴 𝑁 𝑋 = πœ‘ 𝐴 βˆ— πœ‰ 𝑋 , 𝑋 π‘Ž = π‘Ž 𝜏 ( 𝑋 ) , 𝑋 𝑏 = βˆ’ 𝑏 𝜏 ( 𝑋 ) , π‘Ž πœ™ ( 𝑋 ) = 𝑏 𝜌 ( 𝑋 ) , ( 4 . 4 ) for all 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) , where we set πœ‘ = βˆ’ π‘Ž / 𝑏 . Thus 𝑀 is screen conformal.

Substituting (4.1) into 𝑔 ( 𝜁 , 𝜁 ) = 1 , we have 2 π‘Ž 𝑏 = 1 . Consider the local unit timelike vector field 𝑉 βˆ— on 𝑀 and its 1-form 𝑣 βˆ— defined by 𝑉 βˆ— = βˆ’ 𝑏 βˆ’ 1 𝐽 πœ‰ , 𝑣 βˆ— ξ€· ( 𝑋 ) = βˆ’ 𝑔 𝑋 , 𝑉 βˆ— ξ€Έ , βˆ€ 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . ( 4 . 5 ) Let π‘ˆ βˆ— = βˆ’ π‘Ž βˆ’ 1 𝐽 𝑁 . Then π‘ˆ βˆ— is a unit timelike vector field on 𝑆 ( 𝑇 𝑀 ) such that 𝑔 ( 𝑉 βˆ— , π‘ˆ βˆ— ) = 1 . Applying 𝐽 to (4.1) and using (2.1) and 2 π‘Ž 𝑏 = 1 , we have 𝑉 0 = π‘Ž 𝐽 πœ‰ + 𝑏 𝐽 𝑁 = βˆ’ βˆ— + π‘ˆ βˆ— 2 i . e . , π‘ˆ βˆ— = βˆ’ 𝑉 βˆ— . ( 4 . 6 ) From this we show that 𝐽 ( R a d ( 𝑇 𝑀 ) ) = 𝐽 ( l t r ( 𝑇 𝑀 ) ) . Using this and Proposition 3.1, the tangent bundle 𝑇 𝑀 of 𝑀 is decomposed as follows: 𝑇 𝑀 = R a d ( 𝑇 𝑀 ) βŠ• o r t h ξ€½ 𝐽 ( R a d ( 𝑇 𝑀 ) ) βŠ• o r t h 𝐽 ξ€· 𝑆 ξ€· 𝑇 𝑀 βŸ‚ βŠ• ξ€Έ ξ€Έ o r t h 𝐻 βˆ— ξ€Ύ , ( 4 . 7 ) where 𝐻 βˆ— is a nondegenerate and almost complex distribution on 𝑀 with respect to the indefinite cosymplectic structure tensor 𝐽 , otherwise 𝑆 ( 𝑇 𝑀 ) is degenerate. Consider the local unit spacelike vector field π‘Š βˆ— on 𝑆 ( 𝑇 𝑀 ) and its 1-form 𝑀 βˆ— defined by π‘Š βˆ— = βˆ’ 𝐽 𝐿 , 𝑀 βˆ— ξ€· ( 𝑋 ) = 𝑔 𝑋 , π‘Š βˆ— ξ€Έ , βˆ€ 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . ( 4 . 8 ) Denote by 𝑆 βˆ— the projection morphism of 𝑇 𝑀 on 𝐻 βˆ— . Using (4.7), for any vector field 𝑋 on 𝑀 , the vector field 𝐽 𝑋 is expressed as follows: 𝐽 𝑋 = 𝑓 𝑋 + π‘Ž 𝑣 βˆ— ( 𝑋 ) πœ‰ βˆ’ 𝑏 πœ‚ ( 𝑋 ) 𝑉 βˆ— βˆ’ 𝑏 𝑣 βˆ— ( 𝑋 ) 𝑁 + 𝑀 βˆ— ( 𝑋 ) 𝐿 , ( 4 . 9 ) because 𝐽 𝑉 βˆ— = π‘Ž πœ‰ βˆ’ 𝑏 𝑁 , where 𝑓 is a tensor field of type (1, 1) defined by 𝑓 𝑋 = 𝐽 𝑆 βˆ— 𝑋 , βˆ€ 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . ( 4 . 1 0 ) Applying 𝐽 to (2.10) and (2.21) and using (2.2), (2.8) and (4.4) ∼ (4.9), we get 𝑏 βˆ‡ 𝑋 𝑉 βˆ— ξ‚€ 𝐴 = 𝑓 βˆ— πœ‰ 𝑋  ξ€· βˆ’ π‘Ž 𝐡 𝑋 , 𝑉 βˆ— ξ€Έ πœ‰ βˆ’ πœ™ ( 𝑋 ) π‘Š βˆ— βˆ‡ , ( 4 . 1 1 ) 𝑋 π‘Š βˆ— ξ€· 𝐴 = 𝑓 𝐿 𝑋 ξ€Έ ξ€· βˆ’ π‘Ž 𝐷 𝑋 , 𝑉 βˆ— ξ€Έ πœ‰ βˆ’ 2 π‘Ž πœ™ ( 𝑋 ) 𝑉 βˆ— , ξ€· ( 4 . 1 2 ) 𝑏 𝐷 𝑋 , 𝑉 βˆ— ξ€Έ ξ€· = 𝐡 𝑋 , π‘Š βˆ— ξ€Έ , βˆ€ 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . ( 4 . 1 3 )

Example 4.4. Consider a submanifold 𝑀 of 𝑀 = ( 𝑅 5 2 , 𝐽 , 𝜁 , πœƒ , 𝑔 ) given by the equation 𝑋 ξ€· 𝑒 1 , 𝑒 2 , 𝑒 3 ξ€Έ =  𝑒 1 , 𝑒 2 , 𝑒 3 , 𝑒 2 , 1 √ 2 ξ€· 𝑒 1 + 𝑒 3 ξ€Έ ξƒͺ . ( 4 . 1 4 ) By direct calculations we easily check that  𝑇 𝑀 = S p a n πœ‰ = πœ• π‘₯ 1 + πœ• 𝑦 1 + √ 2 πœ• 𝑧 , π‘ˆ = πœ• π‘₯ 1 βˆ’ πœ• 𝑦 1 , 𝑉 = πœ• π‘₯ 2 + πœ• 𝑦 2  , 𝑇 𝑀 βŸ‚ ξ€½ = S p a n πœ‰ , 𝐿 = πœ• π‘₯ 2 βˆ’ πœ• 𝑦 2 ξ€Ύ , R a d ( 𝑇 𝑀 ) = S p a n { πœ‰ } . ( 4 . 1 5 ) We obtain the lightlike transversal and transversal vector bundles  1 l t r ( 𝑇 𝑀 ) = S p a n 𝑁 = 4 ξ‚€ βˆ’ πœ• π‘₯ 1 βˆ’ πœ• 𝑦 1 + √ 2 πœ• 𝑧   , t r ( 𝑇 𝑀 ) = S p a n { 𝑁 , 𝐿 } . ( 4 . 1 6 ) From this results, we show that 𝐽 πœ‰ = π‘ˆ , R a d ( 𝑇 𝑀 ) ∩ 𝐽 ( R a d ( 𝑇 𝑀 ) ) = { 0 } , 𝐽 𝑁 = βˆ’ ( 1 / 4 ) π‘ˆ , 𝐽 𝐿 = βˆ’ 𝑉 , 𝐽 𝑁 = βˆ’ ( 1 / 4 ) 𝐽 πœ‰ and 𝐽 ( R a d ( 𝑇 𝑀 ) = 𝐽 ( l t r ( 𝑇 𝑀 ) , √ 𝜁 = ( 1 / 2 √ 2 ) πœ‰ + 2 𝑁 and 𝐽 𝜁 = 0 . Thus 𝑀 is an ascreen half lightlike submanifold of an indefinite cosymplectic manifold 𝑀 .

Theorem 4.5. Let 𝑀 be an ascreen half lightlike submanifold of an indefinite cosymplectic manifold 𝑀 . If 𝑀 is totally umbilical, then 𝑀 and 𝑆 ( 𝑇 𝑀 ) are totally geodesic.

Proof. Assume that 𝑀 is totally umbilical. From (3.25) and (4.13), we have ξ€· 𝑏 𝛿 𝑔 𝑋 , 𝑉 βˆ— ξ€Έ ξ€· = 𝛽 𝑔 𝑋 , π‘Š βˆ— ξ€Έ , βˆ€ 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . ( 4 . 1 7 ) Replacing 𝑋 by π‘Š βˆ— and 𝑉 βˆ— to this equation by turns, we have 𝛽 = 0 and 𝛿 = 0 , respectively. Thus we have β„Ž = 0 and 𝑀 is totally geodesic. By (4.2), we also have 𝐢 = 0 . Thus 𝑆 ( 𝑇 𝑀 ) is also totally geodesic in 𝑀 .

Taking π‘Œ ∈ Ξ“ ( 𝐻 βˆ— ) . Then we have 𝑓 π‘Œ = 𝐽 π‘Œ ∈ Ξ“ ( 𝐻 βˆ— ) due to (4.9). Applying βˆ‡ 𝑋 to 𝐽 π‘Œ = 𝑓 π‘Œ and using (2.2), (2.8), (4.2), (4.5), and (4.9), we have 𝐡 ξ€· βˆ‡ ( 𝑋 , 𝑓 π‘Œ ) = 𝑏 𝑔 𝑋 π‘Œ , 𝑉 βˆ— ξ€Έ ξ€· βˆ‡ , 𝐷 ( 𝑋 , 𝑓 π‘Œ ) = 𝑔 𝑋 π‘Œ , π‘Š βˆ— ξ€Έ ξ€· βˆ‡ , ( 4 . 1 8 ) 𝑋 𝑓 ξ€Έ ξ€· βˆ‡ π‘Œ = βˆ’ π‘Ž 𝑔 𝑋 π‘Œ , 𝑉 βˆ— ξ€Έ πœ‰ + 2 π‘Ž 𝐡 ( 𝑋 , π‘Œ ) 𝑉 βˆ— βˆ’ 𝐷 ( 𝑋 , π‘Œ ) π‘Š βˆ— , ( 4 . 1 9 ) for all 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . By the procedure same as the proofs of Theorem 3.10 and Theorem 3.11 and by using (4.18) and (4.19), instead of (3.29) and (3.30), and that 𝑆 ( 𝑇 𝑀 ) is integrable due to (4.2), the following two theorems hold.

Theorem 4.6. Let 𝑀 be an ascreen half lightlike submanifold of an indefinite cosymplectic manifold 𝑀 . 𝐻 βˆ— is an integrable distribution on 𝑀 if and only if one has β„Ž ξ€· 𝐻 ( 𝑋 , 𝑓 π‘Œ ) = β„Ž ( 𝑓 𝑋 , π‘Œ ) , βˆ€ 𝑋 , π‘Œ ∈ Ξ“ βˆ— ξ€Έ . ( 4 . 2 0 ) Moreover, if 𝑀 is totally umbilical, then 𝐻 βˆ— is a parallel distribution on 𝑀 .

Theorem 4.7. Let 𝑀 be an ascreen half lightlike submanifold of an indefinite cosymplectic manifold 𝑀 . Then 𝑓 is parallel on 𝐻 βˆ— with respect to the induced connection βˆ‡ if and only if 𝐻 βˆ— is a parallel distribution on 𝑀 .

Theorem 4.8. Let 𝑀 be an ascreen half lightlike submanifold of an indefinite cosymplectic manifold 𝑀 . If 𝑀 is totally umbilical, then 𝑀 is locally a product manifold 𝐿 πœ‰ Γ— 𝐿 𝑉 βˆ— Γ— 𝐿 π‘Š βˆ— Γ— 𝑀 βˆ— , where 𝐿 πœ‰ , 𝐿 𝑉 βˆ— , and 𝐿 π‘Š βˆ— are null, timelike, and spacelike curves tangent to R a d ( 𝑇 𝑀 ) , 𝐽 ( R a d ( 𝑇 𝑀 ) ) , and 𝐽 ( 𝑆 ( 𝑇 𝑀 βŸ‚ ) ) , respectively, and 𝑀 βˆ— is a leaf of 𝐻 βˆ— .

Proof. If 𝑀 is totally umbilical, then 𝐻 βˆ— is a parallel distribution on 𝑀 by Theorem 4.6 and we have 𝐡 = 𝐷 = 𝐴 βˆ— πœ‰ = πœ™ = 0 ; 𝐴 𝐿 𝑋 = 𝜌 ( 𝑋 ) πœ‰ by Theorem 4.5. From (4.4)1, we also have 𝐴 𝑁 = 0 . Using (2.12), (4.11), and (4.12), we have βˆ‡ 𝑋 πœ‰ = βˆ’ 𝜏 ( 𝑋 ) πœ‰ and βˆ‡ 𝑋 𝑉 βˆ— = βˆ‡ 𝑋 π‘Š βˆ— = 0 due to 𝑓 πœ‰ = 0 . This implies that all of the distributions R a d ( 𝑇 𝑀 ) , 𝐽 ( R a d ( 𝑇 𝑀 ) ) , and 𝐽 ( 𝑆 ( 𝑇 𝑀 βŸ‚ ) ) are parallel on 𝑀 . Thus we have 𝑀 = 𝐿 πœ‰ Γ— 𝐿 𝑉 βˆ— Γ— 𝐿 π‘Š βˆ— Γ— 𝑀 βˆ— , where 𝐿 πœ‰ , 𝐿 𝑉 βˆ— , and 𝐿 π‘Š βˆ— are null, timelike, and spacelike curves tangent to R a d ( 𝑇 𝑀 ) , 𝐽 ( R a d ( 𝑇 𝑀 ) ) and 𝐽 ( 𝑆 ( 𝑇 𝑀 βŸ‚ ) ) , respectively, and 𝑀 βˆ— is a leaf of 𝐻 βˆ— .

By straightforward calculations from (4.11) and (4.12) and the same method as the proof of Theorem 3.14, the following theorem holds.

Theorem 4.9. Let 𝑀 be an ascreen half lightlike submanifold of an indefinite cosymplectic manifold 𝑀 . Then one has the following assertions.(i)If 𝑉 βˆ— is parallel with respect to βˆ‡ on 𝑀 , then 𝑀 is irrotational and 𝐴 βˆ— πœ‰ ξ€· 𝑋 = 𝐡 𝑋 , π‘Š βˆ— ξ€Έ π‘Š βˆ— ξ€· , 𝐡 𝑋 , 𝑉 βˆ— ξ€Έ = 0 , 𝜌 ( 𝑋 ) = 0 , βˆ€ 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . ( 4 . 2 1 ) (ii)If π‘Š βˆ— is parallel with respect to βˆ‡ on 𝑀 , then 𝑀 is irrotational and 𝐴 𝐿 ξ€· 𝑋 = 𝐷 𝑋 , π‘Š βˆ— ξ€Έ π‘Š βˆ— ξ€· , 𝐷 𝑋 , 𝑉 βˆ— ξ€Έ = 0 , 𝜌 ( 𝑋 ) = 0 , βˆ€ 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . ( 4 . 2 2 ) Moreover, if 𝑉 βˆ— and π‘Š βˆ— are parallel with respect to βˆ‡ , then one sees that 𝐴 βˆ— πœ‰ = 0 and the screen distribution 𝑆 ( 𝑇 𝑀 ) is totally geodesic in 𝑀 .

Theorem 4.10. Let 𝑀 be an ascreen half lightlike submanifold of an indefinite cosymplectic manifold 𝑀 . If 𝑉 βˆ— and π‘Š βˆ— are parallel with respect to βˆ‡ , then 𝑀 is locally a product manifold 𝐿 πœ‰ Γ— 𝐿 𝑉 βˆ— Γ— 𝐿 π‘Š βˆ— Γ— 𝑀 βˆ— , where 𝐿 πœ‰ , 𝐿 𝑉 βˆ— , and 𝐿 π‘Š βˆ— are null, timelike, and spacelike curves tangent to R a d ( 𝑇 𝑀 ) , 𝐽 ( R a d ( 𝑇 𝑀 ) ) , and 𝐽 ( 𝑆 ( 𝑇 𝑀 βŸ‚ ) ) , respectively, and 𝑀 βˆ— is a leaf of 𝐻 βˆ— .

Proof. If 𝑉 βˆ— is parallel with respect to βˆ‡ , for any π‘Œ ∈ Ξ“ ( 𝐻 βˆ— ) , we have ξ‚€ 𝐴 𝐡 ( 𝑋 , π‘Œ ) = 𝑔 βˆ— πœ‰  ξ€· 𝑋 , π‘Œ = 𝐡 𝑋 , π‘Š βˆ— ξ€Έ 𝑔 ξ€· π‘Œ , π‘Š βˆ— ξ€Έ = 0 , βˆ€ 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . ( 4 . 2 3 ) Thus we get 𝑔 ( βˆ‡ 𝑋 π‘Œ , 𝑉 βˆ— ) = 𝑏 βˆ’ 1 𝐡 ( 𝑋 , 𝑓 π‘Œ ) = 0 because 𝑓 π‘Œ ∈ Ξ“ ( 𝐻 βˆ— ) . Also if π‘Š βˆ— is parallel with respect to βˆ‡ , then, for any π‘Œ ∈ Ξ“ ( 𝐻 βˆ— ) , we have 𝐷 ξ€· 𝐴 ( 𝑋 , π‘Œ ) = 𝑔 𝐿 ξ€Έ ξ€· 𝑋 , π‘Œ = 𝐷 𝑋 , π‘Š βˆ— ξ€Έ 𝑔 ξ€· π‘Œ , π‘Š βˆ— ξ€Έ = 0 , βˆ€ 𝑋 ∈ Ξ“ ( 𝑇 𝑀 ) . ( 4 . 2 4 ) From these results and (4.19), we show that 𝑓 is parallel on 𝐻 βˆ— with respect to βˆ‡ . Thus, by Theorem 4.7, we see that 𝐻 βˆ— is a parallel distribution on 𝑀 . As 𝑉 βˆ— and π‘Š βˆ— are parallel with respect to βˆ‡ and βˆ‡ 𝑋 πœ‰ = βˆ’ 𝜏 ( 𝑋 ) πœ‰ due to 𝐴 βˆ— πœ‰ = 0 , we have our theorem.

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