Research article

Lorentzian approximations for a Lorentzian α-Sasakian manifold and Gauss-Bonnet theorems

  • Received: 29 May 2022 Revised: 16 September 2022 Accepted: 25 September 2022 Published: 09 October 2022
  • MSC : 53C40, 53C42

  • In this paper, we define the Lorentzian approximations of a 3-dimensional Lorentzian α-Sasakian manifold. Moreover, we define the notions of the intrinsic curvature for regular curves, the intrinsic geodesic curvature of regular curves on Lorentzian surfaces and spacelike surfaces and the intrinsic Gaussian curvature of Lorentzian surfaces and spacelike surfaces away from characteristic points. Furthermore, we derive the expressions of those curvatures and prove Gauss-Bonnet theorems for the Lorentzian surfaces and spacelike surfaces in the Lorentzian α-Sasakian manifold.

    Citation: Haiming Liu, Xiawei Chen, Jianyun Guan, Peifu Zu. Lorentzian approximations for a Lorentzian α-Sasakian manifold and Gauss-Bonnet theorems[J]. AIMS Mathematics, 2023, 8(1): 501-528. doi: 10.3934/math.2023024

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  • In this paper, we define the Lorentzian approximations of a 3-dimensional Lorentzian α-Sasakian manifold. Moreover, we define the notions of the intrinsic curvature for regular curves, the intrinsic geodesic curvature of regular curves on Lorentzian surfaces and spacelike surfaces and the intrinsic Gaussian curvature of Lorentzian surfaces and spacelike surfaces away from characteristic points. Furthermore, we derive the expressions of those curvatures and prove Gauss-Bonnet theorems for the Lorentzian surfaces and spacelike surfaces in the Lorentzian α-Sasakian manifold.



    Lorentzian α-Sasakian manifolds were introduced by Yildiz and Murathan in [1]. Then, many researchers began to study properties of α-Sasakian manifolds, such as second order parallel tensors [2], pseudosymmetric Lorentzian α-Sasakian manifolds [3], some special classes of Lorentzian α-Sasakian manifolds [4,5,6], certain derivations [7], Ricci solitons [8,9], Lorentzian α-Sasakian manifolds admitting a quarter-symmetric metric connection [10], semi-symmetry type α-Sasakian manifolds [11] and M-projectively semi-symmetric Lorentzian α-Sasakian manifolds [12]. Recently, Wang studied Gauss-Bonnet theorems in the BCV spaces and the twisted Heisenberg group [13], the affine group and the group of rigid motions of the Minkowski plane [14] by using the method of Riemannian approximations which first took by Balogh, Tyson and Vecchi to prove a Heisenberg version of the Gauss-Bonnet theorem[15,16]. Riemannian approximations can be extended to the case for any Lie group equipped with left-invariant Lorentzian metric g, named Lorentzian approximations. Some typical works of Lorentzian approximations in a Lorentzian Heisenberg group are obtained in [17,18]. Inspired by the above work, we proved Gauss-Bonnet theorems in the rototranslation group [19,20], Lorentzian Sasakian space forms [21] and the group of rigid motions of the Minkowski plane with the general left-invariant metric [22]. However, very little is known about the Gauss-Bonnet theorem in 3-dimensional Lorentzian α-Sasakian manifolds. This paper attempts to solve this question by employing the method of the Lorentzian approximation scheme.

    We restrict our attention to Lorentzian α-Sasakian manifolds. As we know, in [8], a differentiable manifold of dimension (2n+1) is called a Lorentzian α-Sasakian manifold if it admits a (1,1) tensor field ϕ, a vector field ξ, 1-form η and Lorentzian metric g which satisfy on M, respectively, that

    ϕ2=I+ηξ,η(ξ)=1,ηϕ=0,ϕξ=0,
    g(ϕX,ϕY)=g(X,Y)+η(X)η(Y),g(X,ξ)=η(X),
    Xξ=αϕX,(Xη)Y=αg(ϕX,Y),

    where denotes the operator of covariant differentiation with respect to the Lorentzian metric g on M. Meanwhile, a Lorentzian α-Sasakian model of 3-dimensional Lorentzian α-Sasakian manifolds was constructed in [8]. In this paper, we focus on Gauss-Bonnet theorems for the Lorentzian surfaces and spacelike surfaces in the Lorentzian α-Sasakian model. We define the notions of the intrinsic curvature for regular curves, the intrinsic geodesic curvature of regular curves on Lorentzian surfaces and spacelike surfaces and the intrinsic Gaussian curvature of Lorentzian surfaces and spacelike surfaces away from characteristic points. Furthermore, we derive the expressions of those curvatures and prove Gauss-Bonnet theorems for the Lorentzian surfaces and spacelike surfaces in the 3-dimensional Lorentzian α-Sasakian manifold.

    The paper is organized in the following way. Basic notions on (Sα,g) and the Lorentzian approximants (Sα,gL) of the α-Sasakian manifold are given in Section 2. The sub-Lorentzian limit of curvature of curves in (Sα,gL) will be computed. In Sections 3 and 4, we compute sub-Lorentzian limits of geodesic curvature of curves on Lorentzian surfaces and the intrinsic Gaussian curvature of Lorentzian surfaces in (Sα,gL). In Section 5, we prove the Gauss-Bonnet theorem for Lorentzian surfaces. In Section 6, we prove the Gauss-Bonnet theorem for spacelike surfaces. Finally, we summarize the conclusions and add an appendix section on length measure and surface measure.

    In this section, some basic notions on a Lorentzian α-Sasakian manifold will be introduced. First, we recall the Lorentzian α-Sasakian model of 3-dimensional Lorentzian α-Sasakian manifolds constructed in [8]. Let α be some constant, and set Sα={(x,y,z)R3|z>0} equipped with a Lorentzian metric

    g=e2zdx2+e2z(dx+dy)21α2dz2.

    Then, (Sα,g) was called the Lorentzian α-Sasakian model of 3-dimensional Lorentzian α-Sasakian manifold, where (x,y,z) are the standard coordinates of R3. Let E1,E2 and E3 be the vector fields on Sα given by

    E1=αz, E2=ez(x+y), E3=ezy, (2.1)

    which are linearly independent at each point p of Sα. Then,

    x=ez(E2E3), y=ezE3, z=1αE1, (2.2)

    and span{E1,E2,E3}=T(Sα). One can check the following brackets

    [E1,E2]=αE2, [E2,E3]=0, [E1,E3]=αE3. (2.3)

    Let H=span{E1,E2} be the horizontal distribution on Sα. If we let

    θ1=1αdz,θ2=ezdx,θ=ez(dx+dy),

    then H=kerθ. To describe the Lorentzian approximants of Sα, let L>0 and define a metric

    gL=θ1θ1+θ2θ2+Lθθ,

    so that E1,E2,~E3:=L12E3 are a pseudo orthonormal basis on T(Sα) with respect to gL. Hereafter, we denote the Lorentzian approximants to Sα by (Sα,gL) and write SLα instead of (Sα,gL). Note that g=g1 is the Lorentzian metric on Sα. A non-zero vector xSLα is called spacelike, null or timelike if x,x>0, x,x=0 or x,x<0, respectively. We define the norm of the vector xSLα by x∥=x,x. We assume that L is the Levi-civita connection on SLα with respect to gL. Using the Koszul formula and (2.3), we have

    Proposition 2.1. The Levi-civita connection on SLα relative to the coordinate frame E1,E2,~E3 is given by

    LE1E1=0, LE1E2=0, LE1E3=0,LE2E1=αE2, LE2E2=αE1, LE2E3=0,LE3E1=αE3, LE3E2=0, LE3E3=αLE1. (2.4)

    Proof. It follows from a direct application of the Koszul identity, which here simplifies

    2LEiEj,EkL=[Ei,Ej],EkL[Ej,Ek],EiL+[Ek,Ei],EjL, (2.5)

    where i,j,k=1,2,3.

    For a Lorentzian α-Sasakian manifold M, one can compute the curvature tensor of the connection L by the formula RL(X,Y)Z=LXLYZLYLXZL[X,Y]Z or RL(X,Y)Z=α2[g(Y,Z)Xg(X,Z)Y]. Then, we get the following proposition.

    Proposition 2.2. The curvature tensor of SLα is given by

    RL(E1,E2)E1=α2E2, RL(E1,E2)E2=α2E1, RL(E1,E2)E3=0,RL(E1,E3)E1=α2E3, RL(E1,E3)E2=0, RL(E1,E3)E3=α2LE1,RL(E2,E3)E1=0, RL(E2,E3)E2=α2E3, RL(E2,E3)E3=α2LE2. (2.6)

    Proof. We take RL(X,Y)Z=α2[g(Y,Z)Xg(X,Z)Y] to compute curvature tensor of SLα. Taking

    RL(E1,E2)E1=α2[g(E2,E1)E1g(E1,E1)E2],

    for example, we compute

    g(E2,E1)E1=0,g(E1,E1)E2=E2,

    and hence

    RL(E1,E2)E1=α2E2.

    In this section, we will compute the sub-Lorentzian limit of curvature for curves in SLα. Our approach is to define sub-Lorentzian objects as limits of horizontal objects in SLα, where a family of metrics gL is essentially obtained as an anisotropic blow-up of the Lorentzian metric g. At the heart of this approach is the fact that the intrinsic horizontal geometry does not change with L. Let β:ISLα be a regular curve, where I is an open interval in R. The regular curve β is called a spacelike curve, timelike curve or null curve if ˙β(t) is a spacelike vector, timelike vector or null vector at any tI, respectively.

    Definition 3.1. Let β:ISLα be a C1 smooth curve, and we say that β is regular if ˙β0 for every tI. Moreover we say that β(t) is a horizontal point of β if

    θ(˙β(t))=eβ3(˙β2(t)˙β1(t))=0,

    where β(t)=(β1(t),β2(t),β3(t)).

    As is well known, if β is a curve with arc length parametrization, then the standard definition of curvature for β in Riemannian geometry is κLβ:=L˙β˙βL. If β is a curve with an arbitrary parametrization, then we give the definitions as follows:

    Definition 3.2. Let β:ISLα be a C2-smooth regular curve.

    (1) If L˙β˙β is a spacelike vector, we define the curvature κLβ of β at β(t) by

    κLβ:=L˙β˙β2L˙β4LL˙β˙β,˙β2L˙β,˙β3L. (3.1)

    (2) If L˙β˙β is a timelike vector, we define the curvature κLβ of β at β(t) by

    κLβ:=L˙β˙β2L˙β4L+L˙β˙β,˙β2L˙β,˙β3L. (3.2)

    Proposition 3.3. Suppose that β:ISLα is a C2-smooth regular curve.

    (1) If L˙β˙β is a spacelike vector, then

    κLβ={{[1α¨β3+αe2β3˙β21+αL(θ(˙β(t)))2]2+[2˙β3˙β1eβ3+eβ3¨β1]2+L[˙β3θ(˙β(t))+ddt(θ(˙β(t)))]2}×[1α2˙β32+e2β3˙β21+L(θ(˙β(t)))2]2{1α˙β3[1α¨β3+αe2β3˙β21+αL(θ(˙β(t)))2]+eβ3˙β1[2˙β3˙β1eβ3+eβ3¨β1]+Lθ(˙β(t))[˙β3θ(˙β(t))+ddt(θ(˙β(t)))]}2×[1α2˙β32+e2β3˙β21+L(θ(˙β(t)))2]3}12. (3.3)

    In particular, if β(t) is a horizontal point of β,

    κLβ={{[1α¨β3+αe2β3˙β21]2+[2˙β3˙β1eβ3+eβ3¨β1]2+L[ddt(θ(˙β(t)))]2}×[1α2˙β32+e2β3˙β21]2{1α˙β3[1α¨β3+αe2β3˙β21]+eβ3˙β1[2˙β3˙β1eβ3+eβ3¨β1]}2×[1α2˙β32+e2β3˙β21]3}12. (3.4)

    (2) If L˙β˙β is a timelike vector, then

    κLβ={{[1α¨β3+αe2β3˙β21+αL(θ(˙β(t)))2]2+[2˙β3˙β1eβ3+eβ3¨β1]2+L[(˙β3θ(˙β(t)))+ddt(θ(˙β(t)))]2}×[1α2˙β32+e2β3˙β21+L(θ(˙β(t)))2]2+{1α˙β3[1α¨β3+αe2β3˙β21+αL(θ(˙β(t)))2]+eβ3˙β1[2˙β3˙β1eβ3+eβ3¨β1]+Lθ(˙β(t))[˙β3θ(˙β(t))+ddt(θ(˙β(t)))]}2×[1α2˙β32+e2β3˙β21+L(θ(˙β(t)))2]3}12. (3.5)

    In particular, if β(t) is a horizontal point of β,

    κLβ={{[1α¨β3+αe2β3˙β21]2+[2˙β3˙β1eβ3+eβ3¨β1]2+L[ddt(θ(˙β(t)))]2}×[1α2˙β32+e2β3˙β21]2+{1α˙β3[1α¨β3+αe2β3˙β21]+eβ3˙β1[2˙β3˙β1eβ3+eβ3¨β1]}2×[1α2˙β32+e2β3˙β21]3}12. (3.6)

    Proof. By (2.2), we have

    ˙β(t)=1α˙β3E1+eβ3˙β1E2+θ (˙β(t))E3. (3.7)

    By Proposition 2.1 and (3.7), we obtain

    L˙βE1=αeβ3˙β1E2+αθ(˙β(t))E3,
    L˙βE2=αeβ3˙β1E1,
    L˙βE3=αLθ(˙β(t))E1. (3.8)

    Coming by (3.7), we have

    L˙β˙β=[1α¨β3+αe2β3˙β21+αL(θ(˙β(t)))2]E1+[2˙β3˙β1eβ3+eβ3¨β1]E2+[˙β3θ(˙β(t))+ddt(θ(˙β(t)))]E3. (3.9)

    By (3.7), (3.9), and the definition of κLβ, we get Proposition 3.3.

    Definition 3.4. Let β:ISLα be a C2-smooth regular curve. We define the intrinsic curvature κβ of β at β(t) to be

    κβ:=limLκLβ,

    if the limit exists.

    We introduce the following notation : For continuous functions f1,f2:(0,+)R,

    f1(L)f2(L), as L+limLf1(L)f2(L)=1.

    Proposition 3.5. Suppose that β:ISLα is a C2-smooth regular curve in the Lorentzian α-Sasakian manifold.

    (1) If L˙β˙β is a spacelike vector, then κβ does not exist, if θ(˙β(t))0.

    κβ={{[1α¨β3+αe2β3˙β21]2+[2˙β3˙β1eβ3+eβ3¨β1]2}×[1α2˙β32+e2β3˙β21]2{1α˙β3[1α¨β3+αe2β3˙β21]+eβ3˙β1[2˙β3˙β1eβ3+eβ3¨β1]}2×[1α2˙β32+e2β3˙β21]3}12, (3.10)

    if θ(˙β(t))=0 and ddt(θ(˙β(t)))=0.

    limLκLβL=|ddt(θ(˙β(t)))||1α2˙β32+e2β3˙β21|,if θ(˙β(t))=0 and ddt(θ(˙β(t)))0. (3.11)

    (2) If L˙β˙β is a timelike vector, then

    κβ=∣α,if θ(˙β(t))0. (3.12)
    κβ={{[1α¨β3+αe2β3˙β21]2+[2˙β3˙β1eβ3+eβ3¨β1]2}×[1α2˙β32+e2β3˙β21]2+{1α˙β3[1α¨β3+αe2β3˙β21]+eβ3˙β1[2˙β3˙β1eβ3+eβ3¨β1]}2×[1α2˙β32+e2β3˙β21]3}12, (3.13)

    if θ(˙β(t))=0 and ddt(θ(˙β(t)))=0.

    limLκLβL=[ddt(θ(˙β(t)))]2|1α2˙β32+e2β3˙β21|,if θ(˙β(t))=0 and ddt(θ(˙β(t)))0. (3.14)

    Therefore, this situation does not exist.

    Proof. (1) If L˙β˙β is a spacelike vector, we have

    L˙ββ,L˙ββLα2L2(θ(˙β(t)))4 as L+,
    ˙β,˙βLL[θ(˙β(t))]2, L˙β˙β,˙β2LO(L2) as L+.

    Thus,

    L˙ββ,L˙ββL˙β4Lα2 as L+,
    L˙β˙β,˙β2L˙β,˙β3L0 as L+,
    κβ=α2.

    So, using (3.1), we know κβ does not exist, if θ(˙β(t))0. If θ(˙β(t))=0 and ddt(θ(˙β(t)))=0, we get (3.10). If θ(˙β(t))=0 and ddt(θ(˙β(t)))0, then

    L˙ββ,L˙ββLL[ddt(θ(˙β(t)))]2 as L+,
    ˙β,˙βL=1α2˙β32+e2β3˙β12,
    L˙β˙β,˙β2LO(1) as L+.

    By (3.1), we get (3.11).

    (2) If L˙β˙β is a timelike vector, we have

    L˙ββ,L˙ββLα2L2(θ(˙β(t)))4 as L+,
    ˙β,˙βLL[θ(˙β(t))]2, L˙β˙β,˙β2LO(L2) as L+,
    κβ=α2=∣α.

    We get (3.12). If θ(˙β(t))=0 and ddt(θ(˙β(t)))=0, we get (3.13). If θ(˙β(t))=0 and ddt(θ(˙β(t)))0,

    limLκLβL=[ddt(θ(˙β(t)))]2|1α2˙β32+e2β3˙β21|,

    and then, the situation does not exist.

    In this section, we will compute the expressions of intrinsic geodesic curvatures of curves on Lorentzian surfaces in SLα. We will say that a surface SLα is regular if S is a C2-smooth compact and oriented surface. In particular we will assume that there exists a C2-smooth function h:SLαR such that

    S={(x1,x2,x3)SLα:h(x1,x2,x3)=0},

    and SLαh=hx1x1+hx2x2+hx3x30. Let Hh=E1(h)E1+E2(h)E2. A point xS is called characteristic if Hh(x)=(0,0). Our computations will be local and away from characteristic points of S. Let us define first p:=E1h,q:=E2h, and r:=~E3h. Since p2+q2>0, we say SSLα is a horizontal spacelike surface. When L+, p2+q2+r2>0. Then, we define

    l:=p2+q2,lL:=p2+q2+r2,ˉp:=pl,ˉq:=ql,¯pL:=plL,¯qL:=qlL,¯rL:=rlL. (4.1)

    In particular, ˉp2+ˉq2=1. These functions are well defined at every non-characteristic point. Let

    NL=¯pLE1+¯qLE2+¯rL~E3,F1=ˉqE1ˉpE2,F2=¯rLˉpE1¯rLˉqE2+llL~E3. (4.2)

    Then, NL is the unit spacelike normal vector to S, and F1 is a unit timelike vector, while F2 is a unit spacelike vector of S. {F1,F2} is the orthonormal basis of S. Let ˙β=aF1+bF2. We define JL(˙β)=aF2+bF1 if β is a C2-smooth spacelike curve, and we define JL(˙β)=aF2bF1 if β is a C2-smooth timelike curve. Then, gL(˙β,JL(˙β))=0 and (˙β,JL(˙β)) have the same orientation with {F1,F2}.

    For every U,VTS, we define S,LUV=πLUV where π:TSLαTS is the projection. Then, S,L is the Levi-Civita connection on S with respect to the metric gL. By (3.9), (4.2) and

    S,L˙β˙β=L˙β˙β,F1LF1+L˙β˙β,F2LF2, (4.3)

    we have

    S,L˙β˙β={ˉq[1α¨β3+αe2β3˙β21+αL(θ(˙β(t)))2]ˉp[2˙β3˙β1eβ3+eβ3¨β1]}F1+{¯rLˉp[1α¨β3+αe2β3˙β21+αL(θ(˙β(t)))2]¯rLˉq[2˙β3˙β1eβ3+eβ3¨β1]+llLL12[˙β3θ(˙β(t))+ddt(θ(˙β(t)))]}F2. (4.4)

    Therefore, when θ(˙β(t))=0, we have

    S,L˙β˙β={ˉq[1α¨β3+αe2β3˙β21]+ˉp[2˙β3˙β1eβ3+eβ3¨β1]}F1+{¯rLˉp[1α¨β3+αe2β3˙β21]¯rLˉq[2˙β3˙β1eβ3+eβ3¨β1]+llLL12ddt(θ(˙β(t)))}F2. (4.5)

    Definition 4.1. Let SSLα be a Lorentzian regular surface, β:IS be a C2-smooth regular curve.

    (1) If S,L˙β˙β is a spacelike vector, the geodesic curvature κLβ,S of β at β(t) is defined as

    κLβ,S:=S,L˙β˙β2S,L˙β4S,LS,L˙β˙β,˙β2S,L˙β,˙β3S,L. (4.6)

    (2) If S,L˙β˙β is a timelike vector, the geodesic curvature κLβ,S of β at β(t) is defined as

    κLβ,S:=S,L˙β˙β2S,L˙β4S,L+S,L˙β˙β,˙β2S,L˙β,˙β3S,L. (4.7)

    Definition 4.2. Let SSLα be a Lorentzian regular surface, β:IS be a C2-smooth regular curve. We define the intrinsic geodesic curvature κβ,S of β at β(t) to be

    κβ,S:=limL+κLβ,S,

    if the limit exists.

    Proposition 4.3. Let SSLα be a Lorentzian regular surface, β:IS be a C2-smooth regular curve.

    (1) If S,L˙β˙β is a spacelike vector, then κβ,S does not exist, if θ(˙β(t))0.

    κβ,S=0, if θ(˙β(t))=0 and ddt(θ(˙β(t)))=0,
    limL+κLβ,SL=|ddt(θ(˙β(t)))|(1αˉq˙β3+eβ3ˉp˙β1)2, if θ(˙β(t))=0 and ddt(θ(˙β(t)))0. (4.8)

    (2) If S,L˙β˙β is a timelike vector, then

    κβ,S=∣αˉq, if θ(˙β(t))0, (4.9)
    κβ,S=0, if θ(˙β(t))=0 and ddt(θ(˙β(t)))=0,

    limL+κLβ,SL does not exist, if θ(˙β(t))=0 and ddt(θ(˙β(t)))0.

    Proof. (1) If S,L˙β˙β is a spacelike vector, by (3.7) and ˙βTS, we have

    ˙β(t)=aF1+bF2=(aˉq+b¯rLˉp)E1+(aˉpb¯rLˉq)E2+bllLL12E3.

    Thus,

    {aˉq+b¯rLˉp=1α˙β3,aˉpb¯rLˉq=eβ3˙β1,bllLL12=θ(˙β(t)),

    and we have

    {a=1α˙β3ˉq+eβ3˙β1ˉp,b=lLlL12θ(˙β(t)).

    Thus,

    ˙β(t)=(1α˙β3ˉq+eβ3˙β1ˉp)F1+lLlL12θ(˙β(t))F2. (4.10)

    By (4.4), we have

    S,L˙β˙β,S,L˙β˙βS,L={ˉq[1α¨β3+αe2β3˙β21+αL(θ(˙β(t)))2]ˉp[2˙β3˙β1eβ3+eβ3¨β1]}2+{¯rLˉp[1α¨β3+αe2β3˙β21+αL(θ(˙β(t)))2]¯rLˉq[2˙β3˙β1eβ3+eβ3¨β1]+llLL12[˙β3θ(˙β(t))+ddt(θ(˙β(t)))]}2. (4.11)

    Similarly, we have that when θ(˙β(t))0,

    ˙β,˙βS,L=(1α˙β3ˉq+eβ3˙β1ˉp)2+(lLl)2L(θ(˙β(t)))2L(θ(˙β(t)))2 as L+. (4.12)

    By (4.4) and (4.9), we have

    S,L˙β˙β,˙βS,LM0L, (4.13)

    where M0 does not depend on L. By Definition 4.1, (4.11)–(4.13), κβ,S does not exist, if θ(˙β(t))0. When θ(˙β(t))=0 and ddt(θ(˙β(t)))=0, then

    S,L˙β˙β,S,L˙β˙βS,L={ˉq[1α¨β3+αe2β3˙β21]ˉp[2˙β3˙β1eβ3+eβ3¨β1]}2+{¯rLˉp[1α¨β3+αe2β3˙β21]¯rLˉq[2˙β3˙β1eβ3+eβ3¨β1]}2{ˉq[1α¨β3+αe2β3˙β21]ˉp[2˙β3˙β1eβ3+eβ3¨β1]}2 as L+, (4.14)

    and

    ˙β,˙βS,L=(1α˙β3ˉq+eβ3˙β1ˉp)2 as L+, (4.15)
    S,L˙β˙β,˙βS,L=(1α˙β3ˉq+eβ3˙β1ˉp){ˉq[1α¨β3+αe2β3˙β21]ˉp[2˙β3˙β1eβ3+eβ3¨β1]}, (4.16)

    where ˉA=ˉq[1α¨β3+αe2β3˙β21]ˉp[2˙β3˙β1eβ3+eβ3¨β1] and ˉB=1α˙β3ˉq+eβ3˙β1ˉp. By (4.14)–(4.16) and (4.6), we get

    κβ,S=ˉA2ˉB4+ˉA2ˉB2ˉB6=0.

    When θ(˙β(t))=0, and ddt(θ(˙β(t)))0, we have

    S,L˙β˙β,S,L˙β˙βS,LL[ddt(θ(˙β(t)))]2,
    S,L˙β˙β,˙βS,LO(1).

    Therefore, (4.8) holds.

    (2) If S,L˙β˙β is a timelike vector, by similar calculation, we get (2).

    Definition 4.4. Let SSLα be a Lorentzian regular surface, β:IS be a C2-smooth regular curve. The signed geodesic curvature κL,cβ,S of β at β(t) is defined as

    κL,cβ,S:=S,L˙β˙β,JL(˙β)S,L˙β3S,L.

    Definition 4.5. Let SSLα be a Lorentzian regular surface, β:IS be a C2-smooth regular curve. We define the intrinsic geodesic curvature κβ,S of β at the non-characteristic point β(t) to be

    κ,cβ,S:=limL+κL,cβ,S,

    if the limit exists.

    Proposition 4.6. Let SSLα be a Lorentzian regular surface.

    (1) If β:IS is a C2-smooth regular spacelike curve, then

    κ,cβ,S=αˉq, if  θ(˙β(t))0, (4.17)
    κ,cβ,S=0, if  θ(˙β(t))=0 and ddt(θ(˙β(t)))=0,
    limL+kL,cβ,SL=ddt(θ(˙β(t)))(1αˉq˙β3+eβ3ˉp˙β1)2, if  θ(˙β(t))=0 and ddt(θ(˙β(t)))0. (4.18)

    (2) If β:IS is a C2-smooth regular timelike curve, then

    κ,cβ,S=αˉq, if  θ(˙β(t))0, (4.19)
    κ,cβ,S=0, if  θ(˙β(t))=0 and ddt(θ(˙β(t)))=0,
    limL+kL,cβ,SL=ddt(θ(˙β(t)))(1αˉq˙β3+eβ3ˉp˙β1)2, if  θ(˙β(t))=0 and ddt(θ(˙β(t)))0. (4.20)

    Proof. For (4.1), by (4.10), we have

    JL(˙β)=lLlL12θ(˙β(t))F1+(1α˙β3ˉq+eβ3˙β1ˉp)F2. (4.21)

    By (4.4) and (4.21), we have

    S,L˙β˙β,JL(˙β)S,L=lLlL12θ(˙β(t)){ˉq[1α¨β3+αe2β3˙β21+αL(θ(˙β(t)))2]ˉp[2˙β3˙β1eβ3+eβ3¨β1]}+(1α˙β3ˉq+eβ3˙β1ˉp){¯rLˉp[1α¨β3+αe2β3˙β21+αL(θ(˙β(t)))2]¯rLˉq[2˙β3˙β1eβ3+eβ3¨β1]+llLL12[˙β3θ(˙β(t))+ddt(θ(˙β(t)))]}αL32(θ(˙β(t)))3ˉq as L+,
    ˙β2S,L=(1α˙β3ˉq+eβ3˙β1ˉp)2+[lLlL12θ(˙β(t))]2L(θ(˙β(t)))2 as L+.

    Thus, if θ(˙β(t))0, (4.17) holds. When θ(˙β(t))=0 and ddt(θ(˙β(t)))=0, we get

    S,L˙β˙β,JL(˙β)L,S=(1α˙β3ˉq+eβ3˙β1ˉp){¯rLˉp[1α¨β3+αe2β3˙β1]¯rLˉq[2˙β3˙β1eβ3+eβ3¨β1]}O(L12) as L+.

    So, κ,cβ,S=0. When θ(˙β(t))=0 and ddt(θ(˙β(t)))0, we have

    S,L˙β˙β,JL(˙β)L,SL12(1α˙β3ˉq+eβ3˙β1ˉp)ddt(θ(˙β(t))) as L+.

    We get

    limL+kL,cβ,SL=ddt(θ(˙β(t)))(1αˉq˙β3+eβ3ˉp˙β1)2.

    (2) If β:IS is a C2-smooth regular timelike curve, by similar calculation, we get (2).

    In this section, we will compute the expression of the sub-Lorentzian limit of the Gaussian curvature of Lorentzian surfaces in SLα. Then, we will prove a Gauss-Bonnet theorem for Lorentzian surfaces in SLα. To do this, we define the second fundamental form IIL of the embedding of S into SLα by

    IIL=(LF1NL,F1LLF1NL,F2LLF2NL,F1LLF2NL,F2L).

    We have the following theorem.

    Theorem 5.1. For the embedding of S into SLα, the second fundamental form IIL of the embedding of S is given by

    IIL=(h11h12h21h22),

    where

    h11=llL[E1(ˉp)E2(ˉq)]+αˉpL,
    h12=lLlF1,H¯rLL,
    h21=lLlF1,H¯rLL+¯rL2L,
    h22=l2l2LF2,H(rl)LllL¯rL~E3(llL)+(llL)2~E3(¯rL)α¯pL.

    Proof. Since F1,NLL=0,F2,NLL=0, we have

    LF1NL,F1L=LF1F1,NLL,LF2NL,F2L=LF2F2,NLL.

    Using the definition of the connection, the identities in (2.4) and grouping terms, we have

    LF1F1=LˉqE1ˉpE2ˉqE1ˉpE2=[ˉqE1(ˉq)ˉpE2(ˉq)+αˉp2]E1[ˉqE1(ˉp)ˉpE2(ˉp)+αˉpˉq]E2.

    Since ˉp2+ˉq2=1, we have ˉpEiˉp+ˉqEiˉq=0,i=1,2,3. Thus, ˉqE1ˉq=ˉpE1ˉp, ˉqE2ˉq=ˉpE2ˉp. Next, we compute the inner product of this with NL, and we have

    LF1F1,NL=llL[E1(ˉp)E2(ˉq)]α¯pL.

    We get

    h11=LF1F1,NLL=llL[E1(ˉp)E2(ˉq)]+α¯pL.

    To compute h12, using the definition of the connection, we obtain

    LF1F2=LˉqE1ˉpE2¯rLˉpE1¯rLˉqE2+llL~E3=[ˉqE1(¯rLˉp)ˉpE2(¯rLˉp)+α¯rLˉpˉq]E1[ˉqE1(¯rLˉq)ˉpE2(¯rLˉq)+α¯rLˉp2]E2+[ˉqE1(llL)ˉpE2(llL)]~E3.

    We get

    LF1F2,NLL=lLlF1,LH¯rLL,

    and therefore

    h12=LF1F2,NLL=lLlF1,LH¯rLL.

    To compute h21, using the definition of the connection, we obtain

    LF2F1=L¯rLˉpE1¯rLˉqE2+llL~E3ˉqE1ˉpE2.

    We get

    LF2F1,NLL=lLlF1,H¯rLL¯rL2L.

    Therefore,

    h21=lLlF1,H¯rLL+¯rL2L.

    Since F2NL,F2L=F2F2,NLL, we use the definition of connection, the identities in (2.4) and grouping terms. Taking the inner product with NL and under some simplifications similar to Theorem 4.3 in [23], we have

    LF2F2,NLL=l2l2LF2,H(rl)L+llL¯rL~E3(llL)(llL)2~E3(¯rL)+α¯pL,

    and then we get

    h22=F2F2,NLL=l2l2LF2,H(rl)LllL¯rL~E3(llL)+(llL)2~E3(¯rL)α¯pL.

    We define the mean curvature HL of S by

    HL:=tr(IIL)=h11+h22.

    Let

    KS,L(F1,F2)=RS,L(F1,F2)F1,F2S,L, KL(F1,F2)=RL(F1,F2)F1,F2L.

    By the Gauss equation, we have

    KS,L(F1,F2)=KL(F1,F2)+det(IIL). (5.1)

    Proposition 5.2. The horizontal mean curvature H of SSα away from characteristic point is given in the following form:

    H=limL+HL=E1(ˉp)E2(ˉq). (5.2)

    Proof. By

    lLlF2,H¯rL=¯rLˉpE1(¯rL)¯rLˉqE2(¯rL)=ˉprlE1(¯rL)ˉqrlE2(¯rL)O(L12),
    ~E3(¯rL)0,¯pLˉp,
    llL[E1(ˉp)E2(ˉq)]E1(ˉp)E2(ˉq),

    we get (5.2).

    Proposition 5.3. Away from characteristic points, we have

    KS,L(F1,F2)A+O(L1) as L+, (5.3)

    where

    A:=α2(llL)2llLα¯pL[E1(ˉp)E2(ˉq)]α2¯pL2. (5.4)

    Proof. We compute

    RL(F1,F2)F1=α2¯rLˉpE1α2¯rLˉqE2+α2llL~E3,

    and then

    RL(F1,F2)F1,F2L=α2¯rL2ˉp2+α2¯rL2ˉq2+α2(llL)2. (5.5)

    By Proposition 2.2, we find

    KL(F1,F2)=α2¯rL2ˉp2α2¯rL2ˉq2α2(llL)2=α2(llL)2 as L. (5.6)

    By the second fundamental form and H(ˉrL)=L12H(E3h|Hh|)+O(L1) as L+, we get

    det(IIL)=h11h22h12h21={llL[E1(ˉp)E2(ˉq)]+α¯pL}{l2l2LF2,H(rl)LllL~E3(llL)+(llL)2~E3(¯rL)α¯pL}lLlF1,H¯rLL{lLlF1,H¯rLL+¯rL2L}llLα¯pL[E1(ˉp)E2(ˉq)]α2¯pL2 as L+. (5.7)

    By (5.1), (5.6) and (5.7), we get the desired equation.

    We get a Gauss-Bonnet theorem for Lorentzian surface in SLα as follows.

    Theorem 5.4. Let SSLα be a regular Lorentzian surface with finitely many boundary components (S)i,i{1,,n}, given by Euclidean C2-smooth regular and closed spacelike curves βi:[0,2π](S)i. Let A be Gaussian curvature of Σ in Proposition 5.3 and κ,cβi,S the sub-Lorentzian signed geodesic curvature of βi relative to Σ in Proposition 4.6. Supposing that the characteristic set C(S) be the empty set, dσS is defined by (8.5), and ds is defined by (8.1) in Appendix A. Then,

    SAdσS+ni=1βiκ,cβi,Sds=0.

    Proof. By the discussions in [15], suppose that all points satisfy θ(˙β(t))0 on βi. Therefore, using Proposition 4.6, we obtain

    κL,cβi,S=κ,cβi,S+O(L1). (5.8)

    According to the Gauss-Bonnet theorem (see [4], page 90 Theorem 1.4), we get

    SKS,L1LdσS,L+ni=1βiκL,cβi,S1LdsL=0. (5.9)

    Therefore, by (5.8), (5.9), (8.6), (5.3) and (8.4), we get

    (SAdσS+ni=1βiκ,cβi,Sds)+O(L12)=0. (5.10)

    Let L go to infinity and use the dominated convergence theorem, and we get the desired result.

    In this section, we will prove a Gauss-Bonet theorem for spacelike surface in SLα. Let

    p:=E1h,q:=E2h, and r:=~E3h.

    Let p2q2>0,when L+, and we have p2q2r2>0. We define

    l:=p2q2,lL:=p2q2r2,ˉp:=pl,ˉq:=ql,¯pL:=plL,¯qL:=qlL,¯rL:=rlL. (6.1)

    In particular, ˉp2ˉq2=1. These functions are well defined at every non-characteristic point. Let

    NL=¯pLE1+¯qLE2+¯rL~E3,F1=ˉqE1ˉpE2,F2=¯rLˉpE1¯rLˉqE2+llL~E3, (6.2)

    and then NL is the unit timelike normal vector to S, F1 and F2 are the unit spacelike vector of S. {F1,F2} is the orthonormal basis of S. We call S a spacelike surface in Lorentzian α-Sasakian space. We define a linear transformation on TS by JL:TSTS, and the transformation is well defined:

    JL(F1)=F2,JL(F2)=F1. (6.3)

    For every U,VTS, we define S,LUV=πLUV where π:TSLαTS is the projection. Then, S,L is the Levi-Civita connection on S with respect to the metric gL. By (3.9), (6.2) and

    S,L˙β˙β=L˙β˙β,F1LF1+L˙β˙β,F2LF2, (6.4)

    we have

    S,L˙β˙β={ˉq[1α¨β3+αe2β3˙β21+αL(θ(˙β(t)))2]ˉp[2˙β3˙β1eβ3+eβ3¨β1]}F1+{¯rLˉp[1α¨β3+αe2β3˙β21+αL(θ(˙β(t)))2]¯rLˉq[2˙β3˙β1eβ3+eβ3¨β1]+llLL12[˙β3θ(˙β(t))+ddt(θ(˙β(t)))]}F2. (6.5)

    Therefore, when θ(˙β(t))=0, we have

    S,L˙β˙β={ˉq[1α¨β3+αe2β3˙β21]ˉp[2˙β3˙β1eβ3+eβ3¨β1]}F1+{¯rLˉp[1α¨β3+αe2β3˙β21]¯rLˉq[2˙β3˙β1eβ3+eβ3¨β1]+llLL12ddt(θ(˙β(t)))}F2. (6.6)

    Definition 6.1. Let SSLα be a regular spacelike surface, β:IS be a C2-smooth regular curve. We define the geodesic curvature κLβ,S of β at β(t) by

    κLβ,S:=S,L˙β˙β2S,L˙β4S,LS,L˙β˙β,˙β2S,L˙β,˙β3S,L. (6.7)

    Definition 6.2. Let SSLα be a regular spacelike surface, β:IS be a C2-smooth regular curve. The intrinsic geodesic curvature κβ,S of β at β(t) is defined as

    κβ,S:=limL+κLβ,S,

    if the limit exists.

    Proposition 6.3. Let SSLα be a regular spacelike surface, β:IS be a C2-smooth spacelike curve, and then we have the following assertions:

    κβ,S=∣αˉq, if θ(˙β(t))0, (6.8)
    κβ,S=0, if θ(˙β(t))=0 and ddt(θ(˙β(t)))=0,
    limL+κLβ,SL=|ddt(θ(˙β(t)))|(1αˉq˙β3+eβ3ˉp˙β1)2, if θ(˙β(t))=0 and ddt(θ(˙β(t)))0. (6.9)

    Proof. By (3.7) and ˙βTS, we have

    ˙β(t)=(1α˙β3ˉq+eβ3˙β1ˉp)F1+lLlL12θ(˙β(t))F2. (6.10)

    By (6.5), we have

    S,L˙β˙β,S,L˙β˙βS,L={ˉq[1α¨β3+αe2β3˙β21+αL(θ(˙β(t)))2]ˉp[2˙β3˙β1eβ3+eβ3¨β1]}2+{¯rLˉp[1α¨β3+αe2β3˙β21+αL(θ(˙β(t)))2]¯rLˉq[2˙β3˙β1eβ3+eβ3¨β1]+llLL12[˙β3θ(˙β(t))+ddt(θ(˙β(t)))]}2. (6.11)

    Similarly, if θ(˙β(t))0,

    ˙β,˙βS,L=(1α˙β3ˉq+eβ3˙β1ˉp)2+(lLl)2L(θ(˙β(t)))2L(θ(˙β(t)))2 as L+. (6.12)

    By (6.5) and (6.10), we have

    S,L˙β˙β,˙βS,LM0L, (6.13)

    where M0 does not depend on L. By (6.7) and (6.11)-(6.13), (6.8) holds. When θ(˙β(t))=0 and ddt(θ(˙β(t)))=0,

    S,L˙β˙β,S,L˙β˙βS,L={ˉq[1α¨β3+αe2β3˙β21]ˉp[2˙β3˙β1eβ3+eβ3¨β1]}2+{¯rLˉp[1α¨β3+αe2β3˙β21]¯rLˉq[2˙β3˙β1eβ3+eβ3¨β1]}2{ˉq[1α¨β3+αe2β3˙β21]ˉp[2˙β3˙β1eβ3+eβ3¨β1]}2 as L+ (6.14)

    and

    ˙β,˙βS,L=(1α˙β3ˉq+eβ3˙β1ˉp)2 as L+. (6.15)
    S,L˙β˙β,˙βS,L=(1α˙β3ˉq+eβ3˙β1ˉp){ˉq[1α¨β3+αe2β3˙β21]ˉp[2˙β3˙β1eβ3+eβ3¨β1]}. (6.16)

    By (6.14)-(6.16) and (6.7), we get

    κβ,S=0.

    When θ(˙β(t))=0, and ddt(θ(˙β(t)))0, we have

    S,L˙β˙β,S,L˙β˙βS,LL[ddt(θ(˙β(t)))]2,
    S,L˙β˙β,˙βS,LO(1).

    Therefore, (6.9) holds.

    Proposition 6.4. Let SSLα be a regular spacelike surface. β:IS is a C2-smooth regular spacelike curve, and then

    κ,cβ,S=αˉq, if  θ(˙β(t))=0; (6.17)
    κ,cβ,S=0, if  θ(˙β(t))=0 and ddt(θ(˙β(t)))=0;
    limL+kL,cβ,SL=ddt(θ(˙β(t)))(1αˉq˙β3+eβ3ˉp˙β1)2, if  θ(˙β(t))=0 and ddt(θ(˙β(t)))0. (6.18)

    Proof. By (6.3) and (6.10), we have

    JL(˙β)=lLlL12θ(˙β(t))F1(1α˙β3ˉq+eβ3˙β1ˉp)F2. (6.19)

    By (6.5) and (6.19), we have

    S,L˙β˙β,JL(˙β)S,L=lLlL12θ(˙β(t)){ˉq[1α¨β3+αe2β3˙β21+αL(θ(˙β(t)))2]ˉp[2˙β3˙β1eβ3+eβ3¨β1]}(1α˙β3ˉq+eβ3˙β1ˉp){¯rLˉp[1α¨β3+αe2β3˙β21+αL(θ(˙β(t)))2]¯rLˉq[2˙β3˙β1eβ3+eβ3¨β1]+llLL12[˙β3θ(˙β(t))+ddt(θ(˙β(t)))]}αL32(θ(˙β(t)))3ˉq as L+,
    ˙β2S,L=(1α˙β3ˉq+eβ3˙β1ˉp)2+[lLlL12θ(˙β(t))]2L(θ(˙β(t)))2 as L+.

    Therefore, if θ(˙β(t))0, (6.17) holds. When θ(˙β(t))=0 and ddt(θ(˙β(t)))=0, we get

    S,L˙β˙β,JL(˙β)L,S=(1α˙β3ˉq+eβ3˙β1ˉp){¯rLˉp[1α¨β3+αe2β3˙β1]¯rLˉq[2˙β3˙β1eβ3+eβ3¨β1]}O(L12) as L+.

    So, κ,cβ,S=0. When θ(˙β(t))=0 and ddt(θ(˙β(t)))0, we have

    S,L˙β˙β,JL(˙β)L,SL12(1α˙β3ˉq+eβ3˙β1ˉp)ddt(θ(˙β(t))) as L+.

    We get

    limL+kL,cβ,SL=ddt(θ(˙β(t)))(1αˉq˙β3+eβ3ˉp˙β1)2.

    In the following, we investigate the sub-Lorentzian limit of the Gaussian curvature of spacelike surfaces in SLα. The second fundamental form IIL of the embedding of S into SLα is defined as

    IIL=(LF1NL,F1LLF1NL,F2LLF2NL,F1LLF2NL,F2L).

    Similar to Theorem 4.3 in [23], we have the following.

    Theorem 6.5. For the embedding of S into SLα, the second fundamental form IIL of the embedding of S is given by

    IIL=(h11h12h21h22),

    where

    h11=llL[E1(ˉp)E2(ˉq)]αˉpL,
    h12=(lLl2llL)F1,H¯rLL,
    h21=(2llLlLl)F1,H¯rLL¯rL2L2α¯rL¯qL,
    h22=(lLl2llL)F2,H¯rLL(llL)2~E3(rl)2llL¯rL~E3(llL)+α¯pL.

    Proof. We combine

    NL=¯pLE1+¯qLE2+¯rL~E3,F1=ˉqE1ˉpE2,F2=¯rLˉpE1¯rLˉqE2+llL~E3, (6.20)

    and LFiNL,FjL=LFiFj,NLL,i,j=1,2. By direct calculation, we obtain

    LF1F1=[ˉqE1(ˉq)ˉpE2(ˉq)αˉp2]E1[ˉqE1(ˉp)ˉpE2(ˉp)+αˉpˉq]E2.

    Since ˉp2ˉq2=1, we have ˉpEiˉpˉqEiˉq=0,i=1,2. Then, ˉqE1ˉq=ˉpE1ˉp, ˉqE2ˉq=ˉpE2ˉp. Next, we compute the inner product of this with NL, and we have

    LF1F1,NL=llL[E1(ˉp)E2(ˉq)]+αˉpL.

    We obtain

    h11=LF1F1,NLL=llL[E1(ˉp)E2(ˉq)]αˉpL.

    Similarly, we have

    h12=LF1F2,NLL=(lLl2llL)F1,H¯rLL,
    h21=LF2F1,NLL=(2llLlLl)F1,H¯rLL¯rL2L2α¯rL¯qL,
    h22=LF2F2,NLL=(lLl2llL)F2,LH¯rLL(llL)2~E3(rl)2llL¯rL~E3(llL)+α¯pL.

    Thus, Theorem 6.5 holds.

    By the Gauss equation, we have

    KS,L(F1,F2)=KL(F1,F2)det(IIL). (6.21)

    Proposition 6.6. The horizontal mean curvature H of SSα away from characteristic point is given in the following form:

    H=limL+HL=E1(ˉp)+E2(ˉq). (6.22)

    Proof. By

    (lLl2llL)F2,H¯rL=¯rLˉpE1(¯rL)¯rLˉqE2(¯rL)=ˉprlE1(¯rL)ˉqrlE2(¯rL)O(L12),
    ~E3(¯rL)0,¯pLˉp,
    llL[E1(ˉp)E2(ˉq)]E1(ˉp)E2(ˉq),

    we get (6.22).

    Proposition 6.7. Away from characteristic points, we have

    KS,L(F1,F2)C+O(L1) as L+, (6.23)

    where

    C:=α2(llL)2+llLα¯pL[E1(ˉp)E2(ˉq)]+α2¯pL2. (6.24)

    Proof. We compute

    RL(F1,F2)F1=α2¯rLˉpE1+α2¯rLˉqE2α2llL~E3,

    and then

    RL(F1,F2)F1,F2L=α2¯rL2ˉp2α2¯rL2ˉq2α2(llL)2. (6.25)

    So,

    KL(F1,F2)=RL(F1,F2)F1,F2L=α2¯rL2ˉp2+α2¯rL2ˉq2+α2(llL)2 as L+. (6.26)

    By the second fundamental form and H(ˉrL)=L12H(E3h|Hh|)+O(L1) as L+, we get

    det(IIL)=h11h22h12h21llLα¯pL[E1(ˉp)E2(ˉq)]α2¯pL2 as L+. (6.27)

    By (6.21), (6.26) and (6.27), we get the desired equation.

    Theorem 6.8. Let SSLα be a regular spacelike surface with finitely many boundary components (S)i,i{1,,n}, given by Euclidean C2-smooth regular and closed spacelike curves βi:[0,2π](S)i. Suppose that C is defined by (6.24), dσS is defined by (8.8) and κ,cβi,S is the sub-Lorentzian signed geodesic curvature of βi relative to S. If the characteristic set C(S) is the empty set, then

    SCdσS+ni=1βiκ,cβi,Sds=0.

    Proof. By the discussions in [15], we may assume that there are no points satisfying θ(˙β(t))=0 and ddt(θ(˙β(t)))0 on βi. Therefore, using Proposition 6.3, we obtain

    κL,cβi,S=κ,cβi,S+O(L1). (6.28)

    According to the Gauss-Bonnet theorem, we get

    SKS,L1LdσS,L+ni=1βiκL,cβi,S1LdsL=2πX(S)L. (6.29)

    Therefore, by (6.28), (6.29), (8.9), (6.23), (8.3) and (8.4), we get

    (SCdσS+ni=1βiκ,cβi,Sdˉs)+O(L12)=2πX(S)L. (6.30)

    Let L go to infinity and use the dominated convergence theorem, and we get the desired result.

    This paper proved two Gauss-Bonnet theorems for the Lorentzian surfaces and spacelike surfaces in a Lorentzian α-Sasakian manifold by using the method of the Lorentzian approximation scheme. For Lorentzian surfaces, we derive the expressions of the intrinsic curvature for regular curves, the intrinsic geodesic curvature of regular curves on Lorentzian surfaces and the intrinsic Gaussian curvature of Lorentzian surfaces away from characteristic points in the Lorentzian α-Sasakian manifold. Similarly, we get the corresponding results for the spacelike surface.

    To prove Gauss-Bonnet theorems, we need to define the Lorentzian length measure and the Lorentzian surface measure. Let us first consider the case of a regular spacelike curve β:ISLα, and we define the length measure dsL=˙βLdt.

    Lemma 7.1. Let β:ISLα be a C2-smooth spacelike curve. Let

    ds:=|θ(˙β(t))|dt, dˉs:=121|θ(˙β(t))|(1α2˙β23+e2β3˙β21)dt. (7.1)

    Then,

    limL+1LβdsL=bads. (7.2)

    When θ(˙β(t))0, we have

    1LdsL=ds+dˉsL1+O(L2) as L+. (7.3)

    With the situation of θ(˙β(t))=0, we have

    1LdsL=1L1α2˙β23+e2β3˙β21dt. (7.4)

    Proof. We know that

    ˙β(t)L=1α2˙β23+e2β3˙β21+L(θ(˙β(t))),

    and similar to the proof of Lemma 6.1 in [15], we can prove

    limL+1LβdsL=balimL+1L˙β(t)Ldt=balimL+1L1α2˙β23+e2β3˙β21+L(θ(˙β(t)))dt=bads,

    so we get (8.2). When θ(˙β(t))0, we have

    1LdsL=L1(1α2˙β23+e2β3˙β21)+θ(˙β(t))dt.

    Using the Taylor expansion, we can prove

    1LdsL=ds+dˉsL1+O(L2) as L+.

    From the definition of dsL and θ(˙β(t))=0, we get

    1LdsL=1L1α2˙β23+e2β3˙β21dt.

    Proposition 7.2. Let SSLα be a regular Lorentzian C2-smooth surface. Let dσS,L denote the surface measure on S with respect to the Lorentzian metric gL. Let

    dσS:=(ˉpθ2ˉqθ1)θ, dˉσS:=E3hlθ1θ2+(E3h)22l2(ˉpθ2ˉqθ1)θ. (7.5)

    Then,

    1LdσS,L=dσS+dˉσSL1+O(L2), as L+. (7.6)

    If S=f(D) with f=f(h1,h2)=(f1,f2,f3):DR2SLα, then

    limL+1LSdσS,L=D{e4z[(f1)h1(f2)h2(f1)h1(f1)h2(f1)h2(f2)h1+(f1)h2(f1)h2]21α2e2z[(f3)h1(f2)h2(f3)h1(f1)h2(f3)h2(f2)h1+(f3)h2(f1)h1]2}12dh1dh2.

    Proof. It is well known that

    gL(E1,)=θ1, gL(E2,)=θ2, gL(E3,)=Lθ.

    We define F1:=gL(F1,), F2:=gL(F2,), and then

    F1=ˉqθ1ˉpθ2, F2=ˉrLˉpθ1ˉrLˉqθ2+llLL12θ.

    Therefore,

    1LdσS,L=1LF1F2=llL(ˉpθ2+ˉqθ1)θ+1LˉrLθ1θ2.

    Recall

    ˉrL=(E3h)L12p2+q2+L1(E3h)2

    and the Taylor expansion

    1lL=1l12l3(E3h)2L1+O(L2) as L+,

    and we get (8.6). By (2.2), we have

    fh1=(f1)h1x+(f2)h1y+(f3)h1z=(f1)h1[ez(E2E3)]+(f2)h1ezE3+1α(f3)h1E1=1α(f3)h1E1+ez(f1)h1E2+Lez((f1)h1+(f2)h1)~E3,

    and

    fh2=(f1)h2x+(f2)h2y+(f3)h2z=1α(f3)h2E1+ez(f1)h2E2+Lez((f1)h2+(f2)h2)~E3.

    Let

    ˉNL=|E1E2~E31α(f3)h1ez(f1)h1Lez((f1)h1+(f2)h1)1α(f3)h2ez(f1)h2Lez((f1)h1+(f2)h1)|=Le2z[(f1)h1(f2)h2(f1)h1(f1)h2(f1)h2(f2)h1+(f1)h2(f1)h1]E1Lαez[(f3)h1(f2)h2(f3)h1(f1)h2(f3)h2(f2)h1+(f3)h2(f1)h1]E2+1αez[(f3)h1(f1)h2(f1)h1(f3)h2]~E3. (7.7)

    We know that dσS,L=det(gij)dh1dh2, gij=gL(fhi,fhj), and

    det(gij)=ˉNL,ˉNLL=Le4z[(f1)h1(f2)h2(f1)h1(f1)h2(f1)h2(f2)h1+(f1)h2(f1)h1]2+Lα2e2z[(f3)h1(f2)h2(f3)h1(f1)h2(f3)h2(f2)h1+(f3)h2(f1)h1)]2+1α2e2z[(f3)h1(f1)h2(f1)h1(f3)h2]2,

    so by the dominated convergence theorem, we get

    limL+1LSdσS,L=D{e4z[(f1)h1(f2)h2(f1)h1(f1)h2)(f1)h2(f2)h1+(f1)h2(f1)h2)]2+1α2e2z[(f3)h1(f2)h2(f3)h1(f1)h2)(f3)h2(f2)h1+(f3)h2(f1)h1]2}12dh1dh2.

    Proposition 7.3. Let SSLα be a spacelike C2-smooth surface. Let dσS,L denote the surface measure on S with respect to the metric gL. Suppose that

    dσS:=(ˉpθ2ˉqθ1)θ, dˉσS:=E3hlθ1θ2+(E3h)22l2(ˉpθ2ˉqθ1)θ. (7.8)

    Then,

    1LdσS,L=dσS+dˉσSL1+O(L2), as L+. (7.9)

    Proof. It is well known that

    gL(E1,)=θ1, gL(E2,)=θ2, gL(E3,)=Lθ.

    Then,

    F1=ˉqθ1ˉpθ2, F2=ˉrLˉpθ1ˉrLˉqθ2+llLL12θ.

    Therefore,

    1LdσS,L=1LF1F2=llL(ˉpθ2+ˉqθ1)θ1LˉrLθ1θ2.

    Recall

    ˉrL=(E3h)L12p2q2L1(E3h)2

    and the Taylor expansion

    1lL=1l+12l3(E3h)2L1+O(L2) as L+,

    and we get (8.9).

    This research was funded by the Project of Science and Technology of Heilongjiang Provincial Education Department (Grant No. 1354ZD008), the Reform and Development Foundation for Local Colleges and Universities of the Central Government (Excellent Young Talents project of Heilongjiang Province, Grant No. ZYQN2019071) and the Natural Science Foundation of Heilongjiang Province of China (Grant No. LH2021A020).

    The authors declare that there are no conflicts of interests in this work.



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