On Special Berwald Metrics

In this paper, we study a class of Finsler metrics which contains the class of Berwald metrics as a special case. We prove that every Finsler metric in this class is a generalized Douglas-Weyl metric. Then we study isotropic flag curvature Finsler metrics in this class. Finally we show that on this...

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Автори: Tayebi, A., Peyghan, E.
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Опубліковано: Інститут математики НАН України 2010
Назва видання:Symmetry, Integrability and Geometry: Methods and Applications
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Цитувати:On Special Berwald Metrics / E. Tayebi // Symmetry, Integrability and Geometry: Methods and Applications. — 2010. — Т. 6. — Бібліогр.: 16 назв. — англ.

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spelling irk-123456789-1461182019-02-08T01:23:17Z On Special Berwald Metrics Tayebi, A. Peyghan, E. In this paper, we study a class of Finsler metrics which contains the class of Berwald metrics as a special case. We prove that every Finsler metric in this class is a generalized Douglas-Weyl metric. Then we study isotropic flag curvature Finsler metrics in this class. Finally we show that on this class of Finsler metrics, the notion of Landsberg and weakly Landsberg curvature are equivalent. 2010 Article On Special Berwald Metrics / E. Tayebi // Symmetry, Integrability and Geometry: Methods and Applications. — 2010. — Т. 6. — Бібліогр.: 16 назв. — англ. 1815-0659 2010 Mathematics Subject Classification: 53C60; 53C25 http://dspace.nbuv.gov.ua/handle/123456789/146118 en Symmetry, Integrability and Geometry: Methods and Applications Інститут математики НАН України
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
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language English
description In this paper, we study a class of Finsler metrics which contains the class of Berwald metrics as a special case. We prove that every Finsler metric in this class is a generalized Douglas-Weyl metric. Then we study isotropic flag curvature Finsler metrics in this class. Finally we show that on this class of Finsler metrics, the notion of Landsberg and weakly Landsberg curvature are equivalent.
format Article
author Tayebi, A.
Peyghan, E.
spellingShingle Tayebi, A.
Peyghan, E.
On Special Berwald Metrics
Symmetry, Integrability and Geometry: Methods and Applications
author_facet Tayebi, A.
Peyghan, E.
author_sort Tayebi, A.
title On Special Berwald Metrics
title_short On Special Berwald Metrics
title_full On Special Berwald Metrics
title_fullStr On Special Berwald Metrics
title_full_unstemmed On Special Berwald Metrics
title_sort on special berwald metrics
publisher Інститут математики НАН України
publishDate 2010
url http://dspace.nbuv.gov.ua/handle/123456789/146118
citation_txt On Special Berwald Metrics / E. Tayebi // Symmetry, Integrability and Geometry: Methods and Applications. — 2010. — Т. 6. — Бібліогр.: 16 назв. — англ.
series Symmetry, Integrability and Geometry: Methods and Applications
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AT peyghane onspecialberwaldmetrics
first_indexed 2025-07-10T23:12:16Z
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fulltext Symmetry, Integrability and Geometry: Methods and Applications SIGMA 6 (2010), 008, 9 pages On Special Berwald Metrics Akbar TAYEBI † and Esmaeil PEYGHAN ‡ † Department of Mathematics, Faculty of Science, Qom University, Qom, Iran E-mail: akbar.tayebi@gmail.com ‡ Department of Mathematics, Faculty of Science, Arak University, Arak, Iran E-mail: epeyghan@gmail.com, e-peyghan@araku.ac.ir Received November 01, 2009, in final form January 17, 2010; Published online January 20, 2010 doi:10.3842/SIGMA.2010.008 Abstract. In this paper, we study a class of Finsler metrics which contains the class of Berwald metrics as a special case. We prove that every Finsler metric in this class is a generalized Douglas–Weyl metric. Then we study isotropic flag curvature Finsler metrics in this class. Finally we show that on this class of Finsler metrics, the notion of Landsberg and weakly Landsberg curvature are equivalent. Key words: Randers metric; Douglas curvature; Berwald curvature 2010 Mathematics Subject Classification: 53C60; 53C25 1 Introduction For a Finsler metric F = F (x, y), its geodesics curves are characterized by the system of diffe- rential equations c̈i + 2Gi(ċ) = 0, where the local functions Gi = Gi(x, y) are called the spray coefficients. A Finsler metric F is called a Berwald metric if Gi = 1 2Γi jk(x)yjyk is quadratic in y ∈ TxM for any x ∈ M . It is proved that on a Berwald space, the parallel translation along any geodesic preserves the Minkowski functionals [7]. Thus Berwald spaces can be viewed as Finsler spaces modeled on a single Minkowski space. Recently by using the structure of Funk metric, Chen–Shen introduce the notion of isotropic Berwald metrics [6, 16]. This motivates us to study special forms of Berwald metrics. Let (M,F ) be a two-dimensional Finsler manifold. We refer to the Berwald’s frame (`i,mi) where `i = yi/F (y), mi is the unit vector with `im i = 0, `i = gij` i and gij is the fundamental tensor of Finsler metric F . Then the Berwald curvature is given by Bi jkl = F−1 ( −2I,1` i + I2m i ) mjmkml, (1) where I is 0-homogeneous function called the main scalar of Finsler metric and I2 = I,2 + I,1|2 (see [2, page 689]). By (1), we have Bi jkl = − 2I,1 3F 2 ( mjhkl + mkhjl + mlhjk ) yi + I2 3F ( hi jhkl + hi khjl + hi lhjk ) , where hij := mimj is called the angular metric. Using the special form of Berwald curvature for Finsler surfaces, we define a new class of Finsler metrics on n-dimensional Finsler manifolds which their Berwald curvature satisfy in following Bi jkl = (µjhkl + µkhjl + µlhjk)yi + λ ( hi jhkl + hi khjl + hi lhjk ) , (2) where µi = µi(x, y) and λ = λ(x, y) are homogeneous functions of degrees −2 and −1 with re- spect to y, respectively. By definition of Berwald curvature, the function µi satisfies µiy i=0 [12]. mailto:akbar.tayebi@gmail.com mailto:epeyghan@gmail.com file:e-peyghan@araku.ac.ir http://dx.doi.org/10.3842/SIGMA.2010.008 2 A. Tayebi and E. Peyghan The Douglas tensor is another non-Riemanian curvature defined as follows Di jkl := ( Gi − 1 n + 1 ∂Gm ∂ym yi ) yjykyl . (3) Douglas curvature is a non-Riemannian projective invariant constructed from the Berwald curva- ture. The notion of Douglas curvature was proposed by Bácsó and Matsumoto as a generalization of Berwald curvature [4]. We show that a Finsler metric satisfies (2) with vanishing Douglas tensor is a Randers metric (see Proposition 1). A Finsler metric is called a generalized Douglas– Weyl (GDW) metric if the Douglas tensor satisfy in hi αDα jkl|mym = 0 [10]. In [5], Bácsó–Papp show that this class of Finsler metrics is closed under projective transformation. We prove that a Finsler metric satisfies (2) is a GDW-metric. Theorem 1. Every Finsler metric satisfying (2) is a GDW-metric. Theorem 1, shows that every two-dimensional Finsler metric is a generalized Douglas–Weyl metric. For a Finsler manifold (M,F ), the flag curvature is a function K(P, y) of tangent planes P ⊂ TxM and directions y ∈ P . F is said to be of isotropic flag curvature if K(P, y) = K(x) and constant flag curvature if K(P, y) = const. Theorem 2. Let F be a Finsler metric of non-zero isotropic flag curvature K = K(x) on a manifold M . Suppose that F satisfies (2). Then F is a Riemannian metric if and only if µi is constant along geodesics. Beside the Berwald curvature, there are several important Finslerian curvature. Let (M,F ) be a Finsler manifold. The second derivatives of 1 2F 2 x at y ∈ TxM0 is an inner product gy on TxM . The third order derivatives of 1 2F 2 x at y ∈ TxM0 is a symmetric trilinear forms Cy on TxM . We call gy and Cy the fundamental form and the Cartan torsion, respectively. The rate of change of the Cartan torsion along geodesics is the Landsberg curvature Ly on TxM for any y ∈ TxM0. Set Jy := n∑ i=1 Ly(ei, ei, ·), where {ei} is an orthonormal basis for (TxM, gy). Jy is called the mean Landsberg curvature. F is said to be Landsbergian if L = 0, and weakly Landsbergian if J = 0 [13, 14]. In this paper, we prove that on Finsler manifolds satisfies (2), the notions of Landsberg and weakly Landsberg metric are equivalent. Theorem 3. Let (M,F ) be a Finsler manifold satisfying (2). Then L = 0 if and only if J = 0. There are many connections in Finsler geometry [15]. In this paper, we use the Berwald connection and the h- and v-covariant derivatives of a Finsler tensor field are denoted by “|” and “,” respectively. 2 Preliminaries Let M be a n-dimensional C∞ manifold. Denote by TxM the tangent space at x ∈ M , by TM = ∪x∈MTxM the tangent bundle of M , and by TM0 = TM \ {0} the slit tangent bundle on M . A Finsler metric on M is a function F : TM → [0,∞) which has the following properties: (i) F is C∞ on TM0; (ii) F is positively 1-homogeneous on the fibers of tangent bundle TM , and (iii) for each y ∈ TxM , the following quadratic form gy on TxM is positive definite, gy(u, v) := 1 2 d2 dsdt [ F 2(y + su + tv) ] ∣∣ s,t=0 , u, v ∈ TxM. On Special Berwald Metrics 3 Let x ∈ M and Fx := F |TxM . To measure the non-Euclidean feature of Fx, define Cy: TxM × TxM × TxM → R by Cy(u, v, w) := 1 2 d dt [gy+tw(u, v)] |t=0, u, v, w ∈ TxM. The family C := {Cy}y∈TM0 is called the Cartan torsion. It is well known that C = 0 if and only if F is Riemannian [14]. For y ∈ TxM0, define mean Cartan torsion Iy by Iy(u) := Ii(y)ui, where Ii := gjkCijk, gjk is the inverse of gjk and u = ui ∂ ∂xi |x. By Deicke’s theorem, F is Riemannian if and only if Iy = 0 [13]. Let α = √ aij(x)yiyj be a Riemannian metric, and β = bi(x)yi be a 1-form on M with b = √ aijbibj < 1. The Finsler metric F = α + β is called a Randers metric. Let (M,F ) be a Finsler manifold. Then for a non-zero vector y ∈ TxM0, define the Mat- sumoto torsion My : TxM ⊗ TxM ⊗ TxM → R by My(u, v, w) := Mijk(y)uivjwk where Mijk := Cijk − 1 n+1{Iihjk + Ijhik + Ikhij}, hij := FFyiyj = gij − 1 F 2 gipy pgjqy q is the angular metric and Ii := gjkCijk is the mean Cartan torsion. By definition, we have hijy i = 0, hi j = δi j − F−2yiyj , yj = gijy i, hi jhik = hjk and hi i = n− 1. A Finsler metric F is said to be C-reducible if My = 0. This quantity is introduced by Matsumoto [8]. Matsumoto proves that every Randers metric satisfies that My = 0. Later on, Matsumoto–Hōjō proves that the converse is true too. Lemma 1 ([9]). A Finsler metric F on a manifold of dimension n ≥ 3 is a Randers metric if and only if My = 0, ∀ y ∈ TM0. Let us consider the pull-back tangent bundle π∗TM over TM0 defined by π∗TM = {(u, v) ∈ TM0 × TM0| π(u) = π(v)} . Let ∇ be the Berwald connection. Let {ei}n i=1 be a local orthonormal (with respect to g) frame field for the pulled-back bundle π∗TM such that en = `, where ` is the canonical section of π∗TM defined by `y = y/F (y). Let {ωi}n i=1 be its dual co-frame field. Put ∇ei = ωj i⊗ ej , where {ωj i} is called the connection forms of ∇ with respect to {ei}. Put ωn+i := ωi n + d(log F )δi n. It is easy to show that {ωi, ωn+i}n i=1 is a local basis for T ∗(TM0). Since {Ωj i} are 2-forms on TM0, they can be expanded as Ωj i = 1 2Rj iklω k ∧ ωl + Bj iklω k ∧ ωn+l. Let {ēi, ėi}n i=1 be the local basis for T (TM0), which is dual to {ωi, ωn+i}n i=1. The objects R and B are called, respectively, the hh- and hv-curvature tensors of the Berwald connection with the components R(ēk, ēl)ei = Rj iklej and P (ēk, ėl)ei = P j iklej [15]. With the Berwald connection, we define covariant derivatives of quantities on TM0 in the usual way. For example, for a scalar function f , we define f|i and f·i by df = f|iω i + f,iω n+i, where “|” and “,” denote the h- and v-covariant derivatives, respectively. The horizontal covariant derivatives of C along geodesics give rise to the Landsberg curvature Ly : TxM × TxM × TxM → R defined by Ly(u, v, w) := Lijk(y)uivjwk, where Lijk := Cijk|sy s, u = ui ∂ ∂xi |x, v = vi ∂ ∂xi |x and w = wi ∂ ∂xi |x. The family L := {Ly}y∈TM0 is called the Landsberg curvature. A Finsler metric is called a Landsberg metric if L=0. The 4 A. Tayebi and E. Peyghan horizontal covariant derivatives of I along geodesics give rise to the mean Landsberg curvature Jy(u) := Ji(y)ui, where Ji := gjkLijk. A Finsler metric is said to be weakly Landsbergian if J = 0. Given a Finsler manifold (M,F ), then a global vector field G is induced by F on TM0, which in a standard coordinate (xi, yi) for TM0 is given by G = yi ∂ ∂xi − 2Gi(x, y) ∂ ∂yi , where Gi(y) are local functions on TM given by Gi(y) := 1 4 gil(y) { ∂2[F 2] ∂xk∂yl (y)yk − ∂[F 2] ∂xl (y) } , y ∈ TxM. G is called the spray associated to (M,F ). In local coordinates, a curve c(t) is a geodesic if and only if its coordinates (ci(t)) satisfy c̈i + 2Gi(ċ) = 0. For a tangent vector y ∈ TxM0, define By : TxM ⊗ TxM ⊗ TxM → TxM and Ey : TxM ⊗ TxM → R by By(u, v, w) := Bi jkl(y)ujvkwl ∂ ∂xi |x and Ey(u, v) := Ejk(y)ujvk where Bi jkl(y) := ∂3Gi ∂yj∂yk∂yl (y), Ejk(y) := 1 2Bm jkm(y). B and E are called the Berwald curvature and mean Berwald curvature, respectively. Then F is called a Berwald metric and weakly Berwald metric if B = 0 and E = 0, respectively [14]. By definition of Berwald and mean Berwald curvatures, we have yjBi jkl = ykBi jkl = ylBi jkl = 0, yjEjk = ykEjk = 0. The Riemann curvature Ry = Ri kdxk ⊗ ∂ ∂xi |x : TxM → TxM is a family of linear maps on tangent spaces, defined by Ri k = 2 ∂Gi ∂xk − yj ∂2Gi ∂xj∂yk + 2Gj ∂2Gi ∂yj∂yk − ∂Gi ∂yj ∂Gj ∂yk . The flag curvature in Finsler geometry is a natural extension of the sectional curvature in Riemannian geometry was first introduced by L. Berwald [3]. For a flag P = span{y, u} ⊂ TxM with flagpole y, the flag curvature K = K(P, y) is defined by K(P, y) := gy(u,Ry(u)) gy(y, y)gy(u, u)− gy(y, u)2 . When F is Riemannian, K = K(P ) is independent of y ∈ P , and is the sectional curvature of P . We say that a Finsler metric F is of scalar curvature if for any y ∈ TxM , the flag curvature K = K(x, y) is a scalar function on the slit tangent bundle TM0. If K = const, then F is said to be of constant flag curvature. A Finsler metric F is called isotropic flag curvature, if K = K(x). In [1], Akbar-Zadeh considered a non-Riemannian quantity H which is obtained from the mean Berwald curvature by the covariant horizontal differentiation along geodesics. This is a positively homogeneous scalar function of degree zero on the slit tangent bundle. The quantity Hy = Hijdxi⊗dxj is defined as the covariant derivative of E along geodesics [11]. More precisely Hij := Eij|mym. In local coordinates, we have 2Hij = ym ∂4Gk ∂yi∂yj∂yk∂xm − 2Gm ∂4Gk ∂yi∂yj∂yk∂ym − ∂Gm ∂yi ∂3Gk ∂yj∂yk∂ym − ∂Gm ∂yj ∂4Gk ∂yi∂yk∂ym . Akbar-Zadeh proved the following: Theorem 4 ([1]). Let F be a Finsler metric of scalar curvature on an n-dimensional mani- fold M (n ≥ 3). Then the flag curvature K = const if and only if H = 0. On Special Berwald Metrics 5 3 Proof of Theorem 1 Lemma 2. Let (M,F ) be a Finsler manifold. Suppose that the Cartan tensor satisfies in Cijk = Bihjk + Bjhik + Bkhij with yiBi = 0. Then F is a C-reducible metric. Proof. Suppose that the Cartan tensor of the Finsler metric F satisfies in Cijk = Bihjk + Bjhik + Bkhij . (4) Contracting (4) with gij yields Ik = Bih i k + Bjh j k + (n− 1)Bk. (5) Using (5) and Bih i k = Bjh j k = Bk, we get Ii = (n + 1)Bi. Putting this relation in (4), we conclude that F is a C-reducible Finsler metric. � Lemma 3. Let (M,F ) be a Finsler metric. Then F is a GDW-metric if and only if Di jkl|sy s = Tjkly i, (6) for some tensor Tjkl on manifold M . Proof. Let F be is a GDW-metric hi mDm jkl|sy s = 0. This yields Di jkl|sy s = ( F−2ymDm jkl|s ) yi. Therefore Tjkl := F−2ymDm jkl|s. The proof of converse is trivial. � Equation (6) is equivalent to the condition that, for any parallel vector fields U = U(t), V = V (t) and W = W (t) along a geodesic c(t), there is a function T = T (t) such that d dt [Dċ(U, V,W )] = T ċ. The geometric meaning of the above identity is that the rate of change of the Douglas curvature along a geodesic is tangent to the geodesic. Proposition 1. Let (M,F ) be a Finsler manifold satisfies (2) with dimension n ≥ 3. Suppose that the Douglas tensor of F vanishes. Then F is a Randers metric. Proof. Since F satisfies (2), then by considering µiy i = 0 we get 2Ejk = (n + 1)λhij . (7) On the other hand, we have hij,k = 2Cijk − F−2(yjhik + yihjk), which implies that 2Ejk,l = (n + 1)λ,lhjk + (n + 1)λ { 2Cjkl − F−2(ykhjl + yjhkl) } . (8) 6 A. Tayebi and E. Peyghan Putting (2), (7) and (8) in (3) yields Di jkl = {µjhkl + µkhjl + µlhjk − 2λCjkl}yi − ( λylF −2 + λ,l ) hjky i. (9) For the Douglas curvature, we have Di jkl = Di jlk. Then by (9), we conclude that λylF −2 + λ,l = 0. (10) From (9) and (10) we deduce Di jkl = {µjhkl + µkhjl + µlhjk − 2λCjkl}yi. (11) Since F is a Douglas metric, then Cjkl = 1 2λ{µjhkl + µkhjl + µlhjk}. By Lemmas 2 and 1, it follows that F is a Randers metric. � Proof of Theorem 1. To prove the Theorem 1, we start with the equation (11): Di jkl = {µjhkl + µkhjl + µlhjk − 2λCjkl}yi. (12) Taking a horizontal derivation of (12) implies that Di jkl|sy s = {µ′ jhkl + µ′ khjl + µ′ lhjk − 2λ′Cjkl − 2λLjkl}yi. where λ′ = λ|mym and µ′ i = µi|mym. By Lemma 3, F is a GDW-metric with Tjkl = µ′ jhkl + µ′ khjl + µ′ lhjk − 2λ′Cjkl − 2λLjkl. This completes the proof. � The Funk metric on a strongly convex domain Bn ⊂ Rn is a non-negative function on TΩ = Ω × Rn, which in the special case Ω = Bn (the unit ball in the Euclidean space Rn) is defined by the following explicit formula: F (y) := √ |y|2 − (|x|2|y|2 − 〈x, y〉2) 1− |x|2 + 〈x, y〉 1− |x|2 , y ∈ TxBn = Rn, where | · | and 〈·, ·〉 denote the Euclidean norm and inner product in Rn, respectively [14]. The Funk metric on Bn is a Randers metric. The Berwald curvature of Funk metric is given by Bi jkl = 1 2F { hi jhkl + hi khjl + hi lhjk + 2Cjkly i } . Thus the Funk metric is a GDW-metric which does not satisfy (2). Then by Theorem 1, we conclude the following. Corollary 1. The class of Finsler metrics satisfying (2) is a proper subset of the class of generalized Douglas–Weyl metrics. On Special Berwald Metrics 7 4 Proof of Theorem 2 To prove Theorem 2, we need the following. Lemma 4 ([7, 11]). For the Berwald connection, the following Bianchi identities hold: Ri jkl|m + Ri jlm|k + Ri jmk|l = 0, Bi jml|k −Bi jkm|l = Ri jkl,m, (13) Bi jkl,m = Bi jkm,l. Proof of Theorem 2. We have: Ri jkl = 1 3 { ∂2Ri k ∂yj∂yl − ∂2Ri l ∂yj∂yk } . (14) Here, we assume that a Finsler metric F is of isotropic flag curvature K = K(x). In local coordinates, Ri k = K(x)F 2hi k. Plugging this equation into (14) gives Ri jkl = K{gjlδ i k − gjkδ i l}. (15) Differentiating (15) with respect to ym gives a formula for Ri jkl,m expressed in terms of K and its derivatives. Contracting (13) with yk, we obtain Bi jml|ky k = 2KCjmly i. (16) Multiplying (16) with yi implies that Bi jml|ky kyi = 2KF 2Cjml. (17) Since F satisfies (2), then we have Bi jkl|mym = (µ′ jhkl + µ′ khjl + µ′ lhjk)yi + λ′(hi jhkl + hi khjl + hi lhjk). (18) By contracting (18) with yi, we have Bi jkl|mymyi = (µ′ jhkl + µ′ khjl + µ′ lhjk)F 2. (19) By (17) and (19) we get µ′ jhkl + µ′ khjl + µ′ lhjk = 2KCjkl. Contracting with gkl yields µ′ j = 2K n + 1 Ij . Since K 6= 0, then by Deicke’s theorem F is a Riemannian metric if and only if µ′ j = 0. � Theorem 5. Let F be a Finsler metric on an n-dimensional manifold M (n ≥ 3) and satis- fies (2). Suppose that F is of scalar flag curvature K. Then K = const if and only if λ′ = 0. Proof. Contracting i and l in (2) yields 2Ejk = (n + 1)λhjk. By taking a horizontal derivative of this equation, we have 2Hjk = (n + 1)λ′hjk. Therefore Hjk = 0 if and only if λ′ = 0. By Theorem 4, we get the proof. � 8 A. Tayebi and E. Peyghan 5 Proof of Theorem 3 In this section, we are going to prove Theorem 3. Proof of Theorem 2. Let F be a Finsler metric satisfy in following Bi jkl = (µjhkl + µkhjl + µlhjk)yi + λ ( hi jhkl + hi khjl + hi lhjk ) , (20) where µi = µi(x, y) and λ = λ(x, y) are homogeneous functions of degrees −2 and −1 with respect to y, respectively. Contracting (20) with yi yields yiB i jkl = F 2(µjhkl + µkhjl + µlhjk) + λyi ( hi jhkl + hi khjl + hi lhjk ) . (21) On the other hand, we have yiB i jkl = −2Ljkl, (22) yih i m = yi ( δi m − F−2yiym ) = 0. (23) See [14, page 84]. Using (21), (22) and (23), we get Ljkl = −1 2F 2{µjhkl + µkhjl + µlhjk}. (24) By (24), it is obvious that if µi = 0 then Ljkl = 0. Conversely let F be a Landsberg metric. Then we have µjhkl + µkhjl + µlhjk = 0. (25) Contracting (25) with gkl yields µj = 0. Then F is a Landsberg metric if and only if µj = 0. Now, contracting (24) with gkl yields Jj = −1 2(n + 1)F 2µj . (26) By (26), Jj = 0 if and only if µj = 0. Then L = 0 if and only if J = 0. � By using the notion of Landsberg curvature, we define the stretch curvature Σy : TxM ⊗ TxM ⊗ TxM ⊗ TxM → R by Σy(u, v, w, z) := Σijkl(y)uivjwkzl where Σijkl := 2(Lijk|l − Lijl|k). In [3], L. Berwald has introduce the stretch curvature tensor Σ and showed that this tensor vanishes if and only if the length of a vector remains unchanged under the parallel displacement along an infinitesimal parallelogram. Theorem 6. Let (M,F ) be a Finsler manifold on which (2) holds. Suppose that F is a stretch metric. Then µj is constant along any Finslerian geodesics. Proof. Taking a horizontal derivation of (24) yields Lijk|l = −1 2F 2{µi|lhjk + µj|lhki + µk|lhij}. Suppose that Σ = 0. Then by Lijk|l = Lijl|k, we get µi|lhjk + µj|lhki + µk|lhij = µi|khjl + µj|khli + µl|khij . (27) Multiplying (27) with yl implies that µ′ ihjk + µ′ jhki + µ′ khij = 0. (28) By contracting (28) with gjk, we conclude the following (n + 1)µ′ i = 0. 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[16] Tayebi A., Rafie Rad M., S-curvature of isotropic Berwald metrics, Sci. China Ser. A 51 (2008), 2198–2204. http://dx.doi.org/10.1023/B:MAHU.0000038974.24588.83 http://dx.doi.org/10.1007/s10711-007-9218-9 http://dx.doi.org/10.1007/s11425-008-0095-y 1 Introduction 2 Preliminaries 3 Proof of Theorem 1 4 Proof of Theorem 2 5 Proof of Theorem 3 References