On Darboux vector in Lorentzian 5-space

We introduce the Darboux vector in the Lorentzian 5-space. We give some characterizations of this vector in the space. In addition, we consider some special cases in the space.

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Дата:2018
Автори: Iyigün, E., Ійігун, Е.
Формат: Стаття
Мова:Англійська
Опубліковано: Institute of Mathematics, NAS of Ukraine 2018
Онлайн доступ:https://umj.imath.kiev.ua/index.php/umj/article/view/1583
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Назва журналу:Ukrains’kyi Matematychnyi Zhurnal
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Ukrains’kyi Matematychnyi Zhurnal
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author Iyigün, E.
Ійігун, Е.
author_facet Iyigün, E.
Ійігун, Е.
author_sort Iyigün, E.
baseUrl_str https://umj.imath.kiev.ua/index.php/umj/oai
collection OJS
datestamp_date 2019-12-05T09:19:33Z
description We introduce the Darboux vector in the Lorentzian 5-space. We give some characterizations of this vector in the space. In addition, we consider some special cases in the space.
first_indexed 2026-03-24T02:08:32Z
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fulltext UDC 517.5 E. Iyigün (Uludag Univ., Bursa, Turkey) ON DARBOUX VECTOR IN LORENTZIAN 5-SPACE ПРО ВЕКТОР ДАРБУ В 5-ПРОСТОРI ЛОРЕНЦА We introduce the Darboux vector in the Lorentzian 5-space. We give some characterizations of this vector in the space. In addition, we consider some special cases in the space. Введено вектор Дарбу в 5-просторi Лоренца. Наведено деякi харатеристики даного вектора в цьому просторi. Крiм того, розглянуто деякi частиннi випадки в цьому ж просторi. 1. Introduction. Let X = (x1, x2, x3, x4, x5) and Y = (y1, y2, y3, y4, y5) be two non-zero vectors in Lorentzian 5-space \BbbL 5. For X, Y \in \BbbL 5 g(X,Y ) = \langle X,Y \rangle = - x1y1 + 5\sum i=2 xiyi, is called Lorentzian inner product. The couple \bigl\{ \BbbL 5, \langle , \rangle \bigr\} is called Lorentzian 5-space. Then the vector X of \BbbL 5 is called: (i) time-like if \langle X,X\rangle < 0, (ii) space-like if \langle X,X\rangle > 0 or X = 0, (iii) null (or light-like) vector if \langle X,X\rangle = 0 and X \not = 0. The set of a null vectors in Tp(\BbbL 5) is called the nullcone at p \in \BbbL 5. Similarly, an arbitrary curve \alpha = \alpha (s) in \BbbL 5 can be locally be space-like, time-like or null, if all of its velocity vectors \alpha \prime (s) are respectively space-like, time-like or null. Also, recall the norm of a vector X is given by \| X\| = \sqrt{} | \langle X,X\rangle | . Therefore, X is a unit vector if \langle X,X\rangle = \pm 1. Next, vectors X, Y in \BbbL 5 are said to be orthogonal if \langle X,Y \rangle = 0. The velocity of the curve \alpha is given by \| \alpha \prime (s)\| . Thus, a space-like or a time-like \alpha is said to be parametrized by arclength function s, if \langle \alpha \prime (s), \alpha \prime (s)\rangle = \pm 1 [1]. 2. Basic definitions of \BbbL 5 . Definition 1. Let \alpha : I - \rightarrow \BbbL 5 be a curve in \BbbL 5 and k1, k2, k3, k4 be the Frenet curvatures of \alpha . Then for the unit tangent vector V1 = \alpha \prime (s) over M the ith e-curvature function mi, 1 \leq i \leq 5, is defined by mi = \left\{ 0, i = 1, \varepsilon 1\varepsilon 2 k1 , i = 2,\biggl[ d dt (mi - 1) + \varepsilon i - 2mi - 2ki - 2 \biggr] \varepsilon i ki - 1 , 2 < i \leq 5, (1) where \varepsilon i = \langle Vi, Vi\rangle = \pm 1. Definition 2. Let \alpha : I - \rightarrow \BbbL 5 be a unit speed non-null curve. The curve \alpha is called Frenet curve of osculating order d, d \leq 5, if its 5th order derivatives \alpha \prime (s), \alpha \prime \prime (s), . . . , \alpha v(s) are linearly independent and \alpha \prime (s), \alpha \prime \prime (s), . . . , \alpha v\imath (s) are no longer linearly independent for all s \in I. For each Frenet curve of order 5 one can associate an orthonormal 5-frame \bigl\{ V1, V2, V3, V4, V5 \bigr\} along \alpha (such that \alpha \prime (s) = V1) called the Frenet frame k1, k2, k3, k4 : I - \rightarrow \BbbR called the Frenet curvatures, such that the Frenet formulas is defined in the usual way; c\bigcirc E. IYIGÜN, 2018 ISSN 1027-3190. Укр. мат. журн., 2018, т. 70, № 5 635 636 E. IYIGÜN \nabla V1V1 = \varepsilon 2k1V2, \nabla V1V2 = - \varepsilon 1k1V1 + \varepsilon 3k2V3, \nabla V1V3 = - \varepsilon 2k2V2 + \varepsilon 4k3V4, (2) \nabla V1V4 = - \varepsilon 3k3V3 + \varepsilon 5k4V5, \nabla V1V5 = - \varepsilon 4k4V4, where V1, V2, V3, V4, and V5 are orthogonal vectors satisfying equations \langle V1, V1\rangle = - 1, \langle Vi, Vi\rangle = 1, 2 \leq i \leq 5, and \nabla is the Levi-Civita connection of \BbbL 5. Definition 3. Let \alpha be a non-null curve of osculating order 5. The harmonic functions Hj : I - \rightarrow \BbbR , 0 \leq j \leq 3, defined by H0 = 0, H1 = k1 k2 ,\biggl[ d dt (Hj - 1) + \varepsilon j - 2Hj - 2kj \biggr] \varepsilon j kj+1 , 2 \leq j \leq 3, are called the harmonic curvatures of \alpha , where k1, k2, kj , kj+1 are Frenet curvatures of \alpha which are not necessarily constant and \varepsilon j = \langle Vj , Vj\rangle = \pm 1 [2]. Definition 4. Let \alpha be a non-null curve of osculating order 5. Then \alpha is called a general helix of rank 3 if 3\sum i=1 (Hi) 2 = c, holds, where c \not = 0 is a real constant. Corollary 1. If \alpha is a general helix of rank 3, then H2 1 +H2 2 +H2 3 = c. Proof. By the use of above definition, we obtain the corollary. 3. The Darboux vector in \BbbL 5 . Theorem 1. Let \alpha be a non-null curve of osculating order 5 in \BbbL 5, then \nabla VjVi = \varepsilon i mi+1 Vi+1, i, j = 1, \nabla VjVi+1 = - \varepsilon i+1 mi+1 Vi + m\prime i+1 mi+2 Vi+2, i, j = 1, ISSN 1027-3190. Укр. мат. журн., 2018, т. 70, № 5 ON DARBOUX VECTOR IN LORENTZIAN 5-SPACE 637 \nabla VjVi+1 = \biggl( - \varepsilon i\varepsilon i+1mim \prime i - \varepsilon i - 1\varepsilon i+1mi - 1m \prime i - 1 mimi+1 \biggr) Vi+ + \biggl( mi+1m \prime i+1 + \varepsilon i\varepsilon i+1mim \prime i + \varepsilon i - 1\varepsilon i+1mi - 1m \prime i - 1 mi+1mi+2 \biggr) Vi+2, j = 1, i = 2, 3, \nabla VjVi+1 = \biggl( - \varepsilon i\varepsilon i+1mim \prime i - \varepsilon i - 1\varepsilon i+1mi - 1m \prime i - 1 - \varepsilon i - 2\varepsilon i+1mi - 2m \prime i - 2 mimi+1 \biggr) Vi, j = 1, i = 4, where mi are the ith e-curvature functions and \varepsilon i = \langle Vi, Vi\rangle = \pm 1. Corollary 2. Let \alpha be a non-null curve of osculating order 5 in \BbbL 5, then \nabla V1V1 = \varepsilon 1 m2 V2, \nabla V1V2 = - \varepsilon 2 m2 V1 + m\prime 2 m3 V3, \nabla V1V3 = - \varepsilon 2\varepsilon 3 m\prime 2 m3 V2 + \biggl( m3m \prime 3 + \varepsilon 2\varepsilon 3m2m \prime 2 m3m4 \biggr) V4, \nabla V1V4 = \biggl( - \varepsilon 3\varepsilon 4m3m \prime 3 - \varepsilon 2\varepsilon 4m2m \prime 2 m3m4 \biggr) V3 + \biggl( m4m \prime 4 + \varepsilon 3\varepsilon 4m3m \prime 3 + \varepsilon 2\varepsilon 4m2m \prime 2 m4m5 \biggr) V5, \nabla V1V5 = \biggl( - \varepsilon 4\varepsilon 5m4m \prime 4 - \varepsilon 3\varepsilon 5m3m \prime 3 - \varepsilon 2\varepsilon 5m2m \prime 2 m4m5 \biggr) V4. Proof. By the use of a previous theorem, we obtain the corollary. Theorem 2. Let \alpha be a non-null curve of osculating order 5 in \BbbL 5, then \nabla V1V1 = \varepsilon 2k2H1V2, \nabla V1V2 = - \varepsilon 1k2H1V1 + \varepsilon 3 k1 H1 V3, \nabla V1V3 = - \varepsilon 2 k1 H1 V2 + \varepsilon 2\varepsilon 4 H \prime 1 H2 V4, \nabla V1V4 = - \varepsilon 2\varepsilon 3 H \prime 1 H2 V3 + \varepsilon 3\varepsilon 5 \biggl( H2H \prime 2 + \varepsilon 1\varepsilon 2H1H \prime 1 H2H3 \biggr) V5, \nabla V1V5 = - \varepsilon 3\varepsilon 4 \biggl( H2H \prime 2 + \varepsilon 1\varepsilon 2H1H \prime 1 H2H3 \biggr) V4, where H1, H2, H3 are harmonic curvature of \alpha and \varepsilon i = \langle Vi, Vi\rangle = \pm 1 for 1 \leq i \leq 5. Proof. By using definition of harmonic curvatures, we obtain the theorem. Theorem 3. Let \alpha : - \rightarrow \BbbL 5 be a non-null curve of osculating order 5 given over the Frenet frame \bigl\{ V1, V2, V3, V4, V5 \bigr\} . If mi, 2 \leq i \leq 5, are the ith e-curvature functions, Hi, 1 \leq i \leq 3, are the harmonic curvatures and m\prime i = dmi ds , 2 \leq i \leq 5, then the following relations hold: \mathrm{d}\mathrm{e}\mathrm{t}(m\prime 2,m \prime 3,m \prime 4,m \prime 5) = 0 \Leftarrow \Rightarrow 3\sum i=1 (Hi) 2 = \mathrm{c}\mathrm{o}\mathrm{n}\mathrm{s}\mathrm{t}\mathrm{a}\mathrm{n}\mathrm{t}, ISSN 1027-3190. Укр. мат. журн., 2018, т. 70, № 5 638 E. IYIGÜN \mathrm{d}\mathrm{e}\mathrm{t}(m\prime 2,m \prime 3,m \prime 4,m \prime 5) = 0 \Leftarrow \Rightarrow 5\sum i=2 m2 i = \mathrm{c}\mathrm{o}\mathrm{n}\mathrm{s}\mathrm{t}\mathrm{a}\mathrm{n}\mathrm{t}. Proof. The proof can seen by using the definitions of ith e-curvature functions and harmonic curvatures. Definition 5. Let \alpha be a non-null curve of osculating order 5 in \BbbL 5, with Frenet curvatures k1, k2, k3, k4. Let us denote a0 = k2k4, aj = \varepsilon j k2j - 1 k2j aj - 1, 1 \leq j \leq 2, k2j \not = 0. The Darboux vector in \BbbL 5 is defined by D(s) = 2\sum j=0 ajV2j+1 = a0V1 + a1V3 + a2V5, where V2j+1 are the Frenet vectors of \alpha . Corollary 3. Let \alpha be a non-null curve of osculating order 5 in \BbbL 5, then aj aj - 1 = \varepsilon j k2j - 1 k2j , where 1 \leq j \leq 2, k2j \not = 0. Lemma 1. The derivative of the Darboux vector D(s) is [4]. D\prime (s) = a\prime 0V1 + a\prime 1V3 + a\prime 2V5. Definition 6. The point \alpha (s0) is called Darboux vertex of \alpha if the first derivative of the Darboux vector D(s) is vanishing at that point [3]. Theorem 4. Let \alpha be a non-null curve of osculating order 5 in \BbbL 5, with Frenet curvatures k1, k2, k4 and harmonic curvatures H1, H2. Let us denote a0 = k1k4 H1 , a1 = \varepsilon 1H1k2k4, a2 = \varepsilon 1 H \prime 1 H2 k1, where H1 \not = 0, H2 \not = 0, \varepsilon 1 = \langle V1, V1\rangle = \pm 1. Proof. By using definition of harmonic curvature, we get the result. The following theorem is true. Theorem 5. Let \alpha : I - \rightarrow \BbbL 5 be a non-null curve of osculating order 5. Then H1 = \varepsilon 1 a1 a0 , a0 \not = 0, ISSN 1027-3190. Укр. мат. журн., 2018, т. 70, № 5 ON DARBOUX VECTOR IN LORENTZIAN 5-SPACE 639 H2 = \varepsilon 1 a0H1H \prime 1 a2k4 , a2 \not = 0, k4 \not = 0, where H1, H2 are harmonic curvatures of \alpha , k4 is Frenet curvature of \alpha , \varepsilon 1 = \langle V1, V1\rangle = \pm 1 and a0, a1, a2 \in R. Proof. By the use of a previous theorem, we obtain the theorem. Corollary 4. (i) If the vector V1 is space-like, then H1 = a1 a0 , a0 \not = 0, H2 = a0H1H \prime 1 a2k4 , a2 \not = 0, k4 \not = 0. (ii) If the vector V1 is time-like, then H1 = - a1 a0 , a0 \not = 0, H2 = - a0H1H \prime 1 a2k4 , a2 \not = 0, k4 \not = 0. Theorem 6. Let \alpha be a non-null curve of osculating order 5 in \BbbL 5,with Frenet curvatures k1, k2, k3, k4. Then the curve \alpha has a Darboux vertex at point \alpha (s) if and only if \varepsilon i \biggl( ki ki+1 \biggr) \prime = 0, ki+1 \not = 0, 1 \leq i \leq 3, where \varepsilon i = \langle Vi, Vi\rangle = \pm 1. Corollary 5. (i) If the vector V1 is space-like, then (H1) \prime = 0. (ii) If the vector V1 is time-like, then - (H1) \prime = 0. Corollary 6. If \alpha : I - \rightarrow \BbbL 5 has a Darboux vertex at the point \alpha (s0), then \alpha is a general helix of order 3 [3]. 4. ccr-Curve in \BbbL 5 . Definition 7. A curve \alpha : I - \rightarrow \BbbL 5 is said to have constant curvature ratios (that is to say, it is a ccr-curve) if all the quotients \varepsilon i \biggl( ki+1 ki \biggr) are constant, ki \not = 0. Here, ki, ki+1, 1 \leq i \leq 3, are Frenet curvatures of \alpha , and \varepsilon i = \langle Vi, Vi\rangle = \pm 1, 1 \leq i \leq 3. Theorem 7. (i) For i = 1, the ccr-curve is a1 a0(H1)2 . (ii) For i = 2, the ccr-curve is \varepsilon 1 a2H1 (k1)2 . (iii) For i = 3, the ccr-curve is \varepsilon 2\varepsilon 3 a0H2 k2H \prime 1 . Here H1, H2 are harmonic curvatures of \alpha ; k1, k2 are Frenet curvatures of \alpha ; \varepsilon i = \langle Vi, Vi\rangle = = \pm 1, 1 \leq i \leq 3, and a0, a1, a2 \in R. ISSN 1027-3190. Укр. мат. журн., 2018, т. 70, № 5 640 E. IYIGÜN Proof. The proof can be easily seen by using the definitions of the harmonic curvature and ccr-curve. Corollary 7. (i) If the vector V1 is space-like, then the ccr-curve is a2H1 (k1)2 , where \varepsilon 1 = 1. (ii) If the vector V1 is time-like, then the ccr-curve is - a2H1 (k1)2 , where \varepsilon 1 = - 1. (iii) If the vectors V2, V3 are space-like, then the ccr-curve is a0H2 k2H \prime 1 , where \varepsilon 2 = \varepsilon 3 = 1. (iv) If the vector V2 is time-like, then the ccr-curve is - a0H2 k2H \prime 1 , where \varepsilon 2 = - 1 and \varepsilon 3 = 1. (v) If the vector V3 is time-like, then the ccr-curve is - a0H2 k2H \prime 1 , where \varepsilon 3 = - 1 and \varepsilon 2 = 1. Corollary 8. \alpha is a ccr-curve in \BbbL 5 \leftrightarrow \varepsilon 1 (H1) - 1 = \mathrm{c}\mathrm{o}\mathrm{n}\mathrm{s}\mathrm{t}\mathrm{a}\mathrm{n}\mathrm{t}. Corollary 9. For \alpha : I - \rightarrow \BbbL 5 curve, we have \varepsilon i \biggl( ki ki+1 \biggr) \prime = \varepsilon i \biggl( ki+1 ki \biggr) , 1 \leq i \leq 3, that is the Darboux vertex is equal to the constant curvature ratio. Now, we will calculate Darboux vector and Darboux vertex of the unit speed time-like curve in \BbbL 5 studied in [5]. 5. An example. Example 1. Let us consider the following curve: \alpha (s) = \Bigl( \surd 3 \mathrm{s}\mathrm{i}\mathrm{n}\mathrm{h} s, \surd 3 \mathrm{c}\mathrm{o}\mathrm{s}\mathrm{h} s, \mathrm{s}\mathrm{i}\mathrm{n} s, s, \mathrm{c}\mathrm{o}\mathrm{s} s \Bigr) , V1(s) = \alpha \prime (s) = \Bigl( \surd 3 \mathrm{c}\mathrm{o}\mathrm{s}\mathrm{h} s, \surd 3 \mathrm{s}\mathrm{i}\mathrm{n}\mathrm{h} s, \mathrm{c}\mathrm{o}\mathrm{s} s, 1, - \mathrm{s}\mathrm{i}\mathrm{n} s \Bigr) , where \langle \alpha \prime (s), \alpha \prime (s)\rangle = - 1. One can easily see that \alpha (s) is an unit speed time-like curve. We express the following differentiations: \alpha \prime \prime (s) = \Bigl( \surd 3 \mathrm{s}\mathrm{i}\mathrm{n}\mathrm{h} s, \surd 3 \mathrm{c}\mathrm{o}\mathrm{s}\mathrm{h} s, - \mathrm{s}\mathrm{i}\mathrm{n} s, 0, - \mathrm{c}\mathrm{o}\mathrm{s} s \Bigr) \Rightarrow \Rightarrow \alpha \prime \prime \prime (s) = \Bigl( \surd 3 \mathrm{c}\mathrm{o}\mathrm{s}\mathrm{h} s, \surd 3 \mathrm{s}\mathrm{i}\mathrm{n}\mathrm{h} s, - \mathrm{c}\mathrm{o}\mathrm{s} s, 0, \mathrm{s}\mathrm{i}\mathrm{n} s \Bigr) \Rightarrow \Rightarrow \alpha \imath v(s) = \Bigl( \surd 3 \mathrm{s}\mathrm{i}\mathrm{n}\mathrm{h} s, \surd 3 \mathrm{c}\mathrm{o}\mathrm{s}\mathrm{h} s, \mathrm{s}\mathrm{i}\mathrm{n} s, 0, \mathrm{c}\mathrm{o}\mathrm{s} s \Bigr) \Rightarrow \Rightarrow \alpha v(s) = \Bigl( \surd 3 \mathrm{c}\mathrm{o}\mathrm{s}\mathrm{h} s, \surd 3 \mathrm{s}\mathrm{i}\mathrm{n}\mathrm{h} s, \mathrm{c}\mathrm{o}\mathrm{s} s, 0, - \mathrm{s}\mathrm{i}\mathrm{n} s \Bigr) . So, we have the first curvature as \bigm\| \bigm\| \alpha \prime \prime (s) \bigm\| \bigm\| = k1(s) = 2. Moreover we can write second, third, fourth and fifth Frenet vectors of the curve, respectively, V2(s) = \varepsilon 2 \Biggl( \surd 3 2 \mathrm{s}\mathrm{i}\mathrm{n}\mathrm{h} s, \surd 3 2 \mathrm{c}\mathrm{o}\mathrm{s}\mathrm{h} s, - 1 2 \mathrm{s}\mathrm{i}\mathrm{n} s, 0, - 1 2 \mathrm{c}\mathrm{o}\mathrm{s} s \Biggr) , ISSN 1027-3190. Укр. мат. журн., 2018, т. 70, № 5 ON DARBOUX VECTOR IN LORENTZIAN 5-SPACE 641 V3(s) = 1\surd 14 \Bigl( - 3 \surd 3 \mathrm{c}\mathrm{o}\mathrm{s}\mathrm{h} s, - 3 \surd 3 \mathrm{s}\mathrm{i}\mathrm{n}\mathrm{h} s, - 5 \mathrm{c}\mathrm{o}\mathrm{s} s, - 4, 5 \mathrm{s}\mathrm{i}\mathrm{n} s \Bigr) , V4(s) = \mu \biggl( - 1 2 \mathrm{s}\mathrm{i}\mathrm{n}\mathrm{h} s, - 1 2 \mathrm{c}\mathrm{o}\mathrm{s}\mathrm{h} s, - 3 2 \mathrm{s}\mathrm{i}\mathrm{n} s, 0, - 3 2 \mathrm{c}\mathrm{o}\mathrm{s} s \biggr) and V5(s) = \mu \Biggl( - 1\surd 14 \mathrm{c}\mathrm{o}\mathrm{s}\mathrm{h} s, - 1\surd 14 \mathrm{s}\mathrm{i}\mathrm{n}\mathrm{h} s, \sqrt{} 3 14 \mathrm{c}\mathrm{o}\mathrm{s} s, - \sqrt{} 2 7 , - \sqrt{} 3 14 \mathrm{s}\mathrm{i}\mathrm{n} s \Biggr) , where \mu is taken \mp 1 to make +1 determimant of \{ V1(s), V2(s), V3(s), V4(s), V5(s)\} matrix. In ad- dition to, we can write second, third, fourth curvatures and harmonic curvature of \alpha (s), respectively, k2(s) = \surd 14, k3(s) = \sqrt{} 3 14 , k4(s) = \sqrt{} 2 7 , H1 = 2\surd 14 , a0 = 2, a1 = \varepsilon 1 \Biggl( 2 \surd 2\surd 7 \Biggr) , a2 = 0. Now, we will calculate ccr-curves of \alpha (s) in \BbbL 5. If the vector V1 is time-like, then \mu = 1, \varepsilon 1 = - 1 and \varepsilon 2 = \varepsilon 3 = 1 \varepsilon 1 k2 k1 = - \surd 14 2 = \mathrm{c}\mathrm{o}\mathrm{n}\mathrm{s}\mathrm{t}\mathrm{a}\mathrm{n}\mathrm{t}, \varepsilon 2 \mathrm{k}3 \mathrm{k}2 = \surd 3 14 = \mathrm{c}\mathrm{o}\mathrm{n}\mathrm{s}\mathrm{t}\mathrm{a}\mathrm{n}\mathrm{t} and \varepsilon 3 \mathrm{k}4 \mathrm{k}3 = 2\surd 3 = \mathrm{c}\mathrm{o}\mathrm{n}\mathrm{s}\mathrm{t}\mathrm{a}\mathrm{n}\mathrm{t}. Thus, \alpha (s) is a ccr-curve in \BbbL 5. Also, we obtain, respectively, Darboux vector and Darboux vertex of \alpha (s) in \BbbL 5, (i) If the vector V1 is time-like, then \mu = 1, \varepsilon 1 = - 1 and \varepsilon 2 = \varepsilon 3 = 1, D(s) = \Biggl( 20 \surd 3 7 \mathrm{c}\mathrm{o}\mathrm{s}\mathrm{h} s, 20 \surd 3 7 \mathrm{s}\mathrm{i}\mathrm{n}\mathrm{h} s, 24 7 \mathrm{c}\mathrm{o}\mathrm{s} s, 22 7 , - 24 7 \mathrm{s}\mathrm{i}\mathrm{n} s \Biggr) and D\prime (s) = \Biggl( 20 \surd 3 7 \mathrm{s}\mathrm{i}\mathrm{n}\mathrm{h} s, 20 \surd 3 7 \mathrm{c}\mathrm{o}\mathrm{s}\mathrm{h} s, - 24 7 \mathrm{s}\mathrm{i}\mathrm{n} s, 0, - 24 7 \mathrm{c}\mathrm{o}\mathrm{s} s \Biggr) . (ii) If the vector V1 is time-like, then Darboux vector and Darboux vertex are as in (i) when \mu = - 1, \varepsilon 1 = - 1 and \varepsilon 2 = \varepsilon 3 = 1, since a2 = 0. References 1. O’neill B. Semi-Riemannian geometry with applications to relativity. – New York: Acad. Press, 1983. 2. İyigün E., Arslan K. On harmonic curvatures of curves in Lorentzian n-space // Commun. Fac. Sci. Univ. Ank. Ser. A1. – 2005. – 54, № 1. – P. 29 – 34. 3. Öztürk G., Arslan K., Hacısalihoğlu H. H. A characterization of ccr-curves in Rm // Proc. Eston. Acad. Sci. – 2008. – 57, № 4. – P. 217 – 224. 4. Uribe-Vargas R. On singularities, perestroikas and differential geometry of space curves // Enseign. Math. – 2004. – 50. – P. 69 – 101. 5. Turgut M., Lopez-Bonilla J. L., Yılmaz S. On Frenet – Serret invariants of non-null curves in Lorentzian space L5 // World Acad. Sci., Eng. and Technology. – 2009. – 55. – P. 638 – 640. 6. Kocayiğit H., Öztürk G., Bayram B. K., Bulca B., Arslan K. Characterization of curves in E2n+1 with 1-type Darboux vector // Math. Morav. – 2013. – 17, № 2. – P. 29 – 37. Received 09.11.16 ISSN 1027-3190. Укр. мат. журн., 2018, т. 70, № 5
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spelling umjimathkievua-article-15832019-12-05T09:19:33Z On Darboux vector in Lorentzian 5-space Про вектор дарбу в 5-просторi Лоренца Iyigün, E. Ійігун, Е. We introduce the Darboux vector in the Lorentzian 5-space. We give some characterizations of this vector in the space. In addition, we consider some special cases in the space. Введено вектор Дарбу в 5-просторi Лоренца. Наведено деякi харатеристики даного вектора в цьому просторi. Крiм того, розглянуто деякi частиннi випадки в цьому ж просторi. Institute of Mathematics, NAS of Ukraine 2018-05-25 Article Article application/pdf https://umj.imath.kiev.ua/index.php/umj/article/view/1583 Ukrains’kyi Matematychnyi Zhurnal; Vol. 70 No. 5 (2018); 635-641 Український математичний журнал; Том 70 № 5 (2018); 635-641 1027-3190 en https://umj.imath.kiev.ua/index.php/umj/article/view/1583/565 Copyright (c) 2018 Iyigün E.
spellingShingle Iyigün, E.
Ійігун, Е.
On Darboux vector in Lorentzian 5-space
title On Darboux vector in Lorentzian 5-space
title_alt Про вектор дарбу в 5-просторi Лоренца
title_full On Darboux vector in Lorentzian 5-space
title_fullStr On Darboux vector in Lorentzian 5-space
title_full_unstemmed On Darboux vector in Lorentzian 5-space
title_short On Darboux vector in Lorentzian 5-space
title_sort on darboux vector in lorentzian 5-space
url https://umj.imath.kiev.ua/index.php/umj/article/view/1583
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