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AKÜ FEMÜBİD 16 (2016)031301 (569-575) DOI:10.5578/fmbd.32172

AKU J. Sci. Eng. 16 (2016)031301 (569-575)

Araştırma Makalesi / Research Article

On Involutes of Order k of a Space-like Curve in Minkowski 4-space IE

14

Günay Öztürk

Kocaeli University, Art and Science Faculty, Department of Mathematics, Kocaeli, TURKEY e-posta: ogunay@kocaeli.edu.tr

Geliş Tarihi:25.04.2016 ; Kabul Tarihi:07.10.2016

Keywords Involute; Space-like Curve; W-curve; Helix.

Abstract

The orthogonal trajectories of the first tangents of a curve x are called the involutes of x. In this study, we give a characterization of involutes of order k of a space-like curve x with time-like principal normal in Minkowski 4-space IE . 14

4

IE

1

Minkowski 4-uzayında bir Space-like Eğrinin k’yinci Mertebeden İnvolütleri Üzerine

Anahtar kelimeler İnvolüt; Space-like Eğri;

W-eğrisi; Helis.

Özet

Bir x eğrisinin birinci teğetlerinin dik yörüngelerine eğrinin involütleri adı verilir. Bu çalışmada, IE 41 Minkowski 4-uzayında time-like asli normalli bir space-like eğrinin k’yinci mertebeden involütlerinin bir karakterizasyonunu verdik.

© Afyon Kocatepe Üniversitesi

1. Introduction

4

IE Minkowski space-time 1 IE is a pseudo-41 Euclidean space IE provided with the standart flat 4 metric given by

gdx12 dx22 dx32 dx24, (1) where (x1,x2,x3,x4) is a rectangular coordinate system in IE14. Since g is an indefinite metric, recall that a vector v ∈IE41 can have one of the three causal characters; it can be space-like if g(v,v)0 or v0, time-like if g(v,v)0, and null (light-like) if g(v,v)0 and v0. Similarly, an arbitrary curve

) s ( x

x in IE can be locally space-like, time-like 14 or null if all of its velocity vectors x(s) are respectively space-like, time-like or null. Also, recall the norm of a vector v is given by v  g(v,v). Therefore, v is a unit vector if g(v,v)1. Next, vectors v, w in IE14 are said to be orthogonal if

0 ) w , v (

g  . The velocity of the curve x(s) is given by x(s) . Space-like or time-like curve x(s) is said

to be parametrized by arc-length function s, if 1

)) s ( x ), s ( x (

g    (O’Neill, 1983).

Let x(s) be a space-like curve with a time- like principal normal in the space-time IE41, parametrized by arc-length function s. Then we have the following Frenet equations (Walfare, 1995):

























4 3 2 1

3 3 2

2 1

1

4 3 2 1

V V V V

0 k 0 0

k 0 k 0

0 k 0 k

0 0 k 0

V V V V

, (2)

where V , 1 V , 2 V3 and V are the Frenet vectors 4 satisfy the equations:

g(V1,V1)g(V3,V3)g(V4,V4)1, g(V2,V2)1. Here k , 1 k , 2 k3 are respectively, the first, the second and the third curvatures of the curve x(s).

Definition 1. (Yılmaz and Turgut, 2008) Let )

a , a , a , a (

a 1 2 3 4 , b(b1,b2,b3,b4) and )

c , c , c , c (

c 1 2 3 4 be vectors in IE41. The vector

Afyon Kocatepe University Journal of Science and Engineering

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AKÜ FEMÜBİD 16 (2016) 031301 570

product in Minkowski space-time IE is defined by 41 the determinant

4 3 2 1

4 3 2 1

4 3 2 1

4 3 2 1

c c c c

b b b b

a a a a

e e e e c

b a

 , (3)

where e , 1 e , 2 e3 and e are mutually 4 orthogonal vectors satisfying the equations

4 3 2

1 e e e

e    , e2e3e4 e1,

2 1 4

3 e e e

e    , e4e1e2 e3.

Let x(s) be a space-like curve in IE . The 41 Frenet frame vectors V , 1 V , 2 V3, V and Frenet 4 curvatures k1, k2, k3 are given by

) s ( x

) s ( ) x s ( V1

  ,

) s ( x ) s ( x ) s ( x

) s ( x ) s ( x ) s ( ) x s (

V4   





 

∧ ,

) s ( x ) s ( x V

) s ( x ) s ( x ) V

s ( V

4 4

3    

 

 

 , (4)

) s ( x V V

) s ( x V ) V

s ( V

4 3

4 3

2   

 

 

and

2 2

1 x(s)

)) s ( x ), s ( V ( ) g s (

k 

  ,

) s ( k ) s ( x

)) s ( x ), s ( V ( ) g s ( k

1 3 3

2

  , (5)

) s ( k ) s ( k ) s ( x

)) s ( x ), s ( V ( ) g s ( k

2 1 4

) ıv ( 4

3   ,

respectively, where  is vector product in IE 41 (Gluck, 1966).

A curve which has constant first Frenet curvature IE is called a Salkowski curve 14 (Salkowski, 1909). ( or T.C-curve (Kılıç et al. 2008)).

An arbitrary curve is called W-curve or (circular) helix if it has constant Frenet curvatures (Klein and

Lie, 1871). Meanwhile, a curve with constant curvature ratios IE is called a ccr-curve 14 (Monterde, 2007), (Öztürk et al. 2008).

In (Öztürk et al.) (2016), the authors gave a characterization of involutes of order k of a given curve in IE . They obtain some results about the n involutes of order 1, 2, 3 of a given curve in IE , 3 IE4 , respectively.

In the present study, we give a characterization of involutes of order k of a space- like curve x in Minkowski space-time IE . 14

2. Involute curves of order k

Definition 2. Let x(s) be a regular space-like curve in IE given with arc-length parameter s. Then the 41 curves which are orthogonal to the system of k- dimensional osculating hyperplanes of x are called the involutes of k (or k involute) of the curve x th (Balazenka and Zeljka 1999). For simplicity, we call the involutes of order 1, the involute of the given curve.

In order to find the parametrization of involutes x(s) of order k of the curve x in IE , we 14 put

k

1 i

i

i(s)V(s), k 3 )

s ( x ) s (

x , (6)

where i is a differentiable function and s, which is not necessarily an arc-length parameter, is the parameter of x(s).

Furthermore, the involutes

x

of order k of the curve x in IE are detemined by 14

. 3 k i 1 , 0 )) s ( V ), s ( x (

g  i  ≤ ≤ ≤ (7)

2.1. Involute curves of order 1

Theorem 1. Let x(s) be a space-like curve with time-like principal normal in IE given with the 41

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AKÜ FEMÜBİD 16 (2016) 031301 571

Frenet curvatures k , 1 k , 2 k3. Then, the involute

x

of the curve x is a time-like curve with the Frenet frame vectors V1, V2, V3, V4 and Frenet curvatures k1, k2, k3 which are given by

2 1(s) V V  ,

2 2 2 1

3 2 1 1

2 k k

V k V ) k s (

V 

  ,





 

4 2 2 2 1

3 1 2 1

1 1 2 2

2 2 2 1 3

V ) k k ( D

V ) C k A k ( k

V ) C k A k ( k k k W ) 1 s (

V , (8)

2 1 1 3 2 1 4

4 k DV k DV (k A k C)V

W ) 1 s (

V      ,

and

2122

1

k ) k

s (

k ,

) k k ( ) W s (

k 2

2 2 1 2 2



 , (9)



 

 



 

 

2

3 1 2 1

3 1 2 2

2 2 2 1

3 D(k C k A) k k D

) D C k )(

C k A k ( W

k ) k

s ( k

respectively, where k1

) s c ( 

 ,





k1 2k1

A ,

 

k21 k22

B ,



k2 2k2

C ,

k2k3

D ,

and

. ) k k k k ( ) k k ( k k

) C k A k ( ) k k ( D W

2 2 1 2 1 2 2 2 1 2 3 2 2

2 1 2 2 2 2 1 2

 

 

 (10)

Proof. Let x(s)be the involute of a space-like curve x with time-like principal normal in IE . Then by 14 the use of (6) with (7), we get 11(s)0, and furthermore 1(s)(cs) for some constant c. We have the following parametrization

) s ( V ) s c ( ) s ( x ) s (

x    1 (11) Further, differentiating the equation (11), we find

V2

) s (

x  ,

3 2 2 1

1V V k V

k ) s (

x    , (12)

4 3 2 3 2 2

2 2 2 2

1 1 1 1

V k k V ) k 2 k (

V ) k k

( V ) k 2 k ( ) s ( x











 

where (s)1(s)k1(s) is a differentiable function. Substituting





k1 2k1

A ,

 

k21 k22

B ,





k2 2k2

C ,

k2k3

D .

in the last equation, we obtain

4 3 2

1 BV CV DV

AV ) s (

x      .

Furthermore, differentiating x (s) with respect to s, we get

3 3

3 3 2

2 2 1 1

1 )

ıv (

V ) D C k ( V ) D k B k C (

V ) C k A k B ( V ) B k A ( ) s ( x

 







By the use of (12), we find

2 1(s) V V  .

While g(V2,V2)1, we can write 1

) V , V (

g 1 1  which implies that involute

x

is a time-like curve.

Then we can compute the vector form )

s ( x ) s ( x ) s (

x     and V4 of

x

as in the following:



 

 

 

 

 

4 1 2

3 1 1 2 2

V ) C k A k (

DV k DV ) k

s ( x ) s ( x ) s ( x and

2 1 1 3 2 1 4

4

V ) C k A k ( DV k DV W k

1

) s ( x ) s ( x ) s ( x

) s ( x ) s ( x ) s ( ) x s ( V

 

 

 

 

 

where

W D2(k21k22)(k2Ak1C)2 . Similarly, we can compute





 

 

 

4 2 2 2 1

3 1 2 1

1 1 2 2 2

4

V ) k k ( D

V ) C k A k ( k

V ) C k A k ( k ) W

s ( x ) s ( x V

and

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AKÜ FEMÜBİD 16 (2016) 031301 572





 

 

 

 

 

4 2 2 2 1

3 1 2 1

1 1 2 2

2 2 2 1 4 4 3

V ) k k ( D

V ) C k A k ( k

V ) C k A k ( k k k W

1

) s ( x ) s ( x V

) s ( x ) s ( x V V

Finally, if we calculate V3V4x(s) and substitute in (4), we get

2 2 2 1

3 2 1 1

2 k k

V k V ) k s (

V 

  .

Consequently, an easy calculation gives g(V2(s),x(s)) k12k22 ,

2 2 2 1

3 k k

)) W s ( x ), s ( V (

g    , (13)



 

 



 

  2

3 1 2 1

3 1 ) 2

ıv (

4 D(k C k A) k k D

) D C k )(

C k A k ( W )) 1 s ( x ), s ( V (

g .

Hence, from equations (13) and (5), we get (9), which completes the proof.

For the case x is a W-curve, one can get the following results.

Corollary 1 Let x(s) be a space-like curve with time-like principal normal in IE given with the 14 Frenet curvatures k , 1 k , 2 k3. If x is a W-curve, then the Frenet frame vectors V1, V2, V3, V4 and Frenet curvatures k1, k2, k3 of the involute

x

of the curve x are given by

2 1(s) V V  ,

2 2 2 1

3 2 1 1

2 k k

V k V ) k s (

V 

  ,

4 3(s) V

V , (14)

2 2 2 1

3 1 1 2

4 k k

V k V ) k s (

V 

 ,

and

1 2 2 2 1 1 (c s)k

k ) k

s (

k 

  ,

) k k ( k ) s c (

k ) k

s (

k 2

2 2 1 1

3 2

2    , (15)

2 2 2 1 3

3 (c s) k k

) k s (

k    ,

respectively (Turgut et al. 2010).

Corollary 2. Let x(s) be an involute of a space-like curve x with time-like principal normal in IE given 14 with the Frenet curvatures k1,k2,k3. If x is a W- curve, then

x

becomes a ccr-curve.

2.2. Involute of order 2

An involute of order 2 of a space-like curve x in IE has the parametrization 14

) s ( V ) s ( ) s ( V ) s ( ) s ( x ) s (

x  1 1 2 2 (16) where 1, 2 are differential functions satisfying

) s ( k ) s ( 1 ) s

( 2 1

1  



) s ( k ) s ( )

s

( 1 1

2 

 . (17)

From the differentiable equation system (17), we get the following result.

Corollary 3. Let xx(s) be a space-like Salkowski curve with time-like principal normal in IE . Then 41 the involute

x

of order 2 of the curve x has the parametrization (16) given with the coefficient functions

) s k sinh(

c ) s k cosh(

c ) s

( 1 1 2 1

1  

1 1 2

1 1

2 k

) 1 s k cos h(

c ) s k s i nh(

c ) s

(   

where c and 1 c are real constants. 2

Theorem 2. Let xx(s) be a space-like curve with time-like principal normal in IE given with Frenet 14 curvatures k , 1 k , 2 k3. Then the involute

x

of order 2 of the curve x is a space-like curve with the Frenet frame vectors V1, V2, V3, V4 and Frenet curvatures k1, k2, k3 which are given by

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AKÜ FEMÜBİD 16 (2016) 031301 573

V1(s)V3,

2 2 2 3

4 3 2 2

2 k k

V k V ) k s (

V 

  , (18)



 

 

4 3 2 2

2 3 2 3 1 2 2 2 3 2 2 2 3

3 k (kN k L)V

V ) L k N k ( k V ) k k ( K k k W ) 1 s (

V

4

(k2N k3L)V1 k3KV2 k2KV4

W ) 1 s (

V     ,

and

 

2 2 2 3 1

k ) k

s (

k ,

) k k ( ) W s (

k 2

2 2 3

2 2  , (19)





 

 



 

2 3 1

2 3

1 3

2

2 2 2 2 3 3

K k k

) N k L k ( K

) L k K )(

L k N k ( W

k ) k

s (

k ,

where

2 2k

 ,

k1k2

K ,



k2 2k2

L ,





k3 2k3

N ,

and

. ) k k ( k k ) k k k k (

) k k ( K ) L k N k ( W

2 2 2 3 2 2 2 1 2 3 2 3 2

2 2 2 3 2 2 3 2

 

 

Proof. Let xx(s) be the involute of order 2 of a space-like curve with time-like principal normal in

4

IE . Then by the use of (16) with (7), we get 1

V3

) s (

x  , (20) where (s)2(s)k2(s) is a differentiable function.

By the use of (20), we find

3 1(s) V

V .

While g(V3,V3)1, we can write g(V1,V1)1 which implies that involute

x

of order 2 is a space- like curve.

Further, the differentiation of (20) implies that x(s)k2V2V3k4V4, (21)

. V ) k 2 k ( V ) k k

(

V ) k 2 k ( V k k ) s ( x

4 3 3 3 2 3 2

2

2 2 2 1 2 1





 





 

Consequently, substituting

k1k2

K ,





k2 2k2

L ,

 

k22 k23

M ,





 k3 2k3

N ,

in the last vector, we obtain

. NV MV LV KV ) s (

x   1234 (22) Furthermore, differentiating

x 

with respect to s, we get

4 3 3

3 2

2 2 1 1

1 )

ıv (

V ) M k N ( V ) N k L k M (

V ) M k K k L ( V ) L k K ( ) s ( x









 (23)

Hence substituting (20)-(23) into (4) and (5), after making some calculations as in the previous theorem, we obtain the result.

For the case x is a W-curve, one can get the following result.

Corollary 4. Let

x

be an involute of order 2 of a space-like curve with time-like principal normal in

4

IE given with the Frenet curvatures 1 k1,k2,k3. If x is a W-curve, then the Frenet frame vectors V1, V2, V3, V4 and Frenet curvatures k1, k2, k3 of the involute

x

of order 2 of the curve x are given by

3 1(s) V

V ,

2 2 2 3

4 3 2 2

2 k k

V k V ) k s ( V

-

  ,

1 3(s) V

V , (24)

2 2 2 3

4 2 2 3

4 k k

V k V ) k s (

V 

  ,

and

 

2 2 2 3 1

k ) k

s (

k ,

2 2 2 3

2 1

2 k k

k ) k

s (

k   , (25)

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AKÜ FEMÜBİD 16 (2016) 031301 574

2 2 2 3

3 1

3 k k

k ) k

s (

k   ,

where (s)2(s)k2(s).

Corollary 5. Let

x

be an involute of order 2 of a space-like curve x with time-like principal normal in

4

IE given with the Frenet curvatures 1 k1,k2,k3. If x is a W-curve, then

x

becomes a ccr-curve.

2.3. Involute of order 3

An involute of order 3 of a space-like curve x in IE has the parametrization 14

) s ( V ) s ( ) s ( V ) s ( ) s ( V ) s ( ) s ( x ) s (

x  1 1 2 2 3 3 (26)

where 1, 2, 3 are differentiable functions satisfying

) s ( k ) s ( 1 ) s

( 2 1

1  

 ,

) s ( k ) s ( ) s ( k ) s ( )

s

( 1 1 3 2

2  

 , (27)

) s ( k ) s ( )

s

( 2 2

3 

 .

By solving the differential equation system (27), we get the following result.

Corollary 6. Let xx(s) be a space-like W-curve with time-like principal normal in IE . Then the 14 involute

x

of order 3 of the curve x has the parametrization (26) given with the coefficient functions

2 1 2 2 2

3 1

1 c

k s k k

)) ks sin(

c ) ks cos(

c ( ) k s

(   

 ,

2 1 3

2

2 k

) k ks sin(

c ) ks cos(

c ) s

(   

 ,

2 1 1 2

2 1 2

3 2

3 k

k c k

s k k k

)) ks sin(

c ) ks cos(

c ( ) k s

(

,

where k k1k2 , c , 1 c and 2 c3 are real constants.

Theorem 3. Let xx(s) be a space-like curve with time-like principal normal in IE given with Frenet 14 curvatures k , 1 k and 2 k3. Then the involute

x

of order 3 of the curve x is a space-like curve with the

Frenet frame vectors V1, V2, V3, V4 and Frenet curvatures k1, k2, k3 which are given by

4 1(s) V V  ,

3 2(s) V

V , (28)

2 3(s) V

V ,

1 4(s) V V  and

 3

1

) k s (

k ,



2

2

) k s (

k , (29)



1

3

) k s (

k , where (s)3(s)k3(s).

Proof. Let xx(s) be the involute of order 3 of a space-like curve with time-like principal normal in

4

IE . Then by the use of (26) with (7), we get 1

V4

) s (

x  (30) where (s)3(s)k3(s) is a differentiable function.

By the use of (30), we find

4 1(s) V V  .

While g(V4,V4)1, we can write g(V1,V1)1 which implies that involute

x

of order 3 is a space- like curve.

Further, the differentiation of (29) implies that

4 3

3 V V

k ) s (

x    ,

. V ) k (

V ) k 2 k ( V k k ) s ( x

4 2 3

3 3 3 2 3 2

 





 

(31) Consequently, substituting

 k2k3 E

) k 2 k (

F 3 3

 

k23 G

in the last vector, we obtain . GV FV EV ) s (

x   234 (32) Furthermore, differentiating

x 

with respect to s, we get

4 3 3

3 2

2 2 1

1 ) ıv (

V ) F k G ( V ) G k E k F (

V ) F k E ( EV k ) s ( x







 (33)

(7)

AKÜ FEMÜBİD 16 (2016) 031301 575

Hence substituting (30)-(33) into (4) and (5), after some calculations as in the previous theorem, we obtain the result.

Corollary 7. The ivolute

x

of order 3 of a space-like ccr-curve x with time-like principal normal in IE is 14 also a ccr-curve in IE . 14

3. Conclusion

In recent years, many authors have studied with the involute-evolute curve couples in many paper. Turgut et al. (2010) gave the characterization of the involute of order 1 (involute) of a W-curve in IE 14

In this paper, we study involute curves of order k of a space-like curve x with time-like principal normal in Minkowski 4-space IE . First, 41 we investigate an involute curve of order 1 of a given curve. Furthermore, we give the characterizations of the involutes of order 2 and 3.

We obtain the Frenet Frame and Frenet curvatures of the involutes of order k of the curve with respect to the Frenet Frame and Frenet curvatures of the given curve.

Nowadays, as known W-curve (or helix) is very important topic in curve theory, we characterize the involutes of order k of a W-curve in IE . 14

References

Blazenka, D. And Zeljka M.S.,1999. Involutes and evolutes in n-dimensional simply isotropic space. Journal of Information and Organizational Sciences, 2(3), 71-79.

Gluck, H., 1966. Higher curvatures of curves in Euclidean space. American Mathematical Monthly, 73, 699-704.

Kılıc, B., Arslan, K. and Öztürk, G., 2008. Tangentially cubic curves in Euclidean spaces. Differential Geometry- Dynamical Systems, 10, 186-196.

Klein, F. and Lie, S., 1871. Uber diejenigen ebenenen kurven welche durch eingeschlossenes system von einfach unendlich vielen vartauschbaren linearen transformationen in sich übergehen. Mathematische Annalen, 4, 50-84.

Monterde, J., 2007. Curves with constant curvature ratios. Bulletin of Mexican Mathematic Society, Ser. 3A, 13(1), 177-186.

O'Neill, B., 1983. Semi-Riemannian Geometry with Applications to Relativity, Academic Press, New York.

Öztürk, G., Arslan, K. and Hacisalihoglu, H. H., 2008. A characterization of ccr-curves in IRm. Proccedings of Estonian Academy Science, 57(4), 217-224.

Öztürk, G., Arslan, K. and Bulca, B., 2016. A characterization of involutes and evolutes of a given curve in IEn. arxiv.org.

Salkowski E., 1909. Zur transformation von raumkurven.

Mathematische Annalen, 66(4), 517-557.

Turgut, M., Ali, A.T., and Lopez-Bonilla, J. L., 2010. Time- like involutes of a space-like helix in Minkowski space- time. Apeiron, 17(1), 28-41.

Walfare, J., 1995. Curves and surfaces in Minkowski space. PhD thesis, K.U. Leuven, Faculty of Science, Leuven.

Yılmaz, S. and Turgut, M., 2008. On the differential geometry of the curves in Minkowski space-time I.

International Journal of Contemporary Mathematical Science, 3(27), 1343-1349.

Referanslar

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