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On The Volume Of The Trajectory Surface Under The Galilean Motions In The Galilean Space

Mücahit Akb¬y¬k

y

, Salim Yüce

z

Received 15 Feb 2017

Abstract

In this work, the volumes of the trajectory surfaces which are traced by …xed points during 3-parameter Galilean space motions are studied. Also, the well- known classical Holditch theorem [3] is generalized for the volumes of the trajec- tory surfaces in the Galilean space.

1 Introduction

In 1958, H. Holditch, [3], came up with the following outstanding classical theorem: If the endpointsA andB of a …xed line segmentAB with lengtha+bare rotated once along an ovalkin the Euclidean planeE2;then a given …xed pointX(AX=a; XB=b) ofABdescribes a closed not necessarily convex curvekX:The areaF of the Holditch- Ring bounded by the curves kandkX isF = ab:

Later, this theorem was studied by di¤erent methods [1,2,6–10] and in di¤erent spaces [13–15]. One of the generalizations of this theorem is on the volumes of the surfaces of 3-dimensional Euclidean space which are traced by …xed points during 3- parameter motions are given by H. R. Müller [6–8] and W. Blashke [1].

In this paper, the volumes of the trajectory surfaces of …xed points under 3- parameter Galilean space motions are calculated. Also, by the help of a special distance that we have de…ned, we generalize the well-known classical Holditch theorem for the volumes of the trajectory surfaces of …xed points under 3-parameter Galilean space motions.

2 Preliminaries

Galilean geometry G3 can be described as the study of properties of 3-dimensional space with coordinates that are invariant under Galilean transformations

8<

:

x0 =x+a;

y0= (vcos )x+ (cos')y+ (sin')z+b;

z0 = (vsin )x+ ( sin')y+ (cos')z+d:

Mathematics Sub ject Classi…cations: 53A17, 53A35.

yDepartment of Mathematics, Yildiz Technical University, Esenler, Istanbul 34220, Turkey

zDepartment of Mathematics, Yildiz Technical University, Esenler, Istanbul 34220, Turkey

297

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The Galilean transformations consist of translation, rotation and shear motions, and are described by I. M. Yaglom in [11]. In the literature, the basic information about Galilean Geometry is …rstly given by I. M. Yaglom. Then, the di¤erential geometry of curves and surfaces in the Galilean space G3 is worked in detail by O. Röshcel in [9].

Also, the quadrics in the Galilean space are examined by Kamenarovic in [4]. Now, let’s give some basic information about the Galilean space G3. Leta = (x; y; z) and b= (x1; y1; z1)be two vectors in the Galilean space. The scalar product ofa andbis de…ned by

<a;b>G=xx1:

The vectors in the Galilean space are divided into two classes as non-isotropic vectors and isotropic vectors which are of the form a = (x; y; z); x 6= 0 and p = (0; y; z);

respectively:Moreover, the special scalar product of isotropic vectorsp= (0; y; z)and q= (0; y1; z1)is de…ned by

<p;q> =yy1+zz1:

Ifa= (x; y; z)andb= (x1; y1; z1)are vectors in Galilean space, the vector product of a andbis de…ned as the following in [5]:

a b=

0 e2 e3

x y z

x1 y1 z1

:

Letg1be a nonisotropic vector,g2and g3 be isotropic vectors in the Galilean space.

If the vectors g1;g2; and g3 satisfy that <g1;g1 >G=<g2;g2 > =<g3;g3 > = 1 and <g1;g2>G=<g1;g3>G=<g2;g3> = 0;then the vector systemfg1;g2;g3g is called an orthonormal frame of Galilean space. More information about the Galilean geometry can be found in [9, 11].

3 One Parameter Galilean Space Motion

LetR andR0 be two3 dimensional Galilean spaces. Let fO;g1;g2;g3g and fO0;g10;g02;g03g

are orthonormal frames of spaces R and R0, respectively. Assume that the frame fO;g1;g2;g3gmoves with respect to frame fO0;g01;g02;g30g: Then, it is accepted that the space R moves according to the space R0. The spaces R and R0 are called moving space and …xed space, respectively. Moreover, the frames fO;g1;g2;g3g and fO0;g01;g02;g03g are calledmoving frame and …xed frame, respectively. This motion is called one parameter Galilean space motion and is denoted byB=R=R0: Here, the spaces Rand R0 are orientated in the same direction. During the motionB =R=R0; it is clear that

x0 = u+x;

where x0 and x correspond to the position vectors of any pointX 2 R according to the rectangular coordinate systems ofR0,R, respectively, and

u=OO0=u1g1+u2g2+u3g3:

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Here, the vectoruis calledtranslation vector. In the motionB=R=R0, the vectorsx0; x and uare continuously di¤erentiable functions of a real parameter t:If the frames fg1;g2;g3gand fg01;g02;g30g are written as

G= 2 4 g1

g2

g3 3

5 andG0= 2 4 g01

g02 g03

3 5

in the matrix form, respectively, then

G=AG0 andG0=A 1G (1)

are hold. Here,A is an invertible matrix. In this case, by di¤erentiating both sides of the equation (1) and considering that G0 is …xed frame, we get

dG= G; (2)

where =dAA 1. If we calculate from above equation (2) and by the necessary operations with the basis vectorsgi;1 i 3;we get

= 2

4 0 !3 !2

0 0 !1

0 !1 0 3

5; (3)

where !i;1 i 3 are the linear di¤erential forms with respect to t, that is, !i = fi(t)dt:

The vector

!=!1g1+!2g2+!3g3

which is de…ned by nonzero components of is called the instantaneousPfa¢ an vector of the motion B =R=R0.

Especially, if!1= 0; then, the motion ofB consists of only translation and shear motions. The motion doesn’t contain the rotation. We will, therefore, accept!1 6= 0 in this work.

If it is used the equality (3) given for , we get

dg1= !3g2+!2g3; dg2= !1g3; dg3=!1g2: (4) Moreover, if we calculate the exterior derivation of equation (4), by considering that basis vectors gi; i= 1;2;3, are linearly independent, we obtain

d!1= 0; d!2= !3^!1; d!3=!2^!1;

where "^" is the wedge product of the di¤erential forms. Hence, the conditions of integration for components of the pfa¢ an vector of the motionR=R0 are found as

d!1= 0; d!2= !3^!1; d!3=!2^!1: (5) On the other hand, by di¤erentiating of translation vector

O0O= u= u1g1 u2 g2 u3g3

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and by the aid of using the equation (4), we have

0 = du= 1g1+ 2g2+ 3g3;

where

0 = du

and

1= du1; 2= du2+u1!3 u3!1; 3= du3 u1!2+u2!1:

The equations 8

>>

<

>>

:

dg1=!2g3 !3g2; dg2= !1g3; dg3=!1g2;

0= du= 1g1+ 2g2+ 3g3;

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are called derivative equations of motionR=R0. Furthermore,

0=d 0=d 1g1+ (d 2 1^!3+ 3^!1)g2+ (d 3+ 1^!2 2^!1)g3

and because of the fact thatfg1;g2; g3g are linearly independent, we …nd

d 1= 0; d 2= 1^!3 3^!1; d 3= 1^!2+ 2^!1: (7) So, the conditions of integration obtained for the translation vector of the motionR=R0 are equations (7).

Now, let’s examine the velocity vectors of the pointX under the motionR=R0:Let X be any point inR. So, we can write

x= X3 i=1

xigi

with respect to the moving frame fO;g1;g2;g3g. Since we have x0 = u+x

for position vector x0 of the pointX with respect to …xed framefO0;g01; g02;g03g, the di¤erential of position vectorx0 can be expressed as

dx0= du+dx:

By (6), it is calculated as

dx0 = 1g1+ ( 2 x1!3+x3!1)g2+ ( 3+x1!2 x2!1)g3+dx1g1+dx2g2+dx3g3: During the motion R=R0; the velocity vector of any point X 2R with respect to

…xed spaceR0 and moving space Ris calledabsolute velocity XAandrelative velocity XR, respectively. XA and XR are expressed by

XA=dx0

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and

XR=dx1g1+dx2g2+dx3g3:

The di¤erence between the absolute and the relative velocities is calledsliding velocity XF of the pointX and it is stated as

XF = 1g1+ ( 2 x1!3+x3!1)g2+ ( 3+x1!2 x2!1)g3:

In this way, the following theorem can be given:

THEOREM 1. LetX be a point inR and XA;XF; andXR be the absolute, the sliding and the relative velocity of the point X under the motion R=R0, respectively.

Then, the relation between the velocities is given by XA=XF +XR:

If any pointX in Ris …xed, then the relative velocity XR=0and XA=XF

under the motion R=R0: Furthermore, by considering derivative equations (6), the following equation holds:

dx= ( x1!3+x3!1)g2+ (x1!2 x2w1)g3

or

dx=x !

for any …xed pointX inR:So, for any …xed pointX during the motionR=R0, one can state

dx0 = 0+x !:

Also, one can rewrite

dx0= 1g1+ 2g2+ 3g3; where

1= 1; 2= 2+x3!1 !3x1; 3= 3+x1!2 !1x2: (8)

4 The Volume of the Trajectory Surface in G

3

I: Until now, we have considered that the translation vector u and basis vectors gi

for 1 i 3 of the motionB are functions of a real parameter t:From now on, we assume that the translation vector uand basis vectorsgi for1 i 3 of the motion B are functions of real parameterst1; t2andt3:And this motion is called3-parameter Galilean space motion and we shall denote this 3-parameter motion byB3:During the motionB3; !iand i are the linear di¤erential forms with respect tot1; t2andt3:So, the equations (5), (7) and (8) are not changed for the motion B3.

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Under the motion B3; any …xed point X in the moving space R determines a volumetric trajectory surface inR0:The volume element of the trajectory surface ofX under the motionB3, is de…ned by

dJX = 1^ 2^ 3: (9)

Thus, the integration of the volume element over a region Gdetermined by the …xed pointXof the parameter space during the motionB3yields the volume of the trajectory surface, i.e.,

JX = Z

G

dJX:

By putting equation (8) into (9) and after making necessary arrangement, the volume of the trajectory surface of …xed pointX inR during the motionB3 is calculated as

JX=JO+ax21+ X3 i=2

bixix1+ X3 i=1

cixi; (10)

where JO= Z

G

1^ 2^ 3; a= Z

G

1^!2^!3; b2= Z

G

( 1^!1^!3); b3= Z

G

( 1^!1^!2);

c1= Z

G

1^ 2^!2 1^!3^ 3; c2= Z

G

( 1^ 2^!1); c3= Z

G

1^!1^ 3:

JOis the volume of trajectory surface of origin pointO:So, the volumeJXof trajectory surface is a quadratic polynomial ofxi:

THEOREM 2. All …xed points inR whose trajectory surfaces have equal volume under the motionB3lie on the same quadric.

II: LetX = (xi)and Y = (yi)be two …xed points in R and Z = (zi)be another point on the line segment XY; that is, zi = xi + yi; + = 1 in barycentric coordinates. Then, the volume of the region in R0 determined by the …xed point Z under the motionB3, by using equation (10), is obtained as

JZ = 2JX+ 2 JXY + 2JY; where

JXY =JO+ax1y1+1 2

X3 i=2

bi(x1yi+y1xi) +1 2

X3 i=1

ci(xi+yi): (11) Also,JXY is called themixture trajectory surface volume. It is clearly seen thatJXX = JX andJXY =JY X: Since

JX 2JXY +JY =a(x1 y1)2+ X3 i=2

bi(x1 y1) (xi yi); (12)

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we can restate the volume trajectory surface of the …xed pointZ asJZ= JX+ JY a(x1 y1)2+

P3 i=2

bi(x1 y1) (xi yi) :So, we may give following theorem:

THEOREM 3. LetX and Y be two di¤erent …xed points inR;andZ be another point on the segmentXY:During the motionB3, the relation between the volumes of the trajectory surfaces of …xed pointsX; Y andZ is as follows:

JZ = JX+ JY a(x1 y1)2+ X3 i=2

bi(x1 y1) (xi yi)

!

: (13)

We will de…ne the distanceD(X; Y)between the …xed pointsX; Y 2R;by

D2(X; Y) =" a(x1 y1)2+ X3 i=2

bi(x1 y1) (xi yi)

!

; "= 1: (14)

Therefore, by the help of the distance (14), the equation (13) can be restated as follows:

JZ = JX+ JY " D2(X; Y): (15) SinceX; Y andZ are collinear, we can writeD(X; Z) +D(Z; Y) =D(X; Y):Hence, if we represent =D(Z;YD(X;Y)); = D(X;Z)D(X;Y);where D(X; Y)6= 0; i.e.,x16=y1, then from equation (15), we have

JZ = 1

D(X; Y)[D(Z; Y)JX+D(X; Z)JY] "D(Z; Y)D(X; Z): (16) Now, we consider that the …xed points X andY trace the same trajectory surface. In this case, we getJX =JY:Then, from the above equation (16), we get

JX JZ="D(Z; Y)D(X; Z):

So, we may give the following theorem:

THEOREM 4. Let X = (x1; x2; x3) and Y = (y1; y2; y3); where x1 6= y1; be two di¤ erent …xed points in R and Z be another point on the segment XY: Let the

…xed points X and Y trace the same trajectory surface and the …xed pointZ trace the di¤erent trajectory surface during the motion B3. Then, the di¤erence between the volumes of these two trajectory surfaces depends on the distances of Z from the endpoints which are de…ned in (14) with respect to the motionB3:

In case of x1 = y1; then the equation (13) is arranged as JZ = JX+ JY: If the …xed pointsX andY trace the same trajectory surface during the motion B3, we obtain

JX JZ= 0:

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COROLLARY. Let X = (x1; x2; x3) and Y = (y1; y2; y3); where x1 = y1 be two di¤ erent …xed points in R and Z be another point on the segment XY:If the …xed pointsXandY trace the same trajectory surface, the …xed pointZtrace the trajectory surface with same volume during the motionB3.

III:

THEOREM 5. Let us consider a triangle in R whose vertices are points X1 = (x1; x2; x3); X2 = (y1; y2; y3) and X3 = (z1; z2; z3); where x1 6= y1, x1 6= z1 and y16=z1. If the vertices of this triangle trace the same trajectory surface inR0;then a di¤erent point Qon the plane which is determined byX1; X2 and X3 traces another surface. The di¤erence between the volumes of these two trajectory surfaces depends on the distances D(Xk; Q); D(Xk; Qk); D(Qk; Xj) and D(Xi; Qk) which are measured with respect to the motionB3. Here, the pointQiis a intersection point of the segments XiQandXjXk; i; j; k= 1;2;3; 2;3;1; 3;1;2:

PROOF. LetX1= (xi); X2= (yi)and X3 = (zi); x1 6=y1,x1 6=z1 and y1 6=z1

be three non- collinear …xed points in R;andQ= (qi) be another …xed point on the plane which is determined byX1= (xi); X2= (yi)andX3= (zi):Then, for the point Q, we can write

qi = 1x1+ 2yi+ 3zi; 1+ 2+ 3= 1: (17) Under the motion B3, by the help of equations (10), (11) and (17), the volume of the region determined by the point Qcan be calculated as

JQ= 21JX1+ 22JX2+ 23JX3+ 2 1 2JX1X2+ 2 1 3JX1X3+ 2 2 3JX2X3: Also, by considering the equations (12) and (14), we get

JQ = 1JX1+ 2JX2+ 3JX3

"12 1 2D2(X1; X2) +"13 1 3D2(X1; X3) +"23 2 3D2(X2; X3) : Let the pointsQ1= (q1i)are intersection point of the segmentsX1QandX2X3. Then, we can write

q1i = 1yi+ 2zi; qi= 3xi+ 4ai;

where 1+ 2= 3+ 4= 1:Hence, we have 1= 3; 2= 1 4; 2= 2 4i.e.,

1= D(Q; Q1)

D(X1; Q1); 2= D(Q1; X3) D(X2; X3)

D(X1; Q)

D(X1; Q1); 3= D(X2; Q1) D(X2; X3)

D(X1; Q) D(X1; Q1): Similarly, for Q2andQ3;we calculate

i= D(Q; Qi)

D(Xi; Qi) = D(Xj; Q) D(Xj; Qj)

D(Xk; Qj)

D(Xk; Xi) = D(Xk; Q) D(Xk; Qk)

D(Qk; Xj) D(Xi; Xj)

fori; j; k= 1;2;3; 2;3;1; 3;1;2. So, the volume of the trajectory surface determined by the pointQcan be rearranged as

JQ= X3 i=1

D(Q; Qi) D(X; Qi)JXi

X3 i=1

"ij D(Xk; Q) D(Xk; Qk)

2

D(Qk; Xj)D(Xi; Qk): (18)

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During the motionB3;since the pointsX1; X2andX3trace the same trajectory surface in R0; we can write JX1 = JX2 =JX3: So, from the equation 1+ 2+ 3 = 1 and equation (18), we can get

JXi JQ = X3 i=1

"ij

D(Xk; Q) D(Xk; Qk)

2

D(Qk; Xj)D(Xi; Qk);

fori; j; k (cyclic):

Finally, the di¤erence between the volumesJX1 andJQ only depends on distances on triangleX1X42X3 de…ned in (14) according to the motionB3:

References

[1] W. Blaschke, Über Integrale in der Kinematik. Arch. Math., 1(1948). 18–22.

[2] M. Düldül and N. Kuruo¼glu, On the volume of the trajectory surfaces under the homothetic motions, Acta Math. Univ. Comenian., 76(2007), 241–246.

[3] H. Holditch, Geometrical Theorem, Q. J. Pure Appl. Math., 2(1858), 38.

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Wiss. Ges., 30(1979), 54–61.

[7] H. R. Müller, Über den R•auminhalt kinematisch erzeugter, geschlossener Fl•achen, Arch. Math. 38(1982), 43–49.

[8] H. R. Müller, Ein Holditch Satz für Fl•achenstücke imR3;Abh. Braunschw. Wiss.

Ges, 39(1987), 37–42.

[9] O. Röschel, Die Geometrie des Galileischen Raumes, Berichte [Reports], 256.

Forschungszentrum Graz, Mathematisch-Statistische Sektion, Graz, 1985.

[10] A. Tutar and N. Kuruo¼glu, The Steiner formula and the Holditch theorem for the homothetic motions on the planar kinematics, Mech. Mach. Theory, 34(1999), 1–6.

[11] I. M. Yaglom, A simple non-Euclidean Geometry and its Physical Basis, New York, USA: Springer-Verlag, 1979.

[12] H. Y¬ld¬r¬m, S. Yüce and N. Kuruo¼glu, Holditch theorem for the closed space curves in Lorentzian 3-space, Acta Math. Sci. Ser. B Engl. Ed., 31(2011), 172–180.

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[13] H. Y¬ld¬r¬m, Spatial Motions and the Holditch-type theorems in 3-Dimensional Lorentzian space, PhD, Istanbul University, Grad. Sch. of Nat. and Appl. Sci., Istanbul, 2010.

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