ORIGINAL RESEARCH article

Front. Phys., 24 June 2021

Sec. Statistical and Computational Physics

Volume 9 - 2021 | https://doi.org/10.3389/fphy.2021.660241

Normal Curves in 4-Dimensional Galilean Space G4

  • 1. Department of Mathematics, College of Science, University of Bisha, Bisha, Saudi Arabia

  • 2. Department of Mathematics, Faculty of Science, Damanhour University, Damanhour, Egypt

  • 3. Department of Mathematics, Faculty of Science, Tanta University, Tanta, Egypt

Abstract

In this article, first, we give the definition of normal curves in 4-dimensional Galilean space G4. Second, we state the necessary condition for a curve of curvatures τ(s) and σ(s) to be a normal curve in 4-dimensional Galilean space G4. Finally, we give some characterizations of normal curves with constant curvatures in G4.

1. Introduction

Galilean geometry is one of the Cayley-Klein geometries whose motions are the Galilean transformations of classical kinematics [1]. The Galilean transformation group has an important place in classical and modern physics. It is well known that the idea of world lines originates in physics and was pioneered by Einstein. The world line of a particle is just the curve in space-time which indicates its trajectory [2].

In Euclidean 3-space E3, there are three types of curves, namely, osculating, rectifying, and normal curves [3]. The osculating curve in E3 is defined as a curve whose position vector always lies in its osculating plane, which is spanned by the tangent vector T and the normal vector N [3]. The rectifying curve in E3 is defined as a curve whose position vector always lies in its rectifying plane, which is spanned by the tangent vector T and the binormal vector B. Many researchers have investigated rectifying curves in Euclidean, Lorentz-Minkowski, and Galilean space, as can be seen in [46]. Similarly, a normal curve in E3 is defined as a curve whose position vector always lies in its normal plane, which is spanned by the normal vector N and the binormal vector B of the curve. Normal curves in n-dimensional Euclidean space was studied by Ozcan Bekats [7], framed normal curves in Euclidean space was studied by B.D. Yazici, S. O.Karakus, and M. Tosun [8], and normal curves on a smooth immersed surface was investigated by A.A. Shaikh, M.S. Lone, and P.R. Ghosh [9].

There are also many studies related to normal curves in non-Euclidean spaces, for example, normal curves and their characterizations in Lorentzian n-space was studied by Ozgür Boyacıoğlu Kalkan [10] and to the classification of normal and osculating curves in 3-dimensional Sasakian space was studied by M. Kulahck, M. Bahatas, and A. Bilici [11].

In recent years, researchers have begun to introduce curves and surfaces in Galilean and pesedo-Galilean spaces [1224]. Normal and rectifying curves in Galilean G3 were obtained by Handan Oztekin [25]. Also, many studies about Galilean Geometry were found in Reference [1]. Frenet-Serret frame in the Galilean 4-space was constructed by S.Yilmaz [26].

In the present study, we considered a curve in Galilean 4-space G4 whose position vector satisfies the equation α(s) = λ(s)N(s) + μ1(s)B1(s) + μ2(s)B2(s) for differentiable functions λ(s), μ1(s), and μ2(s). N(s), B1(s), and B2(s) are normal, first binormal, and second binormal vectors of the curve in Galilean space G4. In the first part of the study, the necessary condition for a curve to be a normal curve was obtained; then, we considered a special case when the curvatures are constant and got the position vector of the normal curve in G4. At the end of the study, it can be seen that the normal curve in G4 lies on a sphere if constant, where τ and σ are the second and the third curvatures of the normal curve α(s).

2. Preliminaries

In this section, we will give some definitions considered in this study. Let and be two vectors in G4. The Galilean scalar product in G4 is defined by

The norm of the vector is given by

The cross product of any three vectors and in G4 is defined by the relation

where the unit vectors e1 = (1, 0, 0, 0), e2 = (0, 1, 0, 0), e3 = (0, 0, 1, 0), and e4 = (0, 0, 0, 1) [1].

A curve α : IRG4 of C in the Galilean space G4 is defined by α(t) = (x(t), y(t), z(t), w(t)).

If the curve is parameterized by Galilean arc-length s, it is defined by α(s) = (s, y(s), z(s), w(s)).

The Frenet frame for the parameterized curve α(s) = (s, y(s), z(s), w(s)) in G4 is denoted by the following vectors

T(s) = α′(s) = (1, y′(s), z′(s), w′(s)),

B2(s) = ςT(s) × N(s) × B1(s),

Here, the coefficient ς is taken ±1 to make the determinant of the matrix [T, N, B1, B2] = 1.

where T(s), N(s), B1(s) and B2(s) are the tangent, normal, the first binormal, and the second binormal vectors of α(s). k(s) and τ(s) are the first and second curvatures, which are given by the following equations

The third curvature of the parameterized curve α(s) is denoted by . If the curvatures of α(s) are constants, the curve α(s) is called a W-curve. The set {T(s), N(s), B1(s), B2(s), k(s), τ(s), σ(s)} is called Frenet apparatus of the curve α(s). The vectors T(s), N(s), B1(s), and B2(s) are mutually orthogonal.

and

The derivatives of the Frenet equations are defined by [26].

3. Normal Curves in G4

In the following section, we will define the normal curves in Galilean 4-dimensional space and prove that there are no congruent curves to the normal curve α(s); finally, we will provide some characterizations of the normal curves in G4.

Definition 1. Let α : IRG4be a parameterized curve inG4. A curve α(s) is called a normal curve if the orthogonal components ofT(s) contains a fixed point for allsI.

In the following theorem, we indicate the position vector of the normal curve in Galilean 4-space G4.

Theorem 1. The position vector of the normal curve inG4with curvaturesk(s), τ(s), and σ(s) are defined if τ(s) and σ(s) satisfy the following equations:

Proof: The position vector of a normal curve in G4 is defined by

where λ(s), μ1(s), and μ2(s) are smooth functions of s.

By differentiating (Equation 3.1) with respect to s, we obtain

substituting Frenet (Equations 2.1) into Equation 3.2, we have

Hence, we have the following system of differential equations:

and

Since the curvature functions τ(s) and σ(s) must be differentiable functions, so we consider a set of differentiable functions, defined by

where Pn(s) denotes a polynomial function of degree n in s. Here, the curvature functions can be any function of , a linear combination or a product of these functions. It is said that annihilates the function ϒ(s) if . Here, all the member functions of have this property. Consequently, we have two linear differential operators, Φ(Ds) and Ψ(Ds), such that Φ(Ds){τ(s)} = 0 and Ψ(Ds){σ(s)} = 0, where , some of these annihilator operators are listed in Table 1. By applying the operator Θ(Ds) = Φ(Ds)Ψ(Ds) on Equation (3.4), we have

The operator Θ(Ds) annihilates the terms that contain λ(s) and μ2(s), i.e., the right hand side (RHS) of Equation (3.7) contains the derivatives of λ(s) and μ2(s) from order 1 to an order of less than the order of the derivative of μ1(s) by 1 at most. Let the maximum derivative in the left hand side (LHS) of Equation (3.7) be r + 1; then, its RHS can be written as a linear combination of the derivatives of τ(k)(s(rk)(s) and and k ∈ {0, 1, …, r − 1}, consequently, we have

where ar, k, br, k ∈ ℝ. Next by differentiating Equations (3.3) and (3.5), (r − 1 − k) times and applying Leibniz's rule, one gets

and

Applying Equations (3.9) and (3.10) into (3.8) yields

Equation (3.11) is a linear differential equation of order (r + 1) in μ1(s) with differential variable coefficients. Its general solution depends on the nature of the coefficients of its derivatives. However, the power series method can be applied to obtain its solution, especially, for any value of s ∈ ℝ is an ordinary point in all the coefficients of the derivatives , k = 0, 1, …, r.

Table 1

FunctionThe corresponding annihilator operator
Pn(s)
eωs
cos βs\sin βs
sneωs
sneωscos βs

Annihilator operators of some functions.

Next, we studied the case when τ(s) ∈ Pn(s) and σ(s) ∈ Pm(s). When r = max(m, n), then the annihilator operator is , , and consequently, was applied into Equation (3.7) by applying Leibniz's rule, yielding

By using Equations (3.9) and (3.10), Equation (3.12) becomes

Corollary 1. Let α(s) be a normal curve inG4. If the curvatures τ (s) and σ(s) ∈ P1(s), then the position vector of the normal curve inG4is given by

whereC1, C2, C3, cλ, andcμ2are constants; the Fresnel functions, the generalized hypergeometric function,

and (β)nis the shifted factorial, defined by [27]

Proof: We consider a special case, when τ(s), σ(s) ∈ P1(s), i.e., τ(s) = a1s + b1, σ(s) = a2s + b2, then we have r = 1, and and the annihilate operator is (); by substituting into Equation (3.13), one gets

By extracting the summations, we have

By applying the power series method to solve Equation (3.15), where , differentiating it for up to three times, then substituting into Equation (3.15), and collecting the coefficients, one gets

where,

Finally, for a special case, when a1 = a2 = b1 = b2 = 1, the resultant differential equation is

which has the solution

It is worth noting that the generalized hypergeometric function is convergent, when p < q + 1, which holds in the proposed problem. Hence, we can obtain the functions λ(s) and μ2(s), by integrating Equations (3.3) and (3.5) with respect to s, respectively, then we have

and

Corollary 2. The position vector of the normal curve inG4with constant curvatures τ and σ is given by

Proof: The position vector of a normal curve in G4 is defined by

where λ(s), μ1(s), and μ2(s) are differentiable functions of s.

By differentiating Equation (3.17) with respect to s, we obtain

Substituting Frenet Equations (2.1) into Equation (3.18), we have

Hence, we obtain the following differential equations:

If we take the normal curve α(s) with constant curvatures τ and σ, the Equations (3.19) will take the form

By differentiating the second equation of the Equation (3.20) and substituting the first and the third Equation of (3.20), we obtain the following differential equation

By solving the ordinary differential Equation (3.21), we obtain

where c1, c2, c3 and c4 are constants.

In the following corollary, we give some characterizations for the curve to be a normal curve.

Corollary 3. Let α(s) be a normal curve in Galilean 4- spaceG4with non-zero constant curvatures τ and σ. The following statements are satisfied.

  • < + c3,

  • <

  • < + c4,

where c1, c2, c3, and c4 are constants.

Proof: Suppose that α(s) is a normal curve in Galilean 4-space G4 with non-zero constant curvatures τ and σ, then α(s) can be written in the form

α

Taking the inner product of the two sides with N(s), B1(s), and B2(s), the statements are held.

In the following theorem, we prove that, if α(s) is a normal curve, there are no curves which are congruent to α(s).

Theorem 2. Let α(s) be a normal curve in Galilean spaceG4with non-zero constant curvatures τ and σ. Then, there are no curves which are congruent to α(s).

Proof: First, let us define m(s) as follows

Taking the derivative of Equation (3.25) for both sides, we obtain

By substituting from Equations (2.1), (3.22)–(3.24).

m′(s) does not equal to zero, which means that m(s) is not a constant vector. So, α(s) is not congruent to a normal curve.

In the following theorem, we give the necessary condition for the normal curve in Galilean 4-space to lie on a sphere.

Theorem 3. Let α(s) be a normal curve in Galilean 4-spaceG4with non-zero constant curvatures τ and σ. Then, α(s) lies on a sphere if, wherec3andc4are the constants in equations (3.23) and (3.24).

Proof: The inner product of the position vector of α(s) is defined by

g( α(s), α(s)) = < α(s),

By simple computations, we have

< α(s),

If , then < α(s), , which means that α(s) lies on a sphere.

4. Conclusion

In this study, we established the definition of the normal curve in Galilean 4- space G4. Also, we derived the necessary condition for a curve to be a normal curve in G4. We have proved that, if α(s) is a normal curve in G4 with constant curvatures, there is no curve which is congruent to α(s). In the end, the necessary condition for a normal curve to lie on a sphere has been obtained.

Statements

Data availability statement

The original contributions presented in the study are included in the article/supplementary materials, further inquiries can be directed to the corresponding author/s.

Author contributions

All authors listed have made a substantial, direct and intellectual contribution to the work, and approved it for publication.

Acknowledgments

The authors wish to express their sincere thanks to referee for making several useful comments that improved the first version of the paper.

Conflict of interest

The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.

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Summary

Keywords

normal curves, Galilean space, curvatures, W-curve, Frenet apparatus

Citation

Mosa S, El-Fakharany M and Elzawy M (2021) Normal Curves in 4-Dimensional Galilean Space G4. Front. Phys. 9:660241. doi: 10.3389/fphy.2021.660241

Received

29 January 2021

Accepted

18 March 2021

Published

24 June 2021

Volume

9 - 2021

Edited by

Yang-Hui He, City University of London, United Kingdom

Reviewed by

Özlem Yeilta, Gazi University, Turkey; Kazuharu Bamba, Fukushima University, Japan

Updates

Copyright

*Correspondence: Mervat Elzawy ;

†Present address: Mohamed El-Fakharany, Mathematics and Statistics Department, College of Science, Taibah University, Yanbu, Saudi Arabia

This article was submitted to Mathematical and Statistical Physics, a section of the journal Frontiers in Physics

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All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors and the reviewers. Any product that may be evaluated in this article or claim that may be made by its manufacturer is not guaranteed or endorsed by the publisher.

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