STEM 隨筆︰古典力學︰向量【二】

若我們借著維基百科詞條,回顧一下什麼是『歐氏向量』︰

Euclidean vector

A vector pointing from A to B

In mathematics, physics, and engineering, a Euclidean vector (sometimes called a geometric[1] or spatial vector,[2] or—as here—simply a vector) is a geometric object that has magnitude (or length) and direction. Vectors can be added to other vectors according to vector algebra. A Euclidean vector is frequently represented by a line segment with a definite direction, or graphically as an arrow, connecting an initial point A with a terminal point B,[3] and denoted by \overrightarrow{AB}

A vector is what is needed to “carry” the point A to the point B; the Latin word vector means “carrier”.[4] It was first used by 18th century astronomers investigating planet rotation around the Sun.[5] The magnitude of the vector is the distance between the two points and the direction refers to the direction of displacement from A to B. Many algebraic operations on real numbers such as addition, subtraction, multiplication, and negation have close analogues for vectors, operations which obey the familiar algebraic laws of commutativity, associativity, and distributivity. These operations and associated laws qualify Euclidean vectors as an example of the more generalized concept of vectors defined simply as elements of a vector space.

Vectors play an important role in physics: the velocity and acceleration of a moving object and the forces acting on it can all be described with vectors. Many other physical quantities can be usefully thought of as vectors. Although most of them do not represent distances (except, for example, position or displacement), their magnitude and direction can still be represented by the length and direction of an arrow. The mathematical representation of a physical vector depends on the coordinate system used to describe it. Other vector-like objects that describe physical quantities and transform in a similar way under changes of the coordinate system include pseudovectors and tensors.

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須注意『始點』和『終點』在『向量定義』中角色。如是容易區分所謂『自由』或『束縛』向量何謂也,明白『原點』的重要性 。

 Overview

In physics and engineering, a vector is typically regarded as a geometric entity characterized by a magnitude and a direction. It is formally defined as a directed line segment, or arrow, in a Euclidean space.[8] In pure mathematics, a vector is defined more generally as any element of a vector space. In this context, vectors are abstract entities which may or may not be characterized by a magnitude and a direction. This generalized definition implies that the above-mentioned geometric entities are a special kind of vectors, as they are elements of a special kind of vector space called Euclidean space.

This article is about vectors strictly defined as arrows in Euclidean space. When it becomes necessary to distinguish these special vectors from vectors as defined in pure mathematics, they are sometimes referred to as geometric, spatial, or Euclidean vectors.

Being an arrow, a Euclidean vector possesses a definite initial point and terminal point. A vector with fixed initial and terminal point is called a bound vector.[9] When only the magnitude and direction of the vector matter, then the particular initial point is of no importance, and the vector is called a free vector. Thus two arrows \overrightarrow{AB} and  \overrightarrow{A^{'} B^{'}}  in space represent the same free vector if they have the same magnitude and direction: that is, they are equivalent if the quadrilateral ABB′A′ is a parallelogram. If the Euclidean space is equipped with a choice of origin, then a free vector is equivalent to the bound vector of the same magnitude and direction whose initial point is the origin.

The term vector also has generalizations to higher dimensions and to more formal approaches with much wider applications.

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進而深入『抽象』之『向量空間』裡!

Vector space

A vector space (also called a linear space) is a collection of objects called vectors, which may be added together and multiplied (“scaled”) by numbers, called scalars. Scalars are often taken to be real numbers, but there are also vector spaces with scalar multiplication by complex numbers, rational numbers, or generally any field. The operations of vector addition and scalar multiplication must satisfy certain requirements, called axioms, listed below.

Euclidean vectors are an example of a vector space. They represent physical quantities such as forces: any two forces (of the same type) can be added to yield a third, and the multiplication of a force vector by a real multiplier is another force vector. In the same vein, but in a more geometric sense, vectors representing displacements in the plane or in three-dimensional space also form vector spaces. Vectors in vector spaces do not necessarily have to be arrow-like objects as they appear in the mentioned examples: vectors are regarded as abstract mathematical objects with particular properties, which in some cases can be visualized as arrows.

Vector spaces are the subject of linear algebra and are well characterized by their dimension, which, roughly speaking, specifies the number of independent directions in the space. Infinite-dimensional vector spaces arise naturally in mathematical analysis, as function spaces, whose vectors are functions. These vector spaces are generally endowed with additional structure, which may be a topology, allowing the consideration of issues of proximity andcontinuity. Among these topologies, those that are defined by a norm or inner product are more commonly used, as having a notion of distance between two vectors. This is particularly the case of Banach spaces and Hilbert spaces, which are fundamental in mathematical analysis.

Historically, the first ideas leading to vector spaces can be traced back as far as the 17th century’s analytic geometry, matrices, systems of linear equations, and Euclidean vectors. The modern, more abstract treatment, first formulated by Giuseppe Peano in 1888, encompasses more general objects than Euclidean space, but much of the theory can be seen as an extension of classical geometric ideas like lines, planes and their higher-dimensional analogs.

Today, vector spaces are applied throughout mathematics, science and engineering. They are the appropriate linear-algebraic notion to deal with systems of linear equations. They offer a framework for Fourier expansion, which is employed in image compressionroutines, and they provide an environment that can be used for solution techniques for partial differential equations. Furthermore, vector spaces furnish an abstract, coordinate-free way of dealing with geometrical and physical objects such as tensors. This in turn allows the examination of local properties of manifolds by linearization techniques. Vector spaces may be generalized in several ways, leading to more advanced notions in geometry and abstract algebra.

Vector addition and scalar multiplication: a vector v (blue) is added to another vector w (red, upper illustration). Below, w is stretched by a factor of 2, yielding the sum v + 2w.

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思考『觀察者』如何在其『參考系』內作『座標變換』呦?

Conversion between multiple Cartesian bases

All examples thus far have dealt with vectors expressed in terms of the same basis, namely, the e basis {e1, e2, e3}. However, a vector can be expressed in terms of any number of different bases that are not necessarily aligned with each other, and still remain the same vector. In the e basis, a vector a is expressed, by definition, as

\displaystyle \mathbf {a} =p\mathbf {e} _{1}+q\mathbf {e} _{2}+r\mathbf {e} _{3}

The scalar components in the e basis are, by definition,
\displaystyle p=\mathbf {a} \cdot \mathbf {e} _{1} ,
\displaystyle q=\mathbf {a} \cdot \mathbf {e} _{2} ,
\displaystyle r=\mathbf {a} \cdot \mathbf {e} _{3} .
In another orthnormal basis n = {n1, n2, n3} that is not necessarily aligned with e, the vector a is expressed as
\displaystyle \mathbf {a} =u\mathbf {n} _{1}+v\mathbf {n} _{2}+w\mathbf {n} _{3}
and the scalar components in the n basis are, by definition,
\displaystyle u=\mathbf {a} \cdot \mathbf {n} _{1} ,
\displaystyle v=\mathbf {a} \cdot \mathbf {n} _{2} ,
\displaystyle w=\mathbf {a} \cdot \mathbf {n} _{3} .
The values of p, q, r, and u, v, w relate to the unit vectors in such a way that the resulting vector sum is exactly the same physical vector a in both cases. It is common to encounter vectors known in terms of different bases (for example, one basis fixed to the Earth and a second basis fixed to a moving vehicle). In such a case it is necessary to develop a method to convert between bases so the basic vector operations such as addition and subtraction can be performed. One way to express u, v, w in terms of p, q, r is to use column matrices along with a direction cosine matrix containing the information that relates the two bases. Such an expression can be formed by substitution of the above equations to form
\displaystyle u=(p\mathbf {e} _{1}+q\mathbf {e} _{2}+r\mathbf {e} _{3})\cdot \mathbf {n} _{1} ,
\displaystyle v=(p\mathbf {e} _{1}+q\mathbf {e} _{2}+r\mathbf {e} _{3})\cdot \mathbf {n} _{2} ,
\displaystyle w=(p\mathbf {e} _{1}+q\mathbf {e} _{2}+r\mathbf {e} _{3})\cdot \mathbf {n} _{3} .
Distributing the dot-multiplication gives
\displaystyle u=p\mathbf {e} _{1}\cdot \mathbf {n} _{1}+q\mathbf {e} _{2}\cdot \mathbf {n} _{1}+r\mathbf {e} _{3}\cdot \mathbf {n} _{1} ,
\displaystyle v=p\mathbf {e} _{1}\cdot \mathbf {n} _{2}+q\mathbf {e} _{2}\cdot \mathbf {n} _{2}+r\mathbf {e} _{3}\cdot \mathbf {n} _{2} ,
\displaystyle w=p\mathbf {e} _{1}\cdot \mathbf {n} _{3}+q\mathbf {e} _{2}\cdot \mathbf {n} _{3}+r\mathbf {e} _{3}\cdot \mathbf {n} _{3} .
Replacing each dot product with a unique scalar gives
\displaystyle u=c_{11}p+c_{12}q+c_{13}r ,
\displaystyle v=c_{21}p+c_{22}q+c_{23}r ,
\displaystyle w=c_{31}p+c_{32}q+c_{33}r ,
and these equations can be expressed as the single matrix equation
\displaystyle {\begin{bmatrix}u\\v\\w\\\end{bmatrix}}={\begin{bmatrix}c_{11}&c_{12}&c_{13}\\c_{21}&c_{22}&c_{23}\\c_{31}&c_{32}&c_{33}\end{bmatrix}}{\begin{bmatrix}p\\q\\r\end{bmatrix}} .
This matrix equation relates the scalar components of a in the n basis (u,v, and w) with those in the e basis (p, q, and r). Each matrix element cjk is the direction cosine relating nj to ek.[13] The term direction cosine refers to the cosine of the angle between two unit vectors, which is also equal to their dot product.[13] Therefore,
\displaystyle c_{11}=\mathbf {n} _{1}\cdot \mathbf {e} _{1}
\displaystyle c_{12}=\mathbf {n} _{1}\cdot \mathbf {e} _{2}
\displaystyle c_{13}=\mathbf {n} _{1}\cdot \mathbf {e} _{3}
\displaystyle c_{21}=\mathbf {n} _{2}\cdot \mathbf {e} _{1}
\displaystyle c_{22}=\mathbf {n} _{2}\cdot \mathbf {e} _{2}
\displaystyle c_{23}=\mathbf {n} _{2}\cdot \mathbf {e} _{3}
\displaystyle c_{31}=\mathbf {n} _{3}\cdot \mathbf {e} _{1}
\displaystyle c_{32}=\mathbf {n} _{3}\cdot \mathbf {e} _{2}
\displaystyle c_{33}=\mathbf {n} _{3}\cdot \mathbf {e} _{3}
By referring collectively to e1, e2, e3 as the e basis and to n1, n2, n3 as the n basis, the matrix containing all the cjk is known as the “transformation matrix from e to n“, or the “rotation matrix from e to n” (because it can be imagined as the “rotation” of a vector from one basis to another), or the “direction cosine matrix from e to n[13] (because it contains direction cosines). The properties of a rotation matrix are such that its inverse is equal to its transpose. This means that the “rotation matrix from e to n” is the transpose of “rotation matrix from n to e“.

The properties of a direction cosine matrix, C are [[14]]:

  • the determinant is unity, |C| = 1
  • the inverse is equal to the transpose,
  • the rows and columns are orthogonal unit vectors, therefore their dot products are zero.

The advantage of this method is that a direction cosine matrix can usually be obtained independently by using Euler angles or a quaternion to relate the two vector bases, so the basis conversions can be performed directly, without having to work out all the dot products described above.

By applying several matrix multiplications in succession, any vector can be expressed in any basis so long as the set of direction cosines is known relating the successive bases.[13]