lacunary - Mathnotes

Vector Space

Scalars

Note \@{note-3}

Typically, especially in physics, a scalar is simply a number, especially a real number.

Vectors

Note \@{note-5}

Typically, in physics and many other applications, when we say vector we mean a vector in Rn, which is an ordered tuple of real numbers, x=(x1,x2,,xn). This is the algebraic representation of vector x.

The geometric representation of vector x is, in an n dimensional space, an arrow or directed line segment. When starting from the origin, it would be a line segment from 0 to the point (x1,x2,,xn).

Physically, a vector has a magnitude and a direction.

Definition: Free vector \@{free-vector}

A vector whose endpoints are not fixed at particular points is called a free vector.

Definition: Bound vector \@{bound-vector}

A vector with a fixed endpoint is called a bound vector.

Properties of Vectors

Definition: Magnitude (also: norm, length) \@{magnitude}

Let x=(x1,x2,,xn)Rn. The magnitude, or length, x is denoted as ||x|| and is defined as:

||x||=x12+x22++xn2=xx=i=1nxi2

Note \@{note-9}

This is essentially the Pythagorean theorem in n dimensions; in R2 the magnitude of a vector corresponds to the length of the hypotenuse of a right triangle whose other sides are of length x1 and x2.

While we define norm to be equivalent to magnitude here, this is actually a special case of the more general concept of a norm - there are other norms we could define on Rn, but I don't have need to explore that yet.

Definition: Zero Vector \@{zero-vector}

The zero vector (0,0,,0) is denoted as 0 and has no direction.

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Definition: Vector Equality \@{vector-equality}

Two vectors are equal if they have the same coordinates (or equivalently, the same length and direction).

Definition: Unit Vector \@{unit-vector}

If a vector has a length of 1, i.e. if ||x||=1, we say the vector is a unit vector.

Note \@{note-15}

Geometrically, vector addition connects vectors head to tail.

Definition: Vector Subtraction \@{vector-subtraction}

Similarly, vector subtraction can be performed as:

xy=(x1y1,x2y2,,xnyn)

Multiplication

Definition: Inner product (also: Dot Product, Scalar product of two vectors) \@{inner-product}

If x and y are vectors in Rn, then their inner product is defined as

Xy=i=1nxiyi.

Theorem \@{cos-characterization-of-dot-product}

The dot product of u and v is

uv=|u||v|cosθ

where θ is the angle between u and v.

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Definition: Perpendicular (also: orthogonal) \@{perpendicular}

Two vectors u and v are said to be perpendicular or orthogonal if the angle between them is π/2 radians, or, equivalently, if the inner product uv=0.

Definition: Parallel \@{parallel}

Two vectors x and y are said to be parallel if x is a scalar multiple of y, i.e., if there exists some scalar c where x=cy.

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Definition: Cross Product (also: Vector Product, Outer Product) \@{cross-product}

The cross product a×b (read "a cross b") of two vectors a and b is the vector v denoted by

v=a×b.

I. If a=0 or b=0, then we define v=a×b=0.

II. If both vectors are nonzero vectors, then vector v has the length

|v|=|a×b|=|a||b|sinθ,(1)

where θ is the angle between a and b. Furthermore, a and b form the sides of a parallelogram on a plane in space. The area of this parallelogram is precisely given by (1), such that the length |v| of the vector v is equal to the area of the parallelogram.

III. If a and b lie in the same straight line, i.e. a and b have the same or opposite directions, then θ is 0 or 180 so that sinθ=0. In that case |v|=0, so that v=a×b=0.

IV. If cases I and III do not occur, then v is a nonzero vector. The direction of v=a×b is perpendicular to both a and b such that a,b,v, precisely in this order, form a right-handed triple

Referenced by (2 direct)

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Remark \@{remark-23}

If a=(a1,a2,a3) and b=(b1,b2,b3), then we use the symbolic determinant to find the cross product, in this fashion:

v=a×b=|ijka1a2a3b1b2b3|=|a2a3b2b3|i|a1a3b1b3|j+|a1a2b1b2|k.

Definition: Linear Combination \@{linear-combination}

Let v1,v2,,vnRn and c1,c2,,c3R. Then, the vector

v=c1v1+c2v2++cnvn

is called a linear combination of v1,v2,,vn.

Let v1,v2,,vnRn. The set of all linear combinations of v1,v2,,vn is called their span, denoted Span(v1,v2,,vn).

That is:

Span(v1,v2,,vn)={vRn:v=c1v1+c2v2++cnvn for some scalars c1,c2,,cn}