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JEE Main 2026 Preparation: Question Papers, Solutions, Mock Tests & Strategy Unacademy » JEE Study Material » Mathematics » All About Vector Notation

All About Vector Notation

In the following article we are going to know about vector notation in detail.

Table of Content
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Vector notation is a popular notation in mathematics and physics for representing vectors, which might be Euclidean vectors or, more broadly, members of a vector space. 

The standard typographic approach for showing the vector is lower case, upright boldface font, as in v. The International Organization for Standardization (ISO) suggests using a bold italic serif, such as v, or a non-bold italic serif with a right arrow emphasis. Vectors are frequently represented in advanced mathematics as a basic italic font, just like any other variable.

Unit Vector Notation:

The sign “^”, which is often known as a cap or hat, is used to denote a vector. It is provided by a^ = a/|a|, where |a| stands for the vector a’s norm or magnitude. 

Three-dimensional unit vector:

The unit vectors of i, j, and k are commonly the x-, y-, and z-axes respectively. A linear combination of these unit vectors can be used to express any given vector in three-dimensional space. The cross-product of two supplied unit vectors, on the other hand, produces a third vector that is perpendicular (orthogonal) to both of them.

Normal Vector Unit:

A ‘normal vector’ is perpendicular to the surface at a specific point vector. A surface containing the vector is also referred to as “normal.” The unit normal vector, sometimes known as the “unit normal,” is the unit vector obtained after normalizing the normal vector. A non-zero normal vector is divided by its vector norm for this.

Set notation in order

An ordered collection of components surrounded in parentheses or angle brackets can be used to specify a rectangular vector in Rn.

V = (v1, v2 , v3 , v4 ,…, vn-1 , vn)

V= < v1, v2 , v3 , v4 ,…, vn-1 , vn >

V = [ v1, v2 , v3 , v4 ,…, vn-1 , vn]

Polar vectors:

A two-dimensional vector is made up of the two polar coordinates of a point in a plane. A polar vector has two components: a magnitude (or length) and a direction (or angle). The magnitude, which is usually written as r, is the distance between the origin and the point is represented. The angle (the Greek letter theta) is the angle formed by a fixed direction, generally the positive x-axis, and the direction from the origin to the point. It is normally measured counterclockwise.

Direct notation

Simplified autonomous equations that describe r and explicitly can also be used to specify polar vectors. This is cumbersome, but it avoids the misunderstanding that might emerge when using ordered pair or matrix notation with two-dimensional rectangular vectors.

Cylindrical Vector:

A cylindrical vector is a three-dimensional expansion of the idea of polar vectors. In the cylindrical coordinate system, it resembles an arrow. A cylindrical vector is defined by its xy-plane distance, angle, and distance from the xy-plane. The first distance is the magnitude of the vector’s projection onto the xy-plane, which is commonly written as r or ρ (the Greek letter rho). The angle is calculated asθ or φ(the Greek letter phi)  the offset from the line collinear with the x-axis in the positive direction, and is commonly lowered to lie within the range 0 which is less than equal to the angle theta less than  twice of pi. The second distance, commonly denoted by h or z, is the distance between the xy-plane and the vector’s terminus.

Notations for ordered sets and matrices

The second distance component is concatenated as a third component to construct ordered triplets (again, a subset of ordered set notation) and matrices, much as it is for polar vectors. The angle symbol can be used to prefix the angle; the distance-angle-distance combination differentiates cylindrical vectors from spherical vectors in identical notation.

Direct notation

A cylindrical vector can alternatively be defined directly using simplified autonomous equations that determine r (or ρ), θ (or φ), and h (or z). When naming variables, consistency should be used; for example, should not be confused with and so on.

Conclusion:

The quantity with both magnitude and direction are known as vectors. A vector is represented as a line with an arrow pointing in the direction of the vector, and the length of the vector denotes its magnitude. Vectors are therefore represented by arrows and have both beginning and terminal locations.

faq

Frequently asked questions

Get answers to the most common queries related to the JEE Examination Preparation.

What is the best way to write vector notation?

 the best way to write vector notation as an arrow in space when it is merely a list of integers.

What is the vector notation rule?

 Rule 1: a zero vector exists.  Rule 2: A vector A multiplied by a sc...Read full

What are the different kinds of vectors?

 the different kinds of vectors are Zer...Read full

Write down the definition of a vector?

In Mathematics, a vector is a quantity with both magnitude and direction. It is represented by an arrow with the sam...Read full

How to combine vectors?

 Place the first vector on a set of axes with its tail at the origin to add more vectors. Place the tail of the nex...Read full

 the best way to write vector notation as an arrow in space when it is merely a list of integers.

 Rule 1: a zero vector exists. 

Rule 2: A vector A multiplied by a scalar m is a vector with the same direction as before but with the length varied by the factor m. 

Rule 3 – A vector’s negative is the original vector inverted 180 degrees;

 the different kinds of vectors are

  • Zero vector.
  • Unit Vector.
  • Position Vector.
  • Co-initial Vector.
  • Like vector.
  • Unlike Vectors.
  • Co-planar Vector.
  • Collinear Vector

In Mathematics, a vector is a quantity with both magnitude and direction. It is represented by an arrow with the same direction as the value and a length proportionate to the magnitude of the quantity. A vector does not have location, it has magnitude and direction.

 Place the first vector on a set of axes with its tail at the origin to add more vectors. Place the tail of the next vector at the head of the preceding vector. Draw a straight line from the origin to the head of the final vector when there are no more vectors. The total of the vectors is this line.

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