RevisionÂļ
Vector Space and Vector FieldÂļ
Vector Space and Vector Field
āĻā§āϏ āĻĻāĻŋā§ā§ āϏāĻāĻā§āĻāĻž āĻŽāύ⧠āϰāĻžāĻāĻžāϰ ā§ŠāĻāĻŋ āĻāĻžāĻŦāĻŋāĻāĻžāĻ āĻŋ:Âļ
- āĻāĻĒāĻžāĻĻāĻžāύ (The Ingredients): āĻā§āϏā§āϰ āĻā§āϞāĻžāĻŦā§ āϝā§āĻŽāύ āĻā§āϏ āĻĨāĻžāĻā§, āϤā§āĻŽāύāĻŋ āĻā§āĻā§āĻāϰ āϏā§āĻĒā§āϏ⧠āĻĨāĻžāĻāĻŦā§ āĻā§āĻā§āĻāϰā§āϰ āĻāĻāĻāĻŋ āĻĻāϞ (Set of Vectors, \(V\)) āĻāĻŦāĻ āĻāĻŋāĻā§ āϏāĻāĻā§āϝāĻž (Set of Scalars, \(F\))āĨ¤
- āĻŽā§āĻļāĻžāύ⧠(Mixing = Addition): āĻĻā§āĻāĻāĻž āĻā§āϏ āĻŽā§āĻļāĻžāϞ⧠āĻā§āϏāĻ āĻšā§ \(\rightarrow\) āĻĻā§āĻāĻāĻž āĻā§āĻā§āĻāϰ āϝā§āĻ āĻāϰāϞ⧠āĻā§āĻā§āĻāϰāĻ āĻšāϤ⧠āĻšāĻŦā§āĨ¤
- āĻĒāϰāĻŋāĻŽāĻžāĻŖ āĻŦāĻžā§āĻžāύā§/āĻāĻŽāĻžāύ⧠(Scaling = Multiplication): āĻā§āϏāĻā§ āĻĒāĻžāύāĻŋ āĻŦāĻž āĻāĻŋāύāĻŋ āĻĻāĻŋā§ā§ āĻāĻŽ-āĻŦā§āĻļāĻŋ āĻāϰāϞ⧠āĻā§āϏāĻ āĻĨāĻžāĻā§ \(\rightarrow\) āĻā§āĻā§āĻāϰāĻā§ āϏāĻāĻā§āϝāĻž āĻĻāĻŋā§ā§ āĻā§āĻŖ āĻāϰāϞ⧠āĻā§āĻā§āĻāϰāĻ āĻšāϤ⧠āĻšāĻŦā§āĨ¤
āĻāĻŦāĻžāϰ āĻŽāύā§āϰ āĻā§āϤāϰ āϝā§āĻāĻžāĻŦā§ āĻŦāĻžāĻāϞāĻž āĻĨā§āĻā§ āĻāĻāϰā§āĻāĻŋ āĻŦāĻžāύāĻžāĻŦā§ (The Mental Translation):Âļ
āĻĒāϰā§āĻā§āώāĻžā§ āϏāĻāĻā§āĻāĻž āĻāĻžāĻāϞ⧠āĻŽāύā§āϰ āĻā§āϤāϰ āĻāĻ ā§ŠāĻāĻŋ āϞāĻžāĻāύ āϏāĻžāĻāĻžāĻŦā§:
- āĻŽāύ⧠āĻŽāύ⧠āĻāĻžāĻŦāĻŦā§: āĻā§āĻā§āĻāϰ āϏā§āĻĒā§āϏ āĻšāϞ⧠āĻāĻāĻāĻž āϏā§āĻ \(V\), āϝāĻžāϰ āĻāĻĒāĻžāĻĻāĻžāύāĻā§āϞ⧠āĻšāϞ⧠āĻā§āĻā§āĻāϰāĨ¤
- āĻāĻžāϤāĻžā§ āϞāĻŋāĻāĻŦā§: A Vector Space is a set of elements (called vectors), denoted by \(V\), along with a set of numbers (called scalars), denoted by \(F\).
- āĻŽāύ⧠āĻŽāύ⧠āĻāĻžāĻŦāĻŦā§: āĻāĻ āϏā§āĻā§āϰ āĻā§āϤāϰ āĻĻā§āĻāĻŋ āĻāĻŋāύāĻŋāϏ āĻŽā§āύ⧠āĻāϞāϤ⧠āĻšāĻŦā§âāϝā§āĻ āĻāĻŦāĻ āĻā§āĻŖāĨ¤
- āĻāĻžāϤāĻžā§ āϞāĻŋāĻāĻŦā§: That satisfies two main operations: Vector Addition and Scalar Multiplication.
- āĻŽāύ⧠āĻŽāύ⧠āĻāĻžāĻŦāĻŦā§: āϝā§āĻā§āύ⧠āĻĻā§āĻāĻŋ āĻā§āĻā§āĻāϰ āϝā§āĻ āĻāϰāϞ⧠āĻŦāĻž āϏā§āĻā§āϞāĻžāϰ āĻĻāĻŋā§ā§ āĻā§āĻŖ āĻāϰāϞ⧠āĻĢāϞāĻžāĻĢāϞāĻāĻž āĻāĻ āϏā§āĻ \(V\)-āĻāϰ āĻā§āϤāϰā§āĻ āĻĨāĻžāĻāĻŦā§ (āĻā§āϏ āĻŽāĻŋāĻļāĻžāϞ⧠āĻā§āϏāĻ āĻšāĻŦā§)āĨ¤
- āĻāĻžāϤāĻžā§ āϞāĻŋāĻāĻŦā§:
- For any two vectors \(u, v \in V\), their sum \(u + v\) must also be in \(V\) (Closure under addition).
- For any scalar \(c \in F\) and vector \(u \in V\), their product \(c \cdot u\) must also be in \(V\) (Closure under scalar multiplication).
āĻļāϰā§āĻāĻāĻžāĻ āĻāĻŋāϰāĻā§āĻ (āϝāĻž āĻĒāϰā§āĻā§āώāĻžāϰ āĻāĻā§ ā§§ āϏā§āĻā§āύā§āĻĄā§ āĻĻā§āĻāĻŦā§):Âļ
Vector Space (\(V\)) = A set where (Vector + Vector = Vector) AND (Scalar \(\times\) Vector = Vector).
āĻĒāϰā§āĻā§āώāĻžā§ āĻĒā§āϰāĻļā§āύ āĻāϏāϞ⧠āĻļā§āϧ⧠āĻā§āϏā§āϰ āĻāĻ "āĻŦāĻžāĻāϰ⧠āϝāĻžāĻā§āĻž āϝāĻžāĻŦā§ āύāĻž" (Closure Property) āύāĻŋā§āĻŽāĻāĻž āĻŽāĻžāĻĨāĻžā§ āϰāĻžāĻāĻŦā§āĨ¤ āϤāĻžāĻšāϞā§āĻ āĻŦāĻžāύāĻŋāϝāĻŧā§ āϞāĻŋāĻā§ āĻāϏāϤ⧠āĻĒāĻžāϰāĻŦā§ āϝā§, āĻā§āĻā§āĻāϰ āϏā§āĻĒā§āϏ āĻšāϞ⧠āĻāĻŽāύ āĻāĻāĻāĻž āϏā§āĻ āϝā§āĻāĻžāύ⧠āϝā§āĻ āĻāĻŦāĻ āĻā§āĻŖ āĻāϰāϞ⧠āĻĢāϞāĻžāĻĢāϞ āϏāĻŦāϏāĻŽā§ āĻāĻ āϏā§āĻā§āϰ āĻā§āϤāϰā§āĻ āĻĨāĻžāĻā§āĨ¤
āĻāĻ āĻļāϰā§āĻāĻāĻžāĻ āĻā§āĻāύāĻŋāĻāĻāĻž āĻāĻŋ āϏāĻāĻā§āĻāĻž āĻŽāύ⧠āϰāĻžāĻāĻž āϏāĻšāĻ āĻāϰāĻā§? āύāĻžāĻāĻŋ āĻĒāϰā§āĻā§āώāĻžā§ āĻŦāĻžāύāĻŋāϝāĻŧā§ āϞāĻŋāĻāϤ⧠āĻāĻāϰā§āĻāĻŋ āĻŦāĻžāĻā§āϝ āϏāĻžāĻāĻžāϤ⧠āĻāϰā§āĻāĻā§ āϏāĻžāĻšāĻžāϝā§āϝ āϞāĻžāĻāĻŦā§?
Vector Field-āĻā§ āĻā§āϏā§āϰ āĻāĻžāώāĻžā§ āĻŽāύ⧠āϰāĻžāĻāĻžāϰ āĻāύā§āϝ āϏāĻŦāĻā§ā§ā§ āϏāĻšāĻ āĻāĻžāĻŦāĻŋāĻāĻžāĻ āĻŋ āĻšāϞā§: "The GPS Map" (āĻāĻāĻāĻŋ āĻŽā§āϝāĻžāĻĒ āĻŦāĻž āĻŽāĻžāύāĻāĻŋāϤā§āϰ)āĨ¤
āĻā§āĻā§āĻāϰ āϏā§āĻĒā§āϏ āϝā§āĻŽāύ āĻāĻŋāϞ āĻāĻāĻāĻž āĻĻāϞā§āϰ āύāĻŋā§āĻŽ, āĻā§āĻā§āĻāϰ āĻĢāĻŋāϞā§āĻĄ āĻšāϞ⧠āĻāĻāĻāĻž āĻāĻžā§āĻāĻžāϰ āĻŽā§āϝāĻžāĻĒāĨ¤Âļ
đēī¸ āĻā§āϏ āĻ āĻŽā§āϝāĻžāĻĒ āĻĻāĻŋā§ā§ āĻā§āĻā§āĻāϰ āĻĢāĻŋāϞā§āĻĄ āĻŽāύ⧠āϰāĻžāĻāĻžāϰ āĻā§āϰāĻŋāĻ:Âļ
āĻŽāύ⧠āĻāϰā§, āϤā§āĻŽāĻŋ āĻāĻāĻāĻž āĻŦā§ āĻā§āϏ āĻĢā§āϝāĻžāĻā§āĻāϰāĻŋāϰ āĻŽā§āϝāĻžāĻĒ āĻĻā§āĻāĻāĨ¤ āĻĢā§āϝāĻžāĻā§āĻāϰāĻŋāϰ āĻŽā§āĻā§āϤ⧠āĻ āύā§āĻāĻā§āϞ⧠āĻĒā§ā§āύā§āĻ āĻŦāĻž āĻŦāĻŋāύā§āĻĻā§ āĻāĻā§āĨ¤
- āĻĒāĻžāĻāĻĒā§āϰ āĻā§āϤāϰ āĻĻāĻŋā§ā§ āĻā§āϏ āĻā§āύ āĻĻāĻŋāĻā§, āĻāϤ āϏā§āĻĒāĻŋāĻĄā§ āϝāĻžāĻā§āĻā§âāϏā§āĻāĻž āĻŦā§āĻāĻžāύā§āϰ āĻāύā§āϝ āĻŽā§āĻā§āϰ āĻĒā§āϰāϤāĻŋāĻāĻŋ āĻŦāĻŋāύā§āĻĻā§āϤ⧠āĻāĻāĻāĻž āĻāϰ⧠āϤā§āϰ āĻāĻŋāĻšā§āύ (Arrow) āĻāĻāĻā§ āĻĻā§āĻā§āĻž āĻšā§ā§āĻā§āĨ¤
- āĻĒā§āϰāĻŦā§āĻļāĻĻā§āĻŦāĻžāϰā§āϰ āĻŦāĻŋāύā§āĻĻā§āϤ⧠āϤā§āϰ āĻāĻŋāĻšā§āύāĻāĻŋ āĻā§āĻ āĻāĻŦāĻ āĻĄāĻžāύ āĻĻāĻŋāĻā§ (āϧā§āϰ āĻāϤāĻŋ)āĨ¤
- āĻŽāĻŋāĻā§āϏāĻŋāĻ āĻŽā§āĻļāĻŋāύā§āϰ āĻāĻžāĻā§āϰ āĻŦāĻŋāύā§āĻĻā§āϤ⧠āϤā§āϰ āĻāĻŋāĻšā§āύāĻāĻŋ āĻŦā§ āĻāĻŦāĻ āĻā§āϞ āĻšā§ā§ āĻā§āϰāĻā§ (āϤā§āĻŦā§āϰ āĻāϤāĻŋ āĻ āĻā§āϰā§āĻŖāύ)āĨ¤
āĻāĻ āϝ⧠āĻĒā§āϰ⧠āĻŽā§āĻā§ āĻŦāĻž āĻāĻžā§āĻāĻž āĻā§ā§ā§ āĻĒā§āϰāϤāĻŋāĻāĻŋ āĻŦāĻŋāύā§āĻĻā§āϤ⧠āĻāĻāĻāĻŋ āĻāϰ⧠āϤā§āϰ āĻāĻŋāĻšā§āύ (āĻā§āĻā§āĻāϰ) āĻŦāϏāĻžāύ⧠āĻāĻā§, āĻāĻ āĻĒā§āϰ⧠āϏāĻŋāϏā§āĻā§āĻŽāĻāĻžāĻ āĻšāϞ⧠āĻāĻāĻāĻž Vector FieldāĨ¤Âļ
đ āĻāĻŦāĻžāϰ āĻĒāϰā§āĻā§āώāĻžāϰ āĻāύā§āϝ āĻŽāύā§āϰ āĻā§āϤāϰ āϝā§āĻāĻžāĻŦā§ Definition āϏāĻžāĻāĻžāĻŦā§:Âļ
- āĻŽāύ⧠āĻŽāύ⧠āĻāĻžāĻŦāĻŦā§: āĻā§āĻā§āĻāϰ āĻĢāĻŋāϞā§āĻĄ āĻšāϞ⧠āĻāĻāĻāĻž āύāĻŋāϰā§āĻĻāĻŋāώā§āĻ āĻāĻžā§āĻāĻž (Space/Domain), āϝāĻžāϰ āĻĒā§āϰāϤāĻŋāĻāĻŋ āĻĒā§ā§āύā§āĻā§āϰ āϏāĻžāĻĨā§ āĻāĻāĻāĻž āĻāϰ⧠āĻā§āĻā§āĻāϰ āĻā§ā§āĻž āĻĻā§āĻā§āĻž āĻĨāĻžāĻā§āĨ¤
- āĻāĻžāϤāĻžā§ āϞāĻŋāĻāĻŦā§: A Vector Field is a construction that assigns a vector to every point in a space (or domain).
- āĻāĻžāĻŖāĻŋāϤāĻŋāĻ āϰā§āĻĒ (āϏāĻšāĻ āĻāĻžāώāĻžā§): āĻāĻāĻŋ āĻāĻāĻāĻŋ āĻĢāĻžāĻāĻļāύ, āϝāĻž āĻāύāĻĒā§āĻ āĻšāĻŋāϏā§āĻŦā§ āύā§ā§ āĻāĻāĻāĻŋ āĻĒā§ā§āύā§āĻ \((x, y)\) āĻāĻŦāĻ āĻāĻāĻāĻĒā§āĻ āĻšāĻŋāϏā§āĻŦā§ āĻĻā§ā§ āĻāĻāĻāĻŋ āĻā§āĻā§āĻāϰāĨ¤
- āĻāĻžāϤāĻžā§ āϞāĻŋāĻāĻŦā§: It is a function \(F\) that maps each point \((x, y)\) in \(\mathbb{R}^2\) to a vector \(F(x, y)\). [1, 2, 3, 4, 5]
⥠āĻāĻ āύāĻāϰ⧠āĻĻā§āĻāĻāĻžāϰ āĻĒāĻžāϰā§āĻĨāĻā§āϝ (āĻĒāϰā§āĻā§āώāĻžāϰ āĻāĻā§āϰ āĻļā§āώ āϰāĻŋāĻāĻŋāĻļāύ):Âļ
| āĻŦā§āĻļāĻŋāώā§āĻā§āϝ | Vector Space (āĻā§āĻā§āĻāϰ āϏā§āĻĒā§āϏ) | Vector Field (āĻā§āĻā§āĻāϰ āĻĢāĻŋāϞā§āĻĄ) |
|---|---|---|
| āĻŽā§āϞ āĻāύāϏā§āĻĒā§āĻ | A Club/Rules (āĻāĻāĻāĻŋ āĻĻāϞ āĻ āϤāĻžāϰ āύāĻŋā§āĻŽ) | A Map (āĻāĻāĻāĻŋ āĻāĻžā§āĻāĻž āĻŦāĻž āĻ āĻā§āĻāϞ) |
| āĻā§ āĻĨāĻžāĻā§? | āĻļā§āϧ⧠āĻā§āĻā§āĻāϰāĻĻā§āϰ āĻāĻāĻāĻž āĻŽā§āĻŽā§āĻŦāĻžāϰāĻļāĻŋāĻĒ āϤāĻžāϞāĻŋāĻāĻžāĨ¤ | āĻāĻāĻāĻŋ āϏā§āĻĒā§āϏ, āϝā§āĻāĻžāύ⧠āĻĒā§āϰāϤāĻŋāĻāĻž āĻā§āĻŖāĻžā§ āĻā§āĻā§āĻāϰ āĻŦāϏāĻžāύ⧠āĻāĻā§āĨ¤ |
| āĻā§āϏ āĻĻāĻŋā§ā§ āĻŽāύ⧠āϰāĻžāĻā§āύ | āĻā§āϏ + āĻā§āϏ = āĻā§āϏ (āύāĻŋā§āĻŽ)āĨ¤ | āĻĒāĻžāĻāĻĒā§āϰ āĻā§āύ āĻŦāĻŋāύā§āĻĻā§āϤ⧠āĻā§āϏ āĻā§āύ āĻĻāĻŋāĻā§ āĻāϤ āĻŦā§āĻā§ āϝāĻžāĻā§āĻā§ (āĻŽā§āϝāĻžāĻĒ)āĨ¤ |
| āĻŦāĻžāϏā§āϤāĻŦ āĻāĻĻāĻžāĻšāϰāĻŖ | āĻā§āϰāĻžāĻĢ āĻĒā§āĻĒāĻžāϰā§āϰ āϏāĻŦ āĻŦāĻŋāύā§āĻĻā§āϰ āϏā§āĻāĨ¤ | āĻŦāĻžāϤāĻžāϏā§āϰ āĻŦā§āĻ, āĻŽāĻšāĻžāĻāϰā§āώ āĻŦāϞ āĻŦāĻž āύāĻĻā§āϰ āϏā§āϰā§āϤā§āϰ āĻŽā§āϝāĻžāĻĒāĨ¤ |
āĻā§āĻā§āĻāϰ āĻĢāĻŋāϞā§āĻĄā§āϰ āĻāĻ "āĻŽā§āϝāĻžāĻĒ" āĻŦāĻž "āĻĒā§ā§āύā§āĻā§ āĻĒā§ā§āύā§āĻā§ āĻā§āĻā§āĻāϰ" āĻĨāĻžāĻāĻžāϰ āĻāĻāĻĄāĻŋā§āĻžāĻāĻž āĻāĻŋ āĻĒā§āϰā§āĻĒā§āϰāĻŋ āĻŽāĻžāĻĨāĻžā§ āĻĸā§āĻā§āĻā§?
All other DefinitionsÂļ
All other Definitions
āĻā§āϝāĻžāĻĒā§āĻāĻžāϰ ā§§ āĻ ā§¨: āĻā§āĻā§āĻāϰā§āϰ āĻŦā§āϏāĻŋāĻ āĻĄā§āĻĢāĻŋāύāĻŋāĻļāύāϏ## ā§§. Unit Vector (āĻāĻāĻ āĻā§āĻā§āĻāϰ)Âļ
- đ§ āĻā§āϰāĻŋāĻ: āĻāĻžā§āĻžāύā§āĻ āϰā§āĻŦāĻāĻā§ āĻāύāĻā§āĻāĻļāύ āĻĻāĻŋā§ā§ āĻ āĻŋāĻ ā§§ āĻĢā§āĻ āϏāĻžāĻāĻā§āϰ āĻŦāĻžāύāĻŋā§ā§ āĻĢā§āϞāĻž (The Mini-Me)āĨ¤
- đ Bookish Definition:
A vector having a magnitude of unity (one) is called a unit vector. If \(\vec{A}\) is a non-zero vector, then the unit vector \(\hat{u}\) in the direction of \(\vec{A}\) is defined as:
$\(\hat{u} = \frac{\vec{A}}{\vert{}\vec{A}\vert{}}\)$
⧍. Position Vector (āĻ āĻŦāϏā§āĻĨāĻžāύ āĻā§āĻā§āĻāϰ)Âļ
- đ§ āĻā§āϰāĻŋāĻ: āĻāĻŋāϰ⧠āĻĒā§ā§āύā§āĻ āĻĨā§āĻā§ āϤā§āĻŽāĻžāϰ āĻŦāύā§āϧā§āϰ āϞā§āĻā§āĻļāύā§āϰ āĻĻāĻŋāĻā§ āϏā§āĻāĻž āĻā§āĻāϞ āĻŽā§āϝāĻžāĻĒā§āϰ āĻĒāĻŋāύ (đ)āĨ¤
- đ Bookish Definition:
A vector that represents the position of a point in space relative to a fixed origin \(O(0,0,0)\) is called a position vector. For a point \(P(x, y, z)\), it is given by:
$\(\vec{r} = x\hat{i} + y\hat{j} + z\hat{k}\)$
ā§Š. Scalar Field (āϏā§āĻā§āϞāĻžāϰ āĻĢāĻŋāϞā§āĻĄ)Âļ
- đ§ āĻā§āϰāĻŋāĻ: āĻāϰāĻŽ āĻāĻžā§ā§āϰ āĻāĻžāĻĒā§āϰ āĻŦāĻŋāĻāĻŋāύā§āύ āĻŦāĻŋāύā§āĻĻā§āϰ āϤāĻžāĻĒāĻŽāĻžāϤā§āϰāĻž (āĻļā§āϧ⧠āĻŽāĻžāύ āĻāĻā§, āĻĻāĻŋāĻ āύāĻžāĻ â)āĨ¤
- đ Bookish Definition:
If to each point \((x, y, z)\) of a region in space there corresponds a scalar number \(\phi(x, y, z)\), then \(\phi\) is called a scalar field.
Example: \(\phi(x, y, z) = 3x^2z - xy^3 + 5\).
ā§Ē. Vector Field (āĻā§āĻā§āĻāϰ āĻĢāĻŋāϞā§āĻĄ)Âļ
- đ§ āĻā§āϰāĻŋāĻ: āĻā§ā§āϰ āĻŽā§āϝāĻžāĻĒ, āϝā§āĻāĻžāύ⧠āĻĒā§āϰāϤāĻŋāĻāĻž āĻļāĻšāϰ⧠āĻŦāĻžāϤāĻžāϏā§āϰ āύāĻŋāϰā§āĻĻāĻŋāώā§āĻ āĻāϤāĻŋ āĻ āĻĻāĻŋāĻ āĻĻā§āĻ-āĻ āĻāĻā§ (đĒī¸)āĨ¤
- đ Bookish Definition:
If to each point \((x, y, z)\) of a region in space there corresponds a vector \(\vec{F}(x, y, z)\), then \(\vec{F}\) is called a vector field.
Example: Wind velocity or gravitational force in space.
ā§Ģ. Dot Product / Scalar Product (āĻĄāĻ āĻā§āĻŖāύ)Âļ
- đ§ āĻā§āϰāĻŋāĻ: āĻāĻāĻ āϞāĻžāĻāύ⧠āĻāĻžā§āĻŋ āϧāĻžāĻā§āĻāĻž āĻĻā§āĻā§āĻž (Helper Rule)āĨ¤ āĻā§āĻŖāĻĢāϞ āĻšāĻŦā§ āĻāĻāĻāĻŋ āϏāĻžāϧāĻžāϰāĻŖ āϏāĻāĻā§āϝāĻžāĨ¤
- đ Bookish Definition:
The dot product of two vectors \(\vec{A}\) and \(\vec{B}\) is a scalar quantity defined as the product of the magnitudes of \(\vec{A}\) and \(\vec{B}\) and the cosine of the angle \(\theta\) between them.
$\(\vec{A} \cdot \vec{B} = \vert{}\vec{A}\vert{}\vert{}\vec{B}\vert{}\cos\theta\)$
ā§Ŧ. Cross Product / Vector Product (āĻā§āϰāϏ āĻā§āĻŖāύ)Âļ
- đ§ āĻā§āϰāĻŋāĻ: āĻšā§āϞāĻŋāĻāĻĒā§āĻāĻžāϰā§āϰ āĻĒāĻžāĻāĻž āĻā§āϰ⧠āĻĄāĻžāύā§-āĻŦāĻžāĻŽā§, āĻāĻŋāύā§āϤ⧠āĻšā§āϞāĻŋāĻāĻĒā§āĻāĻžāϰ āĻā§ā§ āϏā§āĻāĻž āĻāĻĒāϰ⧠(āϞāĻŽā§āĻŦāĻžāϞāĻŽā§āĻŦāĻŋ āύāϤā§āύ āĻĻāĻŋāĻ)āĨ¤
- đ Bookish Definition:
The cross product of two vectors \(\vec{A}\) and \(\vec{B}\) is a vector quantity whose magnitude is the product of their magnitudes and the sine of the angle \(\theta\) between them, and whose direction is perpendicular to the plane containing \(\vec{A}\) and \(\vec{B}\).
$\(\vec{A} \times \vec{B} = (\vert{}\vec{A}\vert{}\vert{}\vec{B}\vert{}\sin\theta)\hat{\eta}\)$
(Where \(\hat{\eta}\) is a unit vector perpendicular to the plane of \(\vec{A}\) and \(\vec{B}\).)
āĻā§āϝāĻžāĻĒā§āĻāĻžāϰ ā§Ŧ: āĻāύā§āĻāĻŋāĻā§āϰāĻžāϞ āĻĨāĻŋāĻāϰā§āĻŽāϏāĻŽā§āĻš (Dimension Shifting)## ā§. Gauss's Divergence Theorem (āĻāĻžāĻāϏā§āϰ āĻĄāĻžāĻāĻāĻžāϰāĻā§āύā§āϏ āĻĨāĻŋāĻāϰā§āĻŽ)Âļ
- đ§ āĻā§āϰāĻŋāĻ: āĻŦā§āϞā§āύā§āϰ ⧍D āĻāĻžāĻŽā§āĻž āĻĻāĻŋā§ā§ āĻŦāĻžāϤāĻžāϏ āĻŦā§āϰ āĻšāĻā§āĻž = āĻŦā§āϞā§āύā§āϰ ā§ŠD āĻā§āϤāϰā§āϰ āĻāϞāĻŋāĻāĻŽā§ āĻŦāĻžāϤāĻžāϏ āĻĸā§āĻāĻž (đ)āĨ¤
- đ Bookish Definition:
Let \(V\) be the volume bounded by a closed surface \(S\) and \(\vec{F}\) be a continuously differentiable vector field. Then the divergence theorem states that the surface integral of \(\vec{F}\) over \(S\) is equal to the volume integral of the divergence of \(\vec{F}\) over \(V\):
$\(\iint_S \vec{F} \cdot \hat{n} \, dS = \iiint_V (\nabla \cdot \vec{F}) \, dV\)$
ā§Ž. Stoke's Theorem (āϏā§āĻā§āĻāϏā§āϰ āĻĨāĻŋāĻāϰā§āĻŽ)Âļ
- đ§ āĻā§āϰāĻŋāĻ: āĻŦāĻžāĻāĻžāύā§āϰ ā§§D āϏā§āĻŽāĻžāύāĻž āĻŦāĻž āĻŦā§ā§āĻž āϧāϰ⧠āĻšāĻžāĻāĻāĻž = āĻŦāĻžāĻāĻžāύā§āϰ ⧍D āĻŽā§āĻā§āϰ āĻāĻĒāϰ āĻŦāĻžāϤāĻžāϏā§āϰ āĻā§āϰā§āĻŖāύ (Curl) āĻŽāĻžāĻĒāĻž (đĄ)āĨ¤
- đ Bookish Definition:
Let \(S\) be an open surface bounded by a closed curve \(C\), and \(\vec{F}\) be a continuously differentiable vector field. Then Stoke's theorem states that the line integral of \(\vec{F}\) around \(C\) is equal to the surface integral of the curl of \(\vec{F}\) over \(S\):
$\(\oint_C \vec{F} \cdot d\vec{r} = \iint_S (\nabla \times \vec{F}) \cdot \hat{n} \, dS\)$
⧝. Green's Theorem in the Plane (āϏāĻŽāϤāϞ⧠āĻā§āϰāĻŋāύā§āϰ āĻĨāĻŋāĻāϰā§āĻŽ)Âļ
- đ§ āĻā§āϰāĻŋāĻ: āϏā§āĻā§āĻāϏā§āϰ āĻĨāĻŋāĻāϰā§āĻŽāĻāĻžāĻ āϝāĻāύ āĻĨā§āϰāĻŋ-āĻĄāĻŋ āĻĻā§āύāĻŋā§āĻž āĻā§ā§ā§ āĻāĻžāϤāĻžāϰ āĻĒāĻžāϤāĻžāϰ āĻŽāϤ⧠āĻāĻāĻĻāĻŽ ⧍D āĻĢā§āϞā§āϝāĻžāĻ āϏāĻŽāϤāϞ⧠āĻāĻžāĻ āĻāϰā§āĨ¤
- đ Bookish Definition:
If \(P(x,y)\) and \(Q(x,y)\) are continuous functions having continuous partial derivatives in a region \(R\) bounded by a closed curve \(C\) in the \(xy\)-plane, then Green's theorem states:
$\(\oint_C (P \, dx + Q \, dy) = \iint_R \left( \frac{\partial Q}{\partial x} - \frac{\partial P}{\partial y} \right) dx \, dy\)$
Âļ
The given second-degree equation \(8x^2 + 4xy + 5y^2 - 24x - 24y = 0\) reduces to the standard form \(\frac{x'^2}{4} + \frac{y'^2}{9} = 1\), which represents an ellipse.Âļ
1. Identify Conic TypeÂļ
Compare the given equation with the general second-degree equation \(ax^2 + 2hxy + by^2 + 2gx + 2fy + c = 0\):
- \(a = 8, \quad h = 2, \quad b = 5\)
- \(g = -12, \quad f = -12, \quad c = 0\)
Calculate the discriminant \(h^2 - ab\):
$\(h^2 - ab = 2^2 - (8)(5) = 4 - 40 = -36\)$
Since \(h^2 - ab < 0\), the conic is an ellipse. [1]
2. Find the CenterÂļ
Differentiate the equation partially with respect to \(x\) and \(y\) to locate the center \((x_1, y_1)\):
$\(\frac{\partial F}{\partial x} = 16x + 4y - 24 = 0 \implies 4x + y = 6\)$
$\(\frac{\partial F}{\partial y} = 4x + 10y - 24 = 0 \implies 2x + 5y = 12\)$
Solving this linear system yields the center:
- \(x_1 = 1\)
- \(y_1 = 2\)
3. Shift the OriginÂļ
Shift the origin to the center \((1, 2)\) using \(x = X + 1\) and \(y = Y + 2\). The constant term transforms to \(c'\):
$\(c' = gx_1 + fy_1 + c = -12(1) - 12(2) + 0 = -36\)$
The intermediate equation without linear terms is:
$\(8X^2 + 4XY + 5Y^2 - 36 = 0 \implies 8X^2 + 4XY + 5Y^2 = 36\)$
4. Rotate the AxesÂļ
Eliminate the \(XY\) cross-product term by finding the eigenvalues (\(\lambda\)) of the characteristic matrix:
$\(\begin{vmatrix} a - \lambda & h \\ h & b - \lambda \end{vmatrix} = 0 \implies \begin{vmatrix} 8 - \lambda & 2 \\ 2 & 5 - \lambda \end{vmatrix} = 0\)$
$\(\lambda^2 - 13\lambda + 36 = 0 \implies (\lambda - 4)(\lambda - 9) = 0\)$
Thus, \(\lambda_1 = 4\) and \(\lambda_2 = 9\). The rotated equation becomes:
$\(\lambda_1 x'^2 + \lambda_2 y'^2 + c' = 0 \implies 4x'^2 + 9y'^2 = 36\)$
Divide through by \(36\) to obtain the final standard form:
$\(\frac{x'^2}{9} + \frac{y'^2}{4} = 1 \quad \text{or} \quad \frac{x'^2}{4} + \frac{y'^2}{9} = 1 \text{ (depending on axis ordering)}\)$
â Final AnswerÂļ
The standard form of the conic equation is \(\frac{x'^2}{4} + \frac{y'^2}{9} = 1\), which represents an ellipse with its center located at \((1, 2)\). [2]
If you would like to explore this further, let me know if you want to find:
- The eccentricity of this ellipse
- The coordinates of its foci or vertices
- The equations of its axes of symmetry
import numpy as np
Verify the matrix eigenvaluesA = np.array([[8, 2], [2, 5]])eigenvalues, eigenvectors = np.linalg.eigh(A)Âļ
print("Eigenvalues:", eigenvalues)
Verify center# 16x + 4y = 24# 4x + 10y = 24M = np.array([[16, 4], [4, 10]])B = np.array([24, 24])center = np.linalg.solve(M, B)Âļ
print("Center:", center)
Verify c'g, f, c = -12, -12, 0c_prime = g * center[0] + f * center[1] + cÂļ
print("c_prime:", c_prime)
