Vector Algebra: Fundamentals & Geometric Applications - Lecture Notes

Vector Algebra and Scalar Quantities

  • Definition of Physical Quantities:
    • Scalar Quantities: Physical quantities that have only magnitude.
    • Vector Quantities: Physical quantities that have both magnitude and direction and obey the laws of vector algebra (specifically vector addition) are called vectors.
    • The note emphasizes that having magnitude and direction alone is not sufficient; the laws of algebra must be followed (v⃗1+v⃗2\vec{v}_1 + \vec{v}_2).

Representation of a Vector

  • Visual Representation: A vector is represented by a directed line segment (an arrow).
  • Components of the Representation:
    • Tail (Initial Point): The starting point of the vector arrow.
    • Head (Terminal Point): The ending point or tip of the arrow.
    • Length of Arrow: Directly represents the magnitude of the vector.
    • Direction of Arrow: Represents the direction of the vector.
  • Symbolic Representation: A vector is typically denoted as a⃗\vec{a}. Its magnitude is denoted by ∣a⃗∣|\vec{a}|

Special Types of Vectors

  • Zero Vector (Null Vector):

    • Definition: A vector with zero magnitude where the initial and terminal points coincide.
    • Notation: Denoted by 0⃗\vec{0}.
    • Magnitude: ∣0⃗∣=0|\vec{0}| = 0.
    • Direction: The direction of a zero vector is considered arbitrary.
    • Properties:
      • x×0=0x \times 0 = 0 is analogous to k⋅0⃗=0⃗k \cdot \vec{0} = \vec{0}.
      • x+0=xx + 0 = x is analogous to a⃗+0⃗=a⃗\vec{a} + \vec{0} = \vec{a}.
      • x−0=xx - 0 = x is analogous to a⃗−0⃗=a⃗\vec{a} - \vec{0} = \vec{a}.
    • Example: A boy throwing a ball straight up and catching it back; the total displacement of the ball is a null vector.
  • Unit Vector:

    • Definition: A vector whose magnitude is exactly one unit.
    • Purpose: The primary concept of a unit vector is to impart direction to a physical quantity or to write a vector of a specific magnitude in a specific direction.
    • Formula: a^=a⃗∣a⃗∣\hat{a} = \frac{\vec{a}}{|\vec{a}|}.
    • Magnitude: ∣a^∣=1|\hat{a}| = 1.
    • Usage: To write a vector of magnitude 10 along a⃗\vec{a}, compute 10a^10\hat{a}.
  • Equal Vectors:

    • Two vectors are equal (a⃗=b⃗\vec{a} = \vec{b}) if and only if they meet three criteria:
      1. Same Magnitude: ∣a⃗∣=∣b⃗∣|\vec{a}| = |\vec{b}|
      2. Same Direction: The arrows must point the same way.
      3. Same Physical Quantity: They must represent the same type of physical phenomenon.
    • Line of Support: They must have the same or parallel lines of support.

Multiplication of Vectors by Scalars

  • Scalar Multiplication: If a⃗\vec{a} is a vector and mm is a scalar, then ma⃗m\vec{a} is a vector parallel to a⃗\vec{a} with a magnitude ∣m∣|m| times the magnitude of a⃗\vec{a}.
  • Mathematical Properties:
    • m(a⃗)=(a⃗)m=ma⃗m(\vec{a}) = (\vec{a})m = m\vec{a}
    • Associative: m(na⃗)=n(ma⃗)=(mn)a⃗m(n\vec{a}) = n(m\vec{a}) = (mn)\vec{a}
    • Distributive over Vector Addition: m(a⃗+b⃗)=ma⃗+mb⃗m(\vec{a} + \vec{b}) = m\vec{a} + m\vec{b}
    • Distributive over Scalar Addition: (m+n)a⃗=ma⃗+na⃗(m + n)\vec{a} = m\vec{a} + n\vec{a}
  • Important Rule: ∣ka⃗∣=∣k∣∣a⃗∣|k\vec{a}| = |k| |\vec{a}|
    • Example: For −2a⃗-2\vec{a}, the magnitude is ∣−2∣∣a⃗∣=2∣a⃗∣|-2| |\vec{a}| = 2|\vec{a}|

Kaam ki Baat: Unit Vectors in Space

  • Perpendicular to a Given Plane: There are exactly 2 distinct unit vectors perpendicular to a given plane (one pointing upward and one downward).
  • Parallel to a Given Plane: There are infinitely many unit vectors parallel to a given plane.
  • Perpendicular to a Given Line: In 3D space, there are infinitely many distinct unit vectors perpendicular to a given line (forming a disk/plane of vectors around the line).

Localized (Bound) vs. Free Vectors

  • In Mathematics:
    • A vector is viewed as a "directed line segment."
    • We primarily deal with Free Vectors. A free vector can be translated parallel to itself in space without changing its identity or effect. Example: Velocity.
  • In Physics:
    • Localized or Bound Vectors are common. These are vectors where the point of application matters. Moving the vector parallel to itself changes its physical effect. Example: Force.

Collinear (Parallel) Vectors

  • Definition: Two vectors are collinear if their directed line segments are parallel, regardless of their individual directions.
  • Classification:
    • Like Parallel Vectors: Same direction (K>0K > 0).
    • Unlike Parallel Vectors: Opposite directions (K<0K < 0).
  • Mathematical Condition: Two non-zero vectors a⃗\vec{a} and b⃗\vec{b} are collinear if and only if a⃗=Kb⃗\vec{a} = K\vec{b} for some scalar K∈RK \in \mathbb{R}.

Golden Result (G1): Non-Collinear Vectors

  • Theorem: If a⃗\vec{a} and b⃗\vec{b} are two non-zero, non-collinear vectors, then:     xa⃗+yb⃗=0⇒x=0 and y=0x\vec{a} + y\vec{b} = 0 \Rightarrow x = 0 \text{ and } y = 0
  • Proof by Contradiction:
    • Assume x≠0x \neq 0.
    • Then xa⃗=−yb⃗⇒a⃗=(−yx)b⃗x\vec{a} = -y\vec{b} \Rightarrow \vec{a} = (-\frac{y}{x})\vec{b}.
    • This implies a⃗=λb⃗\vec{a} = \lambda\vec{b}, meaning a⃗\vec{a} and b⃗\vec{b} are collinear, which contradicts the initial condition.
  • General Application: If x1a⃗+y1b⃗=x2a⃗+y2b⃗x_1\vec{a} + y_1\vec{b} = x_2\vec{a} + y_2\vec{b}, then x1=x2x_1 = x_2 and y1=y2y_1 = y_2.

Golden Result (G2): The Median Vector

  • Theorem: In triangle ABCABC, if ADAD is the median from vertex AA to side BCBC, then:     AB⃗+AC⃗=2AD⃗\vec{AB} + \vec{AC} = 2\vec{AD}
  • Parallelogram Law Connection: The sum of two vectors emanating from a vertex (AB⃗,AC⃗\vec{AB}, \vec{AC}) is equal to twice the median vector drawn to the opposite side.
  • Extensions:
    • BA⃗+BC⃗=2BE⃗\vec{BA} + \vec{BC} = 2\vec{BE} (where BEBE is the median to ACAC).
    • CA⃗+CB⃗=2CF⃗\vec{CA} + \vec{CB} = 2\vec{CF} (where CFCF is the median to ABAB).

Position Vectors and Coordinate Geometry

  • Definition: The position vector of a point PP relative to a fixed origin OO is denoted as OP⃗\vec{OP}, or simplified as p⃗\vec{p}.
  • Difference Vector: For any two points AA and BB in space:     AB⃗=Position Vector of B−Position Vector of A\vec{AB} = \text{Position Vector of } B - \text{Position Vector of } APQ⃗=OQ⃗−OP⃗\vec{PQ} = \vec{OQ} - \vec{OP}
  • Coordinates in 3D: If point PP has coordinates (x,y,z)(x, y, z), its position vector is:     OP⃗=xi^+yj^+zk^\vec{OP} = x\hat{i} + y\hat{j} + z\hat{k}
  • Magnitude in 3D: The length of the vector OP⃗\vec{OP} is:     ∣OP⃗∣=x2+y2+z2|\vec{OP}| = \sqrt{x^2 + y^2 + z^2}

Section Formula

  • Internal Division: If point PP divides the line segment joining A(a⃗)A(\vec{a}) and B(b⃗)B(\vec{b}) internally in the ratio m:nm:n:     r⃗=mb⃗+na⃗m+n\vec{r} = \frac{m\vec{b} + n\vec{a}}{m+n}
    • Midpoint Formula (when m=nm=n): r⃗=a⃗+b⃗2\vec{r} = \frac{\vec{a} + \vec{b}}{2}
  • External Division: If point PP divides the segment externally in the ratio m:nm:n:     r⃗=mb⃗−na⃗m−n\vec{r} = \frac{m\vec{b} - n\vec{a}}{m - n}
  • General Coordinate Relation: If r⃗=αi^+βj^+γk^\vec{r} = \alpha\hat{i} + \beta\hat{j} + \gamma\hat{k}, then:     α=mx2+nx1m+n,β=my2+ny1m+n,γ=mz2+nz1m+n\alpha = \frac{mx_2 + nx_1}{m+n}, \quad \beta = \frac{my_2 + ny_1}{m+n}, \quad \gamma = \frac{mz_2 + nz_1}{m+n}

Position Vectors of Important Triangle Centers

  • Centroid (GG): The point of intersection (POI) of medians.     g⃗=α⃗+β⃗+γ⃗3\vec{g} = \frac{\vec{\alpha} + \vec{\beta} + \vec{\gamma}}{3}
  • Incentre (II): The POI of internal angle bisectors.     i⃗=aα⃗+bβ⃗+cγ⃗a+b+c\vec{i} = \frac{a\vec{\alpha} + b\vec{\beta} + c\vec{\gamma}}{a+b+c}
    • where a,b,ca, b, c are the lengths of the sides opposite to vertices A,B,CA, B, C.
  • Circumcentre (OO): The POI of perpendicular bisectors of sides.     O⃗circum=α⃗sin⁡(2A)+β⃗sin⁡(2B)+γ⃗sin⁡(2C)sin⁡(2A)+sin⁡(2B)+sin⁡(2C)\vec{O}_{circum} = \frac{\vec{\alpha} \sin(2A) + \vec{\beta} \sin(2B) + \vec{\gamma} \sin(2C)}{\sin(2A) + \sin(2B) + \sin(2C)}
  • Orthocentre (HH): The POI of altitudes.     h⃗=α⃗tan⁡(A)+β⃗tan⁡(B)+γ⃗tan⁡(C)tan⁡(A)+tan⁡(B)+tan⁡(C)\vec{h} = \frac{\vec{\alpha} \tan(A) + \vec{\beta} \tan(B) + \vec{\gamma} \tan(C)}{\tan(A) + \tan(B) + \tan(C)}
  • Euler Line Property: In any triangle, the Orthocentre (HH), Centroid (GG), and Circumcentre (OO) are collinear. The Centroid (GG) divides the segment HOHO in the ratio 2:12:1.

Solved Classroom Problems

  • Problem 1: Length of Median

    • Given sides: AB⃗=3i^+4k^\vec{AB} = 3\hat{i} + 4\hat{k} and AC⃗=5i^−2j^+4k^\vec{AC} = 5\hat{i} - 2\hat{j} + 4\hat{k}.
    • Formula: 2AD⃗=AB⃗+AC⃗=(3+5)i^+(−2)j^+(4+4)k^=8i^−2j^+8k^2\vec{AD} = \vec{AB} + \vec{AC} = (3+5)\hat{i} + (-2)\hat{j} + (4+4)\hat{k} = 8\hat{i} - 2\hat{j} + 8\hat{k}.
    • AD=4i^−j^+4k^AD = 4\hat{i} - \hat{j} + 4\hat{k}.
    • Length: ∣AD⃗∣=42+(−1)2+42=16+1+16=33|\vec{AD}| = \sqrt{4^2 + (-1)^2 + 4^2} = \sqrt{16 + 1 + 16} = \sqrt{33}.
  • Problem 2: Unit Vectors Perpendicular to two given vectors

    • Given: a⃗(1,1,0)\vec{a}(1, 1, 0) and b⃗(0,1,1)\vec{b}(0, 1, 1).
    • The number of unit length vectors perpendicular to two non-parallel vectors in space is 2.
  • Problem 3: Linear Independence/Collinearity

    • Given: a⃗,b⃗,c⃗\vec{a}, \vec{b}, \vec{c} are non-zero, no two collinear. If a⃗+b⃗\vec{a} + \vec{b} is collinear with c⃗\vec{c} and b⃗+c⃗\vec{b} + \vec{c} is collinear with a⃗\vec{a}.
    • Equations: a⃗+b⃗=λc⃗\vec{a} + \vec{b} = \lambda\vec{c} and b⃗+c⃗=μa⃗\vec{b} + \vec{c} = \mu\vec{a}.
    • Through substitution and comparing non-collinear components: λ=−1\lambda = -1 and μ=−1\mu = -1.
    • Result: a⃗+b⃗+c⃗=0⃗\vec{a} + \vec{b} + \vec{c} = \vec{0}.
  • Problem 4: Collinear Points (JEE Mains 2023)

    • Given Points: A(α,10,13)A(\alpha, 10, 13), B(6,11,11)B(6, 11, 11), C(92,β,−8)C(\frac{9}{2}, \beta, -8).
    • Method: Vectors AB⃗\vec{AB} and BC⃗\vec{BC} must be collinear (AB⃗=KBC⃗\vec{AB} = K\vec{BC}).
    • AB⃗=(6−α)i^+j^−2k^\vec{AB} = (6-\alpha)\hat{i} + \hat{j} - 2\hat{k}.
    • BC⃗=−32i^+(β−11)j^−19k^\vec{BC} = -\frac{3}{2}\hat{i} + (\beta-11)\hat{j} - 19\hat{k}.
    • Comparing components: 6−α−3/2=1β−11=−2−19\frac{6-\alpha}{-3/2} = \frac{1}{\beta-11} = \frac{-2}{-19}.
    • Calculated values: 19α=11719\alpha = 117 and 6β=1236\beta = 123.
    • Result: (19α−6β)2=(117−123)2=(−6)2=36(19\alpha - 6\beta)^2 = (117 - 123)^2 = (-6)^2 = 36.
  • Problem 5: Component Rotation (JEE Mains 2021)

    • Vector comp in Rectangular system: (3p,1)(3p, 1).
    • Vector comp in Rotated system: (p+1,10)(p+1, \sqrt{10}).
    • Property: Magnitude remains invariant under rotation.
    • Equation: (3p)2+12=(p+1)2+(10)2⇒9p2+1=p2+2p+1+10(3p)^2 + 1^2 = (p+1)^2 + (\sqrt{10})^2 \Rightarrow 9p^2 + 1 = p^2 + 2p + 1 + 10.
    • 8p2−2p−10=0⇒4p2−p−5=08p^2 - 2p - 10 = 0 \Rightarrow 4p^2 - p - 5 = 0.
    • Roots: p=−1,54p = -1, \frac{5}{4}.

Question & Discussion (TAH and KTK Solutions)

Differential Equations (Revision Practice)

  • TAH 1(a) (Solution by Tushar Verma): Radium decay rate dmdt=−km\frac{dm}{dt} = -km. Resulting law: m=m0(1−α100)t/t0m = m_0(1 - \frac{\alpha}{100})^{t/t_0}.
  • TAH 1(b) (Solution by Rohit Patil): Solve d2ydx2=e2x+ex+2014\frac{d^2y}{dx^2} = e^{2x} + e^x + 2014.
    • Integrating once: dydx=12e2x+ex+2014x+C1\frac{dy}{dx} = \frac{1}{2}e^{2x} + e^x + 2014x + C_1.
    • Final solution: y=14e2x+ex+1007x2+C1x+C2y = \frac{1}{4}e^{2x} + e^x + 1007x^2 + C_1x + C_2.
  • TAH 1(c) (Solution by Tushar Verma/Rohit Patil): Solve d2ydx2=sin⁡2(x)=1−cos⁡(2x)2\frac{d^2y}{dx^2} = \sin^2(x) = \frac{1 - \cos(2x)}{2}.
    • Integrations yield: y=x24+cos⁡(2x)8+C1x+C2y = \frac{x^2}{4} + \frac{\cos(2x)}{8} + C_1x + C_2.
  • TAH 1(d) (Solution by Tushar Verma/Rohit Patil): Solve d2ydx2=14y\frac{d^2y}{dx^2} = \frac{1}{4\sqrt{y}}.
    • Using identity 2dydxd2ydx2=ddx(dydx)22\frac{dy}{dx}\frac{d^2y}{dx^2} = \frac{d}{dx}(\frac{dy}{dx})^2.
    • (dydx)2=y+C1(\frac{dy}{dx})^2 = \sqrt{y} + C_1.
  • TAH 2(a) (Solution by Aditya Singh Tomar): (1+e2x)(dydx+y)=1(1+e^{2x})(\frac{dy}{dx} + y) = 1. Passing through (0,2)(0, 2).
    • Linear differential equation form leads to exy=arctan⁡(ex)+Ce^x y = \arctan(e^x) + C.
    • Limiting value: lim⁡x→∞exy=3π4\lim_{x \to \infty} e^x y = \frac{3\pi}{4}.
  • TAH 3 (Solution by Aditya Singh Tomar): f′(x)=2−f(x)xf'(x) = 2 - \frac{f(x)}{x}.
    • Solving as linear differential equation gives f(x)=x+cxf(x) = x + \frac{c}{x}.
    • Limits check: lim⁡x→0+x2f′(x)=0\lim_{x \to 0^+} x^2 f'(x) = 0.
  • TAH 4 (Solution by Pranay Thakur): Solution of dydx=−x2+3y23x2+y2\frac{dy}{dx} = -\frac{x^2 + 3y^2}{3x^2 + y^2} with y(1)=0y(1) = 0.
    • Result: log⁡e∣x+y∣+2xy(x+y)2=0\log_e |x+y| + \frac{2xy}{(x+y)^2} = 0.
  • TAH 8 (Solution by Himanshu Saini): Solve xlog⁡(x)dydx+y=x2log⁡(x)x \log(x) \frac{dy}{dx} + y = x^2 \log(x).
    • Integrating factor I.F.=log⁡(x)I.F. = \log(x).
    • Solution: ylog⁡(x)=x24(2log⁡(x)−1)+1y \log(x) = \frac{x^2}{4}(2 \log(x) - 1) + 1.
    • Value at x=ex=e: y(e)=e2+44y(e) = \frac{e^2+4}{4}.
  • KTK 1 (Solution by Prithvi Raj): 2x2ydydx−(1−xy2)=02x^2 y \frac{dy}{dx} - (1 - xy^2) = 0.
    • Substitution y2=zy^2 = z. Solution relates to form αx=exp⁡(xβyγ)\alpha x = \exp(x^{\beta} y^{\gamma}).
    • Result: α+β−γ=1\alpha + \beta - \gamma = 1.
  • KTK 5 (Solution by Rohit Patil): (1+x2)dy=y(x−y)dx(1+x^2)dy = y(x-y)dx, y(0)=1y(0)=1.
    • Bernoulli equation solved by setting z=1/yz = 1/y.
    • Solution involves e3β−1=e(3+22)e^{3\beta - 1} = e^{(3 + 2\sqrt{2})}.