Vectors are mathematical quantities that possess both magnitude and direction, obeying specific laws of vector addition (such as the Triangle Law and Parallelogram Law).
Basic Vector Terminologies:
Null Vector (Zero Vector): A vector having zero magnitude (∣A∣=0) and an arbitrary direction. It represents the result of subtracting a vector from itself.
Unit Vector: A dimensionless vector of unit magnitude (∣A^∣=1) that specifies direction. It is calculated by dividing a vector by its magnitude: A^=∣A∣A
Equal Vectors: Two or more vectors are equal (A=B) if and only if they possess identical magnitudes and point in the exact same direction.
Axial Vectors: Vectors associated with rotational motion (such as angular velocity ω, angular acceleration α, and torque τ) whose directions are specified along the axis of rotation using the right-hand screw rule.
Vector Orientations:
Orthogonal Vectors: Two vectors A and B positioned at an angle of θ=90∘. Their dot product is zero (A⋅B=0).
Parallel Vectors: Two vectors positioned at an angle of θ=0∘. They satisfy A=nB, where n is a positive scalar.
Anti-Parallel Vectors: Two vectors positioned at an angle of θ=180∘. They satisfy A=−nB, where n is a positive scalar.
Resolution of a Vector in Two Dimensions:
Any vector V lying in the XY plane can be decomposed into two mutually perpendicular components along the X-axis and Y-axis: V=Vxi^+Vyj^
If α is the angle made by V with the X-axis: Vx=Vcos(α)Vy=Vsin(α)
The magnitude of the vector is given by: ∣V∣=Vx2+Vy2
The direction angle α is determined by: tan(α)=VxVy
Arithmetic Vector Operations:
Given two vectors A=a1i^+b1j^+c1k^ and B=a2i^+b2j^+c2k^:
Expressed in determinant form: A×B=i^a1a2j^b1b2k^c1c2=i^(b1c2−c1b2)+j^(c1a2−a1c2)+k^(a1b2−b1a2)
Fundamental unit vector relationships: i^×i^=j^×j^=k^×k^=0i^×j^=k^,j^×k^=i^,k^×i^=j^j^×i^=−k^,k^×j^=−i^,i^×k^=−j^
Fundamental Vector Addition Laws:
Triangle Law of Vector Addition: If two vectors are represented in magnitude and direction by two sides of a triangle taken in the same order, their resultant is represented by the third side taken in the reverse order.
Parallelogram Law of Vector Addition: If two vectors A and B acting simultaneously at a point are represented in magnitude and direction by two adjacent sides of a parallelogram, their resultant R is given by the diagonal passing through their common point: R=A2+B2+2ABcos(θ)
The angle α that the resultant R makes with vector A is calculated using: tan(α)=A+Bcos(θ)Bsin(θ)
Lami's Theorem: For three coplanar, concurrent, and balanced (equilibrium) forces F1, F2, and F3 making angles α, β, and γ opposite to them respectively: sin(α)F1=sin(β)F2=sin(γ)F3
MOTION WITH UNIFORM ACCELERATION IN A PLANE
Consider a point object moving in the XY plane with a constant acceleration a. Let origin 'O' measure time and position.
At instant t1=0, let the initial position vector be r0 and initial velocity be u. At instant t2=t, let the final position vector be r and final velocity be v.
Initial Velocity: u=uxi^+uyj^, with magnitude u=ux2+uy2
Final Velocity: v=vxi^+vyj^, with magnitude v=vx2+vy2
Acceleration: a=axi^+ayj^, with magnitude a=ax2+ay2
Kinematic Equations per Axis:
Velocity components: vx=ux+axtvy=uy+ayt
Position coordinates / Displacements: x−x0=uxt+21axt2y−y0=uyt+21ayt2
HORIZONTAL PROJECTILE MOTION
A body projected horizontally with an initial velocity u from a height h above ground level describes a parabolic path under the sole influence of gravity.
Motion Components:
Horizontal direction (X-axis): Initial velocity ux=u, Acceleration ax=0.
Vertical direction (Y-axis): Initial velocity uy=0, Acceleration ay=g (downwards). sssssssss
Key Parameters of Horizontal Projectile:
Time of descent (t): h=21gt2⟹t=g2h
The time of descent is completely independent of the horizontal initial velocity u.
Horizontal Range (R): R=uxt=ug2h
Speed at any time t (v): vx=u,vy=gt=2ghv=vx2+vy2=u2+g2t2=u2+2gh
Striking angle with the horizontal (θ): tan(θ)=vxvy=ugt=u2gh
Angle of elevation of projection point from landing point (α): tan(α)=Rh=ug2hh=2ugt=2tan(θ)
Equation of Trajectory: x=ut⟹t=uxy=21gt2=21g(ux)2=2u2gx2
This represents a standard vertical parabola.
OBLIQUE PROJECTILE MOTION
An oblique projectile is any body projected into the air with an initial velocity u making an angle θ (θ=0∘,90∘) with the horizontal, moving freely under gravity.
Basic Assumptions:
Air resistance is neglected.
The curvature and rotation of the earth are neglected.
Acceleration due to gravity (g) is constant in magnitude (9.8m/s2 or 10m/s2) and direction at all points of motion.
Velocity Components and Motion Equations:
Horizontal component: ux=ucos(θ), remains constant throughout flight because ax=0
Vertical component: uy=usin(θ), varies continuously at rate ay=−g
Velocity components at time t: vx=ucos(θ)vy=usin(θ)−gt
Resultant speed at time t: v=vx2+vy2=u2cos2(θ)+(usin(θ)−gt)2=u2+g2t2−2ugtsin(θ)
Direction of velocity at time t relative to horizontal: tan(α)=vxvy=ucos(θ)usin(θ)−gt
Displacements at time t: x=(ucos(θ))ty=(usin(θ))t−21gt2S=x2+y2
Equation of Trajectory: y=xtan(θ)−2u2cos2(θ)gx2=xtan(θ)(1−Rx)
Expressed in polynomial form y=Ax−Bx2 where: A=tan(θ)B=2u2cos2(θ)g
Parameters derived from coefficients A and B: θ=tan−1(A)Range R=BAMaximum Height H=4BA2
Time Parameters of Flight:
Time of ascent (ta) = Time of descent (td) = gusin(θ)
Total Time of Flight (T): T=ta+td=g2usin(θ)
Maximum Height (H): H=2gu2sin2(θ)
At maximum height, vertical component vy=0
Speed is non-zero and at its minimum: vmin=vx=ucos(θ)
Angle between velocity vector v and acceleration vector g at maximum height is exactly 90∘
Horizontal Range (R): R=uxT=(ucos(θ))(g2usin(θ))=gu2sin(2θ)
Maximum horizontal range occurs at projection angle θ=45∘: Rmax=gu2
At maximum range (θ=45∘), maximum height is: H=2gu2sin2(45∘)=4gu2=4Rmax
General relationship between Range and Maximum Height: tan(θ)=R4H⟹R=4Hcot(θ)
When Range equals Maximum Height (R=H): tan(θ)=4⟹θ=tan−1(4)≈76∘
Complementary Angles of Projection:
Two bodies thrown with identical speed u at complimentary angles θ1=θ and θ2=90∘−θ (or 45∘+θ and 45∘−θ) possess identical horizontal ranges: R1=R2=R
Ratios and relationships for complementary projections: T2T1=tan(θ)T1T2=g2usin(θ)⋅g2ucos(θ)=g2R⟹R=21gT1T2H1+H2=2gu2sin2(θ)+2gu2cos2(θ)=2gu2H2H1=tan2(θ)H1H2=4g2u4sin2(θ)cos2(θ)=16R2⟹R=4H1H2
Angles Between Velocity and Acceleration:
During ascent (rising phase): 90∘<θ<180∘
At peak position: θ=90∘
During descent (falling phase): 0∘<θ<90∘
Energy Relations in Oblique Motion:
Initial Kinetic Energy at point of projection: KE0=21mu2
Range along the incline (R): R=gcos2(β)u2[sin(2α+β)+sin(β)]
Maximum Range Condition (Down the plane): 2α+β=2π⟹α=4π−2βRmax=g(1−sin(β))u2
Time of flight T′ corresponding to maximum range: T′=g2Rmax
RELATIVE MOTION IN TWO DIMENSIONS
The motion of a particle P relative to a particle Q in a 2D plane is defined by their vector velocity difference: vP/Q=vP−vQ where vP is the velocity of P w.r.t ground and vQ is the velocity of Q w.r.t ground.
Relative Acceleration: aP/Q=aP−aQ
Relative Displacement: rP/Q=rP−rQ
RAIN-MAN RELATIVE MOTION
When rain is falling downwards with velocity vR and a man moves horizontally with velocity vM, the apparent velocity of rain relative to the man is: vRM=vR−vM
Geometry and Calculation:
If rain falls vertically w.r.t ground (vR=−vRj^) and the man moves east (vM=vMi^): vRM=−vMi^−vRj^vRM=vR2+vM2
Direction to hold umbrella (angle θ with vertical): tan(θ)=∣vR∣∣vM∣=vRvM
Analytical Problem Case Study (Rain-Man):
Scenario: A person in a stationary vehicle holds an umbrella at 60∘ with the vertical. Driving at 20m/s, raindrops appear to fall vertically.
Mathematical breakdown:
When stationary, θ=60∘⟹tan(60∘)=vRvM′=3.
When driving at vM=20m/s, relative rain velocity vRM is vertical.
From vector triangle: sin(60∘)=vRvM⟹23=vR20⟹vR=340m/s
Angular Displacement (θ): Angle turned by the radius vector. Measured in radians (rad).
Small angular displacements (dθ) are vector quantities; finite angular displacements are scalar quantities as they fail vector addition commutativity. θ=radius (r)arc length (l)
Angular Velocity (ω): Rate of change of angular displacement. ω=dtdθ
S.I. Unit: rads−1.
Period (T) and Frequency (f) relations: ω=T2π=2πf
Unit Conversions: 1rps=60rpm=2πrads−11rpm=30πrads−1
Angular Acceleration (α): Rate of change of angular velocity. α=dtdω=dt2d2θ
S.I. Unit: rads−2.
Vector Relations between Linear and Angular Quantities: v=ω×rv=ωr
The directions of v, ω, and r are mutually perpendicular:
v lies along the tangent in the plane of rotation.
ω lies along the axis of rotation perpendicular to the orbital plane.
r lies along the radius vector radially outwards from center.
Equations of Rotational Motion (Constant Angular Acceleration α): ω=ω0+αtθ=ω0t+21αt2ω2−ω02=2αθ
Uniform Circular Motion (UCM):
Motion of a particle along a circular path at constant speed (v = constant).
Scalar quantities that remain constant: Speed, Kinetic Energy, Time Period, Frequency, Angular Speed (ω), Magnitude of Centripetal Acceleration, Magnitude of Centripetal Force.
Vector quantities that continuously change (due to changing direction): Linear Velocity, Centripetal Acceleration, Centripetal Force, Linear Momentum.
Accelerations in Circular Motion:
Centripetal (Radial) Acceleration (ar):
Arises from continuous change in the direction of velocity vector. Directed radially inwards toward the center. ar=ω×v=ω×(ω×r)ar=rv2=ω2r=vω
Tangential Acceleration (at):
Arises from change in magnitude of linear speed (v). Directed along tangent to circle. at=dtdv=αr
Total / Net Acceleration (anet): anet=ar+atanet=ar2+at2=(rv2)2+(αr)2
Classification based on acceleration components:
If at=0,ar=0: Uniform linear motion.
If at=0,ar=0: Uniform circular motion.
If at=0,ar=0: Accelerated linear motion.
If at=0,ar=0: Non-uniform circular motion.
Dynamics of Circular Motion:
Centripetal Force (Fc): Real inward force required to maintain circular motion. Fc=mar=rmv2=mω2r
Work done by centripetal force is strictly zero (W=0) because instantaneous force is perpendicular to velocity (Fc⋅v=0).
Centripetal force is not an additional force; it is provided by physical forces (tension, gravity, normal force, friction).
Example: Mass m attached to string of length l revolved in vertical circle: At lowest position, net force T−mg=lmv2⟹T=mg+lmv2.
Centrifugal Force:
A pseudo force felt in a rotating (non-inertial) frame of reference. Directed radially outwards.
Magnitude Fcf=mω2r=rmv2.
Centripetal and centrifugal forces do not form an action-reaction pair because they are defined in different reference frames.
ANALYTICAL PROBLEMS AND DETAILED DERIVATIONS
Problem 1: Projection at 45∘ with initial speed u=202m/s (g=10m/s2).
Range (R): R=gu2sin(2θ)=10(202)2sin(90∘)=10800×1=80m
Maximum Height (H): H=2gu2sin2(θ)=20800×(1/2)2=20400=20m
Time of Flight (T): T=g2usin(θ)=102×202×(1/2)=4s
Problem 2: Particle thrown from tower of height 40m at angle 45∘ with initial speed u=202m/s (g=10m/s2).
Problem 3: Stone whirled horizontally at height 2.9m on radius 1.5m. String breaks, stone travels horizontal distance 10m as horizontal projectile (g=9.8m/s2).
Flight time: h=21gt2⟹2.9=4.9t2⟹t=4.92.9≈0.769s
Horizontal launch speed: u=tR=5.8/9.810≈13m/s
Centripetal acceleration in circular track: ar=ru2=1.5132=1.5169≈43m/s2
Problem 4: Relative rotation of concentric particles A and B (TA=3min, TB=1min).