Comprehensive Study Notes on Kinematics and Dynamics of Circular Motion

Translational Motion and Angular Variables

  • Position Vector and Polar Coordinates:

    • The position of a particle PP in a plane can be completely specified by its position vector r⃗\vec{r}.
    • The position vector is defined by its magnitude r=OPr = OP (the distance from origin OO to particle PP) and its orientation relative to a fixed reference direction, given by the coordinate angle θ\theta measured from the positive x-axis.
    • The ordered pair (r,θ)(r, \theta) defines the polar coordinates of the particle.
  • Types of Particle Motion in Polar Coordinates:

    • Radial Motion Outward: The particle moves directly away from the origin; magnitude rr increases while angle θ\theta remains constant.
    • Radial Motion Inward: The particle moves directly toward the origin; magnitude rr decreases while angle θ\theta remains constant.
    • Circular Motion Centered at Origin: The particle moves along a circular arc of constant radius rr; only the coordinate angle θ\theta changes with time tt
    • General Motion: If a particle moves on any path other than a radial line or a circle centered at the origin, both coordinates rr and θ\theta vary with time tt
  • Definitions of Angular Variables:

    • Angular Motion: Defined as any change in the direction of position vector r⃗\vec{r}. This occurs whenever a particle moves on a curvilinear path or a straight-line path that does not pass through the origin.
    • Angular Position (θ\theta): The coordinate angle θ\theta made by the position vector r⃗\vec{r} with a reference line at a specific instant.
    • Angular Displacement (Δθ\Delta \theta): The net change in angular position during a specified time interval Δt=t2−t1\Delta t = t_2 - t_1:     Δθ=θ2−θ1\Delta \theta = \theta_2 - \theta_1
    • Angular Velocity (ω\omega): The instantaneous rate of change of angular position θ\theta with respect to time tt:     ω=dθdt\omega = \frac{d\theta}{dt}
    • Angular Acceleration (α\alpha): The instantaneous rate of change of angular velocity ω\omega with respect to time tt:     α=dωdt=d2θdt2=ωdωdθ\alpha = \frac{d\omega}{dt} = \frac{d^2\theta}{dt^2} = \omega \frac{d\omega}{d\theta}
  • Sign Convention and Analogy to Rectilinear Motion:

    • In planar motion, the position vector turns either clockwise or anticlockwise.
    • Assigning one rotational sense as positive and the opposite as negative allows angular kinematic problems involving θ\theta, ω\omega, and α\alpha to be solved using equations directly analogous to 1D rectilinear kinematic problems involving position xx, velocity vv, and acceleration aa

Kinematics of Circular Motion

  • Radius Vector and Path Geometry:

    • In circular translational motion, a particle PP moves along a circular path of constant radius rr.
    • The position vector r⃗=OP⃗\vec{r} = \vec{OP} originating from the center of the circle OO is termed the radius vector.
    • The radius vector is always normal (perpendicular) to the circular path, maintains a constant magnitude rr, and rotates such that its angle θ(t)\theta(t) varies continuously.
  • Classification of Angular Motion:

    • Motion with Uniform Angular Velocity:
    • Characterized by constant angular velocity ω\omega and zero angular acceleration (α=0\alpha = 0).
    • Analogy to uniform rectilinear motion:       θ=θ0+ωt\theta = \theta_0 + \omega t
    • Motion with Uniform Angular Acceleration:
    • Characterized by constant angular acceleration (α=constant\alpha = \text{constant}).
    • Kinematic equations of motion:       ω=ω0+αt\omega = \omega_0 + \alpha tθ=θ0+ω0t+12αt2\theta = \theta_0 + \omega_0 t + \frac{1}{2} \alpha t^2θ=θ0+(ω0+ω2)t\theta = \theta_0 + \left(\frac{\omega_0 + \omega}{2}\right) tω2=ω02+2α(θ−θ0)\omega^2 = \omega_0^2 + 2\alpha(\theta - \theta_0)
    • Motion with Variable Angular Acceleration:
    • Angular acceleration α\alpha is specified as a function of time α(t)\alpha(t), position α(θ)\alpha(\theta), or angular velocity α(ω)\alpha(\omega).
    • Solutions require direct integration or differentiation calculus techniques analogous to variable acceleration in straight-line motion.
  • Linear Velocity and Acceleration Components:

    • Arc Length: Arc length ss covered along the circle is related to angular displacement θ\theta by:     s=rθs = r \theta
    • Linear Speed (vv): Differentiating arc length ss with respect to time tt gives the linear speed:     v=dsdt=rdθdt=ωrv = \frac{ds}{dt} = r \frac{d\theta}{dt} = \omega r
    • Direction of Velocity: Linear velocity v⃗\vec{v} is directed tangentially along the path at every instant.
    • Uniform Circular Motion (UCM):
    • Speed vv is constant, but velocity vector v⃗\vec{v} continuously changes direction.
    • The change in velocity over an infinitesimal interval dtdt is perpendicular to v⃗\vec{v} and points directly toward the center of the path.
    • Infinitesimal velocity magnitude change: ∣dv⃗∣=v dθ|d\vec{v}| = v \, d\theta
    • Centripetal (Normal) Acceleration (aca_c or ana_n):       an=ac=∣dv⃗∣dt=vdθdt=vω=v2r=ω2ra_n = a_c = \frac{|d\vec{v}|}{dt} = v \frac{d\theta}{dt} = v \omega = \frac{v^2}{r} = \omega^2 r
    • Non-Uniform Circular Motion:
    • Speed vv changes with time, giving rise to two perpendicular acceleration components:
      1. Tangential Acceleration (ata_t): Accounts for the rate of change of speed:          at=dvdt=rdωdt=rαa_t = \frac{dv}{dt} = r \frac{d\omega}{dt} = r \alpha
      2. Normal/Centripetal Acceleration (ana_n): Accounts for the rate of change of velocity direction:          an=v2r=ω2ra_n = \frac{v^2}{r} = \omega^2 r
    • Total Linear Acceleration (aa):       a=at2+an2a = \sqrt{a_t^2 + a_n^2}
    • Angle β\beta made by the total acceleration vector a⃗\vec{a} with the radius vector:       tan⁡(β)=atan\tan(\beta) = \frac{a_t}{a_n}
  • Worked Examples and Solutions:

    • Illustration 1: Angular position varies as θ=t3−3t2+4t−2\theta = t^3 - 3t^2 + 4t - 2 (in radians, tt in seconds). Find average angular acceleration αavg\alpha_{avg} between t=2 st = 2\,s and t=4 st = 4\,s
    • Instantaneous angular velocity: ω(t)=dθdt=3t2−6t+4\omega(t) = \frac{d\theta}{dt} = 3t^2 - 6t + 4
    • At t=2 st = 2\,s: ω2=3(2)2−6(2)+4=4 rad/s\omega_2 = 3(2)^2 - 6(2) + 4 = 4\,rad/s
    • At t=4 st = 4\,s: ω4=3(4)2−6(4)+4=28 rad/s\omega_4 = 3(4)^2 - 6(4) + 4 = 28\,rad/s
    • Average angular acceleration:       αavg=ΔωΔt=ω4−ω24−2=28−42=12 rad/s2\alpha_{avg} = \frac{\Delta \omega}{\Delta t} = \frac{\omega_4 - \omega_2}{4 - 2} = \frac{28 - 4}{2} = 12\,rad/s^2
    • Illustration 2: A particle starts from rest (ω0=0\omega_0 = 0) with constant α=3.0 rad/s2\alpha = 3.0\,rad/s^2. An observer starts a stopwatch at t1t_1 and notes an angular displacement of Δθ=120 rad\Delta \theta = 120\,rad in the 4-second interval (Δt=4 s\Delta t = 4\,s) up to t2t_2. How long had the particle been moving before the stopwatch started?
    • Angular displacement equation: Δθ=ω1Δt+12α(Δt)2\Delta \theta = \omega_1 \Delta t + \frac{1}{2} \alpha (\Delta t)^2
    • 120=ω1(4)+12(3.0)(4)2  ⟹  120=4ω1+24  ⟹  ω1=24 rad/s120 = \omega_1 (4) + \frac{1}{2} (3.0)(4)^2 \implies 120 = 4\omega_1 + 24 \implies \omega_1 = 24\,rad/s
    • Using ω1=ω0+αt1\omega_1 = \omega_0 + \alpha t_1:       24=0+3.0t1  ⟹  t1=8.0 s24 = 0 + 3.0 t_1 \implies t_1 = 8.0\,s
    • Illustration 3: Particle moves on a circular path of radius r=8 mr = 8\,m with distance s=23t3+3s = \frac{2}{3}t^3 + 3. Find its speed when tangential and normal accelerations are equal in magnitude.
    • Speed: v=dsdt=2t2v = \frac{ds}{dt} = 2t^2
    • Tangential acceleration: at=dvdt=4ta_t = \frac{dv}{dt} = 4t
    • Normal acceleration: an=v2r=(2t2)28=4t48=t42a_n = \frac{v^2}{r} = \frac{(2t^2)^2}{8} = \frac{4t^4}{8} = \frac{t^4}{2}
    • Setting at=ana_t = a_n:       4t=t42  ⟹  t3=8  ⟹  t=2 s4t = \frac{t^4}{2} \implies t^3 = 8 \implies t = 2\,s
    • Speed at t=2 st = 2\,s: v=2(2)2=8 m/sv = 2(2)^2 = 8\,m/s
    • Illustration 4: Particle moves on a circle of radius r=1.5 mr = 1.5\,m with constant α=2 rad/s2\alpha = 2\,rad/s^2. Initial angular speed at t=0t = 0 is ω0=60π rpm=60π×2π60=2 rad/s\omega_0 = \frac{60}{\pi}\,rpm = \frac{60}{\pi} \times \frac{2\pi}{60} = 2\,rad/s. At t=2 st = 2\,s, find values:
    • Angular speed: ω2=ω0+αt=2+2(2)=6 rad/s\omega_2 = \omega_0 + \alpha t = 2 + 2(2) = 6\,rad/s
    • Angular displacement: θ2=ω0t+12αt2=2(2)+12(2)(2)2=8 rad\theta_2 = \omega_0 t + \frac{1}{2}\alpha t^2 = 2(2) + \frac{1}{2}(2)(2)^2 = 8\,rad
    • Linear velocity: v2=rω2=1.5×6=9 m/sv_2 = r \omega_2 = 1.5 \times 6 = 9\,m/s
    • Tangential acceleration: at=rα=1.5×2=3 m/s2a_t = r \alpha = 1.5 \times 2 = 3\,m/s^2
    • Normal acceleration: an=rω22=1.5×62=54 m/s2a_n = r \omega_2^2 = 1.5 \times 6^2 = 54\,m/s^2
    • Illustration 5: A particle moves in a circle of radius RR starting from rest (ω0=0\omega_0 = 0) with constant tangential acceleration. After t=2 st = 2\,s, the angle between total acceleration a⃗\vec{a} and radius RR is 45∘45^\circ. Find angular acceleration α\alpha
    • Angle 45∘45^\circ implies at=ana_t = a_n
    • αR=ω2R  ⟹  α=ω2\alpha R = \omega^2 R \implies \alpha = \omega^2
    • Since ω=ω0+αt=2α\omega = \omega_0 + \alpha t = 2\alpha:       α=(2α)2=4α2  ⟹  α=14=0.25 rad/s2\alpha = (2\alpha)^2 = 4\alpha^2 \implies \alpha = \frac{1}{4} = 0.25\,rad/s^2
    • Illustration 6: Particle moves in a circle of radius RR such that an=ata_n = a_t at all times. Initial speed at t=0t = 0 is v0v_0. Time taken to complete the first revolution is given as t=αRv0(1−e−βπ)t = \frac{\alpha R}{v_0}(1 - e^{-\beta \pi}). Find α+β\alpha + \beta
    • Differential equation: dvdt=v2R  ⟹  dvv2=dtR\frac{dv}{dt} = \frac{v^2}{R} \implies \frac{dv}{v^2} = \frac{dt}{R}
    • Integrating from v0v_0 to vv:       −1v∣v0v=tR  ⟹  1v0−1v=tR  ⟹  v=v01−v0tR-\frac{1}{v} \Big|_{v_0}^v = \frac{t}{R} \implies \frac{1}{v_0} - \frac{1}{v} = \frac{t}{R} \implies v = \frac{v_0}{1 - \frac{v_0 t}{R}}
    • Integrating ds=v dtds = v \, dt for one revolution (s=2πRs = 2\pi R):       2πR=∫0tv0 dt1−v0tR=−Rln⁡(1−v0tR)2\pi R = \int_0^t \frac{v_0 \, dt}{1 - \frac{v_0 t}{R}} = -R \ln\left(1 - \frac{v_0 t}{R}\right)−2π=ln⁡(1−v0tR)  ⟹  1−v0tR=e−2π  ⟹  t=Rv0(1−e−2π)-2\pi = \ln\left(1 - \frac{v_0 t}{R}\right) \implies 1 - \frac{v_0 t}{R} = e^{-2\pi} \implies t = \frac{R}{v_0}(1 - e^{-2\pi})
    • Comparing with given expression: α=1\alpha = 1, β=2  ⟹  α+β=3\beta = 2 \implies \alpha + \beta = 3

Relative Angular Velocity

  • Relativity of Angular Velocity:
    • Angular velocity is inherently a relative quantity defined with respect to an origin or reference point from which position vectors are drawn; absolute angular velocity does not exist.
    • For a particle PP observed from origin OO and reference point AA:
    • Angular velocity w.r.t. OO: ωPO=dαdt\omega_{PO} = \frac{d\alpha}{dt}
    • Angular velocity w.r.t. AA: ωPA=dβdt\omega_{PA} = \frac{d\beta}{dt}

Angular velocity relative to points O and A

  • Mathematical Definition of Relative Angular Velocity:

    • The angular velocity of particle AA with respect to another moving particle BB (ωAB\omega_{AB}) is defined as the rate at which the position vector of AA relative to BB rotates at that instant:     ωAB=Component of relative velocity of A w.r.t. B perpendicular to line ABSeparation distance between A and B=(vAB)⊥rAB\omega_{AB} = \frac{\text{Component of relative velocity of } A \text{ w.r.t. } B \text{ perpendicular to line } AB}{\text{Separation distance between } A \text{ and } B} = \frac{(v_{AB})_\perp}{r_{AB}}
  • Special Motion Cases:

    • Two Particles on Concentric Circles (Closest Approach):
    • For particles AA and BB on concentric circles of radii rAr_A and rBr_B moving in the same direction at closest separation:       (vAB)⊥=vB−vA(v_{AB})_\perp = v_B - v_ArAB=rB−rAr_{AB} = r_B - r_AωAB=vB−vArB−rA\omega_{AB} = \frac{v_B - v_A}{r_B - r_A}
    • Two Particles on Same or Coplanar Concentric Circles (Uniform Speeds):
    • For particles moving in the same direction with uniform angular speeds ωA\omega_A and ωB\omega_B:
      • Rate of change of line-of-sight angle between radii OAOA and OBOB:         dθdt=ωB−ωA\frac{d\theta}{dt} = \omega_B - \omega_A
      • Time TT taken for one particle to complete one full relative revolution around OO w.r.t. the other:         T=2πωrel=2π∣ω2−ω1∣=T1T2∣T1−T2∣T = \frac{2\pi}{\omega_{rel}} = \frac{2\pi}{|\omega_2 - \omega_1|} = \frac{T_1 T_2}{|T_1 - T_2|}
      • Note: ωB−ωA\omega_B - \omega_A represents the rate of change of angle between lines OAOA and OBOB, which is distinct from the angular velocity of BB w.r.t. AA (the rate of rotation of line ABAB).
  • Illustration 7:

    • Particles PP and QQ are separated by r=10 mr = 10\,m. Velocity of PP is 8 m/s8\,m/s at 30∘30^\circ to line PQPQ. Velocity of QQ is 6 m/s6\,m/s at 30∘30^\circ to line PQPQ in opposite transverse direction.
    • Relative perpendicular velocity component:     (vPQ)⊥=8sin⁡(30∘)−(−6sin⁡(30∘))=8(0.5)+6(0.5)=7 m/s(v_{PQ})_\perp = 8 \sin(30^\circ) - (-6 \sin(30^\circ)) = 8(0.5) + 6(0.5) = 7\,m/s
    • Relative angular velocity:     ωPQ=(vPQ)⊥r=710=0.7 rad/s\omega_{PQ} = \frac{(v_{PQ})_\perp}{r} = \frac{7}{10} = 0.7\,rad/s

Radius of Curvature

  • Concept of Radius of Curvature:

    • Any continuous curved path can be modeled as consisting of an infinite series of infinitesimal circular arcs.
    • The radius of curvature RR at a specific point on a trajectory is the radius of the circular arc that matches the curve's profile at that location.
  • Physical Dynamics Method:

    • Relates particle linear speed vv and normal centripetal force Fc=F⊥F_c = F_\perp or normal acceleration component a⊥a_\perp:     F⊥=mv2R  ⟹  R=mv2F⊥=v2a⊥F_\perp = \frac{m v^2}{R} \implies R = \frac{m v^2}{F_\perp} = \frac{v^2}{a_\perp}
  • Calculus Trajectory Method:

    • Given explicit trajectory equation y(x)y(x), radius of curvature RR is evaluated as:     R=[1+(dydx)2]3/2∣d2ydx2∣R = \frac{\left[1 + \left(\frac{dy}{dx}\right)^2\right]^{3/2}}{\left|\frac{d^2y}{dx^2}\right|}
  • Worked Examples:

    • Illustration 8: Particle projected with speed uu at angle θ\theta with horizontal. Find radius of curvature at point of projection and at peak of trajectory.
    • At projection point:
      • Speed v=uv = u
      • Normal acceleration perpendicular to velocity: a⊥=gcos⁡(θ)a_\perp = g \cos(\theta)
      • Radius of curvature: R=u2gcos⁡(θ)R = \frac{u^2}{g \cos(\theta)}
    • At highest point:
      • Horizontal velocity v=ucos⁡(θ)v = u \cos(\theta)
      • Normal acceleration: a⊥=ga_\perp = g
      • Radius of curvature: R=(ucos⁡(θ))2g=u2cos⁡2(θ)gR = \frac{(u \cos(\theta))^2}{g} = \frac{u^2 \cos^2(\theta)}{g}
    • Illustration 9: Parabolic path y=ax2y = ax^2 with constant speed vv. Find RR at x=0x = 0
    • Calculus approach: dydx=2ax  ⟹  at x=0,dydx=0\frac{dy}{dx} = 2ax \implies \text{at } x=0, \frac{dy}{dx} = 0; d2ydx2=2a\frac{d^2y}{dx^2} = 2aR=[1+0]3/22a=12aR = \frac{[1 + 0]^{3/2}}{2a} = \frac{1}{2a}
    • Kinematic approach: y=ax2  ⟹  vy=2axvxy = ax^2 \implies v_y = 2ax v_x. At x=0x=0, vy=0  ⟹  vx=vv_y = 0 \implies v_x = vay=d2ydt2=2avx2+2axaxa_y = \frac{d^2y}{dt^2} = 2a v_x^2 + 2ax a_x. At x=0x=0, ay=2av2a_y = 2a v^2       Since aya_y is perpendicular to vxv_x, normal acceleration a⊥=2av2a_\perp = 2a v^2R=v2a⊥=v22av2=12aR = \frac{v^2}{a_\perp} = \frac{v^2}{2a v^2} = \frac{1}{2a}

Dynamics of Circular Motion

  • Newton's Second Law Formulation:

    • Circular motion requires a net inward force directed toward the center to supply centripetal acceleration:     Fc=mac=mv2r=mω2rF_c = m a_c = \frac{m v^2}{r} = m \omega^2 r
    • If speed varies, a net tangential force FtF_t is required:     Ft=mat=mdvdtF_t = m a_t = m \frac{dv}{dt}
    • Total net force vector: F⃗net=F⃗c+F⃗t\vec{F}_{net} = \vec{F}_c + \vec{F}_t
    • If speed increases (at>0a_t > 0), FtF_t acts parallel to velocity. If speed decreases (at<0a_t < 0), FtF_t acts antiparallel to velocity.
  • Physical Sources of Centripetal Force:

    • Tension in a whirled string.
    • Gravitational force in planetary and satellite orbits.
    • Electrostatic force in atomic electron orbits.
    • Static friction or normal reaction forces on banked surfaces.
  • Conical Pendulum:

    • Particle of mass mm tied to string of length LL revolving in a horizontal circle of radius r=Lsin⁡(θ)r = L \sin(\theta) at angle θ\theta to vertical.
    • Vertical force balance: Tcos⁡(θ)=mgT \cos(\theta) = mg
    • Horizontal centripetal force: Tsin⁡(θ)=mv2r=mω2rT \sin(\theta) = \frac{m v^2}{r} = m \omega^2 r
    • Dividing equations: tan⁡(θ)=v2rg  ⟹  v=rgtan⁡(θ)\tan(\theta) = \frac{v^2}{rg} \implies v = \sqrt{rg \tan(\theta)}
    • Angular speed: ω=gtan⁡(θ)r=gtan⁡(θ)Lsin⁡(θ)=gLcos⁡(θ)\omega = \sqrt{\frac{g \tan(\theta)}{r}} = \sqrt{\frac{g \tan(\theta)}{L \sin(\theta)}} = \sqrt{\frac{g}{L \cos(\theta)}}
    • Time period of revolution:     Tperiod=2πω=2πLcos⁡(θ)g=2πrgtan⁡(θ)T_{period} = \frac{2\pi}{\omega} = 2\pi \sqrt{\frac{L \cos(\theta)}{g}} = 2\pi \sqrt{\frac{r}{g \tan(\theta)}}
  • Illustrations:

    • Illustration 10: Stone PP of mass mm whirled in free space with string radius RR
    • Gravity is absent (g=0g = 0). Tension provides full centripetal acceleration: T=mv2RT = \frac{m v^2}{R}
    • Force exerted by man holding stationary end: Equal in magnitude to tension T=mv2RT = \frac{m v^2}{R}, directed away from stone.
    • Illustration 11: Boy inside rotating vertical cylindrical container of radius RR, back pressed against inner wall, static friction coefficient μs\mu_s. Platform under feet removed. Find minimum angular speed ωmin\omega_{min} to avoid falling.

Boy inside cylindrical container

* Horizontal normal force: N=mω2RN = m \omega^2 R
* Vertical force balance: fs=mgf_s = mg
* Non-slipping constraint: fs≤μsN  ⟹  mg≤μsmω2Rf_s \le \mu_s N \implies mg \le \mu_s m \omega^2 R
* Minimum angular speed:

      ωmin=gμsR\omega_{min} = \sqrt{\frac{g}{\mu_s R}}

  • Illustration 12: Motorcyclist on horizontal circular track of radius RR accelerates tangentially at constant rate at=aa_t = a. Static friction coefficient μs\mu_s. Find maximum safe speed vmaxv_{max}
    • Normal force: N=mgN = mg
    • Tangential friction force: Ft=maF_t = m a
    • Centripetal friction force: Fc=mv2RF_c = \frac{m v^2}{R}
    • Total friction force f=Ft2+Fc2=ma2+v4R2f = \sqrt{F_t^2 + F_c^2} = m \sqrt{a^2 + \frac{v^4}{R^2}}
    • Setting total friction equal to limiting friction fmax=μsmgf_{max} = \mu_s mg:       ma2+v4R2=μsmg  ⟹  a2+v4R2=μs2g2m \sqrt{a^2 + \frac{v^4}{R^2}} = \mu_s mg \implies a^2 + \frac{v^4}{R^2} = \mu_s^2 g^2vmax=[R2(μs2g2−a2)]1/4v_{max} = \left[ R^2 (\mu_s^2 g^2 - a^2) \right]^{1/4}

Circular Turning on Roads

  • Centripetal Requirements for Vehicles:

    • When vehicles negotiate horizontal circular turns, centripetal acceleration is supplied via friction, road banking, or both.
  • Case 1: By Friction Only (Level Unbanked Road):

    • Centripetal force supplied entirely by static friction f=mv2rf = \frac{m v^2}{r}
    • Limiting friction: fmax=μsN=μsmgf_{max} = \mu_s N = \mu_s mg
    • Safe condition: mv2r≤μsmg\frac{m v^2}{r} \le \mu_s mg
    • Maximum safe turning speed:     vmax=μsgrv_{max} = \sqrt{\mu_s g r}
    • Minimum friction coefficient required:     μs≥v2rg\mu_s \ge \frac{v^2}{rg}
  • Case 2: By Banking of Roads Only (Frictionless Banked Road):

    • Road surface tilted outward at angle θ\theta to horizontal.
    • Horizontal component of normal reaction provides centripetal force: Nsin⁡(θ)=mv2rN \sin(\theta) = \frac{m v^2}{r}
    • Vertical force balance: Ncos⁡(θ)=mgN \cos(\theta) = mg
    • Dividing equations gives design speed:     tan⁡(θ)=v2rg  ⟹  v=rgtan⁡(θ)\tan(\theta) = \frac{v^2}{rg} \implies v = \sqrt{rg \tan(\theta)}
  • Case 3: By Friction and Banking of Road Both:

Banking and Friction diagram

  • Forces acting: Weight mgmg, normal reaction NN, friction ff
  • Friction Direction Behavior:
    1. If vehicle is stationary (v=0v = 0), friction ff acts outward/upward along incline balancing mgsin⁡(θ)mg \sin(\theta).
    2. If v<rgtan⁡(θ)v < \sqrt{rg \tan(\theta)}, vehicle tends to slide down incline; friction ff acts outward/upward along incline.
    3. If v=rgtan⁡(θ)v = \sqrt{rg \tan(\theta)}, friction f=0f = 0
    4. If v>rgtan⁡(θ)v > \sqrt{rg \tan(\theta)}, vehicle tends to skid outward; friction ff acts inward/downward along incline.
  • Maximum Safe Speed (vmaxv_{max}):
    • Friction f=μsNf = \mu_s N acts downward along incline:       Nsin⁡(θ)+fcos⁡(θ)=mv2rN \sin(\theta) + f \cos(\theta) = \frac{m v^2}{r}Ncos⁡(θ)−fsin⁡(θ)=mgN \cos(\theta) - f \sin(\theta) = mg
    • Dividing equations yields:       sin⁡(θ)+μscos⁡(θ)cos⁡(θ)−μssin⁡(θ)=vmax2rg\frac{\sin(\theta) + \mu_s \cos(\theta)}{\cos(\theta) - \mu_s \sin(\theta)} = \frac{v_{max}^2}{rg}vmax=rg(tan⁡(θ)+μs1−μstan⁡(θ))v_{max} = \sqrt{rg \left( \frac{\tan(\theta) + \mu_s}{1 - \mu_s \tan(\theta)} \right)}
  • Minimum Safe Speed (vminv_{min}):
    • Friction f=μsNf = \mu_s N acts upward along incline:       Nsin⁡(θ)−fcos⁡(θ)=mv2rN \sin(\theta) - f \cos(\theta) = \frac{m v^2}{r}Ncos⁡(θ)+fsin⁡(θ)=mgN \cos(\theta) + f \sin(\theta) = mg
    • Dividing equations yields:       vmin=rg(tan⁡(θ)−μs1+μstan⁡(θ))v_{min} = \sqrt{rg \left( \frac{\tan(\theta) - \mu_s}{1 + \mu_s \tan(\theta)} \right)}

Centrifugal Force

  • Definition and Context:

    • Centrifugal force is a pseudo/fictitious inertial force required exclusively when analyzing particle dynamics from a non-inertial reference frame rotating at constant angular velocity ω\omega.
  • Magnitude and Direction:

    • Magnitude: Fcf=mrω2=mv2rF_{cf} = m r \omega^2 = \frac{m v^2}{r}
    • Direction: Radially outward from axis of rotation.
  • Observer Interpretation Differences:

    • Inertial Observer (Ground): Object moves in a circle due to inward real centripetal force.
    • Rotating Frame Observer: Object is stationary or moving relative to rotating frame under balance between radially outward centrifugal pseudo force and internal system forces.
  • Illustrations:

    • Illustration 13: Max speed of car on level curve radius R=30 mR = 30\,m, μ=0.4\mu = 0.4, g=10 m/s2g = 10\,m/s^2vmax=μgR=0.4×10×30=120≈11 m/sv_{max} = \sqrt{\mu g R} = \sqrt{0.4 \times 10 \times 30} = \sqrt{120} \approx 11\,m/s
    • Illustration 14: Banking angle for traffic at v=60 km/h=503 m/sv = 60\,km/h = \frac{50}{3}\,m/s, radius r=0.1 km=100 mr = 0.1\,km = 100\,m, g=10 m/s2g = 10\,m/s^2tan⁡(θ)=v2rg=(50/3)2100×10=2500/91000=518  ⟹  θ=tan⁡−1(518)\tan(\theta) = \frac{v^2}{rg} = \frac{(50/3)^2}{100 \times 10} = \frac{2500/9}{1000} = \frac{5}{18} \implies \theta = \tan^{-1}\left(\frac{5}{18}\right)
    • Illustration 15: Smooth hemispherical bowl radius RR rotates about vertical axis. Small ball rotates at angle α\alpha with vertical. Find ω\omega
    • Vertical force balance: Ncos⁡(α)=mgN \cos(\alpha) = mg
    • Horizontal centripetal force: Nsin⁡(α)=m(Rsin⁡(α))ω2  ⟹  N=mRω2N \sin(\alpha) = m (R \sin(\alpha)) \omega^2 \implies N = m R \omega^2
    • Substituting NN into vertical equation:       (mRω2)cos⁡(α)=mg  ⟹  ω=gRcos⁡(α)(m R \omega^2) \cos(\alpha) = mg \implies \omega = \sqrt{\frac{g}{R \cos(\alpha)}}

Beginner's Practice Problems

  • Beginner's Box 1 (Kinematics):

    1. ω=θ2+2θ\omega = \theta^2 + 2\theta. Angular acceleration α\alpha at θ=1 rad\theta = 1\,rad:
    • α=ωdωdθ=(θ2+2θ)(2θ+2)\alpha = \omega \frac{d\omega}{d\theta} = (\theta^2 + 2\theta)(2\theta + 2)
    • At θ=1\theta = 1: α=(1+2)(2+2)=12 rad/s2\alpha = (1 + 2)(2 + 2) = 12\,rad/s^2 (Option C)
    1. Radii ratio r1:r2=1:2r_1 : r_2 = 1 : 2. Same centripetal acceleration. Speed ratio v1:v2v_1 : v_2:
    • ac=v2r  ⟹  v∝r  ⟹  v1v2=12a_c = \frac{v^2}{r} \implies v \propto \sqrt{r} \implies \frac{v_1}{v_2} = \frac{1}{\sqrt{2}} (Option C)
    1. String length r=80 cm=0.8 mr = 80\,cm = 0.8\,m. 14 revolutions in 25 s25\,s:
    • ω=2π(1425)=2×227×1425=3.52 rad/s\omega = 2\pi \left(\frac{14}{25}\right) = 2 \times \frac{22}{7} \times \frac{14}{25} = 3.52\,rad/s
    • ac=ω2r=(3.52)2×0.8≈9.9 m/s2a_c = \omega^2 r = (3.52)^2 \times 0.8 \approx 9.9\,m/s^2 (Option C)
    1. Radius r=20π mr = \frac{20}{\pi}\,m, starts from rest, speed v=50 m/sv = 50\,m/s after 2 revolutions (s=4πr=80 ms = 4\pi r = 80\,m):
    • v2=2ats  ⟹  2500=2at(80)  ⟹  at=15.6 m/s2v^2 = 2 a_t s \implies 2500 = 2 a_t (80) \implies a_t = 15.6\,m/s^2 (Option C)
    1. Particle on turntable with v1=20 cm/sv_1 = 20\,cm/s, a1=20 cm/s2a_1 = 20\,cm/s^2. Radius halved (r2=r12r_2 = \frac{r_1}{2}) at constant ω\omega:
    • v2=ωr2=10 cm/sv_2 = \omega r_2 = 10\,cm/s
    • a2=ω2r2=10 cm/s2a_2 = \omega^2 r_2 = 10\,cm/s^2 (Option A)
    1. Particle completes first 13\frac{1}{3} circumference in 2 s2\,s, next 13\frac{1}{3} in 1 s1\,s:
    • Total displacement: Δθ=4π3 rad\Delta \theta = \frac{4\pi}{3}\,rad in Δt=3 s\Delta t = 3\,s
    • ωavg=4π/33=4π9 rad/s\omega_{avg} = \frac{4\pi/3}{3} = \frac{4\pi}{9}\,rad/s
    1. θ=ω0t+αt2\theta = \omega_0 t + \alpha t^2 with ω0=1 rad/s\omega_0 = 1\,rad/s, α=1.5 rad/s2\alpha = 1.5\,rad/s^2. Angular velocity at t=2 st = 2\,s:
    • ω=dθdt=ω0+2αt=1+2(1.5)(2)=7 rad/s\omega = \frac{d\theta}{dt} = \omega_0 + 2\alpha t = 1 + 2(1.5)(2) = 7\,rad/s
    1. Angular velocity ω=1.5t3−3t2+2\omega = 1.5 t^3 - 3t^2 + 2. Time when α=0\alpha = 0:
    • α=dωdt=4.5t2−6t=0  ⟹  t=64.5=43 s\alpha = \frac{d\omega}{dt} = 4.5 t^2 - 6t = 0 \implies t = \frac{6}{4.5} = \frac{4}{3}\,s
    1. Disc starts from rest with α=3t−t2\alpha = 3t - t^2. Angular velocity after t=2 st = 2\,s:
    • ω=∫02(3t−t2) dt=[3t22−t33]02=6−83=103 rad/s\omega = \int_0^2 (3t - t^2) \, dt = \left[ \frac{3t^2}{2} - \frac{t^3}{3} \right]_0^2 = 6 - \frac{8}{3} = \frac{10}{3}\,rad/s
  • Beginner's Box 2 (Relative Angular Speed and Radius of Curvature):

    1. Projectile projected with speed uu at angle θ\theta. Radius of curvature near top:
    • R=u2cos⁡2(θ)gR = \frac{u^2 \cos^2(\theta)}{g} (Option B)
    1. Curve y=4x2y = 4x^2. Radius of curvature at origin (x=0x=0):
    • a=4  ⟹  R=12a=18 ma = 4 \implies R = \frac{1}{2a} = \frac{1}{8}\,m (Option C)
    1. Radius of curvature at general point (x,y)(x,y) for y=4x2y = 4x^2:
    • dydx=8x\frac{dy}{dx} = 8x, d2ydx2=8  ⟹  R=[1+(8x)2]3/28\frac{d^2y}{dx^2} = 8 \implies R = \frac{[1 + (8x)^2]^{3/2}}{8} (Option A)
    1. Curve path point PP with v=5 m/sv = 5\,m/s, a=10 m/s2a = 10\,m/s^2 at 30∘30^\circ to velocity:
    • (i) Rate of change of speed at=10cos⁡(30∘)=53 m/s2a_t = 10 \cos(30^\circ) = 5\sqrt{3}\,m/s^2 (Option A)
    • (ii) Radius of curvature R=v2an=5210sin⁡(30∘)=255=5 mR = \frac{v^2}{a_n} = \frac{5^2}{10 \sin(30^\circ)} = \frac{25}{5} = 5\,m (Option C)
    1. Two points of rod move with 3v3v and vv same direction, separation rr:
    • ω=3v−vr=2vr\omega = \frac{3v - v}{r} = \frac{2v}{r}
    1. Two points of rod move with 3v3v and vv opposite directions, separation rr:
    • ω=3v−(−v)r=4vr\omega = \frac{3v - (-v)}{r} = \frac{4v}{r}
  • Beginner's Box 3 (Dynamics & Banking):

Beginner's Box 3 diagram

  1. Rotating setup on frictionless table with l1=l2=ll_1 = l_2 = l:
    • T2=m2ω2(2l)T_2 = m_2 \omega^2 (2l)
    • T1−T2=m1ω2l  ⟹  T1=(m1+2m2)ω2lT_1 - T_2 = m_1 \omega^2 l \implies T_1 = (m_1 + 2m_2) \omega^2 l
    • Ratio T1T2=m1+2m22m2\frac{T_1}{T_2} = \frac{m_1 + 2m_2}{2m_2} (Option B)
  2. Centrifugal force is pseudo force when observed by:
    • Observer moving with the particle (Option C)
  3. Banked curve allows higher speed because:
    • Normal reaction has a horizontal component (Option C)
  4. Mass m=16 kgm = 16\,kg, string r=144 mr = 144\,m, max tension T=16 NT = 16\,N:
    • 16=16v2144  ⟹  vmax=12 m/s16 = \frac{16 v^2}{144} \implies v_{max} = 12\,m/s (Option D)
  5. Motorcyclist in well r=5 mr = 5\,m, min speed vmin=55 m/sv_{min} = 5\sqrt{5}\,m/s, g=10 m/s2g = 10\,m/s^2:
    • vmin2=grμs  ⟹  125=50μs  ⟹  μs=0.4v_{min}^2 = \frac{gr}{\mu_s} \implies 125 = \frac{50}{\mu_s} \implies \mu_s = 0.4
  6. Car at v=30 km/h=253 m/sv = 30\,km/h = \frac{25}{3}\,m/s, radius r=60 mr = 60\,m, g=10 m/s2g = 10\,m/s^2:
    • μs≥v2rg=(25/3)2600=6255400≈0.116\mu_s \ge \frac{v^2}{rg} = \frac{(25/3)^2}{600} = \frac{625}{5400} \approx 0.116
  7. Stone m=0.25 kgm = 0.25\,kg, r=1.5 mr = 1.5\,m, f=40 rpm=23 rev/sf = 40\,rpm = \frac{2}{3}\,rev/s:
    • ω=2π(23)=4π3 rad/s\omega = 2\pi \left(\frac{2}{3}\right) = \frac{4\pi}{3}\,rad/s
    • Tension T=mω2r=0.25×(4π3)2×1.5≈6.58 NT = m \omega^2 r = 0.25 \times \left(\frac{4\pi}{3}\right)^2 \times 1.5 \approx 6.58\,N
    • Max speed at Tmax=200 NT_{max} = 200\,N:        200=0.25vmax21.5  ⟹  vmax=1200=203≈34.64 m/s200 = \frac{0.25 v_{max}^2}{1.5} \implies v_{max} = \sqrt{1200} = 20\sqrt{3} \approx 34.64\,m/s