Rotational Dynamics and Moment of Inertia

Fundamentals of Rotational Dynamics

  • Revolution vs. Rotation:     * Revolution: During revolution, the object undergoes a circular path about some other object or a point outside the object.     * Rotation: During rotation, the motion is about an axis of rotation passing through the object itself.

  • Definition and Characteristics of Circular Motion:     * Circular Motion: The motion of an object around a circular path is called circular motion.     * Accelerated Motion: As the direction of velocity changes at every instant, it is an accelerated motion.     * Periodic Motion: During the motion, the particle repeats its path along the same trajectory. Thus, the motion is periodic in space.

  • Analogy Between Linear and Rotational Quantities:     * Displacement: Linear is ss; Rotational/Angular is θ\theta.     * Velocity: Linear is v=dsdtv = \frac{ds}{dt}; Rotational/Angular is ω=dθdt\omega = \frac{d\theta}{dt}.     * Acceleration: Linear is a=dvdta = \frac{dv}{dt}; Rotational/Angular is α=dωdt\alpha = \frac{d\omega}{dt}.

Angular Kinematics and Relationships

  • Tangential Velocity (vv):     * It describes the motion of an object along the edge of the circle whose direction at any given point on the circle is always along the tangent to that point.     * Vector Form: v=ω×r\vec{v} = \vec{\omega} \times \vec{r}, where r\vec{r} is the position vector and ω\vec{\omega} is the angular velocity.     * Magnitude: v=rωv = r\omega.

  • Direction of Angular Velocity:     * The direction of angular velocity (ω\omega) can be determined using the Right Hand Thumb Rule.

  • Relation Between Angular Velocity, Period, and Frequency:     * n=frequencyn = \text{frequency}     * T=Time periodT = \text{Time period}     * ω=2πT\omega = \frac{2\pi}{T}     * Since n=1Tn = \frac{1}{T}, ω=2πn\omega = 2\pi n.

Uniform and Non-Uniform Circular Motion

  • Uniform Circular Motion (UCM):     * During circular motion, if the speed of the particle remains constant, it is called Uniform Circular Motion (UCM).     * The direction of velocity changes at every instant, remaining always tangential to the path.     * The acceleration responsible for this is the centripetal or radial acceleration (ara_r).     * In UCM, the magnitude of acceleration is constant: a=ω2r=v2r=vωa = \omega^2 r = \frac{v^2}{r} = v\omega.     * This acceleration is always directed towards the center of the circular motion (along r-\vec{r}), hence it is called centripetal.

  • Non-Uniform Circular Motion (NUM):     * During circular motion, if the speed of the particle varies, it is called non-uniform circular motion.     * Example: The starting and stopping of a fan; the speed varies for some time, making it a non-uniform circular motion.     * The acceleration responsible for changing the magnitude of velocity is directed along or opposite to the velocity.     * This acceleration is always tangential and is called tangential acceleration (ata_t).     * As the magnitude of tangential velocity changes, the corresponding angular velocity also changes at every instant due to angular acceleration: α=dωdt\alpha = \frac{d\omega}{dt}.

Dynamics of Circular Motion: Forces

  • Centripetal Force vs. Centrifugal Force:     * Centripetal Force:         * Directed along the radius, towards the center of the circle.         * It is a real force.         * Considered in an inertial frame of reference.         * Vector form: F=mv2rr0\mathbf{F} = -\frac{mv^2}{r} \mathbf{r}_0.     * Centrifugal Force:         * Directed along the radius, away from the center of the circle.         * It is a pseudo force.         * Considered in a non-inertial frame of reference.         * Vector form: F=mv2rr0\mathbf{F} = \frac{mv^2}{r} \mathbf{r}_0.

  • Direction of Angular Acceleration (α\alpha):     * For increasing speed: α\alpha is in the same direction as ω\omega.     * For decreasing speed: α\alpha is in the opposite direction to ω\omega.

Applications of Circular Motion

  • Vehicle on a Horizontal Unbanked Road:     * Forces acting on the car:         1. Weight (mgmg) acting downwards.         2. Normal reaction (NN) that balances the weight (N=mgN = mg).         3. Force of static friction (fsf_s) between road and tires.     * Friction acts as the resultant centripetal force to prevent outward slipping or skidding: fs=mv2rf_s = \frac{mv^2}{r}.     * Derivation:         * fsN=mv2rmg=v2rg\frac{f_s}{N} = \frac{\frac{mv^2}{r}}{mg} = \frac{v^2}{rg}         * As speed increases, fsf_s also increases. At maximum speed, fs=(fs)max=μsNf_s = (f_s)_{max} = \mu_s N.         * μsN=mvmax2r\mu_s N = \frac{m v_{max}^2}{r}         * vmax=μsrgv_{max} = \sqrt{\mu_s rg}, where μs\mu_s is the coefficient of static friction.

  • Well of Death (Maut Ka Kua):     * This is a vertical cylindrical wall of radius rr inside which a vehicle is driven in horizontal circles (often seen in stunts).     * Forces acting on the vehicle:         1. Normal reaction (NN) acting horizontally towards the center.         2. Weight (mgmg) acting vertically downwards.         3. Force of static friction (fsf_s) acting vertically upwards to prevent downward slipping.     * Derivation for Minimum Safest Velocity (vminv_{min}):         * fs=mgf_s = mg         * N=mv2rN = \frac{mv^2}{r}         * To avoid slipping, fsμsNf_s \le \mu_s N         * mgμsmv2rmg \le \mu_s \frac{mv^2}{r}         * gμsv2rv2rgμsg \le \frac{\mu_s v^2}{r} \rightarrow v^2 \ge \frac{rg}{\mu_s}         * vmin=rgμsv_{min} = \sqrt{\frac{rg}{\mu_s}}

Banking of Roads

  • Purpose of Banking:     * On horizontal roads, centripetal force depends on friction. Frictional force has an upper limit and varies with road conditions (e.g., wet surfaces).     * To reduce dependency on friction, the surface of curved roads is tilted with the horizontal at an angle θ\theta. This is called banking of a road.

  • Angle of Banking (Neglecting Friction):     * Weight (mgmg) acts downward; Normal reaction (NN) is perpendicular to the road.     * Components of N:         * Vertical: Ncos(θ)N \cos(\theta) balances mgmg.         * Horizontal: Nsin(θ)N \sin(\theta) provides centripetal force mv2r\frac{mv^2}{r}.     * Equations:         * Nsin(θ)=mv2rN \sin(\theta) = \frac{mv^2}{r}         * Ncos(θ)=mgN \cos(\theta) = mg         * Nsin(θ)Ncos(θ)=mv2rmgtan(θ)=v2rg\frac{N \sin(\theta)}{N \cos(\theta)} = \frac{\frac{mv^2}{r}}{mg} \rightarrow \tan(\theta) = \frac{v^2}{rg}         * Angle of banking: θ=tan1(v2rg)\theta = \tan^{-1}\left(\frac{v^2}{rg}\right).         * Most safe speed: vs=rgtan(θ)v_s = \sqrt{rg \tan(\theta)}.

  • Speed Limits on Banked Roads:     * Lower Speed Limit (v1v_1):         * For v1<rgtan(θ)v_1 < \sqrt{rg \tan(\theta)}, the vehicle tends to slide down. Static friction (fsf_s) acts upwards along the incline.         * v12rg=tan(θ)μs1+μstan(θ)\frac{v_1^2}{rg} = \frac{\tan(\theta) - \mu_s}{1 + \mu_s \tan(\theta)}         * vmin=rg(tan(θ)μs1+μstan(θ))v_{min} = \sqrt{rg \left( \frac{\tan(\theta) - \mu_s}{1 + \mu_s \tan(\theta)} \right)}.     * Upper Speed Limit (v2v_2):         * For v2>rgtan(θ)v_2 > \sqrt{rg \tan(\theta)}, the vehicle tends to skid outward. Static friction (fsf_s) acts downwards along the incline.         * v22rg=tan(θ)+μs1μstan(θ)\frac{v_2^2}{rg} = \frac{\tan(\theta) + \mu_s}{1 - \mu_s \tan(\theta)}         * vmax=rg(tan(θ)+μs1μstan(θ))v_{max} = \sqrt{rg \left( \frac{\tan(\theta) + \mu_s}{1 - \mu_s \tan(\theta)} \right)}.

Pendulums

  • Definitions:     1. Pendulum: A tiny mass connected to a long, flexible, massless, inextensible string suspended from a rigid support.     2. Simple Pendulum: A pendulum where the string oscillates in a single vertical plane.     3. Conical Pendulum: A system where the string moves along the surface of a right circular cone and the point object performs uniform horizontal circular motion.

  • Time Period of a Conical Pendulum:     * Let LL be the length of the string, mm the mass of the bob, and θ\theta the angle with the vertical.     * Forces: Tension (T0T_0) and Weight (mgmg).     1. T0cos(θ)=mgT_0 \cos(\theta) = mg     2. T0sin(θ)=mrω2T_0 \sin(\theta) = m r \omega^2     * Combining these: tan(θ)=rω2g\tan(\theta) = \frac{r\omega^2}{g}.     * From geometry: r=Lsin(θ)r = L \sin(\theta).     * ω2=gsin(θ)rcos(θ)=gsin(θ)Lsin(θ)cos(θ)=gLcos(θ)\omega^2 = \frac{g \sin(\theta)}{r \cos(\theta)} = \frac{g \sin(\theta)}{L \sin(\theta) \cos(\theta)} = \frac{g}{L \cos(\theta)}.     * ω=gLcos(θ)\omega = \sqrt{\frac{g}{L \cos(\theta)}}.     * Time Period (TT): T=2πω=2πLcos(θ)gT = \frac{2\pi}{\omega} = 2\pi \sqrt{\frac{L \cos(\theta)}{g}}.     * Frequency (nn): n=12πgLcos(θ)n = \frac{1}{2\pi} \sqrt{\frac{g}{L \cos(\theta)}}.

  • Factors Governing Frequency of Conical Pendulum:     * Length (LL): n1Ln \propto \frac{1}{\sqrt{L}}. As length decreases, frequency increases.     * Acceleration due to gravity (gg): ngn \propto \sqrt{g}. As gg increases, frequency increases.     * Angle (θ\theta): n1cos(θ)n \propto \frac{1}{\sqrt{\cos(\theta)}}. As θ\theta increases, cos(θ)\cos(\theta) decreases and nn increases.     * Mass: Frequency is independent of the mass of the bob.

Vertical Circular Motion (VCM)

  • Types of VCM:     1. Controlled: Speed is kept constant or not totally controlled by gravity (e.g., giant wheel).     2. Gravity-Controlled: Energy is supplied at the lowest point, and kinematics are governed by gravitation (interconversion of kinetic and gravitational potential energy).

  • Minimum Speeds in Gravity-Controlled VCM:     * Topmost point (A): TA=0T_A = 0. Centripetal force provided by weight: mvA2r=mgvA=rg\frac{mv_A^2}{r} = mg \rightarrow v_A = \sqrt{rg}.     * Lowermost point (B): By conservation of energy (KEB=KEA+PElossKE_B = KE_A + PE_{loss}): vB=5rgv_B = \sqrt{5rg}.     * Middle point (C or D): By conservation of energy: vC=3rgv_C = \sqrt{3rg}.

  • Tension Differences:     * TBTA=6mgT_B - T_A = 6mg     * TCTA=3mgT_C - T_A = 3mg

  • Convex Over-bridge:     * A vehicle at the top of a convex bridge experience weight (mgmg) downwards and Normal reaction (NN) upwards.     * Resultant force: mgN=mv2rmg - N = \frac{mv^2}{r}.     * For the vehicle to maintain contact, N0N \ge 0. This imposes an upper speed limit:     * N=mgmv2rN = mg - \frac{mv^2}{r}. Setting N=0N = 0 gives vmax=rgv_{max} = \sqrt{rg}.

Moment of Inertia (M.I.)

  • Definition: The moment of inertia (II) is the sum of the product of the mass of each particle and the square of its perpendicular distance from the axis of rotation: I=miri2I = \sum m_i r_i^2.

  • Kinetic Energy of a Rotating Body:     * A rigid object consists of particles m1,m2,,mnm_1, m_2, \dots, m_n at distances r1,r2,,rnr_1, r_2, \dots, r_n.     * All particles have the same ω\omega but different linear speeds vi=riωv_i = r_i \omega.     * Individual K.E.i=12mivi2=12miri2ω2\text{K.E.}_i = \frac{1}{2} m_i v_i^2 = \frac{1}{2} m_i r_i^2 \omega^2.     * Total Rotational K.E.=12miri2ω2=12(miri2)ω2\text{Total Rotational K.E.} = \sum \frac{1}{2} m_i r_i^2 \omega^2 = \frac{1}{2} \left( \sum m_i r_i^2 \right) \omega^2.     * Rotational K.E.=12Iω2\text{Rotational K.E.} = \frac{1}{2} I \omega^2.

  • Physical Significance of M.I.:     * M.I. is the rotational analogue of mass (mm). It represents rotational inertia.     * It depends on individual masses and the distribution of these masses about the axis of rotation.

  • Moment of Inertia of Specific Objects:     * Uniform Ring: All mass MM is at distance RR from the axis. I=MR2I = MR^2.     * Uniform Disc: A two-dimensional circular object. Surface density σ=MA=MπR2\sigma = \frac{M}{A} = \frac{M}{\pi R^2}.         * Considered as concentric rings of radius rr and width drdr.         * Mass of elemental ring dm=σ(2πrdr)dm = \sigma(2\pi r dr).         * dI=dm×r2=2πσr3drdI = dm \times r^2 = 2\pi \sigma r^3 dr.         * Integration from 00 to RR: I=0R2πσr3dr=2πσ[r44]0R=πσR42I = \int_0^R 2\pi \sigma r^3 dr = 2\pi \sigma [ \frac{r^4}{4} ]_0^R = \frac{\pi \sigma R^4}{2}.         * Substituting σ=MπR2\sigma = \frac{M}{\pi R^2}: I=πR42MπR2=12MR2I = \frac{\pi R^4}{2} \frac{M}{\pi R^2} = \frac{1}{2} MR^2.

  • Radius of Gyration (KK):     * Defined as the distance from the axis where the entire mass of the object could be concentrated to have the same moment of inertia: I=MK2I = MK^2.     * A larger KK value indicates that the mass is distributed farther from the axis.