Chapter 1 · Physics · 8 questions in the paper · 12 min read
Mechanics
What the syllabus asks for 7
- Physical quantities, vectors and kinematics: dimensions, resolution and polygon law, vector algebra, equations of motion, projectile motion, relative motion
- Newton's laws of motion and friction: conservation of linear momentum, equilibrium and non-equilibrium applications, laws of solid friction
- Work, energy and power: work-energy theorem, kinetic and potential energy, conservation of energy, conservative and non-conservative forces, elastic and inelastic collisions
- Circular motion, gravitation and SHM: centripetal force, conical pendulum, banking, gravitational potential, variation of g, satellites, rocket launch, energy in SHM, spring-mass system, simple pendulum, damped and forced oscillation, resonance
- Rotational dynamics: moment of inertia, radius of gyration, rotational KE, centre of gravity and mass, torque, conservation of angular momentum
- Elasticity: Hooke's law, Young modulus, bulk modulus, modulus of rigidity, Poisson's ratio, elastic energy
- Fluid mechanics: buoyancy, flotation, Archimedes' principle, surface tension, capillarity, viscosity, Newton, Stokes and Poiseuille formulae, Reynolds number, continuity, Bernoulli
Mechanics is about a third of the Physics paper (our estimate: 8 of 27 questions). The official syllabus lists seven sub-areas: kinematics and vectors, Newton's laws and friction, work-energy, circular motion with gravitation and SHM, rotation, elasticity, and fluids. The Section B questions combine two ideas, typically energy with circular motion, momentum with energy loss, or continuity with Bernoulli.
- Dimensions of work, power, pressure, surface tension, viscosity, and dimensional checking.
- Projectile formulas: T=\frac{2u\sin\theta}{g}, H=\frac{u^2\sin^2\theta}{2g}, R=\frac{u^2\sin2\theta}{g}.
- Newton's second law on inclines and with friction; \mu=\tan\theta at the angle of repose.
- Momentum conservation and collisions; kinetic energy lost in a perfectly inelastic collision.
- Circular motion: a=v^2/r, banking \tan\theta=\frac{v^2}{rg}, vertical circle (v_{\text{bottom}}\ge\sqrt{5gr}).
- Gravitation: g'=g\big(\frac{R}{R+h}\big)^2, escape speed \sqrt{2gR}=11.2 km/s, orbital speed, T^2\propto r^3.
- SHM: T=2\pi\sqrt{m/k}, 2\pi\sqrt{l/g}, v_{\max}=A\omega, energy \frac{1}{2}kA^2.
- Rotation: I of standard bodies, \tau=I\alpha, L=I\omega conserved.
- Elasticity: Y=\frac{FL}{A\Delta L}, energy density \frac{1}{2}\times stress \times strain, Poisson's ratio.
- Fluids: Archimedes, surface tension and capillary rise, Stokes' law, continuity A_1v_1=A_2v_2, Bernoulli.
1.1 Physical quantities, vectors and kinematics
Dimensions. [\text{force}]=\text{MLT}^{-2}, [\text{work, energy}]=\text{ML}^2\text{T}^{-2}, [\text{power}]=\text{ML}^2\text{T}^{-3}, [\text{pressure, stress, }Y]=\text{ML}^{-1}\text{T}^{-2}, [\text{surface tension}]=\text{MT}^{-2}, [\text{viscosity }\eta]=\text{ML}^{-1}\text{T}^{-1}, [G]=\text{M}^{-1}\text{L}^3\text{T}^{-2}, [h]=\text{ML}^2\text{T}^{-1}. Only quantities of the same dimensions can be added; dimensional analysis checks a formula but cannot fix numerical constants.
Vectors. Resultant of \vec A,\vec B at angle \theta: R=\sqrt{A^2+B^2+2AB\cos\theta}, direction \tan\alpha=\frac{B\sin\theta}{A+B\cos\theta}. Two equal forces F at 120^\circ give F. Polygon law: vectors drawn head to tail close the polygon when the sum is zero. Resolution: A_x=A\cos\theta, A_y=A\sin\theta. Dot product (work, projection), cross product (torque, magnetic force).
Equations of uniformly accelerated motion: v=u+at, s=ut+\frac{1}{2}at^2, v^2=u^2+2as, s_n=u+\frac{a}{2}(2n-1). Free fall uses a=g=9.8\ \text{m s}^{-2}. Area under the v–t graph is displacement; slope of the x–t graph is velocity.
Projectile (speed u, angle \theta): T=\dfrac{2u\sin\theta}{g}, H=\dfrac{u^2\sin^2\theta}{2g}, R=\dfrac{u^2\sin2\theta}{g} (maximum at 45^\circ, equal for \theta and 90^\circ-\theta), \tan\theta=\frac{4H}{R}. Trajectory y=x\tan\theta-\frac{gx^2}{2u^2\cos^2\theta} is a parabola. Horizontal launch from height h: t=\sqrt{2h/g}.
Relative motion: \vec v_{AB}=\vec v_A-\vec v_B. River crossing: shortest time when heading perpendicular to the bank (time d/v_b); shortest path when \sin\theta=v_r/v_b (needs v_b>v_r). Rain appears to fall at \tan\alpha=v_{\text{man}}/v_{\text{rain}} from the vertical.
1.2 Newton's laws of motion and friction
Laws: (1) inertia; (2) \vec F=\frac{d\vec p}{dt}=m\vec a; (3) action–reaction on different bodies. Impulse =F\Delta t=\Delta p (area under the F–t graph). Momentum conservation holds when no external force acts: m_1u_1+m_2u_2=m_1v_1+m_2v_2; a gun recoils with v_{\text{gun}}=\frac{m_{\text{bullet}}}{M}v.
Equilibrium: \sum\vec F=0 (e.g. Lami's theorem for three concurrent forces). Inclined plane (angle \theta, frictionless): a=g\sin\theta. Atwood machine: a=\dfrac{(m_1-m_2)g}{m_1+m_2}, T=\dfrac{2m_1m_2g}{m_1+m_2}. Lift accelerating up at a: apparent weight m(g+a); down: m(g-a); free fall: zero.
Solid friction. Static f_s\le\mu_sN; kinetic f_k=\mu_kN (\mu_k<\mu_s). Laws (verified with an inclined plane): independent of the area of contact, proportional to normal reaction, independent of speed. Angle of friction \lambda: \tan\lambda=\mu; angle of repose \alpha (a block just slips): \tan\alpha=\mu. On a rough incline a=g(\sin\theta-\mu\cos\theta). Horizontal push P on a block: a=\dfrac{P-\mu mg}{m}.
1.3 Work, energy and power
W=\vec F\cdot\vec s=Fs\cos\theta; area under the F–x graph; spring work \frac{1}{2}kx^2. Work–energy theorem: W_{\text{net}}=\Delta K=\frac{1}{2}mv^2-\frac{1}{2}mu^2. K=\frac{p}{2m}\cdot p=\frac{p^2}{2m}. Gravitational PE =mgh; elastic PE =\frac{1}{2}kx^2. Mechanical energy is conserved under conservative forces (gravity, spring, electrostatic: work independent of path, zero over a closed loop); friction and drag are non-conservative. Power P=\frac{W}{t}=\vec F\cdot\vec v; 1 hp = 746 W; kWh = 3.6\times10^6 J.
Collisions. Momentum is always conserved. Elastic: kinetic energy also conserved, e=1; for equal masses the velocities exchange; for m_1 on a stationary m_2: v_1=\frac{m_1-m_2}{m_1+m_2}u, v_2=\frac{2m_1}{m_1+m_2}u. Perfectly inelastic: bodies stick, v=\frac{m_1u_1+m_2u_2}{m_1+m_2} and the maximum kinetic energy is lost. Coefficient of restitution e=\frac{v_2-v_1}{u_1-u_2}; a ball dropped from h rebounds to e^2h.
1.4 Circular motion, gravitation and SHM
Circular motion. \omega=\frac{2\pi}{T}=2\pi f, v=\omega r, a_c=\frac{v^2}{r}=\omega^2r toward the centre, F_c=\frac{mv^2}{r} (supplied by tension, friction, gravity, normal reaction — not a separate force). Conical pendulum: T\cos\theta=mg, T\sin\theta=\frac{mv^2}{r}, period 2\pi\sqrt{\frac{L\cos\theta}{g}}. Level turn: v_{\max}=\sqrt{\mu rg}. Banking (no friction): \tan\theta=\frac{v^2}{rg}. Vertical circle: T_{\text{top}}=\frac{mv_t^2}{r}-mg; v_{\text{top,min}}=\sqrt{gr}, v_{\text{bottom,min}}=\sqrt{5gr}. Over a convex bridge the apparent weight is m(g-\frac{v^2}{r}).
Gravitation. F=\dfrac{Gm_1m_2}{r^2}, G=6.67\times10^{-11}. g=\dfrac{GM}{R^2}; at height h: g'=g\big(\frac{R}{R+h}\big)^2 (=\frac{g}{4} at h=R); at depth d: g'=g\big(1-\frac{d}{R}\big); with latitude \lambda: g'=g-\omega^2R\cos^2\lambda (zero effect at the poles). Gravitational potential V=-\frac{GM}{r}, PE =-\frac{GMm}{r}. Escape speed v_e=\sqrt{\frac{2GM}{R}}=\sqrt{2gR}=11.2 km/s; v_{\text{orbit}}=\sqrt{\frac{GM}{r}} (near Earth \sqrt{gR}=7.9 km/s), so v_e=\sqrt{2}v_o. Kepler: T^2\propto r^3; T=2\pi\sqrt{\frac{r^3}{GM}}. Orbital energy: K=\frac{GMm}{2r}, E=-\frac{GMm}{2r}. A geostationary satellite has T=24 h, orbit radius \approx42{,}400 km (height \approx36{,}000 km), moves west to east above the equator. Weightlessness in orbit: free fall. Rocket: thrust =v_{\text{rel}}\frac{dm}{dt}; multi-stage design sheds dead mass to reach the required speed.
SHM. a=-\omega^2x, x=A\sin(\omega t+\phi), v=\omega\sqrt{A^2-x^2}, v_{\max}=A\omega, a_{\max}=A\omega^2. Spring–mass T=2\pi\sqrt{\frac{m}{k}} (series springs k=\frac{k_1k_2}{k_1+k_2}, parallel k_1+k_2); simple pendulum T=2\pi\sqrt{\frac{l}{g}} (a seconds pendulum has T=2 s, l\approx0.994 m). Energy E=\frac{1}{2}kA^2=\frac{1}{2}m\omega^2A^2; K=\frac{1}{2}k(A^2-x^2), U=\frac{1}{2}kx^2; both oscillate at twice the frequency; K=U at x=\frac{A}{\sqrt{2}}. Damped oscillations lose amplitude to friction; forced oscillations have the driver's frequency and the amplitude peaks at resonance (f_{\text{driver}}=f_0).
1.5 Rotational dynamics
I=\sum mr^2; K_{\text{rot}}=\frac{1}{2}I\omega^2; \tau=I\alpha=\vec r\times\vec F; L=I\omega; \tau=\frac{dL}{dt}; P=\tau\omega. Radius of gyration k=\sqrt{I/M}.
| Body (axis) | I |
|---|---|
| ring / hollow cylinder (central axis) | MR^2 |
| disc / solid cylinder (central axis) | \frac{1}{2}MR^2 |
| solid sphere (diameter) | \frac{2}{5}MR^2 |
| hollow sphere (diameter) | \frac{2}{3}MR^2 |
| thin rod (centre, perpendicular) / (end) | \frac{ML^2}{12} / \frac{ML^2}{3} |
Parallel-axis theorem I=I_{cm}+Md^2; perpendicular-axis (planar) I_z=I_x+I_y. Rolling without slipping: K=\frac{1}{2}Mv^2\big(1+\frac{k^2}{R^2}\big); down an incline a=\frac{g\sin\theta}{1+k^2/R^2}. Conservation of angular momentum: I_1\omega_1=I_2\omega_2 (a skater pulling arms in spins faster). Centre of mass \frac{\sum m\vec r}{\sum m}; for uniform gravity the centre of gravity coincides with it. A body is in equilibrium when \sum F=0 and \sum\tau=0.
1.6 Elasticity
Stress =\frac{F}{A}, strain =\frac{\Delta L}{L}. Hooke's law: stress \propto strain within the elastic limit. Y=\dfrac{FL}{A\,\Delta L}; bulk modulus K=-\dfrac{\Delta P}{\Delta V/V} (compressibility 1/K); rigidity \eta=\dfrac{F/A}{\theta}. Poisson's ratio \sigma=\frac{\text{lateral strain}}{\text{longitudinal strain}}, between -1 and 0.5. Energy stored =\frac{1}{2}F\Delta L per unit volume \frac{1}{2}\times\text{stress}\times\text{strain}=\frac{\text{stress}^2}{2Y}. Extension \propto\frac{L}{r^2} for the same material and force. Relations: Y=3K(1-2\sigma)=2\eta(1+\sigma). Steel has a higher Y than rubber (it is more elastic in the physics sense). Elastic after-effect, fatigue, yield point, breaking stress are read from the stress–strain graph. Pressure at depth h in the sea decreases the volume of a ball by \frac{\rho gh}{K} (fraction).
1.7 Fluid mechanics
Pressure P=P_0+\rho gh; Pascal's law (hydraulic press, force ratio = area ratio). Archimedes: buoyant force =\rho_{\text{fluid}}Vg; a body floats when its weight equals the buoyancy; ice (900 kg m⁻³) floats with \frac{9}{10} submerged; apparent weight in a liquid =W-F_B.
Surface tension T=\frac{F}{l} (N m⁻¹) =\frac{\text{energy}}{\text{area}}. Excess pressure: bubble with one surface \frac{2T}{r}, soap bubble (two surfaces) \frac{4T}{r}. Work to blow a soap bubble of radius r: 8\pi r^2T. Capillary rise h=\dfrac{2T\cos\theta}{r\rho g} (h\propto1/r; mercury, with \theta>90^\circ, is depressed). Surface tension falls with temperature and with detergent.
Viscosity. F=\eta A\frac{dv}{dx} (Newton). Stokes' law F=6\pi\eta rv; terminal velocity v_t=\dfrac{2r^2(\rho-\sigma)g}{9\eta} (\propto r^2). Poiseuille \dfrac{dV}{dt}=\dfrac{\pi Pr^4}{8\eta l} (\propto r^4). Reynold number R_e=\dfrac{\rho vD}{\eta}; below about 2000 the flow is streamline (laminar), above about 3000 turbulent.
Continuity A_1v_1=A_2v_2 (incompressible). Bernoulli P+\frac{1}{2}\rho v^2+\rho gh=\text{constant} — conservation of energy along a streamline. Uses: Venturi meter, aerofoil lift, atomiser, speed of efflux v=\sqrt{2gh} (Torricelli).
- Centripetal force is not an extra force on a free-body diagram.
- A satellite in orbit is not beyond gravity; it is in free fall.
- In an inelastic collision momentum is conserved, kinetic energy is not.
- Banking-angle questions give v in km/h: convert first.
- Capillary height is inversely proportional to radius; Poiseuille flow goes as r^4.
Formula and fact sheet
| Quantity | Formula |
|---|---|
| range, max height | \frac{u^2\sin2\theta}{g}, \frac{u^2\sin^2\theta}{2g} |
| friction | \mu=\tan\alpha (repose) |
| inelastic KE loss | \frac{1}{2}\frac{m_1m_2}{m_1+m_2}(u_1-u_2)^2 |
| banking | \tan\theta=\frac{v^2}{rg} |
| v_e, v_o | \sqrt{2gR}, \sqrt{gR} |
| SHM | T=2\pi\sqrt{m/k}, 2\pi\sqrt{l/g} |
| rolling ratio | K_{tr}:K_{rot}=1:\frac{k^2}{R^2} |
| Y | \frac{FL}{A\Delta L} |
| capillary | h=\frac{2T\cos\theta}{r\rho g} |
| terminal speed | \frac{2r^2(\rho-\sigma)g}{9\eta} |
| Poiseuille | \frac{\pi Pr^4}{8\eta l} |
Chapter summary
- Check units by dimensions; use \sin2\theta for range, \sin^2\theta for height.
- Momentum is conserved in every collision; kinetic energy only in elastic ones.
- For circular and orbital motion identify what supplies the centripetal force.
- SHM periods depend only on the system constants (m,k or l,g), not on amplitude.
- Angular momentum conservation changes \omega when I changes.
- Elastic energy density is \frac{1}{2}\times stress \times strain.
- Fluids: continuity first for speeds, then Bernoulli for pressure.
Practice questions
Set A — Recall (14 questions)
- The dimensional formula of work isa[MLT^{-2}]b[ML^2T^{-2}]c[ML^2T^{-3}]d[ML^{-1}T^{-2}]
- A projectile is launched at 45^\circ with a speed of 20 m s⁻¹ (g=10 m s⁻²). Its range isa20 mb80 mc40 md10 m
- A force of 10 N acts for 3 s on a 5 kg body initially at rest. Its final speed isa6 m s⁻¹b2 m s⁻¹c15 m s⁻¹d50 m s⁻¹
- The kinetic energy of a 2 kg body moving at 3 m s⁻¹ isa6 Jb18 Jc12 Jd9 J
- The power needed to lift a 100 kg load through 10 m in 10 s (g=10) isa100 Wb1000 Wc10000 Wd10 W
- A body moves at 10 m s⁻¹ on a circle of radius 5 m. Its centripetal acceleration isa2 m s⁻²b50 m s⁻²c20 m s⁻²d10 m s⁻²
- The escape speed from the Earth's surface is nearlya7.9 km s⁻¹b9.8 km s⁻¹c8 km s⁻¹d11.2 km s⁻¹
- If the length of a simple pendulum is made four times, its time periodahalvesbdoublescquadruplesdis unchanged
- The moment of inertia of a solid sphere about a diameter isa\frac{1}{2}MR^2b\frac{2}{3}MR^2c\frac{2}{5}MR^2dMR^2
- The maximum theoretical value of Poisson's ratio isa0.5b1c0.25d0.33
- Ice of density 900 kg m⁻³ floats in water with the fraction submerged equal toa1/10b1/2c3/4d9/10
- Bernoulli's theorem expresses the conservation ofaenergybmomentumcmassdangular momentum
- The SI unit of surface tension isaN mbN m⁻²cN m⁻¹dJ m⁻³
- A block just starts to slide when a plane is tilted to 30^\circ. The coefficient of static friction isa0.866b0.5c1.73d0.577
Answers and explanations — Set A
1. (b) — force × distance. (a) is force.
2. (c) — R=\frac{u^2\sin90^\circ}{g}=\frac{400}{10}=40 m.
3. (a) — impulse: v=\frac{Ft}{m}=\frac{30}{5}=6.
4. (d) — \frac{1}{2}\cdot2\cdot9=9 J.
5. (b) — \frac{mgh}{t}=\frac{100\cdot10\cdot10}{10}=1000 W.
6. (c) — v^2/r=100/5=20.
7. (d) — \sqrt{2gR}=11.2 km s⁻¹; 7.9 km s⁻¹ is the orbital speed near the surface.
8. (b) — T\propto\sqrt{l}.
9. (c) — \frac{2}{5}MR^2; (b) is the hollow sphere.
10. (a) — theory limits: -1<\sigma<0.5.
11. (d) — \rho_{ice}/\rho_{water}=0.9.
12. (a) — it is the work–energy theorem for a flowing fluid.
13. (c) — force per unit length.
14. (d) — \mu=\tan30^\circ=0.577.
Set B — Understanding (10 questions)
- A ball is thrown at 60^\circ to the horizontal with speed 20 m s⁻¹ (g=10). Its maximum height isa10 mb15 mc20 md30 m
- Two forces of 10 N each act at 120^\circ to each other. Their resultant isa20 Nb10\sqrt{3} Nc10 Nd0
- A 2 kg block on a rough floor (\mu=0.2, g=10) is pushed by a 10 N horizontal force. Its acceleration isa5 m s⁻²b3 m s⁻²c4 m s⁻²d2 m s⁻²
- A 2 kg body moving at 4 m s⁻¹ collides and sticks to a stationary 2 kg body. The kinetic energy lost isa4 Jb16 Jc0d8 J
- A frictionless banked road must let a car take a bend of radius 10 m at 10 m s⁻¹ (g=10). The banking angle isa45^\circb30^\circc60^\circd37^\circ
- A particle moves as x=0.1\sin(10t) (SI). Its maximum speed isa0.1 m s⁻¹b10 m s⁻¹c1 m s⁻¹d100 m s⁻¹
- A 2 kg mass hangs on a spring of constant 200 N m⁻¹. The period of its oscillation isa0.2\pi sb2\pi sc0.02\pi sd\pi s
- The time period of a geostationary satellite isa12 hb90 minc6 hd24 h
- A disc of mass 2 kg and radius 0.5 m is acted on by a torque of 0.5 N m about its axis. Its angular acceleration isa2 rad s⁻²b1 rad s⁻²c0.5 rad s⁻²d4 rad s⁻²
- A wire has twice the length and twice the radius of another of the same material. Under the same force its extension isa2 timesb\frac{1}{2} timesc\frac{1}{4} timesdthe same
Answers and explanations — Set B
1. (b) — H=\frac{u^2\sin^2\theta}{2g}=\frac{400\cdot0.75}{20}=15.
2. (c) — equal vectors at 120^\circ give a resultant equal to each.
3. (b) — a=\frac{10-0.2\cdot2\cdot10}{2}=3.
4. (d) — v=2 m s⁻¹; K_i=16 J, K_f=\frac{1}{2}\cdot4\cdot4=8 J; loss 8 J.
5. (a) — \tan\theta=\frac{v^2}{rg}=1.
6. (c) — v_{\max}=A\omega=0.1\times10.
7. (a) — T=2\pi\sqrt{2/200}=0.2\pi s \approx0.63 s.
8. (d) — it must match the Earth's rotation.
9. (a) — I=\frac{1}{2}MR^2=0.25; \alpha=\frac{0.5}{0.25}=2.
10. (b) — \Delta L\propto\frac{L}{r^2}=\frac{2}{4}.
Set C — Application (8 questions)
- A stone is thrown horizontally at 10 m s⁻¹ from a 20 m high tower (g=10). It lands at a horizontal distance ofa10 mb14 mc40 md20 m
- A 1000 kg car moving at 20 m s⁻¹ is stopped by brakes in 40 m. The average braking force isa5000 Nb10000 Nc2500 Nd500 N
- At a height equal to the Earth's radius, the acceleration due to gravity is (g=9.8 at the surface)a4.9 m s⁻²b3.27 m s⁻²c2.45 m s⁻²d1.1 m s⁻²
- A stone on a 0.5 m string is whirled in a vertical circle. The minimum speed at the bottom to complete the circle is (g=10)a5 m s⁻¹b2.5 m s⁻¹c7.07 m s⁻¹d10 m s⁻¹
- A skater spinning at 2 rad s⁻¹ with I=4 kg m² pulls in her arms so that I=1 kg m². Her new angular speed isa0.5 rad s⁻¹b4 rad s⁻¹c8 rad s⁻¹d16 rad s⁻¹
- Water (\rho=1000) flows at 2 m s⁻¹ in a pipe of area 4 cm² that narrows to 1 cm². The pressure drop in the narrow part isa28 kPab30 kPac32 kPad60 kPa
- Water rises 3 cm in a capillary tube. In a tube of half the radius it risesa6 cmb3 cmc12 cmd1.5 cm
- Two identical spheres fall through the same liquid; one has twice the radius. Ratio of terminal speeds (larger : smaller) isa2b8c16d4
Answers and explanations — Set C
1. (d) — t=\sqrt{2h/g}=2 s; x=10\cdot2=20 m.
2. (a) — F=\frac{\frac{1}{2}mv^2}{d}=\frac{200000}{40}.
3. (c) — g'=g\big(\frac{R}{2R}\big)^2=\frac{g}{4}=2.45.
4. (a) — v=\sqrt{5gr}=\sqrt{25}.
5. (c) — L=I\omega: 4\times2=1\times\omega.
6. (b) — v_2=8 m s⁻¹ by continuity; \Delta P=\frac{1}{2}\cdot1000\,(64-4)=30000 Pa.
7. (a) — h\propto\frac{1}{r}: halving the radius doubles the rise.
8. (d) — v_t\propto r^2, ratio 4.