Tamil Nadu HSE First Year Physics study materials
Tamil Nadu HSE First Year Physics study resources

Tamil Nadu HSE First Year Physics cheat sheet

Tamil Nadu HSE First Year Physics · Keep the key ideas within reach.

Quick reference

Nature of Physical World and Measurement

  • Fundamental SI base quantities: length (metre), mass (kilogram), time (second), electric current (ampere), temperature (kelvin), amount of substance (mole), luminous intensity (candela).

  • Dimensional analysis: any physical quantity Q has dimensions expressed as [M^a L^b T^c A^d K^e mol^f cd^g]; only quantities with identical dimensions can be added or equated.

  • Dimensional formula of common quantities: force [MLT^-2], energy/work [ML^2T^-2], power [ML^2T^-3], pressure [ML^-1T^-2], momentum [MLT^-1], angular momentum [ML^2T^-1].

  • Principle of homogeneity: every term in a valid physical equation must have the same dimensions; this checks correctness but cannot determine dimensionless constants.

  • Significant figures: multiplication/division retains the least number of significant figures; addition/subtraction retains the least number of decimal places.

  • Error propagation: for Z = A+B, dZ = dA + dB (absolute); for Z = AB or A/B, fractional error dZ/Z = dA/A + dB/B; for Z = A^n, fractional error = n(dA/A).

  • Percentage error = (mean absolute error / mean value) x 100; mean absolute error = (1/n) sum |a_i - a_mean|.

  • Vernier calliper: least count = 1 main scale division - 1 vernier scale division; if n vernier divisions equal (n-1) MSD, LC = 1 MSD / n.

  • Screw gauge: least count = pitch / number of circular scale divisions; zero error is positive if circular scale zero lies above the reference line, negative if below.

Quick reference

Kinematics

  • Equations of uniformly accelerated motion: v = u + at; s = ut + (1/2)at^2; v^2 = u^2 + 2as; displacement in nth second = u + a(2n-1)/2.

  • Projectile motion: time of flight T = 2u sin(theta)/g; maximum height H = u^2 sin^2(theta)/(2g); horizontal range R = u^2 sin(2theta)/g; maximum range at theta = 45 degrees.

  • Relative velocity: v_AB = v_A - v_B; for two bodies moving in the same direction, relative speed is the difference of speeds.

  • Average velocity = total displacement / total time; average speed = total path length / total time; average speed >= magnitude of average velocity.

  • Distance-time graph slope gives speed; velocity-time graph slope gives acceleration and area under the curve gives displacement.

  • Circular motion: angular velocity omega = d(theta)/dt; tangential acceleration a_t = d|v|/dt; radial acceleration a_r = v^2/r = r omega^2.

  • Uniform circular motion has constant speed but varying velocity direction, so the motion is accelerated; period T = 2 pi r / v.

  • Equations of motion are valid only for constant acceleration; for variable acceleration use calculus: v = dx/dt and a = dv/dt = v dv/dx.

  • Scalars have magnitude only; vectors have magnitude and direction and add by triangle or parallelogram law: R = sqrt(A^2 + B^2 + 2AB cos theta).

Quick reference

Laws of Motion

  • Newton's first law: a body continues in uniform motion or at rest unless acted upon by a net external force; this defines inertial frames.

  • Newton's second law: F_net = dp/dt = ma when mass is constant; the acceleration is along the net force direction.

  • Newton's third law: forces occur in equal and opposite pairs acting on different bodies; action and reaction never cancel on the same body.

  • Friction: limiting friction f_max = mu_s N; kinetic friction f_k = mu_k N, with mu_k < mu_s; static friction adjusts from zero up to f_max.

  • Angle of repose: tan(theta) = mu_s; a block stays at rest on an incline only if tan(theta) <= mu_s.

  • Banking of roads: for zero friction, tan(theta) = v^2/(rg); with friction, maximum safe speed is v = sqrt(rg(tan theta + mu)/(1 - mu tan theta)).

  • Impulse J = F_avg * delta_t = change in momentum; this is useful when force acts for a short time.

  • Apparent weight in a lift: N = m(g + a) when accelerating upward, N = m(g - a) when accelerating downward, N = 0 in free fall.

  • Momentum conservation: if net external force is zero, total momentum of an isolated system remains constant; used in collisions and recoil problems.

Quick reference

Work, Energy and Power

  • Work W = F s cos(theta); work is positive when theta < 90 degrees, zero when theta = 90 degrees, negative when theta > 90 degrees.

  • Work-energy theorem: net work done by all forces equals change in kinetic energy, W_net = (1/2)mv^2 - (1/2)mu^2.

  • Kinetic energy KE = (1/2)mv^2 = p^2/(2m); potential energy of a spring U = (1/2)kx^2.

  • Gravitational potential energy near Earth U = mgh; conservative forces have path-independent work and a defined potential energy.

  • Power P = W/t = F v cos(theta); SI unit watt; 1 horsepower = 746 watt.

  • Conservation of mechanical energy: if only conservative forces act, KE + PE = constant; with friction, mechanical energy decreases by the work done against friction.

  • Collisions: momentum is conserved in all collisions; kinetic energy is conserved only in perfectly elastic collisions.

  • Coefficient of restitution e = relative velocity of separation / relative velocity of approach; e = 1 for elastic, e = 0 for perfectly inelastic collisions.

  • In an elastic collision of equal masses, the bodies exchange velocities; a lighter body rebounds with nearly its own speed when struck by a heavy one.

Quick reference

Motion of System of Particles and Rigid Bodies

  • Centre of mass: R = (sum m_i r_i)/(sum m_i); it moves as if all external forces act at that point.

  • Torque tau = r x F; magnitude tau = r F sin(theta); torque is zero when force passes through the axis.

  • Angular momentum L = I omega; conservation of angular momentum: if external torque is zero, I1 omega1 = I2 omega2.

  • Moment of inertia of a thin rod about its centre: I = ML^2/12; about one end: I = ML^2/3.

  • Moment of inertia of a solid sphere about a diameter: I = (2/5)MR^2; of a hollow sphere: I = (2/3)MR^2; of a disc about its axis: I = (1/2)MR^2.

  • Parallel-axis theorem: I = I_cm + Md^2; perpendicular-axis theorem for a planar lamina: I_z = I_x + I_y.

  • Rolling without slipping: v_cm = R omega; total KE = (1/2)Mv^2 + (1/2)I omega^2 = (1/2)Mv^2(1 + I/(MR^2)).

  • Equilibrium of a rigid body requires both net force zero and net torque zero; for a body to topple, the line of action of weight must pass outside the base.

  • Radius of gyration k relates to moment of inertia by I = Mk^2; it depends on mass distribution and axis, not on the total mass alone.

Quick reference

Gravitation

  • Newton's law of gravitation: F = G m1 m2 / r^2; G = 6.67 x 10^-11 N m^2 kg^-2.

  • Acceleration due to gravity at height h: g_h = g (R/(R+h))^2; at depth d: g_d = g(1 - d/R); at the centre of Earth g = 0.

  • Variation of g with latitude: g_phi = g - R omega^2 cos^2(phi); at the equator the reduction is maximum, at the poles it is zero.

  • Orbital velocity of a satellite near Earth: v_o = sqrt(GM/R) = sqrt(gR) approximately 7.9 km/s.

  • Escape velocity: v_e = sqrt(2GM/R) = sqrt(2gR) approximately 11.2 km/s; independent of the mass of the projected body.

  • Kepler's laws: orbits are ellipses with the Sun at one focus; equal areas in equal times (areal velocity constant); T^2 is proportional to a^3.

  • Total energy of an orbiting satellite E = -GMm/(2r); kinetic energy = GMm/(2r); potential energy = -GMm/r.

  • Geostationary satellite: period 24 hours, equatorial orbit at about 36,000 km altitude, moves west to east.

  • Weightlessness in an orbiting satellite arises because the satellite and everything in it fall with the same centripetal acceleration.

Quick reference

Properties of Matter

  • Stress = force/area; strain = change in dimension / original dimension; Young's modulus Y = stress/strain for longitudinal deformation.

  • Hooke's law: stress is proportional to strain within the elastic limit; the slope of the stress-strain graph gives Young's modulus.

  • Elastic potential energy per unit volume = (1/2) x stress x strain = (1/2)Y(strain)^2.

  • Bulk modulus K = -P/(delta V/V); compressibility is the reciprocal of bulk modulus; shear modulus involves tangential stress.

  • Poisson's ratio = lateral strain / longitudinal strain; theoretical range -1 to 0.5, typical metals around 0.3.

  • Surface tension S = force/length; surface energy = surface tension x change in area; excess pressure inside a soap bubble = 4S/r, inside a liquid drop or bubble = 2S/r.

  • Capillary rise h = 2S cos(theta)/(r rho g); liquid rises when contact angle is acute, is depressed when the angle is obtuse.

  • Bernoulli's theorem: P + (1/2)rho v^2 + rho g h = constant along a streamline for steady, incompressible, non-viscous flow.

  • Viscous force F = eta A dv/dx (Stokes law: F = 6 pi eta r v); terminal velocity v_t = 2r^2(rho - sigma)g/(9 eta).

Quick reference

Heat and Thermodynamics

  • First law of thermodynamics: delta Q = delta U + delta W; sign convention matters - work done by the system is positive.

  • Work done in an isobaric process W = P delta V; in an isothermal process W = nRT ln(V2/V1); in an adiabatic process W = (P1V1 - P2V2)/(gamma - 1).

  • Adiabatic relation: PV^gamma = constant; also TV^(gamma-1) = constant and P^(1-gamma) T^gamma = constant.

  • For a monatomic gas gamma = 5/3; for a diatomic gas gamma = 7/5; gamma = Cp/Cv and Cp - Cv = R.

  • Efficiency of a Carnot engine eta = 1 - T2/T1, with temperatures in kelvin; no engine between the same reservoirs can exceed this.

  • Coefficient of performance of a refrigerator = Q2/W = T2/(T1 - T2).

  • Second law: heat cannot flow spontaneously from a colder to a hotter body without external work; entropy of an isolated system never decreases.

  • Calorimetry: Q = mc delta theta; latent heat Q = mL; principle of mixtures: heat lost = heat gained.

  • Thermal expansion: length L = L0(1 + alpha delta T); area coefficient about 2 alpha; volume coefficient about 3 alpha for isotropic solids.

Quick reference

Kinetic Theory of Gases

  • Ideal gas equation: PV = nRT; in terms of molecules PV = (1/3)Nm v_rms^2.

  • Pressure P = (1/3)(Nm/V) v_rms^2; molecular speeds: v_rms = sqrt(3RT/M), v_avg = sqrt(8RT/(pi M)), v_mp = sqrt(2RT/M).

  • Ordering of speeds: v_mp < v_avg < v_rms; ratio v_rms : v_avg : v_mp = sqrt(3) : sqrt(8/pi) : sqrt(2).

  • Average translational kinetic energy per molecule = (3/2)kT; total internal energy of a monatomic ideal gas U = (3/2)nRT.

  • Degrees of freedom: monatomic f = 3; diatomic f = 5 at ordinary temperature; polyatomic f = 6; equipartition gives (1/2)kT per degree of freedom.

  • Mean free path lambda = 1/(sqrt(2) pi n d^2), where n is number density and d is molecular diameter; it increases as pressure falls.

  • Boyle's law PV = constant at constant T; Charles's law V/T = constant at constant P; Gay-Lussac's law P/T = constant at constant V.

  • Dalton's law of partial pressures: total pressure of a non-reacting gas mixture equals the sum of partial pressures.

  • Real gases deviate from ideal behaviour at high pressure and low temperature; van der Waals equation: (P + a n^2/V^2)(V - nb) = nRT.

Quick reference

Oscillations and Waves

  • SHM: acceleration a = -omega^2 x; displacement x = A sin(omega t + phi); velocity v = omega sqrt(A^2 - x^2); maximum speed = A omega.

  • Time period of a simple pendulum T = 2 pi sqrt(L/g); of a spring-mass system T = 2 pi sqrt(m/k).

  • Total energy in SHM E = (1/2)m omega^2 A^2; kinetic and potential energies vary but their sum stays constant for undamped SHM.

  • Wave equation: v = f lambda; for a stretched string v = sqrt(T/mu) where mu is linear density.

  • Speed of sound in a gas v = sqrt(gamma P/rho) = sqrt(gamma RT/M); it increases with temperature and is independent of pressure at constant temperature.

  • Standing waves on a string fixed at both ends: frequencies f_n = n v/(2L); in a pipe closed at one end only odd harmonics occur, f_n = (2n-1)v/(4L).

  • Beats: beat frequency = |f1 - f2|; produced when two waves of nearly equal frequency superpose.

  • Doppler effect for sound: apparent frequency f' = f (v +/- v_o)/(v -/+ v_s), with upper signs for approach; the effect depends on the medium.

  • Resonance occurs when driving frequency equals the natural frequency, giving maximum amplitude; damping reduces amplitude and slightly lowers the natural frequency.

Quick reference

Practical Physics / Laboratory Skills

  • Before using a vernier calliper or screw gauge, record the zero error and apply it with the correct sign to every reading.

  • Least count of vernier calliper = 1 MSD / number of vernier divisions; of screw gauge = pitch / number of circular scale divisions.

  • For a simple pendulum, time at least 20 oscillations and divide; measure length from the point of suspension to the centre of the bob.

  • For a metre bridge, make all connections tight and tap the jockey gently; insert the key only while taking a reading to avoid heating.

  • In Ohm's law experiments, connect the ammeter in series and the voltmeter in parallel with the resistor, observing correct polarity.

  • Take at least three to five readings over the full range, plot a graph, and find the slope rather than relying on a single reading.

  • Record every measurement with its unit and the correct number of significant figures; report the result as mean value plus or minus mean absolute error.

  • In resonance column experiments, use a tuning fork of known frequency and locate resonance by the loudest sound, measuring from the water level.

  • In optics experiments, keep the optical bench aligned, avoid parallax while reading positions, and use a distant object to find the focal length of a concave mirror.