Chapter 1: Elasticity
Elasticity is the property of a material to return to its original shape after deformation. Stress (σ = F/A, unit: Pa) is force per unit area; strain is fractional deformation (dimensionless). Hooke's Law: within the elastic limit, stress ∝ strain. Three elastic moduli — Young's (Y, linear deformation), Bulk (B, volumetric deformation), Shear (G, tangential deformation) — all share dimensions [ ] and unit Pa. The stress-strain curve sequence is: proportional limit → elastic limit → yield point → ultimate stress → breaking point. The slope of the linear region = Y. Compressibility = 1/B. NEET extension formula: = FL/(AY).
Chapter 2: Fluid Statics
Pascal's Law: pressure applied to an enclosed fluid is transmitted equally in all directions. Application: hydraulic press, / = /. Pressure at depth h: P = + ρgh (Pa). This chapter is less frequently tested independently but supports Bernoulli's equation questions.
Chapter 3: Fluid Dynamics
For ideal, incompressible, non-viscous, streamline flow: Equation of continuity (v_{1} = v_{2}) ensures mass conservation — narrower pipe → higher speed. Bernoulli's equation (P + ½ρ + ρgh = constant) is energy conservation per unit volume. Key applications: Venturi meter, pitot tube, spray gun, airplane lift. Higher velocity → lower pressure.
Chapter 4: Viscosity and Terminal Velocity
Viscosity η: [ ] (Pa·s). Newton's viscosity law: F = ηA(dv/dx). Stokes drag: F = 6πηrv. Terminal velocity v_t = 2(ρ − σ)g/(9η). Key NEET result: v_t ∝ . Poiseuille's law for pipe flow: Q = πr^{4}$$\Delta P/(8ηL) — flow rate depends on (radius to the fourth power).
Chapter 5: Surface Tension
S = F/L = Energy/Area; [ ] (N/m). Excess pressure — liquid drop: = 2S/R; soap bubble: = 4S/R (two surfaces). Capillary rise: h = 2S cosθ/(ρgr). Water-glass: acute θ → rise; Mercury-glass: obtuse θ → depression. Surface energy = S × .
Chapter 6: Heat Transfer
Three modes — conduction (Fourier's law: Q/t = KA /L), convection (Newton's cooling: dT/dt = −k(T − )), radiation (Stefan-Boltzmann: P = σ, σ = W ). Thermal expansion: β = 3α (volume), 2α (area). T must be in Kelvin for radiation calculations.