Phys 2101 Gabriela González2!• Ch 2,4 - Kinematics: motion in 1,2 and 3D: x(t), v(t), a(t) • Ch 5,6 - Dynamics: F = ma • Ch 7,8 - Energy: potential, kinetic, Work-Energy theorem • Ch 9 – Center of mass, linear momentum : collisions. • Ch 10, 11 - Rotation: τ=Iα, rotational energy, rolling, angular momentum, rigid bodies • Ch 12: Equilibrium, elasticity: F=0, τ=0 • Ch 13: Gravitation: F = Gm1m2/r2, U = - GMm/r, Kepler’s laws • Ch 14: Fluids: at rest, p-p0=ρgh, buoyant force • Ch 15: Oscillations: x(t) = xm sin(ωt+φ), potential, kinetic energy • Ch 16: Waves: y(x,t) = ym cos(kx-ωt+φ), standing waves • Ch 18, 19, 20: Thermodynamics: temperature, ideal gases, heat, internal energy, work, entropy, heat engines.3!• Ch 2,4 - Kinematics: motion in 1,2 and 3D: x(t), v(t), a(t) • Ch 5,6 - Dynamics: F = ma • Ch 10, 11: Rotation τ=Iα, rolling4!• Ch 7,8 - Energy: potential, kinetic, Work-Energy theorem • Ch 9 - Particles, collisions: Linear momentum. • Ch 10, 11 – Rotation: rotational energy, angular momentum • Ch 12: Equilibrium, elasticity: F=0, τ=05!• Ch 13: Gravitation: F = Gm1m2/r2, U = - GMm/r: for two and for several masses! • Ch 14: Fluids: at rest. Buoyant force.6!• Ch 15 - Oscillations: x(t) = xm cos(ωt+φ), • Ch 16: Waves Traveling y(x,t) = ym sin(kx-ωt+φ); Superposition (interference, standing waves)7!• Ch 18: Temperature and heat, Thermal expansion Heat capacity, specific heat, heat of transformation: Q = c m ΔT, Q = L m8!• Ch 18: First law of thermodynamics ΔEint = Q – W p, V diagrams • Ch 19: Kinetic theory Ideal gases: pV = nRT Specific heat: Q = nCPΔT or n CV ΔT; CV=(f/2)R; CP =CV+R Eint= (f/2) nRT9!10!Ch 20: Reversible and irreversible processes: entropy Second law of thermodynamics: ΔS ≥ 0 Heat engines: ε = W/QH ≤ εC = 1- TL/TH Refrigerators: K=QL/W ≤Kc=TL /(TH-TL)11!• Mild (low C): revisit homework sets; revisit your exams; read chapter summaries; read formula sheet • Medium (Solid C): read class slides; revisit class problems; do all checkpoints, solve ~1/2 questions; read all problems; solve a few old exams • Hot (B): read whole chapters; solve all questions; solve ~1/2 problems solve many old exams • Tabasco hot (A): solve ALL problems, invent new problems solve all old exams PHYS 2101 PHYS 2101 PHYS 2101 PHYS 2101 Save some time to sleep before the
View Full Document