(Probable) Exam #2 Topics
Forces
Newton III Pairs
Gravity F=GMm/r2, g=acceleration at earth surface = GM/r2
Orbit weightlessness in orbit
Normal Force Not always mg. Compression of material like a spring
Tension Stretching of material like a spring
Friction Non-conservative, Fstatic <= msN, Fdynamic = mdN, ABS
Static Friction equals applied force up to Fstatic_max, then breaks free
Sliding (= Kinetic) Always same once broken free
Free Body Diagrams
Coupled masses Airtrack cart and falling weight, monkey, inclined plane
Uniform circular motion Must accelerate to go in a circle with a = mv2/r. Loop-de-loop
A force must cause this acceleration. Rotor ride, vomit comet
Energy
Work W=∫F·dx . Positive if F and dx in same direction.
Dot product: amount of force along motion/motion along force
Change in energy. Ef = Ei + W
Mechanical Energy Conservative/non-conservative forces
Kinetic Energy Some of individual kinetic energies
Potential Energy Gravity, springs, easily turned into kinetic energy, not friction
Graphs Turning points, F = -dU/dx = -slope of U(x)
Energy transfer Between kinetic and potential energy
Power Energy/time
Conservation When is mechanical energy conserved?
Internal Energy E = K + Ugravity + Uspring + Uheat + Uchem + Unuclear + mc2 + etc.
Momentum
Momentum vectors, conserved separately each direction
Impulse Impulse = change in momentum, rose, sledge hammer
P conserved if impulse=0: Fext=0 or tà 0
Padding Same impulse, longer time means smaller force
Collisions small time: small impulse: p conserved
Inelastic p conserved, E lost: stuck together is pure inelastic
Elastic p conserved, E conserved: How to solve
Center of mass How to find, Useful frame of reference
Rocket Newton III or impulse explanation
Relativistic Energy and Momentum
Definitions p=ϒmv, E=ϒmc2, ϒ=1/sqrt(1-v2/c2)
Definition of Kinetic Energy E=mc2 + K
Workhorse E2 = m2c4 + p2c2
Binding Energy