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Dive deep into the concepts of work, kinetic energy, potential energy, and conservation principles. Learn about impulse, momentum, and systems of particles. Explore the center of mass, conservation of momentum, and elastic & inelastic collisions. Gain insights into rocket propulsion and more in this enlightening lecture review.
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Review from Last Lecture • Work • Kinetic Energy • Potential Energy • For conservative forces • Work-Energy Theorem • Total Energy • Constant for conservative forces • Stability • At a fixed point
Examples: Gravitational Field • Find maximum r for given initial v • Particle will escape if denominator is zero
Impulse • Imagine the force involved in hitting a golf ball • Force changes very quickly • How can we use Newton’s Laws if we don’t know the force at every time? • Integrate with respect to time • Call this the “impulse”
Impulse • What exactly is force the derivative of? • Call p = mv the momentum of a particle • The impulse, then, is the change in momentum
System of Particles 1 • Consider a system of several particles • Each particle obeys Newton’s Laws: • This force can be split into internal and external parts • Now sum up the forces on all the particles • For the internal forces we have • Thus 2 3
System of Particles 1 • Continuing with our system • Internal forces cancel, so • The sum of derivatives is the derivative of the sums • We can treat the motion of a system of particles as the change in the total system’s momentum! 2 3
Center of Mass 1 • If what does refer to? • Well so • Thus • This “average” position is called the Center of Mass 2 3
Center or Mass • What’s the Center of Mass for a continuous object? • Change sum into an integral (using density r) • Note that the total mass is also an integral • So CM is still really the “average” position • “Add” up the positions of each little bit of mass • Divide by the “number” of little bits of mass
Center of Mass • Can find center of mass of an object by hanging it from two places • Center of mass will always be below the hanging point
Center of Mass • Example: CM of a right triangle
Conservation of Momentum • Since the total momentum of a system of particles is only changed by external forces, the momentum of an isolated system is constant • For this we say, “momentum is conserved” • The total momentum is conserved even though parts of the system may be doing wild things
Elastic and Inelastic Collisions • In an elastic collision the total kinetic energy is conserved • Momentum is conserved in any collision • Example: • What are signs of final velocities?
Elastic and Inelastic Collisions • Example (cont.): • Consider reference frame where CM is at rest
Elastic and Inelastic Collisions • In an inelastic collision the total kinetic energy is not conserved • Momentum is conserved in any collision • Example: case where particles stick together
Elastic and Inelastic Collisions • Example: Ballistic Pendulum
Collisions in 2D • Use Conservation of Momentum in each direction • Consider case where one particle is at rest • In CM frame particles are back-to-back!
Rocket Propulsion • “Rockets can’t fly in vacuum. What do they have to push against?” • Nonsense. Rockets don’t push; they conserve momentum, and send parts (fuel) away from the body as fast as possible
Rocket Propulsion • How fast do rockets accelerate? • Start at rest, with mass M+Dm • Some time Dt later, have expelled Dm at speed ve, to conserve momentum, rest of rocket (M) must have velocity (in the other direction) of Dv = ve Dm/M
Rocket Propulsion • How fast do rockets accelerate? • Thrust: (instantaneous) force on rocket