12.07.2015 Views

Simple Nature - Light and Matter

Simple Nature - Light and Matter

Simple Nature - Light and Matter

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Radial acceleration at the surface of the Earth example 14⊲ What is your radial acceleration due to the rotation of the earthif you are at the equator?⊲ At the equator, your distance from the Earth’s rotation axis isthe same as the radius of the spherical Earth, 6.4 × 10 6 m. Yourangular velocity isω =2π radians1 daywhich gives an acceleration of= 7.3 × 10 −5 s −1 ,a r = ω 2 r= 0.034 m/s 2 .The angular velocity was a very small number, but the radius wasa very big number. Squaring a very small number, however, givesa very very small number, so the ω 2 factor “wins,” <strong>and</strong> the finalresult is small.If you’re st<strong>and</strong>ing on a bathroom scale, this small acceleration isprovided by the imbalance between the downward force of gravity<strong>and</strong> the slightly weaker upward normal force of the scale on yourfoot. The scale reading is therefore a little lower than it shouldbe.4.2.3 DynamicsIf we want to connect all this kinematics to anything dynamical,we need to see how it relates to torque <strong>and</strong> angular momentum.Our strategy will be to tackle angular momentum first, since angularmomentum relates to motion, <strong>and</strong> to use the additive propertyof angular momentum: the angular momentum of a system of particlesequals the sum of the angular momenta of all the individualparticles. The angular momentum of one particle within our rigidlyrotating object, L = mv ⊥ r, can be rewritten as L = r p sin θ,where r <strong>and</strong> p are the magnitudes of the particle’s r <strong>and</strong> momentumvectors, <strong>and</strong> θ is the angle between these two vectors. (The rvector points outward perpendicularly from the axis to the particle’sposition in space.) In rigid-body rotation the angle θ is 90 ◦ ,so we have simply L = rp. Relating this to angular velocity, wehave L = rp = (r)(mv) = (r)(mωr) = mr 2 ω. The particle’s contributionto the total angular momentum is proportional to ω, witha proportionality constant mr 2 . We refer to mr 2 as the particle’scontribution to the object’s total moment of inertia, I, where “moment”is used in the sense of “important,” as in “momentous” — abigger value of I tells us the particle is more important for determiningthe total angular momentum. The total moment of inertia268 Chapter 4 Conservation of Angular Momentum

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