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C.1 Calculus and Vectors

Solutions to Practice Problems from Chapter 1.9

C.2 Newtonian Review

Solutions to Practice Problems from Chapter 2.8

C.3 Simple Harmonic Motion

Solutions to Practice Problems from Chapter 3.9

C.4 Introduction to Non-Inertial and Rotating Frames

Solutions to Practice Problems from Chapter 4.8

C.5 Applications of Non-Inertial and Rotating Frames

Solutions to Practice Problems from Chapter 5.8

C.6 Momentum and Variable Mass

Solutions to Practice Problems from Chapter 6.8

C.7 Torques and Angular Momentum

Solutions to Practice Problems from Chapter 7.9

C.8 Work and Energy

Solutions to Practice Problems from Chapter 8.10

C.9 Applications of Energy Conservation

Solutions to Practice Problems from Chapter 9.6

C.10 Central Forces and Motion in Space

Solutions to Practice Problems from Chapter 10.9

Problem 10-2: Question

Feff=L2+2mmr3r^F_{eff}= \frac{L^{2}+ 2m}{mr^{3}} \hat{r}

Problem 10-3: Question

Ueff,max=m2LU_{eff,\max}= -\dfrac{m}{2L}, stable

Problem 10-5: Question

L=2mkR3,v=2kR2L = 2m\sqrt{k} R^{3}, v = 2\sqrt{k} R^{2}

Problem 10-6: Question

Feff=L2mr3γr23γεr4F_{eff}= \frac{L^{2}}{mr^{3}} - \frac{\gamma}{r^{2}} - \frac{3\gamma \varepsilon}{r^{4}}

Problem 10-2: Question

Ueff=12L2mr2+γr12εr2U_{eff}= \frac{1}{2} \frac{L^{2}}{mr^{2}} + - \frac{\gamma}{r} - \frac{1}{2} \varepsilon r^{2}

Problem 10-3: Question

L=3AβmR5eβR3L = \sqrt{3A\beta mR^{5}e^{\beta R^{3}}}

Problem 10-4: Question

a) For small values of r,L2mr2>>Ar2r, \frac{L^{2}}{mr^{2}} >> Ar^{2}, so the centrifugal potential dominates UeffU_{eff}. For large values of r,L2mr2<<Ar2r, \frac{L^{2}}{mr^{2}} << Ar^{2}, so the central force potential dominates UeffU_{eff}.

b)r=(L22Am)1/4\mathrm{b}) r = \Bigg(\frac{L^{2}}{2Am} \Bigg)^{1/4}
c)E=2AL2m\mathrm{c}) E = \sqrt{\frac{2AL^{2}}{m}}

Problem 10-5: Question

a)r˙=2ALmr3/2\mathrm{a}) \dot{r} = 2\sqrt{A}\frac{L}{mr^{3/2}}
b)E=L22m[4Ar3+1r2]+U(r)\mathrm{b}) E = \frac{L^{2}}{2m} \bigg[\frac{4A}{r^{3}} + \frac{1}{r^{2}} \bigg] + U(r)
c)U(r)=EL22m[4Ar3+1r2]\mathrm{c}) U(r) = E - \frac{L^{2}}{2m} \bigg[\frac{4A}{r^{3}} + \frac{1}{r^{2}} \bigg]
d)Fr=L2m(6Ar4+1r3)\mathrm{d}) F_{r}= - \frac{L^{2}}{m} \bigg(\frac{6A}{r^{4}} + \frac{1}{r^{3}} \bigg)

Problem 10-6: Question

a) For small values of r,1r31r2r, \frac{1}{r^{3}} \gg \frac{1}{r^{2}}. For large values of r,1r31r2r, \frac{1}{r^{3}} \ll \frac{1}{r^{2}}.

C.11 Orbits and Kepler’s Laws

Solutions to Practice Problems from Chapter 11.7

C.12 The Lagrange Method

Solutions to Practice Problems from Chapter 12.8