From ab03acdfba14a176ac72e5eebc432bcf71e645e7 Mon Sep 17 00:00:00 2001 From: Erik Strand <erik.strand@cba.mit.edu> Date: Thu, 14 Feb 2019 00:32:20 -0500 Subject: [PATCH] Tex up my solutions --- _posts/2019-02-13-pset1.md | 260 ++++++++++++++++++++++++++++++++++++- 1 file changed, 259 insertions(+), 1 deletion(-) diff --git a/_posts/2019-02-13-pset1.md b/_posts/2019-02-13-pset1.md index 9024bae..b498d6c 100644 --- a/_posts/2019-02-13-pset1.md +++ b/_posts/2019-02-13-pset1.md @@ -6,27 +6,73 @@ title: Problem Set 1 ### (a) -How many atoms are there in a yoctamole? +How many atoms are there in a yoctomole? + +Yocto is the SI prefix for $$10^{-24}$$. So there are +$$ +\frac{N_a}{\si{\mol}} \cdot 10^{-24} += \frac{6.022 \cdot 10^{23}}{\si{\mol}} \cdot 10^{-24} += 0.6022 +$$ +atoms in a yoctomole. ### (b) How many seconds are there in a nanocentury? Is the value near that of any important constants? +Nano is the SI prefix for $$10^{-9}$$. + +$$ +\num{1e-9} \si{century} +\cdot \frac{100 \si{years}}{1 \si{century}} +\cdot \frac{365 \si{days}}{1 \si{year}} +\cdot \frac{24 \si{hours}}{1 \si{day}} +\cdot \frac{60 \si{minutes}}{1 \si{hour}} +\cdot \frac{60 \si{\s}}{1 \si{minute}} += 3.15 \si{\s} +$$ + +This is relatively close to $$\pi$$. + ## 2.2 A large data storage system holds on the order of a petabyte. How tall would a 1 petabyte stack of CDs be? How does that compare to the height of a tall building? +CDs are nominally $$1.2 \si{\mm}$$ thick, and store 650 megabytes. (Some actually store more because +they store data in regions the Orange Book standard reserves for manufacturing error.) + +$$ +10^{15} \si{bytes} \cdot \frac{\num{1.2e-3} \si{\m}}{\num{6.5e6} \si{bytes}} += 1.8 \si{\km} +$$ + +Currently the tallest building in the world is $$0.8 \si{km}$$ (the Burj Khalifa). The Jeddah +Tower, currently under construction, is intended to be $$1 \si{km}$$. So for the foreseeable future +the stack of CDs would be roughly twice as tall as any other human-built structure. + ## 2.3 If all the atoms in our universe were used to write an enormous binary number, using one atom per bit, what would that number be (converted to base 10)? +There are about $$10^{80}$$ atoms in the observable universe. So if each of these was used to +encode one bit, we'd have $$10^{80}$$ bits of information. If all of this was used to store one big +unsigned integer, the largest representable value would be $$2^{10^{80}} - 1$$ (not that the 1 makes +any noticeable difference). Every decimal digit encodes $$\log_2(10) \approx 3.32$$ bits of +information, so $$10^{80}$$ bits is equivalent to $$10^{80} / \log_2(10) \approx \num{3e79}$$ +decimal digits of information. Thus the largest representable unsigned integer can also be written +as $$10^\num{3e79}$$. + ## 2.4 Compare the gravitational acceleration due to the mass of the Earth at its surface to that produced by a 1 kg mass at a distance of 1 m. Express their ratio in decibels. +The acceleration due to gravity at the surface of the Earth is $$9.8\si{m.s^{-2}}$$, while that of +a $$1\si{kg}$$ mass at $$1\si{m}$$ is $$G \cdot 1\si{kg} / 1\si{m^2} = \num{6.67e-11} \si{m.s^{-2}}$$. +In decibels this is $$20 \cdot \log_{10} \frac{9.8}{\num{6.67e-11}} = 223 \si{db}$$. + ## 2.5 ### (a) @@ -35,37 +81,152 @@ Approximately estimate the chemical energy in a ton of TNT. You can assume that nitrogen is the primary component; think about what kind of energy is released in a chemical reaction, where it is stored, and how much there is. +TNT is a chemical explosive, meaning its potential energy is stored in chemical bonds. Chemical +bonds are just (relatively) stable atomic states involving multiple atoms (i.e. shared electrons). +I don't know what compounds result from the combustion of TNT, but since it's an exothermic reaction +the atoms must end up in lower energy states on average. So for a rough estimate, I'll compute the +number of nitrogen atoms per ton of TNT, and assume we free around 1 eV per atom during combustion. + +$$ +1 \si{ton} \cdot \frac{\num{907.18e3} \si{g}}{\si{ton}} +\cdot \frac{\si{mol}}{14 \si{g}} +\cdot \frac{\num{6.022e23} \si{atoms}}{\si{mol}} +\cdot \frac{1 \si{eV}}{\si{atom}} +\cdot \frac{\num{1.6e-19} \si{J}}{\si{eV}} += \num{6e9} \si{J} +$$ + +This is off by a factor of about 1.5, which isn't so bad for not knowing what the reaction is. + ### (b) Estimate how much uranium would be needed to make a nuclear explosion equal to the energy in a chemical explosion in 10,000 tons of TNT (once again, think about where the energy is stored). +Nuclear explosions utilize nuclear energy instead of atomic (electromagnetic) energy. So we're +dealing with a typical energy of $$10^6 \si{eV}$$ rather than $$1 \si{eV}$$. On top of that, we're +getting about that much energy per proton or neutron, rather than per atom. Most uranium has 238 +nucleons, but fissionable uranium has only 235. However we're penalized for atomic mass: uranium is +much heavier than nitrogen so there are less atoms of it per ton. So overall uranium should be about +$$10^6 \cdot 235 \cdot 14/235 = \num{1.4e7}$$ times as potent as TNT per unit mass. Thus $$10^4$$ +tons of TNT is roughly equivalent to $$10^4 / \num{1.4e7} = \num{7e-4}$$ tons of fissionable +uranium, which is about 650 grams. + ### (c) Compare this to the *rest mass energy* $$E = mc^2$$ of that amount of material (Chapter 15), which gives the maximum amount of energy that could be liberated from it. +$$ +E = mc^2 = 0.65 \si{kg} \cdot (\num{3e8} \si{m/s})^2 = \num{5.8e16} \si{J} +$$ + +For fun, let's compare this to the gravitational binding energy of the planet. We can calculate this +by calculating the energy required to remove a thin spherical shell of matter from the Earth (moving +it infinitely far away), and integrating this over the radius of the Earth. For each shell, the +spherical ball of matter inside behaves like a point mass, so the binding energy is just +$$G M m / r$$. Assume a constant density $$\rho$$, so that the mass of a sphere of radius $$r$$ is +$$(4/3) \pi r^3 \rho$$, and the mass of the shell on top of it is $$4 \pi r^2 \rho \mathrm{d}r$$. +Thus the binding energy of the shell is $$G ((4/3) \pi r^3 \rho) (4 \pi r^2 \rho \mathrm{d}r) / r$$. +The total energy needed to unbind the Earth is + +$$ +\begin{align*} +E &= \int_0^R \frac{16}{3} G \pi^2 \rho^2 r^4 \mathrm{d}r \\ +&= \frac{16}{3} G \pi^2 \rho^2 \left[ \frac{1}{5} r^5 \right]_0^R \\ +&= \frac{16}{15} G \pi^2 \rho^2 \frac{1}{5} R^5 \\ +\end{align*} +$$ + +Since $$\rho$$ must be $$\frac{3 M}{4 \pi R^3}$$, we have + +$$ +\begin{align*} +E &= \frac{3 G M^2}{5 R} \\ +&= \frac{3 \cdot (\num{6.67e-11} \si{m^3.kg^{-1}.s^{-2}}) \cdot (\num{6e24} \si{kg})^2}{5 \cdot (\num{6.4e6} \si{m})} \\ +&= \num{2e32} \si{J} +\end{align*} +$$ + +So you'd need a lot more than a kilogram of antimatter to turn the Earth to dust. In fact, you'd +need about 3 exagrams (you get twice as much bang for the buck with antimatter since you're +converting it and an equivalent mass of regular matter into energy). Wikipedia tells me this is +about the mass of all coal deposits on Earth. Luckily, we can't currently produce (and catch) more +than billions of antiprotons, which puts us about 14 orders of magnitude away from creating a single +gram. (This also makes it the world's most valuable substance by mass.) + ## 2.6 ### (a) What is the approximate de Broglie wavelength of a thrown baseball? +A baseball weighs $$1.45^{-1} \si{kg}$$. A major league fastball is around 100 miles per hour, +so 160 km per hour, but I'll just go with 100 km per hour since we're not all professional pitchers. + +$$ +\lambda = \frac{h}{p} += \frac{\num{6.626e-34} \si{J.s}}{\num{1.45e-1} \si{kg} \cdot 10^2 \si{km/hour}} +\cdot \frac{\si{hour}}{60 \si{minutes}} \cdot \frac{\si{minute}}{60 \si{s}} += \num{1.3e-35} \si{m} +$$ + ### (b) Of a molecule of nitrogen gas at room temperature and pressure? (This requires either the result of Section 3.4.2, or dimensional analysis.) +By the equipartition theorem, there is $$\frac{1}{2} k T$$ energy in the x, y, and z components +of the molecule's velocity. We know $$E = \frac{1}{2} m v^2$$, and $$p = m v$$, so +$$p = \sqrt{m k T}$$. Since the x, y, and z components add in quadrature, a typical total momentum +will be $$\sqrt{3 m k T}$$. The mass of a molecule of N2 is + +$$ +2 \cdot \frac{14 \si{g}}{\si{mol}} \cdot \frac{\si{mol}}{\num{6.022e23}} += \num{4.6e-23} \si{g} += \num{4.6e-26} \si{kg} +$$ + +Thus + +$$ +\lambda = \frac{h}{p} += \frac{h}{\sqrt{3 m k T}} += \frac{\num{6.626e-34} \si{J.s}}{\sqrt{3 \cdot \num{4.6e-26} \si{kg} \cdot \num{1.38e-23} \si{J/K} \cdot 300 \si{K}}} += \num{2.7e-11} \si{m} +$$ + ### (c) What is the typical distance between the molecules in this gas? +The typical distance can be estimated based on the number of particles per volume. If the volume is +$$V$$, then we can arrange $$n$$ particles on a cubic lattice with a spacing of $$(V / n)^{1/3}$$. +By the ideal gas law, $$V/n = RT/P$$, so the typical distance is + +$$ +\left( \frac{V}{n} \right) ^ \frac{1}{3} += \left( \frac{R T}{P} \right) ^ \frac{1}{3} += \left( \frac{8.3 \si{J/mol/K \cdot 300 K}}{10^5 \si{Pa}} \cdot \frac{\si{mol}}{\num{6.022e23}} \right) ^ \frac{1}{3} += \num{3.5e-9} \si{m} +$$ + ### (d) If the volume of the gas is kept constant as it is cooled, at what temperature does the wavelength become comparable to the distance between the molecules? +The typical spacing depends on the volume of the gas and number of molecules, both of which are +fixed in this scenario. So we just need to solve + +$$ +\num{3.5e-9} \si{m} = \lambda = \frac{h}{\sqrt{3 m k T}} +\implies T = \frac{h^2}{3 m k \lambda^2} += \frac{(\num{6.626e-34} \si{J.s})^2}{3 \cdot \num{4.6e-26} \si{kg} \cdot \num{1.38e-23} \si{J/K} \cdot (\num{3.5e-9} \si{m})^2} += 0.02 K +$$ + ## (2.7) ### (a) @@ -73,24 +234,121 @@ does the wavelength become comparable to the distance between the molecules? The potential energy of a mass m a distance r from a mass $$M$$ is $$−GMm/r$$. What is the escape velocity required to climb out of that potential? +Assuming small and slow enough masses that relativistic corrections are negligible, we just need to +solve + +$$ +E = \frac{1}{2} m v^2 = \frac{G M m}{r} \implies v = \sqrt{\frac{2 G M}{r}} +$$ + ### (b) Since nothing can travel faster than the speed of light (Chapter 15), what is the radius within which nothing can escape from the mass? +$$ +c = \sqrt{\frac{2 G M}{r}} \implies r = \frac{2 G M}{c^2} +$$ + +This derivation is very much not rigorous, since neither the gravitational potential nor kinetic +energy is expressed relativistically (in fact there's no such thing as a gravitational potential in +general relativity, since gravity isn't a force). But remarkably we do end up with the real +Schwarzschild radius. + ### (c) If the rest energy of a mass $$M$$ is converted into a photon, what is its wavelength? +$$ +E = M c^2 = \frac{h c}{\lambda} \implies \lambda = \frac{h c}{M c^2} = \frac{h}{M c} +$$ + ### (d) For what mass does its equivalent wavelength equal the size within which light cannot escape? +$$ +\frac{h}{M c} = \frac{2 G M}{c^2} \implies M = \sqrt{\frac{h c}{2 G}} = \num{3.9e-8} \si{kg} +$$ + ### (e) What is the corresponding size? +Plugging the above formula for $$M$$ into $$\lambda = h/(M c)$$, we find that + +$$ +\lambda = \sqrt{\frac{2 h G}{c^3}} = \num{5.7e-35} \si{m} +$$ + ### (f) What is the energy? + +$$ +E = \frac{hc}{\lambda} = \sqrt{\frac{h c^5}{2 G}} = \num{3.5e9} \si{J} +$$ + +### (g) + +What is the period? + +$$\tau = 1/f$$ and $$\lambda = c / f = c \tau$$, so + +$$ +\tau = \lambda / c = \sqrt{\frac{2 h G}{c ^ 5}} = \num{1.9e-43} \si{s} +$$ + + +## 2.8 + +Consider a pyramid of height H and a square base of side length L. A sphere is +placed so that its center is at the center of the square at the base of the pyramid, +and so that it is tangent to all of the edges of the pyramid (intersecting each edge +at just one point). + +### (a) + +How high is the pyramid in terms of L? + +To fit within the square base, the radius of the sphere must be $$L / 2$$. Now imagine rotating the +square base 90 degrees along one of its diagonals: since the axis of rotation goes through the +center of the sphere, the edges are still tangent. So the height of the pyramid is the same as the +distance from the center of the sphere to any corner of the base square, namely $$L / \sqrt{2}$$. +(This could also be calculated using triangle similarities, but that's a lot more tedious.) + +### (b) + +What is the volume of the space common to the sphere and the pyramid? + +The sphere is tangent to three points on each planar "wall" of the pyramid. The intersection of +each of these planes with the sphere is a circle, and the spherical caps on top of these circles are +the portions outside the pyramid. So we can compute the volume of the intersection of the sphere and +the pyramid by subtracting the volume of these caps from the volume of the (half) sphere. + +The volume of the caps can be computed via an integral over perpendicular distance from the planes, +but to do so we need to know how far these planes are from the center of the sphere. If we align +two of the base square's corners with the X and Y axes (so the base square is the set of points with +L1 norm of 1), and the top of the pyramid along Z, then the normal vector of the planar wall in the +first octant is $$(1/\sqrt{3}, 1/\sqrt{3}, 1/\sqrt{3})$$. The vector from the center of the sphere +to the X base corner is $$(L/\sqrt{2}, 0, 0)$$, so the distance from the center of the sphere to the +plane is $$(L/\sqrt{2}, 0, 0) \cdot (1/\sqrt{3}, 1/\sqrt{3}, 1/\sqrt{3}) = L/\sqrt{6}$$. (Again this +could also be derived from triangle similarities.) + +Thus the volume of a single cap is + +$$ +\begin{align*} +V_\text{cap} &= \int_\frac{L}{\sqrt{6}}^\frac{L}{2} \pi r^2 \mathrm{d}x \\ +&= \int_\frac{L}{\sqrt{6}}^\frac{L}{2} \pi \left( \frac{L^2}{4} - x^2 \right) \mathrm{d}x \\ +&= \left[ \frac{\pi L^2}{4} x \right]_\frac{L}{\sqrt{6}}^\frac{L}{2} - \left[ \frac{\pi x^3}{3} \right]_\frac{L}{\sqrt{6}}^\frac{L}{2} \\ +&= \pi L^3 \left( \frac{1}{12} - \frac{7}{36 \sqrt{6}}\right) +\end{align*} +$$ + +And the volume shared by the sphere and pyramid is + +$$ +\frac{1}{2} \cdot V_\text{sphere} - 4 \cdot V_\text{cap} = \pi L^3 \left( \frac{7}{9 \sqrt{6}} - \frac{1}{4} \right) +$$ -- GitLab