In class, we assumed that all monatomic gases have 3 degrees of freedom (\(f = 3\)). In this question, we explore the possibility that a monatomic gas might have additional degrees of freedom due to the electrons orbiting the nucleus. To answer this question, you will need to use the equipartition theorem and understand how quantized energy levels affect the application of the equipartition theorem.
Helium is a monatomic gas at room temperature. An atom of helium can store energy by bumping its electron from its lowest orbital energy level to a higher orbital energy level. In particular, moving an electron from the lowest state to the first excited state would store an energy of 24.6 eV (24.6 electron-volts). Give a quantitative explanation (i.e. by comparing quantities) that shows we can ignore this energy storage mode when calculating the heat capacity of helium gas at ordinary temperatures.
At \(T=293\) K, \(k_\text{B}T \approx 0.025\) eV. Thus, a system that accepts an energy quanta 24.6 eV is very unlikely to get that energy from the surrounding environment when \(T=293\) K, because that is 1000 times higher than \(k_BT\).
Adapted from Q2M.1 from Chpt 2 of Unit Q, 3rd Edition
Waves of pressure (sound waves) can travel through air. When there are boundary conditions on a sound wave, the allowed frequencies become discretized (i.e. there is a discrete set of possible values). The same thing happens in quantum mechanics with "matter waves". Before getting fully into quantum mechanics, I want to warm up with musical examples. The PDE for pressure waves in a column of air is \begin{align} \frac{\partial^2p}{\partial t^2}=v_\text{s}^2\frac{\partial^2p}{\partial x^2} \end{align} where \(p\) is the pressure at time \(t\) and position \(x\), and \(v_\text{s}\) is a constant called the the speed of sound in air. We will look for solutions of the form \(p(x,t) = \sin(kx)\cos(wt) + \text{constant}\). The pressure at the open end of a pipe is fixed at 1 atmosphere (this boundary condition is called a node, because pressure doesn't fluctuate). If a pipe has a closed end (which may or may not be true for a flute) the pressure at the closed end can fluctuate up and down (this boundary condition would be called an anti-node).
If the flute has two open ends, there will be a pressure node at each end. Thus, the smallest value of \(k\) would be \(\pi/L\). This would give a standing wave \(P=P_0 \sin k x \sin k v t + (1\text{ atm})\) that will satisfy the PDE and the boundary conditions.
This curve would oscillate at an angular frequency \(\omega = v \pi/L\). The cycles per second frequency is \begin{align} f &= \frac{\omega}{ 2\pi} \\ &= \frac{v \pi}{2 \pi L}\\ &= \frac{v}{2 L} \\ &= \frac{340 \text{ m/s}}{2(0.6\text{ m})} = 262 \text{ Hz} \end{align}![]()
If the flute had one open end and one closed end, we expect a pressure node at one end and anti-node at the other end. The smallest value of \(k\) would be \((\pi/2)/L\).
This would give an angular frequency of \(\omega = v \pi /(2 L)\) and the cycles per second freqency is \begin{align} f &= \frac{\omega}{ 2\pi} \\ &= \frac{v \pi}{4 \pi L}\\ &= \frac{v}{4 L} \\ &= \frac{340 \text{ m/s}}{4(0.6\text{ m})} = 131 \text{ Hz} \end{align} I conclude that we should model the flute as open at both ends. The mouth piece has an open hole, and the "foot" of the flute has an open hole. Interestingly, a trumpet has a pressure anti-node at the mouth piece... so the boundary conditions for a trumpet are different than a flute.![]()
Some other standing waves that satify the PDE and boundary conditions for a flute that is 0.6 m in length are
So, the lowest three frequencies are 262 Hz, 524 Hz, and 786 Hz.![]()
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At 290 K we have \(v = 340\) m/s. The temperature rises to 300 K (\(3.4\%\) increase). We know \(v = \sqrt{\gamma P_0/\rho_0}\) where \(\gamma\) is a dimensionless number. When the flute warms up, \(P_0\) does not change (\(P_0 = 1\) atm). When the flute warms up, the density of air, \(\rho_0\), will change. Air behaves like an ideal gas, therefore \begin{align} P_0 V = N k_\text{B} T \rightarrow \frac{N}{V} = \frac{P_0}{k_\text{B} T} \end{align} The mass of air per unit volume is \begin{align} \rho_0 = \frac{m N}{V} = \frac{m P_0}{k_\text{B}T} \quad \text{ where $m$ is average mass of an air molecule} \end{align} We can can substitute that into the velocity equation \begin{align} v = \sqrt{\frac{\gamma P_0 k_\text{B} T}{m P_0}} = \sqrt{\frac{\gamma k_\text{B} T}{m}} \end{align} When \(T\) increases by \(3.4\%\), \(v\) will increase by \(\frac{1}{2}3.4\% = 1.7\%\). We can see this by finding the ratio of \(v_1\) and \(v_2\). \begin{align} \frac{v_2}{v_1} = \frac{\sqrt{\frac{\gamma k_\text{B} T_2}{m}}}{\sqrt{\frac{\gamma k_\text{B} T_1}{m}}} = \sqrt{\frac{T_2}{T_1}} = \sqrt{\frac{300}{290}} = 1.017 \end{align} The pitch of the flute will be \(\omega = k v\) or \(f = k v /(2 \pi)\). The allowed wavenumbers, \(k\), will be the same. Therefore the pitch of the flute increases by \(1.7\%\). This is more than \(1/6\) of a chromatic step. The flute player will have to adjust the length of their flute.
In this question, you analyze a frequency spectrum recorded from a bugle (a demonstration might be done during class). We'll compare the real bugle data to a coarse-grain model, and consider what might be missing from the coarse-grain model.
I found two articles on the internet (links 1 & 2 below) that helped me understand the physics of standing waves in brass instruments.
The resonances from a straight, closed-open pipe produces a complex and otherworldly set of superimposed frequencies, as exemplified by the ethereal sound of the didgeridoo. To get the “classical” pattern of frequencies, the shape of the flare and bell is critical (trumpets, trombones and bugles all have a similiar flare and bell).
The spectrogram shown below was recorded when I played a note on the bugle. This note is a superposition of the bugle's 2nd resonance (240 Hz), the 4th resonance (480 Hz), the 6th resonance (720 Hz) and so forth. Other resonances were not excited when I played this note. (Other resonances could be excited if I played a different note). I am using a standard convention of numbering the lowest resonant frequency as #1, the next highest resonant frequency as #2, and so forth.
Some helpful figures from the internet articles:
The graphs below show waves that have an anti-node a \(x=0\) and a node at \(x=L\). Outside bugle (\(x>L\)) the air pressure returns to normal. I have not shown the small ripple of sound leaving the bugle because pressure oscillations inside the bugle are much bigger than outside).
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Examining the graphs above, the first resonance fits a quarter wavelength inside the bugle (\(\lambda _1/4 =L\)). The second resonance fits three "quarter wavelengths" inside the bugle. The third resonance fits five "quarter wavelengths" inside the bugle. The four resonance fits seven "quarter wavelengths" inside the bugle. Therefore, the wavelengths are \begin{align} \lambda _1 = 4L\\ \lambda _2 = 4L/3\\ \lambda _3 = 4L/5\\ \lambda _4 = 4L/7\\ \end{align} The corresponding frequencies (\(f=v / \lambda\)) are \begin{align} f_1=v/4L\\ f_2=3v/4L\\ f_3=5v/4L\\ f_4=7v/4L\\ \end{align}
- Using the straight-pipe model to get \(f_4=480\) Hz, the length of the pipe would be... \begin{align} f_4&=\frac{7v}{4L}\\ L&=\frac{7v}{4f_4}\\ &=\frac{7(340 \text{ m/s})}{4(480 \text{ s}^{-1})}\\ &=1.24 \text{ m} \end{align}
If we assume \(L = 1.24\) m, the numerical values for other resonant frequencies are \begin{align} f_1 = v/4L = 340 \text{ m/s}/(4\times1.24 \text{m}) = 69 \text{ Hz}\\ f_2 = 3v/4L = 206 \text{ Hz}\\ f_3 = 5v/4L = 343 \text{ Hz}\\ f_4 = 7v/4L = 480 \text{ Hz}\\ \end{align}
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In summary, when we fit the model to the data using the \(f_4\) resonance, the \(f_2\) resonance does not fit. The measured \(f_2\) is higher than predicted by the straight-pipe model. How do I make sense of this? The information from Univ. of New South Wales says: "in the rapidly flaring bell, the long waves (with the low pitches) could be said to be 'least able to follow' the curve of the bell and so are effectively reflected earlier than are the shorter waves. (This is because their wavelengths are very much longer than the radius of curvature of the bell.) One might say therefore that the long waves 'see' an effectively shorter pipe."