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Molecular Vibrations

From the ladder to a spectrum

Lecture 4.2 found the vibrational levels of a bond, Ev=ℏω(v+12)E_v = \hbar\omega\left(v + \frac{1}{2}\right), evenly spaced by ℏω\hbar\omega. A molecule absorbs a photon when the photon energy hνh\nu matches the gap between two levels. This lecture asks which gaps light can actually bridge, what the measured lines reveal about bonds, and how real molecules differ from the perfect spring.

Spectroscopists count in wavenumbers

Infrared spectra are plotted against the wavenumber ν~=1/λ\tilde{\nu} = 1/\lambda, the number of wavelengths per centimeter. It is proportional to the photon’s energy and frequency:

E=hν=hcλ=hc ν~E = h\nu = \frac{hc}{\lambda} = hc\,\tilde{\nu}

So any energy divided by hchc becomes a wavenumber. For the oscillator, with ℏω=hc ν~\hbar\omega = hc\,\tilde{\nu}:

quantityvaluewhat it tells you
1 cm−1^{-1}1.986×10−231.986\times10^{-23} J =1.240×10−4= 1.240\times10^{-4} eV =0.01196= 0.01196 kJ/molthe conversion factor hchc
1 eV8066 cm−1^{-1}a typical chemical-bond scale is a few eV
kBTk_BT at 300 K208 cm−1^{-1}below this, levels are thermally populated
bond vibrations200 to 4400 cm−1^{-1}wavelengths 2.3 to 50 μm: the infrared

Which transitions light can drive

Start with a puzzle. N2_2 vibrates at 2330 cm−1^{-1} and HCl at 2886 cm−1^{-1}. Both lie in the middle of the infrared, and both ladders have rungs spaced to match an infrared photon. Yet the air, mostly N2_2, is transparent to that light, while HCl gas absorbs it strongly. Matching the photon to a gap is only the tuning. Something else decides whether the molecule can take the photon at all.

Light pushes on the dipole

Light is an oscillating electric field, written E\mathcal{E} here because EE is an energy. Its wavelength, a few micrometers, is about 3×1043\times10^4 times the length of the HCl bond. So the field is uniform across the molecule, and it does the one thing a uniform field can do: push positive charges one way and negative charges the other. It therefore couples to the dipole moment MM, with energy −ME-M\mathcal{E}. (Chemistry texts often write the dipole moment as μ\mu, but here μ\mu is the reduced mass, and a lowercase dd would look like a differential.)

The dipole depends on the bond length: M(x)M(x), with x=R−Rex = R - R_e the stretch. The force the field exerts on the stretch is

F=−ddx(−M(x) E)=M′(x) EF = -\frac{d}{dx}\Big(-M(x)\,\mathcal{E}\Big) = M'(x)\,\mathcal{E}

The field’s handle on the bond is the slope of the dipole, not the dipole itself. A vibrating bond with M′≠0M' \neq 0 is a tiny antenna: its dipole oscillates at the vibration frequency and couples to light at that frequency.

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Fig. Top: HCl vibrating, with the partial charges δ+\delta+ on H and δ−\delta- on Cl. Its dipole (orange bar) grows and shrinks with the bond length, so M(t)M(t) oscillates about its equilibrium value MeM_e; that oscillation couples to light. Bottom: N2_2 has no dipole at any bond length, so there is nothing for the light to push on. The stretch is exaggerated.

A stationary state is not an antenna

The classical picture says what to look for: a dipole that oscillates. An energy eigenstate cannot supply one. Its density ∣ψv∣2|\psi_v|^2 never changes in time (Lecture 3.7), so its average dipole is constant. A molecule that absorbs a photon passes through a superposition of the two levels, and Lecture 3.7 showed that a superposition moves at the Bohr frequencies. Apply that result to the dipole. Take real coefficients and the real oscillator states:

Ψ(x,t)=cv ψv e−iEvt/ℏ+cv′ ψv′ e−iEv′t/ℏ\Psi(x, t) = c_v\,\psi_v\,e^{-iE_vt/\hbar} + c_{v'}\,\psi_{v'}\,e^{-iE_{v'}t/\hbar}

The density has two constant parts and one cross term, whose two phases combine into a cosine (eiθ+e−iθ=2cos⁡θe^{i\theta} + e^{-i\theta} = 2\cos\theta):

∣Ψ∣2=cv2 ψv2+cv′2 ψv′2+2cvcv′ ψvψv′cos⁡ωv′vt,ωv′v=Ev′−Evℏ|\Psi|^2 = c_v^2\,\psi_v^2 + c_{v'}^2\,\psi_{v'}^2 + 2c_vc_{v'}\,\psi_v\psi_{v'}\cos\omega_{v'v}t, \qquad \omega_{v'v} = \frac{E_{v'} - E_v}{\hbar}

Weight it by the dipole and integrate, ⟨M⟩=∫M(x) ∣Ψ∣2 dx\langle M\rangle = \int M(x)\,|\Psi|^2\,dx:

Two readings of the same integral are worth keeping:

The same integral decided which lines an electron in a box can emit in Lecture 3.7, where parity removed the frequency ω31\omega_{31}. Here it decides which rungs light can climb.

Each term of the dipole has one job

Expand the dipole about ReR_e:

M(x)=Me+M′x+12M′′x2+…,M′=(∂M∂x)ReM(x) = M_e + M'x + \frac{1}{2}M''x^2 + \dots, \qquad M' = \left(\frac{\partial M}{\partial x}\right)_{R_e}

Sandwich it between two vibrational states:

⟨v′∣M^∣v⟩=Me ⟨v′∣v⟩+M′ ⟨v′∣x^∣v⟩+12M′′ ⟨v′∣x^2∣v⟩+…\langle v'|\hat{M}|v\rangle = M_e\,\langle v'|v\rangle + M'\,\langle v'|\hat{x}|v\rangle + \frac{1}{2}M''\,\langle v'|\hat{x}^2|v\rangle + \dots
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Fig. What each term of the dipole does to the ground state, in units with α=1\alpha = 1. Top: multiplying ψ0\psi_0 (gray dashed) by 1, xx or x2x^2 gives the orange function. xψ0x\psi_0 lies exactly on ψ1/2\psi_1/\sqrt{2} (teal dotted), and x2ψ0x^2\psi_0 is 12ψ0\frac{1}{2}\psi_0 plus ψ2/2\psi_2/\sqrt{2}. Bottom: the components ⟨v′∣⋅∣0⟩\langle v'|\cdot|0\rangle of each result. The purple bar (v′=0v' = 0) leaves the molecule where it was; the orange bars are transitions.

Slosh or breathe

The widget shows the antenna at work. It mixes v=0v = 0 with a higher level v′v' and draws the density, the dipole function M(x)M(x), and the swing of ⟨M⟩(t)\langle M\rangle(t). Switch the terms of M(x)M(x) on and off and watch which lines light up.

One rung at a time

The slope term is by far the largest, so keep it alone. Position connects only neighboring levels, ⟨v′∣x^∣v⟩=0\langle v'|\hat{x}|v\rangle = 0 unless v′=v±1v' = v \pm 1, so in a harmonic bond light climbs one rung at a time, and every allowed jump absorbs the same wavenumber ν~\tilde{\nu}.

Where the molecules start

A spectrum also depends on which levels are occupied. By the Boltzmann factor, the population of v=1v = 1 relative to v=0v = 0 is e−ν~/(kBT/hc)e^{-\tilde{\nu}/(k_BT/hc)}; for HCl at 300 K that is e−2886/208≈10−6e^{-2886/208} \approx 10^{-6} (Lecture 4.1). Nearly every molecule starts in v=0v = 0, so the absorption is the single jump 0→10 \to 1, called the fundamental: one strong line per infrared-active vibration.

Stiffness and mass set the wavenumber

The vibrational wavenumber has two knobs, ν~=12πck/μ\tilde{\nu} = \frac{1}{2\pi c}\sqrt{k/\mu}: a stiff bond raises it, heavy atoms lower it. The force constant follows from a measured wavenumber, k=μ (2πcν~)2k = \mu\,(2\pi c\tilde{\nu})^2:

moleculeν~\tilde{\nu} (cm−1^{-1})μ\mu (u)kk (N/m)infrared
H2_244010.504575inactive
HF41380.957966active
HCl29910.980516active
HBr26490.995411active
HI23091.000314active
N2_223597.002295inactive
CO21706.861902active
NO19047.471595active
O2_215808.001177inactive
Cl2_256017.5323inactive
I2_221563.5172inactive
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Fig. Harmonic wavenumbers of common diatomic molecules. Top row: one partner is hydrogen, so μ≈1\mu \approx 1 u (0.5 u for H2_2). Bottom row: two heavy atoms. Filled circles absorb infrared light; hollow ones have no dipole at any bond length and do not.

Real bonds are anharmonic

The harmonic levels assume the parabola continues forever. The real bond potential (the Morse curve of Lecture 4.1) is steeper on the compressed side and flattens toward dissociation on the stretched side. Near the bottom the two agree; higher up they do not:

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Fig. Vibrational levels of HCl in the harmonic approximation (left) and in a Morse potential fitted to HCl (right); the lowest three levels are teal. The harmonic steps are equal and never end. The Morse steps shrink as the energy rises, and above the last level the atoms come apart. DeD_e is the depth of the well from its bottom, D0D_0 the energy needed to dissociate from v=0v = 0.

The levels of the Morse potential can be found exactly. The harmonic formula gains one correction term:

G(v)=ν~e(v+12)−ν~exe(v+12)2G(v) = \tilde{\nu}_e\left(v + \frac{1}{2}\right) - \tilde{\nu}_ex_e\left(v + \frac{1}{2}\right)^2
G(v+1)−G(v)=ν~e−ν~exe[(v+32)2−(v+12)2]=ν~e−2ν~exe(v+1)G(v + 1) - G(v) = \tilde{\nu}_e - \tilde{\nu}_ex_e\left[\left(v + \tfrac{3}{2}\right)^2 - \left(v + \tfrac{1}{2}\right)^2\right] = \tilde{\nu}_e - 2\tilde{\nu}_ex_e(v + 1)

It falls by 2ν~exe2\tilde{\nu}_ex_e per rung and reaches zero near v+1=1/2xev + 1 = 1/2x_e. A Morse bond has a finite number of bound levels; above them, the atoms are free.

Overtones and hot bands

In an anharmonic well the selection rule Δv=±1\Delta v = \pm 1 is no longer strict. The states are not exactly harmonic, so x^\hat{x} connects levels further apart, and the dipole has its own curvature M′′M''. Jumps 0→20 \to 2, 0→30 \to 3, ... become weakly allowed: the overtones, each tens of times weaker than the one before.

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Fig. Left: absorption from v=0v = 0 of HCl to v=1v = 1 (fundamental), v=2v = 2 (first overtone) and v=3v = 3 (second overtone), drawn on the anharmonic ladder. Right: the lines they produce, on a logarithmic intensity scale (schematic). Because the steps shrink, the first overtone sits below twice the fundamental.

Polyatomic molecules: one oscillator per normal mode

A molecule with NN atoms has 3N−63N - 6 normal modes (3N−53N - 5 if linear), Lecture 4.1. Near equilibrium the vibrational Hamiltonian is a sum of independent harmonic oscillators, one per mode, so by the separable-Hamiltonian rule of Lecture 4.1 the energies add. Each mode has its own wavenumber, and its own selection rule:

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Fig. The normal modes of CO2_2, with the measured wavenumbers. The orange arrow is the molecule’s dipole moment, computed from partial charges +2q+2q on C and −q-q on each O. In the symmetric stretch the two halves cancel at every instant, so the dipole stays zero. In the antisymmetric stretch and the bend it swings, along the axis and across it. The bend can happen in two perpendicular planes, so there are two bends with the same wavenumber.

Reading an infrared spectrum

In a larger molecule, a bond such as C=O or O−-H vibrates almost like an isolated diatomic spring. Its wavenumber depends mostly on the two atoms and the bond order, and hardly on the rest of the molecule. These group frequencies let a chemist read functional groups off a spectrum:

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Fig. Typical wavenumber ranges of common bond stretches. Below about 1500 cm−1^{-1} (gray), single-bond stretches and bends overlap into a pattern unique to each molecule, its fingerprint.

Amide I vibration of a protein probed by two-dimensional infrared spectroscopy

The amide I vibration of a protein backbone, mostly the C=O stretch of each amide group (left), probed by two-dimensional infrared spectroscopy (right).

Normal mode analysis: finding the modes

The normal modes of water in Lecture 4.1 came from a computer. Here is how they are found, in five steps. The tools are the Taylor expansion of Lecture 4.1 and the matrices of Lecture 3.5.

Step 1: the potential near the minimum, in every coordinate at once

For one bond, Lecture 4.1 expanded the potential about its minimum and kept the first term that survives:

V(x)≈12k x2,k=d2Vdx2V(x) \approx \frac{1}{2}k\,x^2, \qquad k = \frac{d^2V}{dx^2}

A molecule has many displacements x1,x2,…x_1, x_2, \dots, one per atomic coordinate. The Taylor expansion works the same way with all of them at once:

V=Vmin⁡+∑i∂V∂xi xi+12∑i,j∂2V∂xi ∂xj xixj+…V = V_{\min} + \sum_i \frac{\partial V}{\partial x_i}\,x_i + \frac{1}{2}\sum_{i,j}\frac{\partial^2 V}{\partial x_i\,\partial x_j}\,x_ix_j + \dots

Measure VV from the minimum, where every slope ∂V/∂xi\partial V/\partial x_i vanishes. The first term that survives is again the quadratic one:

V≈12∑i,jKij xixj,Kij=∂2V∂xi ∂xjV \approx \frac{1}{2}\sum_{i,j} K_{ij}\,x_ix_j, \qquad K_{ij} = \frac{\partial^2 V}{\partial x_i\,\partial x_j}

The matrix KK of second derivatives is the Hessian: a force constant for every pair of coordinates. A diagonal entry KiiK_{ii} is the stiffness against moving coordinate ii alone. An off-diagonal entry KijK_{ij} says how moving coordinate jj changes the force on coordinate ii.

Step 2: Newton’s equations are coupled

The force on coordinate ii is minus the slope of the potential, −∂V/∂xi=−∑jKijxj-\partial V/\partial x_i = -\sum_j K_{ij}x_j. (For CO2_2: −∂V/∂x1=k(x2−x1)-\partial V/\partial x_1 = k(x_2 - x_1), which is minus the first row of KK times x\mathbf{x}.) So

mi x¨i=−∑jKij xjm_i\,\ddot{x}_i = -\sum_j K_{ij}\,x_j

Because of the off-diagonal entries, the equation for each atom contains the positions of its neighbors: the atoms are coupled. Pull one oxygen of CO2_2 and let go, and the motion of each atom is a tangle:

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Fig. CO2_2 after its left oxygen is pulled outward and released (one spring per bond, center of mass fixed). Top: the displacement of each atom mixes two frequencies, and energy passes back and forth between the atoms. Bottom: the same motion written in the normal coordinates of Step 4 is two independent cosines, one per mode.

Step 3: weight by the masses, and look for a mode

The masses differ from atom to atom. In the coordinates qi=mi xiq_i = \sqrt{m_i}\,x_i every atom behaves as if it had unit mass:

q¨i=−∑jFij qj,Fij=Kijmimj\ddot{q}_i = -\sum_j F_{ij}\,q_j, \qquad F_{ij} = \frac{K_{ij}}{\sqrt{m_im_j}}

A normal mode is all the atoms moving in step. Look for a motion in which every coordinate oscillates at the same frequency, keeping fixed proportions u\mathbf{u}:

q(t)=ucos⁡ωt\mathbf{q}(t) = \mathbf{u}\cos\omega t

This is a guess, an ansatz, like the Gaussian tried for the oscillator ground state in Lecture 4.2: substitute it into Newton’s equation and see which u\mathbf{u} and ω\omega make it work. Step 4 justifies it, by showing that every motion is a sum of such solutions. Two time derivatives give q¨=−ω2 ucos⁡ωt\ddot{\mathbf{q}} = -\omega^2\,\mathbf{u}\cos\omega t. Newton’s equation gives q¨=−Fucos⁡ωt\ddot{\mathbf{q}} = -F\mathbf{u}\cos\omega t. The two agree at every instant only if

F u=ω2 uF\,\mathbf{u} = \omega^2\,\mathbf{u}

Finding the normal modes means finding the eigenvectors of FF (the shapes of the motion) and its eigenvalues (the squared frequencies). CO2_2’s 3×33\times3 matrix has three: a translation with ω=0\omega = 0, the symmetric stretch and the antisymmetric stretch (worked out below). FF is a real symmetric matrix, Fij=FjiF_{ij} = F_{ji}, like the Hermitian matrices of Operators 2, so its eigenvalues are real and its eigenvectors are perpendicular:

F uk=ωk2 uk,uk⋅ul=δklF\,\mathbf{u}_k = \omega_k^2\,\mathbf{u}_k, \qquad \mathbf{u}_k\cdot\mathbf{u}_l = \delta_{kl}

Step 4: project onto the modes, and they come apart

Step 3 found special motions, each at a single frequency. Now show that every motion is made of them, and that they never disturb one another.

  1. The eigenvectors are axes. With nn coordinates there are nn perpendicular unit eigenvectors, a full set of axes for q\mathbf{q}. Any configuration is a combination of them,

q=∑kQk uk,Qk=uk⋅q\mathbf{q} = \sum_k Q_k\,\mathbf{u}_k, \qquad Q_k = \mathbf{u}_k\cdot\mathbf{q}

The normal coordinate QkQ_k is the component of q\mathbf{q} along the axis uk\mathbf{u}_k. Three symbols carry the whole argument, so keep them apart:

symbolwhat it ischanges in time?CO2_2 example
q(t)\mathbf{q}(t)the configuration: every mass-weighted displacement at time tt, one entry per coordinateyes(mO x1, mC x2, mO x3)(\sqrt{m_O}\,x_1,\ \sqrt{m_C}\,x_2,\ \sqrt{m_O}\,x_3)
uk\mathbf{u}_knormal mode kk: a fixed unit vector, the shape of the motion, an eigenvector of FFnousym=(−1,0,1)/2\mathbf{u}_{\text{sym}} = (-1, 0, 1)/\sqrt{2}
Qk(t)Q_k(t)the normal coordinate: one number, how much of mode kk is present now, Qk=uk⋅qQ_k = \mathbf{u}_k\cdot\mathbf{q}yesQsym(t)=Acos⁡ωsymtQ_{\text{sym}}(t) = A\cos\omega_{\text{sym}}t

The configuration is (how much) times (shape), summed over the modes. It has the structure of a state written in a basis, ψ=∑ncnψn\psi = \sum_n c_n\psi_n (Lecture 3.6): q\mathbf{q} plays ψ\psi, the fixed uk\mathbf{u}_k play the basis functions ψn\psi_n, and the QkQ_k play the coefficients cnc_n, found by the same kind of projection. The difference is that the QkQ_k oscillate as cosines, where the cnc_n only turn their phases. In the guess of Step 3, a single Qk(t)=cos⁡ωktQ_k(t) = \cos\omega_kt and every other QQ is zero.

  1. Project Newton’s equation onto one axis. Take the dot product of q¨=−Fq\ddot{\mathbf{q}} = -F\mathbf{q} with uk\mathbf{u}_k, one step at a time:

Q¨k=uk⋅q¨the axis uk does not move=−uk⋅(Fq)Newton’s equation=−(Fuk)⋅qF is symmetric=−ωk2 uk⋅quk is an eigenvector=−ωk2 Qk\begin{aligned} \ddot{Q}_k &= \mathbf{u}_k\cdot\ddot{\mathbf{q}} && \text{the axis } \mathbf{u}_k \text{ does not move} \\ &= -\mathbf{u}_k\cdot(F\mathbf{q}) && \text{Newton's equation} \\ &= -(F\mathbf{u}_k)\cdot\mathbf{q} && F \text{ is symmetric} \\ &= -\omega_k^2\,\mathbf{u}_k\cdot\mathbf{q} && \mathbf{u}_k \text{ is an eigenvector} \\ &= -\omega_k^2\,Q_k \end{aligned}

The third line moves FF from one side of the dot product to the other. That is allowed for a symmetric matrix: a⋅(Fb)=∑ijaiFijbj=∑ijbjFjiai=(Fa)⋅b\mathbf{a}\cdot(F\mathbf{b}) = \sum_{ij}a_iF_{ij}b_j = \sum_{ij}b_jF_{ji}a_i = (F\mathbf{a})\cdot\mathbf{b}.

  1. Read the result. Only QkQ_k appears on the right: no other normal coordinate. Each one obeys its own spring equation, Qk(t)=Akcos⁡(ωkt+φk)Q_k(t) = A_k\cos(\omega_kt + \varphi_k), whatever the others are doing. The modes are independent, as in the bottom panel of the figure above.

Step 5: the Hamiltonian becomes a sum

The same change of coordinates splits the energy. In the mass-weighted coordinates the kinetic energy is ∑i12mix˙i2=12∑iq˙i2\sum_i \frac{1}{2}m_i\dot{x}_i^2 = \frac{1}{2}\sum_i\dot{q}_i^2 and the potential energy is 12∑ijKijxixj=12∑ijFijqiqj\frac{1}{2}\sum_{ij}K_{ij}x_ix_j = \frac{1}{2}\sum_{ij}F_{ij}q_iq_j, so

H=12 q˙⋅q˙+12 q⋅FqH = \frac{1}{2}\,\dot{\mathbf{q}}\cdot\dot{\mathbf{q}} + \frac{1}{2}\,\mathbf{q}\cdot F\mathbf{q}

Now insert q=∑kQkuk\mathbf{q} = \sum_k Q_k\mathbf{u}_k. Every product of two different eigenvectors is zero, uk⋅ul=δkl\mathbf{u}_k\cdot\mathbf{u}_l = \delta_{kl}, so the double sums collapse to single sums:

q˙⋅q˙=∑k,lQ˙kQ˙l uk⋅ul=∑kQ˙k2,q⋅Fq=∑k,lQkQl uk⋅(Ful)=∑k,lQkQl ωl2 δkl=∑kωk2Qk2\dot{\mathbf{q}}\cdot\dot{\mathbf{q}} = \sum_{k,l}\dot{Q}_k\dot{Q}_l\,\mathbf{u}_k\cdot\mathbf{u}_l = \sum_k\dot{Q}_k^2, \qquad \mathbf{q}\cdot F\mathbf{q} = \sum_{k,l}Q_kQ_l\,\mathbf{u}_k\cdot(F\mathbf{u}_l) = \sum_{k,l}Q_kQ_l\,\omega_l^2\,\delta_{kl} = \sum_k\omega_k^2Q_k^2
H=∑k(12Q˙k2+12ωk2Qk2)=∑kHkH = \sum_k\left(\frac{1}{2}\dot{Q}_k^2 + \frac{1}{2}\omega_k^2Q_k^2\right) = \sum_k H_k

The widget runs the CO2_2 stretches live. Choose how much of each mode the molecule holds, or pull one oxygen, and compare the two ways of splitting the same energy:

numpy finds the same three modes from the mass-weighted matrix:

omega^2 in units of k/mO: [0.    1.    3.667]
antisymmetric / symmetric frequency: 1.915
antisymmetric mode, O C O: [ 1.    -2.667  1.   ]

Problems

Problem 1: Bond order from wavenumbers

The C−-O stretch of methanol absorbs near 1033 cm−1^{-1}, the C=O stretch of formaldehyde near 1746 cm−1^{-1}, and the C≡\equivO stretch of carbon monoxide at 2143 cm−1^{-1}. Treat each as a C−-O diatomic spring and find the ratio of the three force constants. How close is it to 1 : 2 : 3?

Problem 2: Which molecules absorb?

Which of these have an infrared-active fundamental: HBr, O2_2, NO, H2_2? For the linear molecule OCS (O=C=S), which of its four modes absorb? Compare with CO2_2 and explain the difference.

Problem 3: How many bound levels?

Using ν~e=2990\tilde{\nu}_e = 2990 cm−1^{-1} and ν~exe=52\tilde{\nu}_ex_e = 52 cm−1^{-1} for HCl, find the highest bound vibrational level and the well depth DeD_e that this Morse potential implies. Compare with the actual De=4.62D_e = 4.62 eV.

Problem 4: Hot bands as a thermometer

Find the wavenumber of the HCl hot band v=1→2v = 1 \to 2. Estimate its intensity relative to the fundamental at 300 K and at 1000 K, assuming both transitions are equally strong per molecule. Why could the ratio serve as a thermometer?

Problem 5: Why bonds to hydrogen absorb high

A C−-H stretch absorbs near 2900 cm−1^{-1} and a C−-C stretch near 1000 cm−1^{-1}. Compute both force constants, treating each bond as a diatomic spring. Is the C−-H bond much stiffer?

Problem 6: Nitrous oxide

N2_2O is linear, N=N=O. How many normal modes does it have? Its stretches absorb near 1285 and 2224 cm−1^{-1} and its bend near 589 cm−1^{-1}, and all of them are infrared active. Why is the “symmetric” stretch active here when the one in CO2_2 is not?

Problem 7: A Birge-Sponer estimate

For an anharmonic bond the gap ΔG(v)=G(v+1)−G(v)\Delta G(v) = G(v + 1) - G(v) falls linearly with vv. Using the HCl constants of the overtone example, sketch ΔG\Delta G against vv, find where it reaches zero, and use the area under the line (the sum of all the gaps) to estimate D0D_0. Compare with the measured 4.43 eV.

Problem 8: One line, four units

Carbon monoxide absorbs at 2143 cm−1^{-1}. Give the photon’s wavelength, frequency and energy (in eV and kJ/mol), and the fraction of CO molecules in v=1v = 1 at 300 K.