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Solutions to Problems 10: Order of Magnitude Physics 1) Electrical ...

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<strong>Solutions</strong> <strong>to</strong> <strong>Problems</strong> <strong>10</strong>: <strong>Order</strong> <strong>of</strong> <strong>Magnitude</strong> <strong>Physics</strong><br />

1) <strong>Electrical</strong> conductivity σ (in the cgs system) has units <strong>of</strong> s −1 . Construct an example <strong>of</strong><br />

a physical process whose characteristic timescale is σ −1 .<br />

Conductivity describes the rate at which charges spread under the influence <strong>of</strong> an<br />

electric field. Consider, therefore, what happens when a charge concentration is created in<br />

a conducting medium. The charge flux is better known as the current density ⃗ J = qn〈v〉,<br />

where q is the charge per carrier, n is the volume density <strong>of</strong> carriers, and 〈v〉 is their mean<br />

drift speed under the influence <strong>of</strong> the electric field. When the mean free path is short<br />

compared <strong>to</strong> the length on which the charge density varies, ⃗ J = σE ⃗ = −σ∇V, for electric<br />

potential V.<br />

We also know from Poisson’s Law that ∇· ⃗E = 4πqn, so the conservation equation for<br />

charge is<br />

q ∂n<br />

∂t +∇·⃗J = 0<br />

q ∂n<br />

∂t +4πσnq = 0<br />

if σ is independent <strong>of</strong> position. As this equation makes clear, the charge density declines<br />

exponentially with timescale σ −1 .<br />

2) There are four quantities with units s −1 relevant <strong>to</strong> the way electromagnetic waves<br />

interact with metals, <strong>of</strong> which three are independent: the conductivity, the conduction<br />

electron collision frequency, the conduction electron plasma frequency, and the frequency<br />

<strong>of</strong> electron transitions from bound states <strong>to</strong> the Fermi level <strong>of</strong> the conduction band.<br />

a) Estimate all four in a typical metal.<br />

We begin with the bound state transition frequency. These transitions have an energy<br />

scale corresponding <strong>to</strong> a slightly inner-shell, i.e., the effective nuclear charge is ≃ 2–3<br />

because a few electrons per a<strong>to</strong>m are out in the conduction band. A<strong>to</strong>mic transition<br />

energies scale ∝ Z 2 , so instead <strong>of</strong> being several eV, they are perhaps ≃ 20 eV. The<br />

corresponding frequency (in radian units) is ω tr ≃ 6×<strong>10</strong> 17 s −1 .<br />

The conduction electron plasma frequency is (4πn e e 2 /m e ) 1/2 , but only the electrons<br />

near enough the Fermi level <strong>to</strong> be able <strong>to</strong> move <strong>to</strong> new states can participate, a fraction<br />

∼ k B T/E F . If the mean volume per a<strong>to</strong>m is ∼ (3Å) 3 and 2 electrons per a<strong>to</strong>m are in the<br />

conduction band, the <strong>to</strong>tal number density <strong>of</strong> conduction electrons is 7×<strong>10</strong> 22 cm −3 . The<br />

Fermi wavenumber k F ∼ (3n e /8π) 1/3 ≃ 2×<strong>10</strong> 7 cm −1 (8π instead <strong>of</strong> 4π because there are<br />

two electron spin states). The Fermi energy E F = (¯hk F ) 2 /2m e = 2 × <strong>10</strong> −13 erg. Then<br />

k B T/E F ≃ 0.2, and<br />

ω p ≃ 7×<strong>10</strong> 15 s −1 .<br />

Given k F , the typical electron speed at the Fermi surface is v F = ¯hk F /m e ≃ 2 ×<br />

<strong>10</strong> 7 cm/s (an amusing numerical coincidence). If the scattering length for collisions with


phonons is 30 Å, we find<br />

Lastly, the conductivity is<br />

If ω < ν c ,<br />

On the other hand, if ω > ν c ,<br />

ν c = 7×<strong>10</strong> 13 s −1 .<br />

σ = ω2 p /4π<br />

ν c −iω .<br />

σ low ≃ 7×<strong>10</strong> 17 s −1 .<br />

σ high ≃ 5i×<strong>10</strong> 17 ω −1<br />

14 s−1 ,<br />

where ω has been scaled in units <strong>of</strong> <strong>10</strong> 14 s −1 .<br />

Thus, if the wave frequency is in the near-infrared or lower (ω < ν c ), the transition<br />

frequencyandtheconductivityaresimilar,theplasmafrequencyistwoorders<strong>of</strong>magnitude<br />

smaller, and the collision frequency is two orders <strong>of</strong> magnitude smaller yet. On the other<br />

hand, asthewavefrequencymovesin<strong>to</strong>theopticalorUVband, theconductivitydiminishes<br />

and becomes mostly imaginary.<br />

b) If their values are ordered according your estimate, discuss the implications for waves<br />

<strong>of</strong> various frequencies encountering the metal: which pass through, which reflect, which are<br />

absorbed, ...?<br />

At very low frequencies (ω < ν c = 7×<strong>10</strong> 13 s −1 ), the conductivity is real and greater<br />

than the wave frequency. In this domain, kc ≃ ± √ 2πi(1+i) √ σω. Complex wavenumbers<br />

indicate decay; the wave is absorbed as it enters the conducting medium.<br />

For all ω > ν c , σ = σ high . When the conductivity has this form, the dispersion relation<br />

is ω 2 = k 2 c 2 +ω 2 p . Thus, for ν c < ω < ω p , the wave is also evanescent inside the conduc<strong>to</strong>r,<br />

and its energy is absorbed.<br />

On the other hand, for ω p < ω < ω tr , the wave can propagate within the conduc<strong>to</strong>r,<br />

but with reduced wave number. Part <strong>of</strong> its energy will be transmitted and part reflected.<br />

Finally, for ω > ω tr , again there is partial transmission and partial reflection, but<br />

the part that enters the medium will be subject <strong>to</strong> absorption by boosting electrons from<br />

bound states <strong>to</strong> the conduction band.<br />

3) Consider the spectroscopy <strong>of</strong> H 2 O molecules.<br />

a) Estimate their characteristic vibrational frequency.<br />

When we first discussed material properties, we estimated the effective spring constant<br />

<strong>of</strong>amolecularbondbyK ∼ 2E b /a 2 . Thecharacteristicscale<strong>of</strong>thevibrationalfrequency is<br />

then ω vib ∼ (2E b /a 2 µ) 1/2 , where µ is the reduced mass <strong>of</strong> the two molecules participating<br />

in the bond. Here, because m H = m O /16, µ ≃ m H . With a binding energy ∼ 3 eV and a<br />

bond length ∼ 1 Å,<br />

ω vib ∼ 2×<strong>10</strong> 13 s −1 .<br />

2


Also because m H ≪ m O , the oxygen a<strong>to</strong>m hardly participates in the motion, so the two<br />

bonds really can be considered separately. Note here and in the next portion <strong>of</strong> this<br />

question that the frequency in Hz is ω/2π.<br />

b) Estimate their characteristic rotational frequency. At room temperature, what’s the highest<br />

rotational quantum number you’d expect <strong>to</strong> be substantially populated? Because water<br />

is an asymmetric molecule, its energy levels also depend on a second quantum number, but,<br />

in the order <strong>of</strong> magnitude spirit, we’ll ignore it here.<br />

The quantum mechanical expression for the energy <strong>of</strong> a rotational state with <strong>to</strong>tal<br />

quantum number J is ¯h 2 J(J + 1)/2I, where I is the moment <strong>of</strong> inertia. If it were a<br />

spherical molecule, the energy differences would be (J + 1)¯h 2 /I when J is the quantum<br />

number <strong>of</strong> the lower state. Water is definitely not spherical, so the axial quantum number<br />

also should be considered, but we’ll ignore that fact in the order <strong>of</strong> magnitude spirit.<br />

Once again because m H ≪ m O , we’ll take the oxygen a<strong>to</strong>m as coinciding with the<br />

center <strong>of</strong> mass <strong>of</strong> the whole molecule. Because the molecule is planar but not linear, two<br />

<strong>of</strong> the principal moments are the same and the third different, but we’ll ignore that, <strong>to</strong>o.<br />

We’ll simply make I ∼ 2m H (sinφa) 2 ≃ 2×<strong>10</strong> −40 gm cm 2 , where sinφ ∼ 1/ √ 2 describes<br />

the degree <strong>to</strong> which this isn’t a linear molecule. We then find that<br />

ω rot ∼ (J +1)¯h/I = 6×<strong>10</strong> 12 (J +1) s −1 .<br />

At the highest rotational quantum number substantially populated, ¯h 2 J ∗ (J ∗ +1)/2I ∼<br />

k B T, so<br />

J ∗ ∼ (2Ik B T) 1/2 /¯h ∼ 4.<br />

c) Estimate their cross section for absorbing pho<strong>to</strong>ns in either rotational or vibrational<br />

transitions when these molecules are in the air.<br />

As shown in class, electric dipole transitions have cross sections in the frame <strong>of</strong> the<br />

a<strong>to</strong>m or molecule<br />

σ(ω) ∼ α fs a 2 0 |M|2 ω 0 Γ/2<br />

(ω −ω 0 ) 2 +(Γ/2) 2,<br />

where Γ is the deexcitation rate <strong>of</strong> the upper state and ω 0 is the resonance frequency.<br />

In air, the molecules are all moving with random thermal motions, so it makes sense <strong>to</strong><br />

analyze the situation in the lab frame and allow for Doppler shifts due <strong>to</strong> the thermal<br />

motions. Because <strong>of</strong> them, even pho<strong>to</strong>ns that are exactly at resonance in the lab frame<br />

are typically <strong>of</strong>f resonance by ∼ (c s /c)ω 0 ∼ <strong>10</strong> −6 in the molecule frame, or an absolute<br />

frequency <strong>of</strong>fset ∼ <strong>10</strong> 7 (ω 0 /<strong>10</strong> 13 s −1 ) s −1 . On the other hand, the collision rate is<br />

∼ nσ coll c s ∼ 2.5×<strong>10</strong> 9 s −1 ,<br />

rather larger than the frequency <strong>of</strong>fset due <strong>to</strong> thermal motions.<br />

Thus, the “pressure broadening” is likely the dominant element, making the cross<br />

section<br />

σ ∼ α fs a 2 0 |M|2 ω 0 /Γ ∼ 1×<strong>10</strong> −15 ω 0<br />

<strong>10</strong> 13 s −1 cm2 .<br />

3


Here we have taken the scaled dipole moment |M| ≃ 1 (it’s actually ≃ 0.8).<br />

4) Microwave ovens generate power at ≃ 6 GHz, and typically produce ∼ 1 kW. It happens<br />

that the lowest frequency rotational transition in water occurs at ≃ 22 GHz. That such<br />

a transition exists should come as a surprise because the characteristic frequency you estimated<br />

in Problem 3 is considerably higher. Its origin turns out <strong>to</strong> lie in a coincidence:<br />

centrifugal bond-stretching leads <strong>to</strong> a near match in energy between a particular state within<br />

the J = 5 set and another particular state in the J = 6 set. In any event, the microwave<br />

frequency is well below even this resonance.<br />

a) Estimate how deeply in<strong>to</strong> the food the microwaves penetrate.<br />

As noted in the solution <strong>to</strong> part c) <strong>of</strong> the previous problem, the cross section for<br />

absorption <strong>of</strong> an electromagnetic wave in a rotational transition <strong>of</strong> water is ∝ [(ω −<br />

ω 0 ) 2 + (Γ/2) 2 ] −1 . In the problem at hand, however, the frequency <strong>of</strong>fset is ≃ 16 GHz∼<br />

1 ×<strong>10</strong> 11 s −1 . The collision rate is even greater, ∼ 5 ×<strong>10</strong> 12 s −1 . Consequently, the pho<strong>to</strong>n<br />

absorption cross section is still determined primarily by the intrinsic breadth <strong>of</strong> the<br />

resonance Γ. In this context, it is 5×<strong>10</strong> −21 cm 2 because the resonance frequency is only<br />

∼ <strong>10</strong> 11 s −1 and the collision rate is rather greater.<br />

The number density <strong>of</strong> water molecules is 6×<strong>10</strong> 23 /18 = 3×<strong>10</strong> 22 cm −3 . However, only<br />

a fraction <strong>of</strong> them are in the ground state <strong>of</strong> the relevant transition. If its ground state<br />

is J = 5, its population is reduced by perhaps a fac<strong>to</strong>r <strong>of</strong> 2 because the energy <strong>to</strong> reach<br />

it is ∼ k B T. More importantly, each angular momentum state has a multiplicity 2J +1,<br />

so that there are 35 states at lower or comparable energy. Thus, the fraction <strong>of</strong> water<br />

molecules in the J = 5 state might be ∼ 1% <strong>of</strong> the <strong>to</strong>tal. The predicted absorption length<br />

is then ∆r ≃ 0.7 cm.<br />

b) The interaction between microwaves and water molecules can also be viewed in terms<br />

<strong>of</strong> classical physics because there are very many pho<strong>to</strong>ns in the microwaves. From that<br />

point <strong>of</strong> view, the interaction between microwaves and molecules is through the classical<br />

<strong>to</strong>rque ⃗ d · ⃗E that tries <strong>to</strong> swing the dipole in<strong>to</strong> alignment with the electric field. What is<br />

the instantaneous energy advantage <strong>to</strong> alignment?<br />

The potential energy <strong>of</strong> a dipole in an external field is ∆E = − ⃗ E·⃗d. We already know<br />

the magnitude <strong>of</strong> the permanent dipole in water. The magnitude <strong>of</strong> the electric field can<br />

be estimated from the power <strong>of</strong> the oven and its electromagnetic “reverberation time”.<br />

We’ll assume that the food in the oven absorbs any wave energy that strikes it (<strong>to</strong> be<br />

justified below), but also that it occupies only ∼ <strong>10</strong>% <strong>of</strong> the cross sectional area <strong>of</strong> the<br />

oven. If so, the waves are absorbed after ∼ <strong>10</strong> crossings <strong>of</strong> the oven. At c, each crossing<br />

takes 1.6×<strong>10</strong> −9 s for a typical oven, 1/2 m across. Consequently, the electromagnetic field<br />

energy in the oven at any given time is ∼ 1×<strong>10</strong> −5 J, or ∼ <strong>10</strong>0 erg. Half <strong>of</strong> this energy is<br />

in electric field, half in magnetic. Given a volume ∼ (1/8) m 3 ∼ <strong>10</strong> 5 cm 3 , that’s an energy<br />

density ∼ <strong>10</strong> −3 erg cm −3 . Setting this energy density equal <strong>to</strong> E 2 /8π implies an rms field<br />

strength E rms ∼ 0.15 dyne/esu. Applied <strong>to</strong> a dipole the size <strong>of</strong> water’s (2×<strong>10</strong> −18 esu cm),<br />

the alignment energy is<br />

∆ǫ = −3×<strong>10</strong> −19 erg.<br />

Note that this is much smaller than the energy <strong>of</strong> the rotational transition nearest in<br />

frequency.<br />

4


c) Extra Credit: Those <strong>of</strong> you with more background in statistical mechanics may want <strong>to</strong><br />

pursue the consequences <strong>of</strong> the fact that ∆ǫ ≪ kT for the rate at which the microwaves<br />

heat the water. Hint: How does the collision frequency compare <strong>to</strong> the wave frequency?<br />

What follows from that comparison?<br />

Asestimated inthe previousproblem, the collisionfrequency is∼ 5×<strong>10</strong> 12 s −1 , which is<br />

≫ ω. That means a typical molecule undergoes many many collisions with other molecules<br />

during a time when the electric field hardly changes at all due <strong>to</strong> its oscillation. If the<br />

field were truly constant, the collisions would lead <strong>to</strong> a thermodynamic equilibrium in<br />

which the small energy advantage <strong>of</strong> aligning the dipoles with the field leads <strong>to</strong> a slightly<br />

greater population pointing in that direction. Approximating the distribution function<br />

<strong>of</strong> dipole directions as an exactly isotropic component plus an exactly aligned and an<br />

exactly anti-aligned component, the relative probability <strong>of</strong> the aligned and anti-aligned are<br />

e ±∆ǫ/kT . Because ∆ǫ/kT ≪ 1, the exponential can be expanded <strong>to</strong> first-order in terms<br />

<strong>of</strong> its argument, and the population contrast in the aligned and anti-aligned directions<br />

is ∼ ±∆ǫ/kT ≃ 7 × <strong>10</strong> −6 . There are slightly more aligned molecules, and they have<br />

slightly lower potential energy; there are slightly fewer anti-aligned molecules, and they<br />

have slightly higher potential energy. The result is that the system as a whole has a<br />

potential energy ∼ 2(∆ǫ) 2 /kT per molecule lower than it would otherwise.<br />

After what, on the collision timescale, is a very long time, the direction <strong>of</strong> the electric<br />

field changes sign. At this point, the relative roles <strong>of</strong> aligned and anti-aligned switch. Now<br />

the effect <strong>of</strong> the electric field is <strong>to</strong> swing the newly anti-aligned molecules in<strong>to</strong> alignment.<br />

As they rotate, there are many collisions, and the work done by the field is transformed<br />

in<strong>to</strong> heat. Thus, every sign flip in the field (which happens twice per wave period) injects<br />

∼ ∆ǫ) 2 /kT per molecule <strong>of</strong> heat in<strong>to</strong> the water. The heating rate per molecule is therefore<br />

H ∼ [(∆ǫ) 2 /kT]4πω,<br />

where the extra fac<strong>to</strong>r <strong>of</strong> two comes from two sign flips per wave period.<br />

Note that because H ∝ (∆ǫ) 2 , and ∆ǫ ∝ | ⃗ E|, the heating rate is proportional <strong>to</strong> the<br />

microwave power, as it should be.<br />

d) What would you predict for the heating rate if a small sample <strong>of</strong> ice were placed in a<br />

microwave oven?<br />

Zero. Water molecules in ice can’t rotate, so they cannot be put in<strong>to</strong> an excited state<br />

<strong>of</strong> rotation.<br />

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