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Change variables in equation 7.83 to λ=hc/ϵ and thus derive a formula for the photon spectrum as a function of wavelength. Plot this spectrum, and find a numerical formula for the wavelength where the spectrum peaks, in terms of hc/kT. Explain why the peak does not occur at hc/(2.82kT).

Short Answer

Expert verified

Hence, formula for the photon spectrum as a function of wavelength isu(l)=8π(kT)4(hc)31l51e1/l-1

Step by step solution

01

Given information

Changing variables in equation 7.83 to λ=hc/ϵ and thus deriving a formula for the photon spectrum as a function of wavelength.

02

Explanation

The equation 7.83 is:

UV=8π(hc)30ϵ3eϵ/kT-1dϵ(1)

Change the variables to the wavelength using,

ϵ=hcλdϵ=-hcλ2dλ

Substitute this into (1)

UV=-8π(hc)30(hc)4λ51ehc/kTλ-1dλ

03

Calculations

By changing the integration boundaries, at ϵ=0the wavelength isand atϵ=the wavelength is zero.

localid="1647752119716">UV=8πhc01λ51ehc/kTλ-1dλUV=8πhc01λ51ehc/kTλ-1dλ

Changing the function to be dimensionless variables,

l=kThcλ

Hence,

UV=8π(kT)4(hc)301l51e1/l-1dλ

u(l)=8π(kT)4(hc)31l51e1/l-1

Using python to solve this function. The code is:

The graph is:

The peak occurs at l=0.2014

0.2014=kThcλλ=0.2014hckTλ=hc4.965kT

This isn't the same as the solution to problem 7.37. This is due to the nonlinear relationship between energy and wavelength; for example, the energy difference between 1 eV and 2 eV is the same for 101 eV and 102 eV, but the wavelengths that correspond to these two intervals are not.

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Most popular questions from this chapter

(a) As usual when solving a problem on a computer, it's best to start by putting everything in terms of dimensionless variables. So define t=T/Tcc=μ/kTc,andx=ϵ/kTc. Express the integral that defines μ, equation 7.122, in terms of these variables. You should obtain the equation

(b) According to Figure 7.33, the correct value of cwhen T=2Tcis approximately -0.8. Plug in these values and check that the equation above is approximately satisfied.

(c) Now vary μ, holding Tfixed, to find the precise value of μfor . Repeat for values of T/Tcranging from 1.2up to 3.0, in increments of 0.2. Plot a graph of μas a function of temperature.

Suppose that the concentration of infrared-absorbing gases in earth's atmosphere were to double, effectively creating a second "blanket" to warm the surface. Estimate the equilibrium surface temperature of the earth that would result from this catastrophe. (Hint: First show that the lower atmospheric blanket is warmer than the upper one by a factor of 21/4. The surface is warmer than the lower blanket by a smaller factor.)

Near the cells where oxygen is used, its chemical potential is significantly lower than near the lungs. Even though there is no gaseous oxygen near these cells, it is customary to express the abundance of oxygen in terms of the partial pressure of gaseous oxygen that would be in equilibrium with the blood. Using the independent-site model just presented, with only oxygen present, calculate and plot the fraction of occupied heme sites as a function of the partial pressure of oxygen. This curve is called the Langmuir adsorption isotherm ("isotherm" because it's for a fixed temperature). Experiments show that adsorption by myosin follows the shape of this curve quite accurately.

Sometimes it is useful to know the free energy of a photon gas.

(a) Calculate the (Helmholtz) free energy directly from the definition

(Express the answer in terms of T' and V.)

(b) Check the formula S=-(F/T)Vfor this system.

(c) Differentiate F with respect to V to obtain the pressure of a photon gas. Check that your result agrees with that of the previous problem.

(d) A more interesting way to calculate F is to apply the formula F=-kTlnZ separately to each mode (that is, each effective oscillator), then sum over all modes. Carry out this calculation, to obtain

F=8πV(kT)4(hc)30x2ln1-e-xdx

Integrate by parts, and check that your answer agrees with part (a).

At the center of the sun, the temperature is approximately 107K and the concentration of electrons is approximately 1032 per cubic meter. Would it be (approximately) valid to treat these electrons as a "classical" ideal gas (using Boltzmann statistics), or as a degenerate Fermi gas (with T0 ), or neither?

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