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Starting from equation 7.83, derive a formula for the density of states of a photon gas (or any other gas of ultra relativistic particles having two polarisation states). Sketch this function.

Short Answer

Expert verified

Hence, the formula for density of states of a photon gas isg(ϵ)=8πVϵ2(hc)3

Step by step solution

01

Given information

The equation 7.83 is

UV=8π(hc)3∫0∞ϵ3eϵ/kT-1dϵ

02

Explanation

The equation 7.83 is:

UV=8π(hc)3∫0∞ϵ3eϵ/kT-1dϵ

We can write the equation as:

localid="1647752992962">U=∫0∞ϵ8πVϵ2(hc)31eϵ/kT-1dϵ(1)

Distribution function for Planck's constant is given as:

n¯Pl=1eϵ/kT-1

Substituting this into (1)

U=∫0∞ϵ8πVϵ2(hc)3n¯Pldϵ

Hence the energy density for Planck's constant is

g(ϵ)=8πVϵ2(hc)3

Using Python to solve this function, the code is:

The graph is:

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Most popular questions from this chapter

Use the results of this section to estimate the contribution of conduction electrons to the heat capacity of one mole of copper at room temperature. How does this contribution compare to that of lattice vibrations, assuming that these are not frozen out? (The electronic contribution has been measured at low temperatures, and turns out to be about40% more than predicted by the free electron model used here.)

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(c) Now assume that every conduction electron comes from an ionized donor atom. In this case the number of conduction electrons is equal to the number of donors that are ionized. Use this condition to derive a quadratic equation for Ncin terms of the number of donor atoms Nd, eliminatingµ. Solve for Ncusing the quadratic formula. (Hint: It's helpful to introduce some abbreviations for dimensionless quantities. Tryx=NcNd,t=kTland so on.)

(d) For phosphorus in silicon, the ionization energy is localid="1650039340485" 0.044eV. Suppose that there are 1017patoms per cubic centimeter. Using these numbers, calculate and plot the fraction of ionized donors as a function of temperature. Discuss the results.

Number of photons in a photon gas.

(a) Show that the number of photons in equilibrium in a box of volume V at temperature T is

N=8πVkThc3∫0∞x2ex-1dx

The integral cannot be done analytically; either look it up in a table or evaluate it numerically.

(b) How does this result compare to the formula derived in the text for the entropy of a photon gas? (What is the entropy per photon, in terms of k?)

(c) Calculate the number of photons per cubic meter at the following temperatures: 300 K; 1500 K (a typical kiln); 2.73 K (the cosmic background radiation).

In Section 6.5 I derived the useful relation F=-kTln(Z)between the Helmholtz free energy and the ordinary partition function. Use analogous argument to prove that ϕ=-kT×ln(Z^), where Z^ is the grand partition function and ϕis the grand free energy introduced in Problem 5.23.

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