Suppose you had three (noninteracting) particles, in thermal equilibrium in a one-dimensional harmonic oscillator potential, with a total energyE=92hω .

(a) If they are distinguishable particles (but all with the same mass), what are the possible occupation-number configurations, and how many distinct (threeparticle) states are there for each one? What is the most probable configuration? If you picked a particle at random and measured its energy, what values might you get, and what is the probability of each one? What is the most probable energy?

(b) Do the same for the case of identical fermions (ignoring spin, as we did in Section 5.4.1).

(c) Do the same for the case of identical bosons (ignoring spin).

Short Answer

Expert verified

(a) Distinguishable particles: there are three possible configurations for occupation numbers. One configuration has one state, other 6 and third 3. The most probable configuration is the second one with probability 6/10 . Most probable energy for distinguishable particles is ground state.

b) Fermions: fermions can occur only in one configuration. And in that configuration all three energies are equally probable.

c) Bosons: they occur only in one state of each configuration. Most probable energy isE1 .

Step by step solution

01

Define Fermions and bosons

  • Fermions are typically associated with matter, whereas bosons are commonly associated with force carrier particles.
  • However, in today's particle physics, the distinction between the two concepts is blurred.
  • Under extreme conditions, weakly interacting fermions can also exhibit bosonic behavior.
02

Determining the possible occupation number configurations

There are three particles in a harmonic oscillator. Total energy of the system isE0=9hω2. There is need to find all possible configurations of particles if they are distinguishable, fermions or bosons. Total energy of system in harmonic potential is:

E=hω(n1+n2+n3+32)9hω2=hω(n1+n2+n3+32)92=(n1+n2+n3+32)n1+n2+n3=3

Possible configurations are

n1=n2=n3=1:(1,1,1)n1=0,n2=1,n3=2:,0,1,2,(2,0,1),(2,1,0),(0,2,1),(1,2,0),(1,0,2)n1=n2=0,n3=3:(3,0,0),(0,3,0),(0,0,3)

(a)

Distinguishable particles

We are interested in occupation-number configurations

(1)All three-particle in-state;1;(0,3,0,0,0,.........)

(2)All three-particle in a different state;(1,1,1,0,0,.......)

(3)Two particles in the ground state one are third;(2,0,0,1,0,.........)

Second configuration is the most probable one, because there are six possibilities for it to happen. First one has only one possibility, and third one three.

Now we need to find the most probable energy. EnergyE0=hωlcan be measured in two configurations: second and third. Second configuration appears 6 times in 10 (total number of possibilities) and to measure energyE0we have chance of 1/3 . Third configuration appears 3 times in 10, and to measure energy we have chance of 2.1/3 . So total probability of measuring energyE0is:

p0=61013+31023=25E0=hω2p1=61013+110=310E1=3hω2p2=61013=15E2=5hω2p3=31013=110E3=7hω2p0=61013

Most probable energy isE0 .

Therefore in distinguishable particles, there are three possible configurations for occupation numbers. One configuration has one state, other 6 and third 3.The most probable configuration is the second one with probability 6/10 . Most probable energy for distinguishable particles is ground state.

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Most popular questions from this chapter

(a) Find the percent error in Stirling’s approximation for z = 10 ?

(b)What is the smallest integer z such that the error is less than 1%?

Certain cold stars (called white dwarfs) are stabilized against gravitational collapse by the degeneracy pressure of their electrons (Equation 5.57). Assuming constant density, the radius R of such an object can be calculated as follows:

P=23EtotV=23h2kF510π2m=(3π2)2/3h25mp5/3(5.57)

(a) Write the total electron energy (Equation 5.56) in terms of the radius, the number of nucleons (protons and neutrons) N, the number of electrons per nucleon d, and the mass of the electron m. Beware: In this problem we are recycling the letters N and d for a slightly different purpose than in the text.

Etot=h2V2π2m0kFK4dk=h2kF5V10π2m=h2(3π2Nd)5/310π2mV-2/3(5.56)

(b) Look up, or calculate, the gravitational energy of a uniformly dense sphere. Express your answer in terms of G (the constant of universal gravitation), R, N, and M (the mass of a nucleon). Note that the gravitational energy is negative.

(c) Find the radius for which the total energy, (a) plus (b), is a minimum.

R=(9π4)2/3h2d5/3GmM2N1/3

(Note that the radius decreases as the total mass increases!) Put in the actual numbers, for everything except , using d=1/2 (actually, decreases a bit as the atomic number increases, but this is close enough for our purposes). Answer:

(d) Determine the radius, in kilometers, of a white dwarf with the mass of the sun.

(e) Determine the Fermi energy, in electron volts, for the white dwarf in (d), and compare it with the rest energy of an electron. Note that this system is getting dangerously relativistic (seeProblem 5.36).

(a)Use Equation5.113 to determine the energy density in the wavelength rangedλ. Hint: setρ(ω)=ρ-(λ), and solve forρ(λ)-

(b)Derive the Wien displacement law for the wavelength at which the blackbody energy density is a maximum
λmax=2.90×10-3mKT

You'll need to solve the transcendental equation(5×x)=5e-x, using a calculator (or a computer); get the numerical answer accurate to three significant digits.

(a) Figure out the electron configurations (in the notation of Equation

5.33) for the first two rows of the Periodic Table (up to neon), and check your

results against Table 5.1.

1s22s22p2(5.33).

(b) Figure out the corresponding total angular momenta, in the notation of

Equation 5.34, for the first four elements. List all the possibilities for boron,

carbon, and nitrogen.

LJ2S+1 (5.34).

Evaluate the integrals (Equation5.108 and 5.109) for the case of identical fermions at absolute zero. Compare your results with equations 5.43 and5.45. (Note for electrons there is an extra factor of 2 in Equations 5.108 and 5.109. to account for the spin degeneracy.)

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