Nuclear density is approximately 1017 kg/m3. (a) Treating them as a gas of fermions bound together by the (no electrostatic) "strung attraction." calculate EFfor the neutrons in lead-206 (82 protons and 124 neutrons). (b) Treating them the same way. what would EFbe for the protons? (c) In fact, the energies of the most energetic neutrons and protons, those at the Fermi energy, are essentially equal in lead-206? What has been left out of pars (a) or (b) that might account for this?

Short Answer

Expert verified
  1. The Fermi energy of neutron in lead 206 is 21.8 MeV.
  2. The Fermi energy of the protons in lead 206 is 16.5 MeV.

Step by step solution

01

A concept of Fermi energy:

Formula used:

Fermi energy is a term in quantum mechanics usually referring to the energy difference between the highest and lowest occupied states of a single particle in a quantum system of non-interacting fermions at absolute zero temperature.

The Fermi energy EFis given by-

EF=π2h2m[32s+1π2NV]23

Here, V is the volume, N is the number of particles, s is the spin of particles, D is the density, m is the mass of the particle

D=MV ….. (2)

Convert the atomic mass of the lead-206 to standard units as below.

Nuclear density of lead- 206 , D = 1717kg/m3

m=(206amu)1.66×10-27kg1amu=3.42×10-25kg

02

Solve for Fermi energy:

To get the Fermi energy of the neutrons, it would help to get a simpler expression.

Fermi energy first, Equation (1) is used, with s being (since as a fermion, it's a spin:

EF=π2h2m32s+1π2NV23=π2h2m3212+1π2NV23=h22m3π3N232πV23EF=h22m3π3N232πV23

03

Express for the volume:

Now equation (2) can be used to get an expression for the volume V, so that can be inserted for

V there:

D=MVV=MD

And plug that in the prior equation.

EF=h22m3π2V23=h22m3π2NMD23EF=h22m3π2NDM23......(3)

04

(a) Define the Fermi energy:

Let m is the mass of the neutron, and M is the mass of the entire nucleus. The N doesn't need be converted since the actual number of neutrons is known. So then insert the 124 for N then, along with 1017 kg/m3 for the density D of nuclear material 3.42x10-25 kg for 1.67x10-27 k, the mass of the neutron, m and 1.055x10-34 J.s for hin equation (3).

EF=h22m3π2NDM23

Substitute known numerical values in the above equation.

EF=1.055×10-34J.s221.67×10-27kg3×3.1421241017kgm33.42×10-25kg23=0.333×10-411072.447×104223=0.333×1041105.02×1028=3.49×10-12J

They can be converted to MeV .

EF=3.49×10-12J1eV1.6×10-19J1MeV106eV=21.8MeV

The Fermi energy of the neutrons in lead 206 is 21.8 MeV.

05

(b) The Fermi energy of the protons in lead  :

Nuclear density of lead is, D = 1017 kg/m3

The number of protons, N = 82

Fermi energy is given as,

EF=h22m3π2NDM23=1.055×10-34J·s221.67×10-27kg3×3.142821017kgm33.42×10-25kg23=0.333×10-4179.7×1028=2.65×10-12J

That can be converted to MeV as follow.

EF=2.65×10-121eV1.6×10-19J1MeV106eV=16.5MeV

The Fermi energy of the protons in lead 206 is 16.5 MeV.

06

(c) explain that the two have them have about the same energy:

The two energies can possibly be made more similar if the repulsive energy for the protons is included in the calculations for the Femi energy. Given all the protons have the same charge and are very close together, there is a great deal of repulsive energy that exists between them. So that repulsive energy could add to the calculated Fermi energy for the protons to get the value closer to that of the neutrons, since it's observed that the two have them have about the same energy.

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

Heat capacity (at constant volume) is defined asU/T. (a) Using a result derived in Example 9.6. obtain an expression for the heat capacity per unit volume, inJ/Kmi3, of a photon gas. (b) What is its value at300K?

According to Wien's law, the wavelengthλmaxat which the thermal emission of electromagnetic energy from a body of temperatureTis maximum obeysλmaxT=2.898×103mK.Show that this law follows from equation (9-47). To do this. Usef=c/λto expressin terms ofλrather than f, then obtain an expression that, when solved, would yield the wavelength at which this function is maximum. The transcendental equation cannot be solved exactly, so it is enough to show thatλ=(2.898×103mK)/T solves it to a reasonable degree of precision.

Show that in the limithω0kBT. Equation (9.15) becomes (9.28).

Discusses the energy balance in a white dwarf. The tendency to contract due to gravitational attraction is balanced by a kind of incompressibility of the electrons due to the exclusion principle.

(a) Matter contains protons and neutrons, which are also fanions. Why do the electrons become a hindrance to compression before the protons and neutrons do?

(b) Stars several times our Sun's mass has sufficient gravitational potential energy to collapse further than a white dwarf; they can force essentially all their matter to become neutrons (formed when electrons and protons combine). When they cool off, an energy balance is reached like that in the white dwarf but with the neutrons filling the role of the incompressible fermions. The result is a neutron star. Repeat the process of Exercise 89. but assume a body consisting solely of neutrons. Show that the equilibrium radius is given by

R=322G(3π22mn8M)1/3

(c) Show that the radius of a neutron star whose mass is twice that of our Sun is only about10km .

The maximum wavelength light that will eject electrons from metal I via the photoelectric effect is410nm. For metal2, it is280nm. What would be the potential difference if these two metals were put in contact?

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.

Sign-up for free