Suppose you had three particles, one in stateψa(x), one in stateψb(x), and one in stateψc(x). Assuming ψa,ψb, andψc are orthonormal, construct the three-particle states (analogous to Equations 5.15,5.16, and 5.17) representing

(a) distinguishable particles,

(b) identical bosons, and

(c) identical fermions.

Keep in mind that (b) must be completely symmetric, under interchange of any pair of particles, and (c) must be completely antisymmetric, in the same sense. Comment: There's a cute trick for constructing completely antisymmetric wave functions: Form the Slater determinant, whose first row isψa(x1),ψb(x1),ψc(x1) , etc., whese second row isψa(x2),ψb(x2),ψc(x2) , etc., and so on (this device works for any number of particles).

Short Answer

Expert verified

a) The distinguishable particles: ψx1,x2,x3isψax1ψbx2ψcx3

b) The identical bosons

ψ1,ψ2,ψ3,-16ψax1ψbx2ψcx3+ψax1ψbx2ψcx3+ψax1ψbx2ψcx3+16ψax1ψbx2ψcx3+ψax1ψbx2ψcx3+ψax1ψbx2ψcx3

c) The identical fermions

ψ1,ψ2,ψ3,-16ψax1ψbx2ψcx3+ψax1ψbx2ψcx3+ψax1ψbx2ψcx3+16ψax1ψbx2ψcx3+ψax1ψbx2ψcx3+ψax1ψbx2ψcx3

Step by step solution

01

Definition of identical bosons ,identical ferminos and slater determinant

  • "Particles come in two types: the particles that make up matter, known as 'fermions,' and the particles that transport forces, known as 'bosons,' according to Carroll.
  • Fermions take up space, whereas bosons can be stacked on top of one another.
  • A Slater determinant is a formula in quantum mechanics that describes the wave function of a multi-fermionic system.
  • It satisfies anti-symmetry criteria, and thus the Pauli principle, by changing sign when two electrons are exchanged (or other fermions)

02

Determine the Slater determinant

WhenNfermionsarepresent,thewholewavefunctioncanberepresentedas:x2,...,xN)=1N!ψax1ψbx1...ψNx1ψax1ψbx1...ψNx2...ψaxNψbxN...ψNxNTheSlaterdeterminantisthenameforthisformula.

03

Determine the distinguishable particles

(a)

The total wave function for identifiable particles is simply the combination of three wave functions:

ψx1,x2,x3=ψax1ψbx2ψcx3

04

Determine the  identical bosons

(b)

When we permute any two particles, the entire wave function for identical bosons must be symmetric:

ψx1,x2,x3,-16ψax1ψbx2ψcx3+ψax1ψbx2ψcx3+ψax1ψbx2ψcx3+16ψax1ψbx2ψcx3+ψax1ψbx2ψcx3+ψax1ψbx2ψcx3

05

Determine the  identical fermions

(c)

When we permute any two fermions, the whole wave function must be antisymmetric for identical fermions:

ψx1,x2,x3,-16ψax1ψbx2ψcx3+ψax1ψbx2ψcx3+ψax1ψbx2ψcx3+16ψax1ψbx2ψcx3+ψax1ψbx2ψcx3+ψax1ψbx2ψcx3

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Most popular questions from this chapter

Check the equations 5.74, 5.75, and 5.77 for the example in section 5.4.1

(a) Find the chemical potential and the total energy for distinguishable particles in the three dimensional harmonic oscillator potential (Problem 4.38). Hint: The sums in Equations5.785.78and5.795.79can be evaluated exactly, in this case−−no need to use an integral approximation, as we did for the infinite square well. Note that by differentiating the geometric series,

11-x=n=0xn

You can get

ddx(x1-x)=n=1(n+1)xn

and similar results for higher derivatives.

(b)Discuss the limiting caserole="math" localid="1658400905376" kBThω.
(c) Discuss the classical limit,role="math" localid="1658400915894" kBThω, in the light of the equipartition theorem. How many degrees of freedom does a particle in the three dimensional harmonic oscillator possess?

Find the average energy per free electron (Etot/Nd), as a fraction of the

Fermi energy. Answer:(3/5)EF

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).

In view ofProblem 5.1, we can correct for the motion of the nucleus in hydrogen by simply replacing the electron mass with the reduced mass.

(a) Find (to two significant digits) the percent error in the binding energy of hydrogen (Equation 4.77) introduced by our use of m instead of μ.

E1=-m2h2e24π'2=-13.6eV(4.77).

(b) Find the separation in wavelength between the red Balmer lines n=3n=2for hydrogen and deuterium (whose nucleus contains a neutron as well as the proton).

(c) Find the binding energy of positronium (in which the proton is replaced by a positron—positrons have the same mass as electrons, but opposite charge).

(d) Suppose you wanted to confirm the existence of muonic hydrogen, in which the electron is replaced by a muon (same charge, but 206.77 times heavier). Where (i.e. at what wavelength) would you look for the “Lyman-α” line n=2n=1?.

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