(a) Using Equations 5.59 and 5.63, show that the wave function for a particle in the periodic delta-function potential can be written in the form

ψ(X)=C[sinkx+e-ikasina-x]0xa

(b) There is an exception; At the top of a band where z is an integer multiple ofπyielsψ(x)=0 yields .

Find the correct wave function for the case. Note what happens toψeach delta function.

Short Answer

Expert verified

(a) Using the equation given in textbook, we derived the wave function for periodic delta potential

(b)The correct wave function for the wave is ψx=Asinkx

Step by step solution

01

Define Schrödinger equation

  • A differential equation that describes matter in quantum mechanics in terms of the wave-like properties of particles in a field. Its answer is related to a particle's probability density in space and time.
  • The time-dependent Schrödinger equation is represented as

ddtψt>=H^ψt

02

Showing the wave function

(a)

To show that wave function for a particle in the periodic delta potential is:

ψx=Csinkx+e-ikasinka-xfor0xa

We start from equations 5.59 and 5.63:

ψx=Asinkx+BcoskxAsinka=eika-coskaBB=Asinkaeika-coska

We insert previous expression for B in wave function ψx:

ψx=Asinkx+Asinkaeika-coskacoskx=Aeikasinkx-sinkxcoska+sinkacoskaeika-coska=Aeikaeika-coskasinkx-eika-sinkxcoska+eika-sinkacoskaψx=Csinkx+eika-sinka-x

Therefore using the equation given in textbook, we derived the wave function for periodic delta potential.

03

Observing from graph

(b)

fz=cosz+βsinzz

Forβ=10 .From equation 5.64 we have:

coska=coskx+mah2ksinka

In this case is an integer multiple ofπ, then we havez=ka=nπ, where is nan integer. This implies:

sinka=sinKa=0coska=cosKa=-1n=cosKa+isinKa=eiKa=-1n

Constant C from previous task is then C=A0which implies that A=0 or B=0 .So the equation 5.62 is:

2h2B=kA-e-iKakAcoska-Bsinka=kA--1nkA12-B.0=kA-kAB=0

So, from equation 5.59, we are left with only Asinkxterm:

ψx=Asinkx

At each delta functionψx=0, so the wave function doesn't "see" any potential.

Hence the correct wave function for the wave is ψx=Asinkx

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Most popular questions from this chapter

Thebulk modulus of a substance is the ratio of a small decrease in pressure to the resulting fractional increase in volume:

B=-VdPdV.

Show thatB=(5/3)P, in the free electron gas model, and use your result in Problem 5.16(d) to estimate the bulk modulus of copper. Comment: The observed value is 13.4×1010N/m2, but don’t expect perfect agreement—after all, we’re neglecting all electron–nucleus and electron–electron forces! Actually, it is rather surprising that this calculation comes as close as it does.

Suppose you could find a solutionψ(r1,r2,...,rz)to the Schrödinger equation (Equation 5.25), for the Hamiltonian in Equation 5.24. Describe how you would construct from it a completely symmetric function, and a completely anti symmetric function, which also satisfy the Schrödinger equation, with the same energy.

role="math" localid="1658219144812" H^=j=1Z-ħ22mj2-14πo,0Ze2rj+1214πo,0j1Ze2rj-rk (5.24).

role="math" localid="1658219153183" H^ψ=E (5.25).

Imagine two noninteracting particles, each of mass m, in the infinite square well. If one is in the stateψn(Equation 2.28 ), and the other in state ψ1(ln), calculate localid="1658214464999" (x1-x2)2, assuming (a) they are distinguishable particles, (b) they are identical bosons, and (c) they are identical fermions.

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).

The ground state of dysprosium (element 66, in the 6th row of the Periodic Table)

is listed as Is5. What are the total spin, total orbital, and grand total angular

momentum quantum numbers? Suggest a likely electron configuration for

dysprosium.

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