/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none} Q18P (a) Using Equations 5.59 and 5.6... [FREE SOLUTION] | 91Ó°ÊÓ

91Ó°ÊÓ

(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]0≤x≤a

(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

¾±Ä§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-xfor0≤x≤a

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:

2³¾Î±h2B=kA-e-iKakAcoska-Bsinka=kA--1nkA12-B.0=kA-kA⇒B=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

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 91Ó°ÊÓ!

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

Obtain equation 5.76 by induction. The combinatorial question is this: How many different ways you can put N identical balls into d baskets (never mind the subscriptfor this problem). You could stick all of them into the third basket, or all but one in the second basket and one in the fifth, or two in the first and three in the third and all the rest in the seventh, etc. Work it out explicitly for the casesN=1,N=2,N=3andN=4; by that stage you should be able to deduce the general formula.

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-ħ22m∇j2-14πo,0Ze2rj+1214πo,0∑j≠1Ze2rj-rk (5.24).

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

(a) Calculate<1/r1-r2>for the stateψ0(Equation 5.30). Hint: Dod3r2integral

first, using spherical coordinates, and setting the polar axis alongr1, so

that

ψ0r1,r2=ψ100r1ψ100r2=8Ï€²¹3e-2r1+r2/a(5.30).

r1-r2=r12+r22-2r1r2³¦´Ç²õθ2.

Theθ2integral is easy, but be careful to take the positive root. You’ll have to

break ther2integral into two pieces, one ranging from 0 tor1,the other fromr1to∞

Answer: 5/4a.

(b) Use your result in (a) to estimate the electron interaction energy in the ground state of helium. Express your answer in electron volts, and add it toE0(Equation 5.31) to get a corrected estimate of the ground state energy. Compare the experimental value. (Of course, we’re still working with an approximate wave function, so don’t expect perfect agreement.)

E0=8-13.6eV=-109eV(5.31).

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=23h2kF510Ï€2m=(3Ï€2)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=h2V2π2m∫0kFK4dk=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=(9Ï€4)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).

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).

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.