Solve the time-independent Schrodinger equation with appropriate boundary conditions for the “centered” infinite square well: V(x)=0(for-a<x<+a), V(x)=α(otherwise). Check that your allowed energies are consistent with mine (Equation 2.30), and confirm that your ψ'scan be obtained from mine (Equation 2.31) by the substitution x → (x + a)/2 (and appropriate renormalization). Sketch your first three solutions, and compare Figure 2.2. Note that the width of the well is now 2a.

Short Answer

Expert verified

Therefore, the allowed energies are consistent with Mr Griffith’s equations and confirm that the wave functions can be obtained from (Equation 2.31) by the substitution x → (x + a)/2.

Step by step solution

01

Given data

For a centered infinite square well.

Vx,t=Vx=0,-a<x<a,otherwise

02

Using the Schrodinger equation

Schrodinger equation is given by:

iψt=-22m(2ψx2+V(x,t)ψ(x,t)

03

For a centred infinite square well

Vx,t=Vx=0,-a<x<aotherwise

Therefore,

iψt=-22m2ψx2+()ψ(x,t),|x|aiψt=-22m2ψx2,|x|<a

Only ψ(x,t)=0can satisfy the equation on the interval |x|a.

Since the wave function needs to be continuous, it leads to two boundary conditions,localid="1658309909151" ψ(-a,t)=0andlocalid="1658309919201" ψ(a,t)=0for -a<x<a.

Assuming a product solution of the formψ(x,t)=ψ(x)ϕ(t).

iħtψxϕt=-ħ22m2x2ψxϕtiħψxϕ't=-ħ22mψ''xϕt (1)

04

Defining the boundary conditions

To define the boundary conditions,

Forψ(-a,t)=0

ψ(-a)ϕ(t)=0ψ(-a)=0

And,

Forψ(a,t)=0

ψ(a)ϕ(t)=0ψ(a)=0

05

Reducing the Schrodinger equation into an ordinary differential equation

Dividing both sides of the partial differential equation (1) by ψ(x)ϕ(t)as:

ϕ'(t)ϕ(t)/ϕ(t)=-22mψ''(x)ψ(x)

This should be equal to a constant E for a function of t to be equal to a function of x as:

ϕ'(t)ϕ(t)=E-22mψ''(x)ψ(x)=E

Therefore, the time-dependent Schrodinger equation can be written as:

d2ψdx2=-2mE2ψ

Puttinglocalid="1658309929287" E=μ2to check if there are positive eigenvalues as:

d2ψdx2=-2mμ22ψ

06

The general solution

ψ(x)=C1cos2mμx+C2sin2mμxψ(-a)=C1cos2mμa+C2sin2mμaψ(-a)=0C1cos2mμa+C2sin2mμa=0

C2=C1cos2mμsin2mμ

And,

ψ(a)=C1cos2mμa+C2sin2mμaψ(a)=0C1cos2mμa+C1cos2mμa2sin2mμasin2mμa=02C1sin2mμacos2mμa=0sin22mμa=0

Since,sin2x=2sinxcosx

Therefore, the sine’s argument is an integral multiple of π.

22mμa=nπ, n=0,±1,±2,...

μ=nπ2a2m

Since, E=μ2

En=2n2π24a2(2m)

And the eigenfunctions,

ψ(x)=C1cos2mμx+C2sin2mμx

ψx=C1cos2mμħx+C1cos2mμħasin2mμħasin2mμħxψx=C1sin2mμħasin2mμħa+x

So,

ψn(x)=Asinnπ2a(a+x)

Solve the ordinary differential equation for this value of E

iϕ'(t)ϕ(t)=Enϕ'(t)ϕ(t)=iEnddtlnϕ(t)=iEnϕ(t)=e-iEnt/

Here, nis a natural number as for n=0 , Eigen value is 0, and for negative n, the values of E being redundant.

07

Normalizing

1=-aa[ψ(x)]2dx1=-aaA2sin2nπ2a(a+x)dx1=A2-aa121-cosnπ2a(a+x)dx

Substituting,

u=nπa(a+x)du=nπadxdx=anπdu

so,

1=A202nπ12(1-cosu)anπdu1=A2a2nπ(u-sinu)|02nπ1=A2a2nπ(2nπ)1=A2aA=1a

Therefore, the Eigen functions for the positive eigenvalues are:

ψn(x)=1asinnπ2a(a+x)

08

Checking for zero eigenvalues

ForE=0

d2ψdx2=0

The general solution is a straight line,

ψ(x)=C3x+C4ψ(-a)=-C3a+C4-C3a+C4=0

And,

ψ(a)=C3a+C4C3a+C4=0

Solving the two equations gives C3=0and C4=0, resulting in ψx=0. Therefore, zero is not an eigenvalue.

09

Checking for negative eigenvalues

E=-γ2d2ψdx2=2mγ2h2ψ

General solution,

ψ(x)=C5cosh2mγx+C6sin2mγx

So,

ψ(-a)=C5cosh2mγaa-C6sin2mγaC5cosh2mγa-C6sin2mγa=0C6=C5cosh2mγasin2mγa

And,

ψa=C5cosh2mγħa+C6sin2mγħaC5cosh2mγħa+C6sin2mγħa=0C5cosh2mγħa+C5cosh2mγħasin2mγħasin2mγħa=0

2C5sinh2mγacosh2mγa=0C5sinh22mγa=0

No non-zero value of γcould make the equation 0; therefore C5=0, hence,localid="1658309948676" C6=0, resulting ψx=0. Therefore, there are no negative eigenvalues.

10

Plotting the graphs

Since,

Vx,tVx=,x00,0<x<2a,x2a

To obtain the centred infinite square well, its width is to be doubled as:

Vx,t=Vx=,a+x00,0<a+x<2a,a+x2aVx,t=Vx=,x-a0,-a<x<2a,x2a

And replacing with to center the well about the origin.

En=n2π222m(2a)2ψn(x)=22asinnπ2a(a+x)ψn(x)=1asinnπ2a(a+x)

Takinga=1and plotting for the first three eigenstates:

For infinite square well:

n=1

n=2

n=3

For centred infinite square well:

n=1

n=2

n=3

Therefore, the allowed energies are consistent with Mr Griffith’s equations and confirm that the wave functions can be obtained from (Equation 2.31) by the substitution x → (x + a)/2.

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Most popular questions from this chapter

Consider the potential V(x)=-h2a2msech2(ax)where a is a positive constant, and "sech" stands for the hyperbolic secant

(a) Graph this potential.

(b) Check that this potential has the ground state

ψ0(x)and find its energy. Normalize and sketch its graph.

(C)Show that the function ψ2(x)=A(ik-atanhaxik+a)ekx

(Where k=2mEihas usual) solves the Schrödinger equation for any (positive) energy E. Sincetanhz-1asas This represents, then, a wave coming in from the left with no accompanying reflected wave (i.e., no term . What is the asymptotic formψk(x) of at large positive x? What are R and T, for this potential? Comment: This is a famous example of a reflectionless potential-every incident particle, regardless of its energy, passes right through.

Find x,p,x2,p2,T, for the nth stationary state of the harmonic oscillator, using the method of Example 2.5. Check that the uncertainty principle is satisfied.

This is a strictly qualitative problem-no calculations allowed! Consider the "double square well" potential (Figure 2.21). Suppose the depth V0and the width a are fixed, and large enough so that several bound states occur.

(a) Sketch the ground state wave function Ψ1and the first excited state localid="1658211858701" Ψ2(i) for the case b = 0 (ii) forbaand (iii) for ba

(b) Qualitatively, how do the corresponding energies(E1andE2)and vary, as b goes from 0 to ? Sketch E1(b)and E2(b)on the same graph.

(c) The double well is a very primitive one-dimensional model for the potential experienced by an electron in a diatomic molecule (the two wells represent the attractive force of the nuclei). If the nuclei are free to move, they will adopt the configuration of minimum energy. In view of your conclusions in (b), does the electron tend to draw the nuclei together, or push them apart? (Of course, there is also the internuclear repulsion to consider, but that's a separate problem.)

Derive Equations 2.167 and 2.168.Use Equations 2.165 and 2.166 to solve C and D in terms of F:

C=(sin(la)+iklcos(la))eikaF;D=(cos(la)iklsin(la))eikaF

Plug these back into Equations 2.163 and 2.164. Obtain the transmission coefficient and confirm the equation 2.169

a) Construct ψ2(x)

b) Sketch ψ0,ψ1andψ2

c) Check the orthogonality ofψ0ψ1ψ2 by explicit integration.

Hint:If you exploit the even-ness and odd-ness of the functions, there is really only one integral left to do.

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