a) Check that Arj1(kr)satisfies the radial equation with V(r)=0and I=1.

(b) Determine graphically the allowed energies for the infinite spherical well, when I=1. Show that for large n,En1(h2π2/2ma2)(n+1/2)2. Hint: First show that j1(x)=0x=tanx. Plot xandtanxon the same graph, and locate the points of intersection.

Short Answer

Expert verified

a) The two terms are equal and the proposed solution satisfies the radial differential equation.

b) The high energies are roughly given by:

En=h2k22m=h2π22ma2n+122

Step by step solution

01

Concept used

The Schrodinger equation is given by:

-h22md2udr2+[V(r)+h22mI(I+1)r2]u=Eu

02

Given information from question

a)

Using the standard substitution ur=Rr/rthe radial part of the Schrodinger equation reads:

-h22md2udr2+[V(r)+h22mI(I+1)r2]u=Eu

Now, if we set I=1and Vr=0the latter expression simplifies to:

h22md2udr2+h22m2r2u=Eu

Next, we multiply both sides by 2m/h2and define k22mE/h2, so the previous equation becomes:

-d2udr2+2r2-k2u=0

The spherical Bessel function must now be inserted into the final differential equation. We are aware that:

j1=sinkrkr2-coskrkr

As a result, we must examine the following solution:

ur=Arj1=Asinkrk2r-coskrk

The second derivative of the urfunction is required to check whether the solution satisfies the given differential equation. So, we find:

dudr=Akcoskrk2r-sinkrk2r2+ksinkrkd2udr2=A-sinkrr-2coskrkr2+2sinkrk2r3+kcoskr

This must be equal to the term2/r2-k2u in order for the differential equation to be satisfied. Therefore, we will calculate it explicitly:

2r2-k2u=A2r2-k2sinkrk2r-coskrk=AAsinkrk2r3-sinkrr-2coskrkr2+kcoskr=A-sinkrr-2coskrkr2+2sinkrk2r3+kcoskr

As a result, the two terms are equal, and the proposed solution is radial differential equation-satisfying.

03

Given information from question

b)

Since, we are dealing with infinite well, our wave function must vanish at r=a. This implies that urhas to vanish. Therefore:

ur=0Asinkak2a-coskakka=tanka

This is a transcendental equation.

04

Graph of the intersection of two functions

By identifying intersections of two functions, we may solve it graphically.

Here, the red curve shows the tangent curve and blue curve is x-curve.

As energy increases, kincreases and intersections occur near ka=n+12π. As a result, the high energies are nearly equal to:

En=h2k22m=h2π22ma2n+122

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Most popular questions from this chapter

(a) Prove that for a particle in a potential V(r)the rate of change of the expectation value of the orbital angular momentum L is equal to the expectation value of the torque:

ddt<L>=<N>

Where,

N=r×(VV)

(This is the rotational analog to Ehrenfest's theorem.)

(b) Show that d<L>/dt=0for any spherically symmetric potential. (This is one form of the quantum statement of conservation of angular momentum.)

(a) Construct the wave function for hydrogen in the state n=4,I=3,m=3. Express your answer as a function of the spherical coordinates r,θandϕ.

(b) Find the expectation value of role="math" localid="1658391074946" rin this state. (As always, look up any nontrivial integrals.)

(c) If you could somehow measure the observable Lx2+Ly2on an atom in this state, what value (or values) could you get, and what is the probability of each?

Deduce the condition for minimum uncertainty inSx andSy(that is, equality in the expression role="math" localid="1658378301742" σSxσSy(ħ/2)|<Sz>|, for a particle of spin 1/2 in the generic state (Equation 4.139). Answer: With no loss of generality we can pick to be real; then the condition for minimum uncertainty is that bis either pure real or else pure imaginary.

A hydrogenic atom consists of a single electron orbiting a nucleus with Z protons. (Z=1 would be hydrogen itself,Z=2is ionized helium ,Z=3is doubly ionized lithium, and so on.) Determine the Bohr energies En(Z), the binding energyE1(Z), the Bohr radiusa(Z), and the Rydberg constant R(Z)for a hydrogenic atom. (Express your answers as appropriate multiples of the hydrogen values.) Where in the electromagnetic spectrum would the Lyman series fall, for Z=2and Z=3? Hint: There’s nothing much to calculate here— in the potential (Equation 4.52) Ze2, so all you have to do is make the same substitution in all the final results.

V(r)=-e24πo0˙1r (4.52).

a) Check that the spin matrices (Equations 4.145 and 4.147) obey the fundamental commutation relations for angular momentum, Equation 4.134.

Sz=h2(100-1)(4.145).Sx=h2(0110),sy=h2(0-ii0)(4.147).[Sx,Sy]=ihSz,[Sy,Sz]=ihSx,[Sz,Sx]=ihSy(4.134).(b)ShowthatthePaulispinmatrices(Equation4.148)satisfytheproductruleσx(0110),σy(0-ii0),σz(100-1)(4.148).σjσk=δjk+io'IjklσI,(4.153).

Wheretheindicesstandforx,y,orz,ando'jklistheLevi-Civitasymbol:+1ifjkl=123,231,or2=312;-1ifjkl=132,213,or321;otherwise.

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