[Attempt this problem only if you are familiar with vector calculus.] Define the (three-dimensional) probability current by generalization of Problem 1.14:

J=ih2m(ψψ*-ψ*ψ)

(a) Show that satisfies the continuity equation .J=-t|ψ|2which expresses local conservation of probability. It follows (from the divergence theorem) that sJ.da=-ddtv|ψ|2d3rwhere Vis a (fixed) volume and is its boundary surface. In words: The flow of probability out through the surface is equal to the decrease in probability of finding the particle in the volume.

(b) FindJfor hydrogen in the staten=2,l=1,m=1 . Answer:

h64ma5re-r/asinθϕ^

(c) If we interpretmJas the flow of mass, the angular momentum is

L=m(r×J)d3r

Use this to calculate Lzfor the stateψ211, and comment on the result.

Short Answer

Expert verified

(a) Jsatisfies the continuity equation.

(b) The value of J is h64πma5re-rasinθϕ^.

(c) The valueLzish64πa54!a5432π.

Step by step solution

01

Define probability current

A mathematical quantity that describes the flow of probability is the probability current. If one imagines probability as a heterogeneous fluid, the probability current is the rate at which the fluid flows. It's a real-world vector that moves through space and time.

02

Prove that continuity equation is satisfied

(a)

The probability current is,

J=ih2mψψ*-ψ*ψ

Show that Jsatisfies the continuity equation

role="math" localid="1656046663375" .J=ih2mψ.ψ*+ψ2ψ*-ψ*.ψ-ψ*2ψ=ih2mψ2ψ*-ψ*2ψConsidertheSchrodingersequation,ihψt=-h2m2ψ+2ψ=-ihψt2mh22ψ*=*-ihψ*t2mh2.J=ih2m.2mh2ψ*+ihψ*t-ψ*-ihψt=ihihψψ*t+ψ*ψt=-tψ*ψ.J=-tψ2

Hence, J satisfies the continuity equation.

03

Determine J for hydrogen

(b)

At time t, the wave function for the hydrogen atom is ψmim=RnlrYlmθ,ϕeiEnthψ211=R21rY11θ,ϕeiEnthNow,apply,R21r=124a32raexp-r2aAlso,Y11θ,ϕ=-38πsinθeψ211=-1πa.18a2re-r2asinθee-iE2thForsphericalcoordinates,ψ=ψrr^+1rψθθ^+1rsinθ.ψϕϕ^ψ211=-1πa18a21-r2ae-r2asinθee-iE2thr^+1rre-r2acosθee-iE2thθ^+1rsinθre-r2asinθie.e-iE2thϕ=1-r2ar^+cosθθ^+isinθϕ1rψ211Replaceiby-itogetψ*211,ψ211*=1-r2ar^+cosθθ^-isinθϕ1rψ211*SubstitutethetwoexpressionsintotheequationforJ,

J=ih2m{ψ2111-r2ar^+cosθθ^-isinθϕ^1rψ211*]-ψ211*1-r2ar^+cosθθ^1rψ211=ih2m1-r2ar^+cosθθ^-isinθϕ-1-r2ar^-cosθθ^1sinθϕ^1rψ2112=ih2m-2irsinθψ2112ϕ^=hm1πa164a4r2e-rasin2θrsinθϕ=h64πma5re-rasinθϕ^Therefore,thevalueofJish64πma5re-rasinθϕ.^

04

Evaluate the value of  Lz

(c) The value of J from part (b),

J=h64πma5re-rasinθϕ^Now,r×J¯=h64πma5re-rasinθr^×ϕ^Consider,r^×ϕ^=-θ^Andz^.θ^=-sinθSo,r×J¯z=h64πma5r2e-rasin2θAs,Lz=mr×J¯zd3rLz=mh64πma5r2e-rasin2θr2sinθdrdθdϕ=h64πma50ar4e-radr0πsin3θdθ02π=h64πma54!a5432πHence,thevalueLzish64πa54!a5432π.

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Most popular questions from this chapter

Consider the earth–sun system as a gravitational analog to the hydrogen atom.

(a) What is the potential energy function (replacing Equation 4.52)? (Let be the mass of the earth, and M the mass of the sun.)

V(r)=-e24π00,1r

(b) What is the “Bohr radius,”ag,for this system? Work out the actual number.

(c) Write down the gravitational “Bohr formula,” and, by equating Ento the classical energy of a planet in a circular orbit of radius r0, show that n=r0/ag.From this, estimate the quantum number n of the earth.

(d) Suppose the earth made a transition to the next lower level(n-1) . How much energy (in Joules) would be released? What would the wavelength of the emitted photon (or, more likely, gravitation) be? (Express your answer in light years-is the remarkable answer a coincidence?).

(a) What isL+Y1I? (No calculation allowed!)

(b) Use the result of (a), together with Equation 4.130 and the fact thatLzY1I=hIYII to determineYII(θ,ϕ) , up to a normalization constant.

(c) Determine the normalization constant by direct integration. Compare your final answer to what you got in Problem 4.5.

The fundamental commutation relations for angular momentum (Equation 4.99) allow for half-integer (as well as integer) eigenvalues. But for orbital angular momentum only the integer values occur. There must be some extra constraint in the specific formL=r×p that excludes half-integer values. Let be some convenient constant with the dimensions of length (the Bohr radius, say, if we're talking about hydrogen), and define the operators

q112[x+a2/ħpy];p112[px-(ħ/a2)y];q212[x-(a2/ħ)py];p212[px-(ħ/a2)y];

(a) Verify that [q1,q2]=[p1,p2]=0;[q1,p1]=[p2,q2]=iħ. Thus the q's and the p's satisfy the canonical commutation relations for position and momentum, and those of index 1are compatible with those of index 2 .

(b) Show that[q1,q2]=[p1,p2]Lz=ħ2a2(q12-q22)+a22ħ(p12-p22)

(c) Check that , where each is the Hamiltonian for a harmonic oscillator with mass and frequency .

(d) We know that the eigenvalues of the harmonic oscillator Hamiltonian are , where (In the algebraic theory of Section this follows from the form of the Hamiltonian and the canonical commutation relations). Use this to conclude that the eigenvalues of must be integers.

(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?

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