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Use Equation 4.32 to construct Yll(θ,ϕ)andy32(θ.ϕ) . (You can take P32from Table 4.2, but you'll have to work outPll from Equations 4.27 and 4.28.) Check that they satisfy the angular equation (Equation 4.18), for the appropriate values of l and m .

Short Answer

Expert verified

The angular equation is

Yll(θ,φ)=1l!(2l+1)!4π(-12eiφsinθ)lYll(θ,φ)=141052πe2iφsin2θcosθ

Step by step solution

01

Define the Schrodinger equation

A differential equation 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.

02

Determine the terms in equation

Equations 4.27, 4.28 and 4.32, are given by:

Plm(x)=1-x2m/2ddxmPl(x)Pl(x)=12ll!ddxl(x2-1)l Ylm(θ,ϕ)=σ(2l+1)4π(l-m)!(l+m)!eimϕPlm(cosθ)

Using these equations, we need to construct Ylland Y32, from (3) we have:

Yll=(-1)l(2l+1)4π1(2l)!eilϕPll(cos(θ))

Using (1) we can write as:

Pll(x)=(1-x2)1/2ddxlPl(x)

Substitute from (2) with Pl

Pll(x)=12ll!(1-x2)1/2ddx2l(x2-1)l

but (x2-1)l=x2l+....,, where the rest of the term has a power less than 2l, which means that when we differentiate localid="1658135583492" (x2-1)l,2l times then all the terms vanishes except the first term with the power of 2l, so:

Pll(x)=12ll!(1-x2)1/2ddx2lx2l

but,

localid="1658135800919" ddxnxn-n!

thus:

Pll=(2l)!2ll!(1-x2)1/2

for x=cos(θ),1-x2=sin2(θ)we get:

Pll=(2l)!2ll!sinl(θ)

Substitute into (4) with Pll, so we get:

Yll=(-1)l(2l+1)4π(2l)!eilϕ(2l)2ll!sinl(0)=(-1)l(2l)!(2l+1)4πeilϕ(2l)2ll!sinl(θ)=1l!(2l+1)4π-12eiϕsinθlYll=1l!(2l+1)!4π-12eiϕsinθl

03

Determine the terms in Schrodinger equation

Now we need to findy32, following the same method, from equations (1), (2) and (3) we have:

Y32=74π.15!e2iϕp32(cos(θ))P32(x)=(1-x2)ddx2p3(x)p3(x)=18.3!ddx3(x2-1)3

First we do the differentiation in the last equation as:

P3=18.3.2ddx26x(x2-1)2=18ddx(x2-1)2+4x2(x2-1)=184x(x2-1)+8x(x2-1)+4x2.2x=12(x3-x+2x3-2x+2x3)=12(5x3-3x)

Then we substitute into the second one, and also do the differentiation as:

P32(x)=12(1-x2)ddx2(5x3-3x)=12(1-x2)ddx(15x2-3)=12(1-x2)30x=15x(1-x2)

forx=cos(θ),1-x2=sin2(θ)we get:

P32(cos(θ))=sin2(θ)cos(θ)

Now substitute into the first one, so we get:

Y32=74π15!15e2iϕcos(θ)sin2(θ)=141052πe2iϕsin2(θ)cos(θ)Y32=141052πe2iϕsin2(θ)cos(θ)

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Most popular questions from this chapter

Determine the commutator of S2withSZ(1)(whereSS(1)+S(2)) Generalize your result to show that

[S2,S1]=2Ih(S1×S2)

Comment: Because Sz(1)does not commute with S2, we cannot hope to find states that are simultaneous eigenvectors of both. In order to form eigenstates ofS2weneed linear combinations of eigenstates ofSz(1). This is precisely what the Clebsch-Gordan coefficients (in Equation 4.185) do for us, On the other hand, it follows by obvious inference from Equation 4.187that the sumrole="math" localid="1655980965321" S(1)+S(2)does commute withdata-custom-editor="chemistry" S2, which is a special case of something we already knew (see Equation 4.103).

(a)Derive Equation 4.131 from Equation 4.130. Hint: Use a test function; otherwise you're likely to drop some terms.

(b)Derive Equation 4.132 from Equations 4.129 and 4.131 .Hint : Use Equation 4.112.

The raising and lowering operators change the value of m by one unit:

L±flm=(Alm)flm+1, (4.120).

Where Almare constant. Question: What is Alm, if the Eigen functions are to be normalized? Hint: First show thatL±is the Hermitian conjugate of L±(Since LxandLyare observables, you may assume they are Hermitian…but prove it if you like); then use Equation 4.112.

An electron is in the spin state

χ=A3i4

(a) Determine the normalization constant .

(b) Find the expectation values of Sx,Sy , and Sz.

(c) Find the "uncertainties" ,σSx , σSyandσSz . (Note: These sigmas are standard deviations, not Pauli matrices!)

(d) Confirm that your results are consistent with all three uncertainty principles (Equation 4.100 and its cyclic permutations - only with in place ofL, of course).

What is the most probable value of r, in the ground state of hydrogen? (The answer is not zero!) Hint: First you must figure out the probability that the electron would be found between r and r + dr.

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