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(a) Use the recursion formula (Equation 4.76) to confirm that whenI=n-1 the radial wave function takes the form

Rn(n-1)=Nnrn-1e-r/na and determine the normalization constant by direct integration.

(b) Calculate 200a and <r2> for states of the form n(n-1)m

(c) Show that the "uncertainty" in r(r) is<r>/2n+1for such states. Note that the fractional spread in decreases, with increasing (in this sense the system "begins to look classical," with identifiable circular "orbits," for large ). Sketch the radial wave functions for several values of, to illustrate this point.

Short Answer

Expert verified

(a) The normalization constant Nnby direct integration isNn=2nan+1212n!

(b) The value of rand r2is r=n+12naand r2=n+12n+1na2

(c) The uncertainty isr=r2n+1

Step by step solution

01

Determine the recursion formula

A recursive formula is one that defines each term in a series in terms of the term before it (s). As an example: An arithmetic sequence's recursive formula is an=an-1+dgeometric sequence's recursive formula is an=an-1r.

02

Determine the normalization constant Nn by direct integration

(a)

The radial equation is given by:

Nn=2nan+1212n!

where:

V=j0cjj=r=-2mEh

and the coefficients turned out to satisfy the recursion formula:

cj+1=2j+I+1-2nj+1j+2I+1cj

let I=n-1thus:

Rnn-1=1rne-pv

but:

c1=2n-n12nc0=0=rnav=c0

so:

Rnn-1r=c0annrn-1e-r/an

combine the constant out front into a single constant, Nn=c0/ann, so:

Rnn-1=Nnrn-1e-r/na

Normalize the wave function, that is:

role="math" localid="1656315281010" 0R2r2dr=1

to do the integral I used the integral-calculator.com. Thus:

0R2r2dr=Nn20r2ne-2r/nadr=Nn22n!na22n+1=1

Nn=2nan+1212n!

Therefore, the normalization constant Nnby direct integration isNn=2nan+1212n!

03

Determine the value of <r> and  <r2>

(b)

Now find the expectation value of r and r2 , first we find it for rIthen we let I=1and I=2as:

rI=0R2rI+2dr=Nn20r2n+Ir-2r/na

for I=1, we have:

r=2na2n+112n!2n+1!na22n+2=n+12na

r=n+12na

For I=2:

r2=2na2n+112n!2n+2!na22n+3=2n+22n+1na2=n+12n+1na2

role="math" localid="1656316300775" r2=n+12n+1na2

Therefore, the value of rand r2is r=n+12naandr2=n+12n+1na2

04

Determine the uncertainty equation 

(c)

The uncertainty in ris given by:

localid="1656316682565" r2=r2-r2

substitute from part bto get:

localid="1656316692244" r2=n+12n+1na2-n+122na2=12n+12na2=22n+1/2r2

Thus :

r=r2n+1

Now we need to sketch few wave functions with different nvalues, combine Nnwith Rnn-1in part a, so we get:

Rnn-1=2nan+1212n!rn-1e-r/nato plot this function /set a=1(for simplicity) and plot rfrom 0 to 200 (actully from 0 to 200a ), I used python to plot it and the code is shown in the following picture:

Therefore, the uncertainty isr=r2n+1

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Most popular questions from this chapter

Construct the spin matrices(Sx,Sy鈥塧苍诲Sz) , for a particle of spin 1. Hint: How many eigenstates ofSz are there? Determine the action of Sz, S+, and Son each of these states. Follow the procedure used in the text for spin 1/2.

If the electron were a classical solid sphere, with radius

rc=e24O0mc2

(the so-called classical electron radius, obtained by assuming the electron's mass is attributable to energy stored in its electric field, via the Einstein formula E=mc2), and its angular momentum is (1/2)h then how fast (in m/sm/s) would a point on the "equator" be moving? Does this model make sense? (Actually, the radius of the electron is known experimentally to be much less than5.1561010m/src, but this only makes matters worse).

Construct the matrixSrrepresenting the component of spin angular momentum along an arbitrary directionr. Use spherical coordinates, for which

r蝉颈苍胃肠辞蝉桅+蝉颈苍胃蝉颈苍桅+肠辞蝉胃k [4.154]

Find the eigenvalues and (normalized) eigen spinors ofSr. Answer:

x+(r)=(cos/2e颈蠒sin/2); x+(r)=(e颈蠒sin(/2)-cos(/2)) [4.155]

Note: You're always free to multiply by an arbitrary phase factor-say,ei-so your answer may not look exactly the same as mine.

Because the three-dimensional harmonic oscillator potential (Equation 4.188)is spherically symmetric, the Schr枚dinger equation can be handled by separation of variables in spherical coordinates, as well as cartesian coordinates. Use the power series method to solve the radial equation. Find the recursion formula for the coefficients, and determine the allowed energies. Check your answer against Equation4.189.

For the most general normalized spinor (Equation 4.139),

compute{Sx},{Sy},{Sz},{Sx2},{Sy2},and{Sx2}.checkthat{Sx2}+{Sy2}+{Sz2}={S2}.

X=(ab)=aX++bX(4.139).

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