Warning: foreach() argument must be of type array|object, bool given in /var/www/html/web/app/themes/studypress-core-theme/template-parts/header/mobile-offcanvas.php on line 20

Work out the radial wave functions R30,R31,andR32using the recursion formula. Don’t bother to normalize them.

Short Answer

Expert verified

The workout radial wave functions are:R30=c03a1-23ra+227ra2e-r/3aR31=c09a2r1-16rae-r/3aR32=c027a3r2e-r/3a

Step by step solution

01

Definition of the radial wave function

The probability of finding an electron in some finite volume element around a point at a distance of r from the nucleus is given by the radial wave function R(r), which is simply the value of the wave function at some radius r.

02

Determine the radial wave function

R30,R31,andR32,We need to work out the radial wave functions and we will use:

Rnl(r)=1runl(r)

Where,

role="math" localid="1658143292950" unl(p)=ρl+1e-pvnl(p)

Thus,

Rnl(r)=1runl(r)Rnl(r)=1rpl+1e-pvnl(p) (1)

Where,

vnl(p)=j=0cjpjcj+1=2(j+l+1)-2n(j+1)(j+2)(l+1))cj (2)

ForR30the values aren=3andl=0 , we have:

v30(p)=c0+c1p+c2p2

where the constant can be determined using the second equation in (2) as:

c1=2(1-3)(1)(2)c0=-2c0c2=2(2-3)(2)(3)c1=-13c1=23c0c3=2(3-3)(3)(4)c2=0

Substitute into (1) to get the expression as:

R30=1rr3ae-r/3ac0-2c0r3a+23c0r3a2R30=c03a1-23ra+227ra2e-r/3a

03

Find the radial wave function for R31 and R32

For R31the values are n=3and localid="1658144737944" l=1, we have:

V31(p)=c0+c1p+c2p2

where the constant can be determined using the second equation in (2) as:

c1=2(2-3)14c0=-12c0c2=2(2-3)25c1=0

Substitute into (1) to get:

R31=1rr3a2e-r/3ac0-12c0r3a=c09a2r1-16rae-r/3aR31=c09a2r1-16rae-r/3a

For R32the values are n=3andl=2 , we have:

v32(p)=c0+c1p+c2p2

where the constant can be determined using the second equation in (2) as:

c1=2(3-3)(1)(6)c0=0c2=2(3-3)(2)(5)c1=0

Substitute into (1) to get:

R32=1rr3a3e-r/3a(c0)=c027a3r2e-r/3aR32=c027a3r2e-r/3a

Thus the Radial wave functions are:

role="math" localid="1658145305610" R30=c03a1-23ra+227ra2e-r/3aR31=c09a2r1-16rae-r/3aR32=c027a3r2e-r/3a

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

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).

Work out the normalization factor for the spherical harmonics, as follows. From Section 4.1.2we know that

Ylm=BlmeimϕPlmcosθ

the problem is to determine the factor (which I quoted, but did not derive, in Equation 4.32). Use Equations 4.120, 4.121, and 4.130to obtain a recursion

relation giving Blm+1 in terms of Blm. Solve it by induction on to get Blm up to an overall constant Cl, .Finally, use the result of Problem 4.22 to fix the constant. You may find the following formula for the derivative of an associated Legendre function useful:

1-x2dPlmdx=1-x2Plm+1-mxPlm [4.199]

(a) Work out the Clebsch-Gordan coefficients for the case s1=1/2,s2=anything. Hint: You're looking for the coefficients A and Bin

|sm=A|1212|s2(m-12)+B|12(-12)|s2(m+12)

such that|sm is an eigenstate of . Use the method of Equations 4.179 through 4.182. If you can't figure out whatSx(2) (for instance) does to|s2m2 , refer back to Equation 4.136 and the line before Equation 4.147. Answer:

;role="math" localid="1658209512756" A=s2+12±m2s2+1;B=±s2+12±m2s2+1

where, the signs are determined bys=s2±1/2 .

(b) Check this general result against three or four entries in Table 4.8.

(a) Construct the spatial wave function (ψ)for hydrogen in the state n=3,I=2,m=1.Express your answer as a function of r,θ,ϕ,anda(the Bohr radius) only—no other variables (p,z,etc.) or functions (p,v,etc.), or constants (A,c0,etc.), or derivatives, allowed (π is okay, and e, and 2, etc.).

(b) Check that this wave function is properly normalized, by carrying out the appropriate integrals over, θ,andϕ.

(c) Find the expectation value of rsin this state. For what range of s (positive and negative) is the result finite?

(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.)

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.

Sign-up for free