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

(a) NormalizeR20 (Equation 4.82), and construct the functionψ200.

(b) NormalizeR21(Equation 4.83), and construct the function.

Short Answer

Expert verified

(a) By normalizing the equation, we get

c0=2a,ψ200=12πa12a1-r2ae-r2a

(b) By normalizing the equation, we get

c0=23a,ψ211=-18πra5/2e-r/2asin(θ)eiϕψ21-1=-18πra5/2e-r/2asin(θ)eiϕψ210=-18πra5/2e-r/2acos(θ)

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

First, we need to work out the radial wave functions R20,andR21,we will use:

Rnl(r)=1runl(r)

Where,

unl(p)=pl+1e-pvnl(p)

Thus,

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

Where,

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

ForR20 the values aren=2 andl=0 , we have:

v20(p)=c0+c1p

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

c1=2(1-2)(1)(2)c0=-c0

Substitute into (1) to get :

R20=12ae-r/2ac01-r2a

And forR21 we have,

R21(r)=1ru21(r)=r(2a)2e-r2ac0

03

Normalize the radial wave function

Toc0findnormalize the radial function in the equation as,

0r2R20(r)2dr=0c02r212a1-r2a2e-r/adr

Letz=r/a, so:

c02a2a301-z22e-zz2dz=1c02a40z2-z3+14z4e-zdz=1

using the integral:

0xne-x=Τ(n+1)=n!

we get:

c02a42!-3!+4!4=1c02a42-6+244=1a2c02=1c0=2a

the complete wave function is:

ψ200=R20(r)y00(ϕ,θ)

where (from table 4.3):

y00=-14π

Then,

ψ200=12πa12a1-r2ae-r2a

04

Normalize the radial wave function in equation(4)

To findc0, we normalize the radial function in equation (4) following the same method in part (a) wherez=r/a, so we get:

1=c04a22a50z4e-zdz1=c02a16241=32ac02c0=23a

In this case there are 3 wave functions corresponding ton=2,l=1for which we need the spherical harmonics:

y11=-38π1/2sin(θ)eiϕy1-1=-38π1/2sin(θ)eiϕy10=-38π1/2cos(θ)

The corresponding wave functions are:

ψ211=-18πra5/2e-r/2asin(θ)eiϕψ21-1=-18πra5/2e-r/2asin(θ)eiϕψ210=-18πra5/2e-r/2acos(θ)

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

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 .

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]

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).

(a) For a functionf(ϕ)that can be expanded in a Taylor series, show that f(ϕ+φ)=eiLzφ/f(ϕ) (where is an arbitrary angle). For this reason, Lz/ is called the generator of rotations about the Z-axis. Hint: Use Equation 4.129 , and refer Problem 3.39.More generally, L·n^/ is the generator of rotations about the direction n^, in the sense that exp(iL·n^φ/)effects a rotation through angleφ (in the right-hand sense) about the axis n^ . In the case of spin, the generator of rotations is S·n^/. In particular, for spin 1/2 χ'=ei(σ·n^)φ/2χtells us how spinors rotate.

(b) Construct the (2×2)matrix representing rotation by 180about the X-axis, and show that it converts "spin up" χ+into "spin down"χ- , as you would expect.

(c) Construct the matrix representing rotation by 90about the Y-axis, and check what it does to

χ+

(d) Construct the matrix representing rotation by 360about the -Zaxis, If the answer is not quite what you expected, discuss its implications.

(e) Show thatei(σ·n^)φ/2=cos(φ/2)+i(n^·σ)sin(φ/2)

The electron in a hydrogen atom occupies the combined spin and position stateR211/3Y10χ++2/3Y11χ-

(a) If you measured the orbital angular momentum squared L2, what values might you get, and what is the probability of each?

(b) Same for the component of orbital angular momentum Lz.

(c) Same for the spin angular momentum squaredS2 .

(d) Same for the component of spin angular momentum Sz.

Let JL+Sbe the total angular momentum.

(e) If you measureddata-custom-editor="chemistry" J2 , what values might you get, and what is the probability of each?

(f) Same forJz .

(g) If you measured the position of the particle, what is the probability density for finding it atr , θ,ϕ ?

(h) If you measured both the component of the spin and the distance from the origin (note that these are compatible observables), what is the probability density for finding the particle with spin up and at radius ?

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