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) Figure out the electron configurations (in the notation of Equation

5.33) for the first two rows of the Periodic Table (up to neon), and check your

results against Table 5.1.

1s22s22p2(5.33).

(b) Figure out the corresponding total angular momenta, in the notation of

Equation 5.34, for the first four elements. List all the possibilities for boron,

carbon, and nitrogen.

LJ2S+1 (5.34).

Short Answer

Expert verified

(a)

Hydrogen:(1s);helium:(1s)2;lithium:(1s)2(2s);beryllium:(1s)2(2s)2;boron:(1s)2(2s)2(2p);carbon:(1s)2(2s)2(2p)2;nitrogen:(1s)2(2s)2(2p)3;oxygen:(1s)2(2s)2(2p)4;fluorine:(1s)2(2s)2(2p)5;neon:(1s)2(2s)2(2p)6;

(b)S1/2,2S3/2,P1/2,2P3/2,24P1/2,P3/2,4P5/2,44D3/2,D5/2.22D1/2,D3/2,44D5/2,4D7/2,4F5/2,F7/2,22F3/2,F5/2,4F7/2,44F9/24.

Step by step solution

01

(a) Figuring out the electron configuration

Hydrogen:1s;helium:1s2;lithium:1s22s;beryllium:1s22s2;boron:1s22s22p;carbon:1s22s22p2;nitrogen:1s22s22p3;oxygen:1s22s22p4;fluorine:1s22s22p5;neon:1s22s22p6;

These values agree with those in Table 5.1-no surprises so far.

02

(b) Figuring out the corresponding total angular momenta 

Hydrogen:S1/22;helium:S01;lithium:S1/22;beryllium:S01;

S0. (These four are unambiguous, because the orbital angular momentum is zero in all cases.) For boron, the spin (1/2) and orbital (1) angular momenta could add to give 3/2 or 1/2, so the possibilities are For carbon, the two p electrons could combine for orbital angular momentum 2, 1, or 0, and the spins could add to 1 or 0:

S0,S1,31P1,P2,3P1,P0,331D2,D3,D2,3D1,331

For nitrogen, the 3 p electrons can add to orbital angular momentum 3, 2, 1, or 0, and the spins to 3/2 or 1/2:

S1/2,2S3/2,P1/2,2P3/2,24P1/2,P3/2,4P5/2,44D3/2,D5/2.22D1/2,D3/2,44D5/2,4D7/2,4F5/2,F7/2,22F3/2,F5/2,4F7/2,44F9/24.

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

In view ofProblem 5.1, we can correct for the motion of the nucleus in hydrogen by simply replacing the electron mass with the reduced mass.

(a) Find (to two significant digits) the percent error in the binding energy of hydrogen (Equation 4.77) introduced by our use of m instead of ฮผ.

E1=-m2h2e24ฯ€โˆž'2=-13.6eV(4.77).

(b) Find the separation in wavelength between the red Balmer lines n=3โ†’n=2for hydrogen and deuterium (whose nucleus contains a neutron as well as the proton).

(c) Find the binding energy of positronium (in which the proton is replaced by a positronโ€”positrons have the same mass as electrons, but opposite charge).

(d) Suppose you wanted to confirm the existence of muonic hydrogen, in which the electron is replaced by a muon (same charge, but 206.77 times heavier). Where (i.e. at what wavelength) would you look for the โ€œLyman-ฮฑโ€ line n=2โ†’n=1?.

The density of copper is8.96g/cm3,and its atomic weight is63.5g/mole

(a) Calculate the Fermi energy for copper (Equation 5.43). Assume d = 1, and give your answer in electron volts.

EF=ฤง22m3ฯฯ€22/3 (5.43).

(b) What is the corresponding electron velocity? Hint: SetEF=1/2mv2Is it safe to assume the electrons in copper are nonrelativistic?

(c) At what temperature would the characteristic thermal energyrole="math" localid="1656065555994" (kBT,wherekBkBis the Boltzmann constant and T is the Kelvin temperature) equal the Fermi energy, for copper? Comment: This is called the Fermi temperature,TF

. As long as the actual temperature is substantially below the Fermi temperature, the material can be regarded as โ€œcold,โ€ with most of the electrons in the lowest accessible state. Since the melting point of copper is 1356 K, solid copper is always cold.

(d) Calculate the degeneracy pressure (Equation 5.46) of copper, in the electron gas model.

P=23EtotV=23ฤง2kF510ฯ€2m=3ฯ€22/3ฤง25mฯ5/3

(a)Use Equation5.113 to determine the energy density in the wavelength rangedฮป. Hint: setฯ(ฯ‰)dฯ‰=ฯ-(ฮป)dฮป, and solve forฯ(ฮป)-

(b)Derive the Wien displacement law for the wavelength at which the blackbody energy density is a maximum
ฮปmax=2.90ร—10-3mKT

You'll need to solve the transcendental equation(5ร—x)=5e-x, using a calculator (or a computer); get the numerical answer accurate to three significant digits.

(a) Using Equations 5.59 and 5.63, show that the wave function for a particle in the periodic delta-function potential can be written in the form

ฯˆ(X)=C[sinkx+e-ikasina-x]0โ‰คxโ‰คa

(b) There is an exception; At the top of a band where z is an integer multiple ofฯ€yielsฯˆ(x)=0 yields .

Find the correct wave function for the case. Note what happens toฯˆeach delta function.

(a) Find the percent error in Stirlingโ€™s approximation for z = 10 ?

(b)What is the smallest integer z such that the error is less than 1%?

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