(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.

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Most popular questions from this chapter

(a) If ψaandψb are orthogonal, and both normalized, what is the constant A in Equation 5.10?

(b) Ifrole="math" localid="1658225858808" ψa=ψb (and it is normalized), what is A ? (This case, of course, occurs only for bosons.)

(a) Write down the Hamiltonian for two noninteracting identical particles in the infinite square well. Verify that the fermion ground state given in Example 5.1 is an eigenfunction of H, with the appropriate eigenvalue.

(b) Find the next two excited states (beyond the ones in Example 5.1) - wave functions and energies - for each of the three cases (distinguishable, identical bosons, identical fermions).

(a) Calculate<1/r1-r2>for the stateψ0(Equation 5.30). Hint: Dod3r2integral

first, using spherical coordinates, and setting the polar axis alongr1, so

that

ψ0r1,r2=ψ100r1ψ100r2=8πa3e-2r1+r2/a(5.30).

r1-r2=r12+r22-2r1r2cosθ2.

Theθ2integral is easy, but be careful to take the positive root. You’ll have to

break ther2integral into two pieces, one ranging from 0 tor1,the other fromr1to

Answer: 5/4a.

(b) Use your result in (a) to estimate the electron interaction energy in the ground state of helium. Express your answer in electron volts, and add it toE0(Equation 5.31) to get a corrected estimate of the ground state energy. Compare the experimental value. (Of course, we’re still working with an approximate wave function, so don’t expect perfect agreement.)

E0=8-13.6eV=-109eV(5.31).

Evaluate the integrals (Equation5.108 and 5.109) for the case of identical fermions at absolute zero. Compare your results with equations 5.43 and5.45. (Note for electrons there is an extra factor of 2 in Equations 5.108 and 5.109. to account for the spin degeneracy.)

Suppose you could find a solutionψ(r1,r2,...,rz)to the Schrödinger equation (Equation 5.25), for the Hamiltonian in Equation 5.24. Describe how you would construct from it a completely symmetric function, and a completely anti symmetric function, which also satisfy the Schrödinger equation, with the same energy.

role="math" localid="1658219144812" H^=j=1Z-ħ22mj2-14πo,0Ze2rj+1214πo,0j1Ze2rj-rk (5.24).

role="math" localid="1658219153183" H^ψ=E (5.25).

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