(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).

Short Answer

Expert verified

a=32a4a.a42-2.2a83-a.a82=32a116-1128-164=54a.bVeee24π'<1r1-r2>=54e24π'1a=5m4h2e24π'2=52-E1=5213.6eV

Step by step solution

01

(a) Calculating <1/r1-r2>for the state ψ0

<1r1-r2>=8πa32e-4r1+r2/ar21+r22-2r1r2cosθ2d3r2d3r1.=2π0e-4r1+r2/a0πsinθ2r21+r22-2r1r2cosθ22r22dar2.x

a=1r1r2r12+r22-2r1r2cosθ2|0π=1r1r2r12+r22+2r1r2-r12+r22+2r1r2.=1r1r2r1+r2-r1-r2=2/r1r2<r12/r2r2>r1.=4πe-4r1/a1r10r1r22e-4r2/adr2+r1r2e-4r2/adr2.1r10r1r22e-4r1/adr2=1r1-a4r22e-4r2/a+a2a42e-4r2/a-4r2a-1|0r1=-a4r1r12e-4r1/a+ar12e-4r1/a+a28e-4r1/a-a28.r1r2e-4r2/adr2=a42e-4r2/a-4r2a-1|r1=ar14e-4r1/a+a216e-4r1/a=4πa332r1e-4r1/a+-ar4-a28-a332r1+ar14+a216e-8r1/a

=πa28ar1e-4r1/a-2+ar1e-8r1/a.

<1r1-r2>=8πa4.4π0ar1e-4r1/a-2+ar1e-8r1/ar12dr1.=32a4a.0r1e-4r1/adr1-20r12e-8r1/adr1-a0r1e-8r1/adr1.=32a4a.a42-2.2a83-a.a82=32a116-1128-164=54a.

02

(b) Estimating the electron interaction energy

Veee24π'<1r1-r2>=54e24π'1a=54mhe24π'2=52-E1=5213.6eV.E0+Vee=-109+34eV=-75eV,whichisprettyclosetotheexperimentalvalue-79eV).

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Most popular questions from this chapter

(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).

Imagine two non interacting particles, each of mass , in the one dimensional harmonic oscillator potential (Equation 2.43). If one is in the ground state, and the other is in the first excited state, calculate (x1-x2)2assuming
(a) they are distinguishable particles, (b) they are identical bosons, and (c) they are identical fermions. Ignore spin (if this bothers you, just assume they are both in the same spin state.)

Use the method of Lagrange multipliers to find the rectangle of largest area, with sides parallel to the axes that can be inscribed in the ellipse(xa)2+(yb)2=1. What is the maximum area?

Derive the Stefan-Boltzmann formula for the total energy density in blackbody radiation

EV=(π2kB415ħ3C3)T4=7.57×10-16Jm-3K-4T4

Suppose you had three particles, one in stateψa(x), one in stateψb(x), and one in stateψc(x). Assuming ψa,ψb, andψc are orthonormal, construct the three-particle states (analogous to Equations 5.15,5.16, and 5.17) representing

(a) distinguishable particles,

(b) identical bosons, and

(c) identical fermions.

Keep in mind that (b) must be completely symmetric, under interchange of any pair of particles, and (c) must be completely antisymmetric, in the same sense. Comment: There's a cute trick for constructing completely antisymmetric wave functions: Form the Slater determinant, whose first row isψa(x1),ψb(x1),ψc(x1) , etc., whese second row isψa(x2),ψb(x2),ψc(x2) , etc., and so on (this device works for any number of particles).

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