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Typically, the interaction potential depends only on the vectorr=r1-r2between

the two particles. In that case the Schrodinger equation seperates, if we change variables from r1,r2andR=(m1r1+m2r2)I(m1+m2)(the center of mass).

(a)Show that

localid="1655976113066" r1=R+(μ/m1)r,r2=R-(μ/m)r,and1=(μ/m)R+r,2=(μ/m1)R-r,where

localid="1655976264171" μ=m1m2m1+m2(5.15).

is the reduced mass of the system

(b) Show that the (time-independent) Schrödinger equation (5.7) becomes

-h22m112ψ-h22m222ψ+=-h22(m1+m2)R2ψ-h22μr2ψ+V(r)ψ=.(5.7).

(c) Separate the variables, letting ψ(R,r)=ψR(R)ψr(r)Note that ψRsatisfies the

one-particle Schrödinger equation, with the total mass (m1+m2)in place of m, potential zero, and energy ERwhile ψrsatisfies the one-particle Schrödinger equation with the reduced mass in place of m, potential V(r) , and energy localid="1655977092786" Er. The total energy is the sum: E=ER+Er. What this tells us is that the center of mass moves like a free particle, and the relative motion (that is, the motion of particle 2 with respect to particle 1) is the same as if we had a single particle with the reduced mass, subject to the potential V. Exactly the same decomposition occurs in classical mechanics; it reduces the two-body problem to an equivalent one-body problem.

Short Answer

Expert verified

(a)=(m2m1+m2)X-(1)x=μm1(R)x,so2=μm1R-r.

(b)-h22m1+m2R2ψ-h22μr2ψ+V(r)ψ=Eψ.

(c)-h22(m1+m2)2ψR=ERψR,-h22μ2ψr+V(r)ψr=Erψr,withER+Er=E.

Step by step solution

01

(a)Showingr1=R+(μ/m1)r, r2=R-(μ/m2)r,and ∇1=(μ/m2) ∇R+∇r,∇2=(μ/m1) ∇R-∇r, 

m1+m2R=m1r1+m2m2=m1r1+m2r1-r=m1+m2r1-m2rr1=R+m2m1+m2r=R+μm1rm1+m2R=m1r2+r+m2r2=m1+m2r2+m1rr2=R-m1m1m2r=R-μm2r.

Let R = (X, Y,Z); r = (x,y, z).

1x=x1=Xx1X+xx1x.=m1m1+m2X+1x=μm2RX+rX,so1=μm2R+r.2x=x2=Xx2X+xx2x.=m2m1+m2X-1x=μm1RX+rX,so2=μm1R+r.

02

(b)Showing the (time-independent) Schrödinger equation

12ψ=1.1ψ=1.μm2Rψ+rψ.=μm2R.μm2Rψ+rψ+r.μm2Rψ+rψ.=μm22R2ψ+2μm2r.Rψ+r2ψ.Likewise,22ψ=μm1R2ψ-2r.R+r2ψ.

Hψ=-h22m112ψ-h22m222ψ+Vr1,r2ψ.=-h22μ2m1m2R2+2μm1m2r.R+1m1r2+μ2m1m12R2-2μm2m1r.R+1m2r2ψ+Vrψ=-h22μ2m1m21m2+1m2R2+1m2+1m2R2ψ+Vrψ=Eψ.But1m2+1m2=m1+m2m1m2=1μ,soμ2m1m21m2+1m2=μ2m1m2=m1m2m1m2m1m2=1m1+m2-h22m1+m2R2ψ-h22μR2ψ+Vrψ=Eψ.

03

(c) Separating the variables, letting ψ(R,r)=ψR(R)ψr(r)

putinψ=ψrrψRR,anddividebyψrψR:-h22m1+m21ψRR2ψR+-h22μ1ψrr2ψr+Vr.

The first term depends only on R, the second only on r, so each must be a constant; call

them ERandEr, respectively. Then:

-h22(m1+m2)2ψR=ERψR,-h22μ2ψr+V(r)ψr=Erψr,withER+Er=E.

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Most popular questions from this chapter

Find the average energy per free electron (Etot/Nd), as a fraction of the

Fermi energy. Answer:(3/5)EF

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).

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.)

(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

ψ(X)=C[sinkx+e-ikasina-x]0xa

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

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

(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).

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