a) Check that the spin matrices (Equations 4.145 and 4.147) obey the fundamental commutation relations for angular momentum, Equation 4.134.

Sz=h2(100-1)(4.145).Sx=h2(0110),sy=h2(0-ii0)(4.147).[Sx,Sy]=ihSz,[Sy,Sz]=ihSx,[Sz,Sx]=ihSy(4.134).(b)ShowthatthePaulispinmatrices(Equation4.148)satisfytheproductruleσx(0110),σy(0-ii0),σz(100-1)(4.148).σjσk=δjk+io'IjklσI,(4.153).

Wheretheindicesstandforx,y,orz,ando'jklistheLevi-Civitasymbol:+1ifjkl=123,231,or2=312;-1ifjkl=132,213,or321;otherwise.

Short Answer

Expert verified

(a)Sx,Sy=ihSz-(b)σjσk=δjk+iojkl'σI-I

Step by step solution

01

(a) Checking the spin matrices obey the fundamental commutation relations for angular momentum.

The spin matrices are

Sz=h2100-1Sx=h20110,Sy=h20-ii0Sx,Sy=SxSy-SySx=h2201100-ii0-0-ii00110.=h24i00-i--i00i=h242i00-2i=ihh22100-1Sx,Sy=ihSz

02

(b) Showing the Pauli spin matrices satisfies the product rule.

σxσx=1001=1=σyσy=σzσz,Soσjσj=1forj=x,y,orz.σxσy=i00-i=iσz;σyσz=0ii0=iσx;σzσx=01-10=iσy.σyσx=-i00-i=iσz;σzσy=0-i-i0=-iσx;σxσz=0-110=-iσy.

Equation 4.153 packages all this in a single formula.

σjσk=δjk+iIojklσI.'

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Most popular questions from this chapter

Consider the three-dimensional harmonic oscillator, for which the potential is

V(r)=122r2

(a) Show that separation of variables in cartesian coordinates turns this into three one-dimensional oscillators, and exploit your knowledge of the latter to determine the allowed energies. Answer:

En=(n+3/2)hω

(b) Determine the degeneracyofd(n)ofEn.

[Refer to. Problem 4.59for background.] Suppose A=B02(X^-yI^) andφ=Kz2, where B0 and Kare constants.

(a) Find the fields E and B.

(b) Find the allowed energies, for a particle of mass m and charge q , in these fields, Answer: E(n1,n2)=(n1+12)ħω1+(n2+12)ħω2,(n1,n2=0,1,2,...)whereω1qB0/mandω22qK/m. Comment: If K=0this is the quantum analog to cyclotron motion;ω1 is the classical cyclotron frequency, and it's a free particle in the z direction. The allowed energies,(n1+12)ħω1, are called Landau Levels.

Use equations 4.27 4.28 and 4.32 to constructy00,y21Check that they are normalized and orthogonal

The (time-independent) momentum space wave function in three dimensions is defined by the natural generalization of Equation 3.54:

Φ(p,t)=12πhe-ipx/hψ(x,t)dx(3.54).ϕ(p)1(2πh)3/2e-i(p.r)Ihψ(r)d3r.(4.223).

(a)Find the momentum space wave function for the ground state of hydrogen (Equation 4.80). Hint: Use spherical coordinates, setting the polar axis along the direction of p. Do the θ integral first. Answer:

ψ100(r,θ,ϕ)=1πa3e-r/a(4.80).ϕ(p)=1π(2ah)3/21[1+ap/h2]2.(4.224).

(b) Check that Φ(p)is normalized.

(c) Use Φ(p)to calculate <p2>, in the ground state of hydrogen.

(d) What is the expectation value of the kinetic energy in this state? Express your answer as a multiple of E1, and check that it is consistent with the virial theorem (Equation 4.218).

<T>=-En;<V>=2En(4.218).

(a) Use the recursion formula (Equation 4.76) to confirm that whenI=n-1 the radial wave function takes the form

Rn(n-1)=Nnrn-1e-r/na and determine the normalization constant by direct integration.

(b) Calculate 200a and <r2> for states of the form ψn(n-1)m·

(c) Show that the "uncertainty" in r(δr) is<r>/2n+1for such states. Note that the fractional spread in decreases, with increasing (in this sense the system "begins to look classical," with identifiable circular "orbits," for large ). Sketch the radial wave functions for several values of, to illustrate this point.

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