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For the most general normalized spinor (Equation 4.139),

compute{Sx},{Sy},{Sz},{Sx2},{Sy2},and{Sx2}.checkthat{Sx2}+{Sy2}+{Sz2}={S2}.

X=(ab)=aX++bX(4.139).

Short Answer

Expert verified

By solving we find the above value to beSx2+Sy2+Sz2=h24.

Step by step solution

01

Calculating

ComputingSx,Sy,Sz,Sx2,Sy2andSz2

Sx=h2a*b*0110(-)ba=h2a*b*(-)bah2a*b+b*a=hReab*.

Sy=h2a*b*0-ii0ab=h2a*b*-ibia

=h2-ia*b+iab*=h2iab*-a*b=-hlmab*.

Sz=h2a*b*100-1ab=h2a*b*a-b=h2a*a-b*b=h2a2b2.

Sx2=h2401100110=h240110=h24

Sy2=h2401100110=h24

localid="1655968926137" Sz2=h2401100110=h24soSx2=Sy2=Sz2=h24

02

Checking that<Sx2>+<Sy2>+<Sz2>+<S2>.

Sx2+Sy2+Sz2=34h2=ss+1h2=12?12+1h2=34h2=S2

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Most popular questions from this chapter

What is the probability that an electron in the ground state of hydrogen will be found inside the nucleus?

  1. First calculate the exact answer, assuming the wave function is correct all the way down tor=0. Let b be the radius of the nucleus.
  2. Expand your result as a power series in the small numbera=2bla, and show that the lowest-order term is the cubic:P≈(4l3)(bla)3. This should be a suitable approximation, provided thatb≪a(which it is).
  3. Alternatively, we might assume thatψ(r)is essentially constant over the (tiny) volume of the nucleus, so thatP≈(4l3)πb3lψ(0)l2.Check that you get the same answer this way.
  4. Useb≈10-15manda≈0≈5×10-10mto get a numerical estimate forP. Roughly speaking, this represents the fraction of its time that the electron spends inside the nucleus:"

[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)ħӬ1+(n2+12)ħӬ2,(n1,n2=0,1,2,...)whereӬ1≡qB0/mandӬ2≡2qK/m. Comment: If K=0this is the quantum analog to cyclotron motion;Ӭ1 is the classical cyclotron frequency, and it's a free particle in the z direction. The allowed energies,(n1+12)ħӬ1, are called Landau Levels.

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

Φ(p,t)=12πh∫∞∞e-ipx/hψ(x,t)dx(3.54).ϕ(p)≡1(2πh)3/2∫e-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,Ï•)=1Ï€²¹3e-r/a(4.80).Ï•(p)=1Ï€(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).

Consider the observablesA=x2andB=Lz .

(a) Construct the uncertainty principle forσAσB

(b) EvaluateσB in the hydrogen stateψn/m .

(c) What can you conclude about<xy>in this state?

a) Check that Arj1(kr)satisfies the radial equation with V(r)=0and I=1.

(b) Determine graphically the allowed energies for the infinite spherical well, when I=1. Show that for large n,En1≈(h2π2/2ma2)(n+1/2)2. Hint: First show that j1(x)=0⇒x=tanx. Plot xandtanxon the same graph, and locate the points of intersection.

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