(a) Work out all of the canonical commutation relations for components of the operator r and p : [x,y],[x,py],[x,px],[py,pz],and so on.

(b) Confirm Ehrenfest’s theorem for 3 dimensions

ddt<r>=1m<p>andddt<p>=<-v>

(Each of these, of course, stand for three equations- one for each component.)

(c) Formulate Heisenberg’s uncertainty principle in three dimensions Answer:

σxσph2;σyσph2;σzσph2

But there is no restriction on, say, σxσpy.

Short Answer

Expert verified

(a)The canonical commutation relations is [x^,y^]f=[y^,x^]f

(b) Ehrenfest’s theorem is dddt=-V

(c) The Heisenberg’s uncertainty principle is σxσpyh2δij

Step by step solution

01

Define the Schrödinger equation

A differential equation describes matter in quantum mechanics in terms of the wave-like properties of particles in a field. Its answer is related to a particle's probability density in space and time.

02

Determine the canonical commutation relations 

x^,y^=-y^,x^From the axioms of quantum mechanics, we get that

x^f=xf and
p^i=-ihri

By definition, we also know that
δij=1
if otherwise,
δij=0

This letter of definition leads to the following useful identities

A^,B^=-B^,A^

A^B^,C^=B^A^,C^+A^B^,C^A^2,B^=A^A^,B^+A^,B^A^

Let, f be a twice continuously differentiable function,

x^,y^f=x^y^-y^x^fx^,y^f=x^y^f-y^x^fx^,y^f=xyf-yxfx^,y^f=yxf-xyfx^,y^f=y^x^-x^y^fx^,y^f=y^,x^f

But since we also know thatx^,y^=-y^,x^, this implies that x^,y^=y^,x^=0

By symmetry, we then see that for all i,j

03

Determine the Ehrenfest’s theorem

ri,rj=rj,ri=0

Now consider p^y,p^z

p^y,p^zf=-ih(2yz-2zy)fp^y,p^zf=-ih(2fyz-2fzy)p^y,p^zf=0

By equality of mixed second partial derivatives,

By symmetry, we then see that for all, i,j

p^i,p^j=p^j,p^i=0

Next, consider x^p^yapplying this operator to the function f , we find that

x^p^yf=x^p^yf-p^yx^fx^p^yf=-ih(xfy-(xf)y)x^p^yf=-ih(xfy-fy)x^p^yf=0

By symmetry, we then see that for all

r^ip^j=p^jr^i=0

But we also want to know what r^ip^j is when i=j so we considerx^p^x

x^p^xf=x^p^xf-p^xx^fx^p^xf=-ih(xfx-(xf)xx^p^xf=-ih(xfx-f-fx)x^p^xf=ihf

r^ip^j=ihfor all i follows by symmetry

Together with the above result ijwe see that for all i,j

r^ip^j=p^jr^i=ihδijdx^df=ihH^,x^H^=p22m+V^(r)andp2=px2+py2+pz2H^,x^=12mp2,x+V,xH^,x^=12mpx2,x+py2,x+pz2,x+Vx-xVH^,p^x=12mpx2,px+VpxH^,p^x=VpxV,px=-ih(Vfx-(Vf)x)=ihVxf

V,px=ihvxH^,p^x=ihvxdp^xdt=ihihvxdpdt=-V

by the symmetry ofx,y,z

04

Determine the Heisenberg’s uncertainty principle

σxσpx=12ix,px=12iih=h2σyσpy=12iy,py=12iih=h2σzσpz=12iz,pz=12iih=h2σxσpy=12ix,py=0σxσpyh2δijbythesymmetryx,y,z

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Most popular questions from this chapter

(a) For a functionf(ϕ)that can be expanded in a Taylor series, show that f(ϕ+φ)=eiLzφ/f(ϕ) (where is an arbitrary angle). For this reason, Lz/ is called the generator of rotations about the Z-axis. Hint: Use Equation 4.129 , and refer Problem 3.39.More generally, L·n^/ is the generator of rotations about the direction n^, in the sense that exp(iL·n^φ/)effects a rotation through angleφ (in the right-hand sense) about the axis n^ . In the case of spin, the generator of rotations is S·n^/. In particular, for spin 1/2 χ'=ei(σ·n^)φ/2χtells us how spinors rotate.

(b) Construct the (2×2)matrix representing rotation by 180about the X-axis, and show that it converts "spin up" χ+into "spin down"χ- , as you would expect.

(c) Construct the matrix representing rotation by 90about the Y-axis, and check what it does to

χ+

(d) Construct the matrix representing rotation by 360about the -Zaxis, If the answer is not quite what you expected, discuss its implications.

(e) Show thatei(σ·n^)φ/2=cos(φ/2)+i(n^·σ)sin(φ/2)

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)=0x=tanx. Plot xandtanxon the same graph, and locate the points of intersection.

An electron is in the spin state

χ=A3i4

(a) Determine the normalization constant .

(b) Find the expectation values of Sx,Sy , and Sz.

(c) Find the "uncertainties" ,σSx , σSyandσSz . (Note: These sigmas are standard deviations, not Pauli matrices!)

(d) Confirm that your results are consistent with all three uncertainty principles (Equation 4.100 and its cyclic permutations - only with in place ofL, of course).

(a) Apply S_tolocalid="1656131461017" 10>(Equation4.177), and confirm that you getlocalid="1656131442455" 2h1-1>.

(b) ApplyS+to[00>(Equation4.178), and confirm that you get zero.

(c) Show thatlocalid="1656131424007" 11>andlocalid="1656131406083" 1-1>(Equation4.177) are eigenstates ofS2, with the appropriate eigenvalue

(a) Work out the Clebsch-Gordan coefficients for the case s1=1/2,s2=anything. Hint: You're looking for the coefficients A and Bin

|sm=A|1212|s2(m-12)+B|12(-12)|s2(m+12)

such that|sm is an eigenstate of . Use the method of Equations 4.179 through 4.182. If you can't figure out whatSx(2) (for instance) does to|s2m2 , refer back to Equation 4.136 and the line before Equation 4.147. Answer:

;role="math" localid="1658209512756" A=s2+12±m2s2+1;B=±s2+12±m2s2+1

where, the signs are determined bys=s2±1/2 .

(b) Check this general result against three or four entries in Table 4.8.

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