(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) 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.

Determine the commutator of S2withSZ(1)(whereSS(1)+S(2)) Generalize your result to show that

[S2,S1]=2Ih(S1×S2)

Comment: Because Sz(1)does not commute with S2, we cannot hope to find states that are simultaneous eigenvectors of both. In order to form eigenstates ofS2weneed linear combinations of eigenstates ofSz(1). This is precisely what the Clebsch-Gordan coefficients (in Equation 4.185) do for us, On the other hand, it follows by obvious inference from Equation 4.187that the sumrole="math" localid="1655980965321" S(1)+S(2)does commute withdata-custom-editor="chemistry" S2, which is a special case of something we already knew (see Equation 4.103).

An electron is at rest in an oscillating magnetic field

B=B0cos(ωt)k^

whereB0 andω are constants.

(a) Construct the Hamiltonian matrix for this system.

(b) The electron starts out (at t=0 ) in the spin-up state with respect to the x-axis (that is:χ(0)=χ+(x)). Determine X(t)at any subsequent time. Beware: This is a time-dependent Hamiltonian, so you cannot get in the usual way from stationary states. Fortunately, in this case you can solve the timedependent Schrödinger equation (Equation 4.162) directly.

(c) Find the probability of getting-h/2 , if you measure Sx. Answer:

sin2(γB02ωsin(ωt))

(d) What is the minimum field(B0) required to force a complete flip inSx ?

What is the most probable value of r, in the ground state of hydrogen? (The answer is not zero!) Hint: First you must figure out the probability that the electron would be found between r and r + dr.

Work out the spin matrices for arbitrary spin , generalizing spin (Equations 4.145 and 4.147), spin 1 (Problem 4.31), and spin (Problem 4.52). Answer:

Sz=(s0000s-10000s-200000-s)Sx=2(0bs0000bs0bs-10000bs-10bs-20000bs-200000000b-s+10000b-s+10)Sy=2(0-ibs0000ibs0-ibs-10000-ibs-10-ibs-20000-ibs-200000000-ibs+10000-ibs+10)

where,bj(s+j)(s+1-j)
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