(a) For a function f(x)that can be expanded in a Taylor series, show that f(x+x0)=eip^x0Ihf(x)

wherex_{0}

is any constant distance). For this reason, p^/his called the generator of translations in space. Note: The exponential of an operator is defined by the power series expansion: eQ^1+Q^+(1/2)Q^2+(1/3!)Q^3+...

(b) If ψ(x,t)satisfies the (time-dependent) Schrödinger equation, show that ψ(x,t+t0)=e-iH^t0/hψ(x,t)

where t_{0}is any constant time); -H^/his called the generator of translations in time.

(c) Show that the expectation value of a dynamical variableQ(x,p,t), at time , t+t0can be written34

<Q>t+t0=<ψx,t|eiH^t0/hQ^x^,p^,t+t0e-iH^t0/h|ψx,t>

Use this to recover Equation 3.71. Hint: Lett0=dt, and expand to first order in dt.

Short Answer

Expert verified

Required answers are

afx+x0=eipx0/hfxbψx,t+t0=e-iHt0/hψx,t+t0cQt-t0=ψx,t|e-iHt0/hQx,p,t+t0e-iHt0/h|ψx,t

Step by step solution

01

Step 1(a) : Taylor series about x0

Taylor series about x0

Consider the function offxwhich can be expanded using Taylor series. By expanding in a Taylor series aboutx0, we get:

fx+x0=n=01n!x0nddxnfx

momentum operator is given by:

p=hiddxddx=iph

02

solve for f(x+x0)

fx+x0=n=01n!x0niphnfx=n=01n!ipx0hnfx

But the power series expansion is given by:

eQ^=1+Q+12!Q^2+13!Q^3+...=n=01n!Q^n

Using this expansion, the above equation becomes:

fx+x0=eipx0/hfx

03

Step 3(b) : Taylor series aboutt0

Now consider the function ofψx,twhich can be expanded using Taylor series. By expanding in a Taylor series aboutt0, we get:

localid="1656049111899" ψx,t+t0=n=01n!x0nddtnψx,t+t0

04

solve forψ(x,t+t0)

But,

ihψt=Hψ

But this doesn't mean,role="math" localid="1656049008992" iht=H these two operators have the same effect only when they are acting on solutions to the time dependent Schrodinger equation. Apply this operator two times, we get:

ihtψ=ihHψ=Hiht=H2ψ

And so on, so we can write:

t=-ihH

Substitute into the above equation we get:

ψx,t+t0=n=01n!x0n-ihHnψx,t+t0

using the power series expansion, we get

ψx,t+t0=e-iHt0/hψx,t+t0

05

Step 5(c) : show that the expectation value

Now we need to show that the expectation value of a dynamical variableQx,p,t, at timet+t0is:

Qt+t0=ψx,t|eiH^t0/hQ^x^,p^,t+t0eiH^t0/h|ψx,t

we start with:

Qt+t0=ψx,t+t0|Qx,p,t+t0|ψx,t+t0

but ψx,t+t0=eiH^t0/hψx,tandeiH^t0/hI=eiH^t0/h, so we can write:

Qt+t0=ψx,t|eiH^t0/hQx,p,t+t0e-iH^t0/h|ψx,t

now let t0=dtbe very small, then we can expand to the first order using the expansion of the exponential, as:

Qt+dQdtdt=ψx,t|a˙|ψx,t

Where,

a˙=1+iHhdtQx,p,t+Qtdt1-iHhdt=Qx,p,t+iHhdtQ-Q1-iHhdt+Qtdt=Q+ihH,Qdt+Qtdtψx,ta˙ψx,t=Qt+ihH,Qdt+QtdtdQdt=ihH,Q+Qt

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Most popular questions from this chapter

Let Q^be an operator with a complete set of orthonormal eigenvectors:localid="1658131083682" Q^en>=qnen(n=1,2,3,....) Show thatQ^can be written in terms of its spectral decomposition:Q^=nqnen><en|

Hint: An operator is characterized by its action on all possible vectors, so what you must show is thatQ^={nqnen><en|} for any vector α>.

The Hamiltonian for a certain three-level system is represented by the matrix

H=hω[100020002] Two other observables, A and B, are represented by the matrices A=λ[010100002],B=μ[200001010],where ω, , and μ are positive real numbers.

(a)Find the Eigen values and (normalized) eigenvectors of H, A and B.

(b) Suppose the system starts out in the generic staterole="math" localid="1656040462996" |S(0)>=(c1c2c3)

with |c1|2+|c2|2+|c3|2=1. Find the expectation values (at t=0) of H, A, and B.

(c) What is |S(t)>? If you measured the energy of this state (at time t), what values might you get, and what is the probability of each? Answer the same questions for A and for B.

Consider the wave functionΨ(x,0)={12ei2πx/λ,-<x<0,

wherenis some positive integer. This function is purely sinusoidal (with wavelengthλ)on the interval-<x<, but it still carries a range of momenta, because the oscillations do not continue out to infinity. Find the momentum space wave functionΦ(p,0). Sketch the graphs of|Ψ(x,0)|2and|Φ(p,0)|2, and determine their widths,wxandwp(the distance between zeros on either side of the main peak). Note what happens to each width asn. Usingwxandwpas estimates ofxandp, check that the uncertainty principle is satisfied. Warning: If you try calculatingσp, you're in for a rude surprise. Can you diagnose the problem?

Suppose Ψ(x,0)=Ax2+a2.(-<x<)for constantsA and a.

(a) Determine A, by normalizingΨ(x,0)

(b) Find, and(at time).

(c) Find the momentum space wave functionΦ(p,0), and check that it is normalized.

(d) UseΦ(p,0)to calculatep,p2, andσp(at timet=0).

(e) Check the Heisenberg uncertainty principle for this state.

Consider the operator Q^=d2/dϕ2, where (as in Example 3.1)ϕ is the azimuthal angle in polar coordinates, and the functions are subject to Equation 3.26. Is Q^Hermitian? Find its eigenfunctions and eigenvalues. What is the spectrum of Q^? Is the spectrum degenerate?

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