570 Quantum time-dependent statistical mechanics
d. Calculate the energy spectrumQ(ω) forω >0. Interpret your results,
and in particular, explain how the allowed absorptions and emissions
are manifest in your final expression. Plot the absorption part of your
spectrum. Where do you expect the peak intensity to occur?
Hint: Consider using a convergence factor, exp(−ǫ|t|), and letǫgo to 0
at the end of the calculation.
e. Based on your results from parts a–d, plot the spectrum three-dimensional
rigid rotor, for which the energy eigenvalues areElm= ̄h^2 l(l+ 1)/ 2 Iand
m=−l,...,lis the quantum number for thez-component of angular
momentum. Where do you expect the peak intensity to occur in the 3-
dimensional case?
14.7. Derive a discrete path-integral representation for the Kubo-transformed quan-
tum time correlation functionKAB(t) defined in eqn. (14.6.11).
14.8. Consider two spin-1/2 particles at fixed points in space a distanceRapart
and interacting with a magnetic fieldB= (0, 0 ,B). The particles carry charge
qand−q, respectively. The Hamiltonian of the system is
Hˆ=−γB·Sˆ−q
2
R
,
whereSˆ=Sˆ 1 +Sˆ 2 is the total spin, andγis the spin gyromagnetic ratio.
a. What are the allowed energy levels of this system?
b. Suppose that a time-dependent perturbation of the form
Hˆ 1 (t) =−γb·Sˆe−t^2 /τ^2 ,
whereb= (b, 0 ,0) is applied att=−∞. Att=−∞, the system is in its
unperturbed ground state. To first order in perturbation theory, what is
the probability, ast−→∞, that the system will make a transition from
its ground state to a state with energy−q^2 /R?
14.9. Thedensity of vibrational states, also known as thepower spectrum orspec-
tral density, is the Fourier transform of the velocity autocorrelation function:
I(ω) =
1
√
2 π
∫∞
−∞
dt e−iωtCvv(t).
I(ω) encodes information about the vibrational modes of a system; however,
it does not provide any information about net absorption intensities. For
the two model velocity autocorrelation functions in Problem 13.1, calculate
the density of vibrational states and interpret them in terms of the physical
situations described by these two model correlation functions.