Categories:
Physics,
Quantum mechanics,
Two-level system.
Optical Bloch equations
For an electron in a two-level system with time-independent states
∣g⟩ (ground) and ∣e⟩ (excited),
consider the following general solution
to the time-dependent Schrödinger equation:
∣Ψ⟩=cg∣g⟩e−iεgt/ℏ+ce∣e⟩e−iεet/ℏ
Perturbing this system with
an electromagnetic wave
introduces a time-dependent sinusoidal term H^1 to the Hamiltonian.
In the electric dipole approximation,
H^1 is given by:
H^1(t)=−p^⋅E(t)p^≡qx^E(t)=E0cos(ωt)
Where E is an electric field,
and p^ is the dipole moment operator.
From Rabi oscillation,
we know that the time-varying coefficients cg and ce
can then be described by:
dtdcgdtdce=i2ℏq⟨g∣x^∣e⟩⋅E0ei(ω−ω0)tce=i2ℏq⟨e∣x^∣g⟩⋅E0e−i(ω−ω0)tcg
Where ω0≡(εe−εg)/ℏ is the resonance frequency.
We want to rearrange these equations a bit,
so we split the field E as follows,
where the amplitudes E0− and E0+
may be slowly-varying with respect to the carrier wave e±iωt:
E(t)≡E−(t)+E+(t)≡E0−eiωt+E0+e−iωt
Since E is real, E0+=(E0−)∗.
Similarly, we define the transition dipole moment p0−:
p0−≡q⟨e∣x^∣g⟩p0+≡(p0−)∗=q⟨g∣x^∣e⟩
With these, the equations for cg and ce can be rewritten as shown below.
Note that E− and E+ include the driving plane wave, and the
rotating wave approximation is still made:
dtdcgdtdce=ℏip0+⋅E−e−iω0tce=ℏip0−⋅E+eiω0tcg
For ∣Ψ⟩ as defined above,
the corresponding pure density operator
ρ^ is as follows:
ρ^=∣Ψ⟩⟨Ψ∣=[cece∗cgce∗eiω0tcecg∗e−iω0tcgcg∗]≡[ρeeρgeρegρgg]
We take the t-derivative of the matrix elements,
and insert the equations for cg and ce:
dtdρggdtdρeedtdρgedtdρeg=dtdcgcg∗+cgdtdcg∗=ℏip0+⋅E−cecg∗e−iω0t−ℏip0−⋅E+cgce∗eiω0t=dtdcece∗+cedtdce∗=ℏip0−⋅E+cgce∗eiω0t−ℏip0+⋅E−cecg∗e−iω0t=dtdcgce∗eiω0t+cgdtdce∗eiω0t+iω0cgce∗eiω0t=ℏip0+⋅E−cece∗−ℏip0+⋅E−cgcg∗+iω0cgce∗eiω0t=dtdcecg∗e−iω0t+cedtdcg∗e−iω0t−iω0cecg∗e−iω0t=ℏip0−⋅E+cgcg∗−ℏip0−⋅E+cece∗−iω0cecg∗e−iω0t
Recognizing the density matrix elements allows us
to reduce these equations to:
dtdρggdtdρeedtdρgedtdρeg=ℏi(p0+⋅E−ρeg−p0−⋅E+ρge)=ℏi(p0−⋅E+ρge−p0+⋅E−ρeg)=iω0ρge+ℏip0+⋅E−(ρee−ρgg)=−iω0ρeg+ℏip0−⋅E+(ρgg−ρee)
These equations are correct if nothing else is affecting ρ^.
But in practice, these quantities decay due to various processes,
e.g. spontaneous emission.
Suppose ρee decays with rate γe.
Because the total probability ρee+ρgg=1, we have:
(dtdρee)e=−γeρee⟹(dtdρgg)e=γeρee
Meanwhile, for whatever reason,
let ρgg decay into ρee with rate γg:
(dtdρgg)g=−γgρgg⟹(dtdρgg)g=γgρgg
And finally, let the diagonal (perpendicular) matrix elements
both decay with rate γ⊥:
(dtdρeg)⊥=−γ⊥ρeg(dtdρge)⊥=−γ⊥ρge
Putting everything together,
we arrive at the optical Bloch equations governing ρ^,
which are the basis of the
Maxwell-Bloch equations
and by extension all laser theory:
dtdρggdtdρeedtdρgedtdρeg=γeρee−γgρgg+ℏi(p0+⋅E−ρeg−p0−⋅E+ρge)=γgρgg−γeρee+ℏi(p0−⋅E+ρge−p0+⋅E−ρeg)=−(γ⊥−iω0)ρge+ℏip0+⋅E−(ρee−ρgg)=−(γ⊥+iω0)ρeg+ℏip0−⋅E+(ρgg−ρee)
Some authors simplify these equations a bit by choosing
γg=0 and γ⊥=γe/2.
References
- F. Kärtner,
Ultrafast optics: lecture notes,
2005, Massachusetts Institute of Technology.
- H.J. Metcalf, P. van der Straten,
Laser cooling and trapping,
1999, Springer.