Categories:
Physics,
Quantum mechanics.
Berry phase
Consider a Hamiltonian H^ that does not explicitly depend on time,
but does depend on a given parameter R.
The Schrödinger equations then read:
iℏdtd∣Ψn(t)⟩H^(R)∣ψn(R)⟩=H^(R)∣Ψn(t)⟩=En(R)∣ψn(R)⟩
The general full solution ∣Ψn⟩ has the following form,
where we allow R to evolve in time,
and we have abbreviated the traditional phase of the “wiggle factor” as Ln:
∣Ψn(t)⟩=exp(iγn(t))exp(−iLn(t)/ℏ)∣ψn(R(t))⟩Ln(t)≡∫0tEn(R(t′))dt′
The geometric phase γn(t) is more interesting.
It is not included in ∣ψn⟩,
because it depends on the path R(t)
rather than only the present R and t.
Its dynamics can be found by inserting the above ∣Ψn⟩
into the time-dependent Schrödinger equation:
dtd∣Ψn⟩=idtdγn∣Ψn⟩−ℏidtdLn∣Ψn⟩+exp(iγn)exp(−iLn/ℏ)dtd∣ψn⟩=idtdγn∣Ψn⟩+iℏ1En∣Ψn⟩+exp(iγn)exp(−iLn/ℏ)∣∇Rψn⟩⋅dtdR=idtdγn∣Ψn⟩+iℏ1H^∣Ψn⟩+exp(iγn)exp(−iLn/ℏ)∣∇Rψn⟩⋅dtdR
Here we recognize the Schrödinger equation, so those terms cancel.
We are then left with:
−idtdγn∣Ψn⟩=exp(iγn)exp(−iLn/ℏ)∣∇Rψn⟩⋅dtdR
Front-multiplying by i⟨Ψn∣ gives us
the equation of motion of the geometric phase γn:
dtdγn=−An(R)⋅dtdR
Where we have defined the so-called Berry connection An as follows:
An(R)≡−i⟨ψn(R)∣∇Rψn(R)⟩
Importantly, note that An is real,
provided that ∣ψn⟩ is always normalized for all R.
To prove this, we start from the fact that ∇R1=0:
0=∇R⟨ψn∣ψn⟩=⟨∇Rψn∣ψn⟩+⟨ψn∣∇Rψn⟩=⟨ψn∣∇Rψn⟩∗+⟨ψn∣∇Rψn⟩=2Re{−iAn}=2Im{An}
Consequently, An=Im⟨ψn∣∇Rψn⟩ is always real,
because ⟨ψn∣∇Rψn⟩ is imaginary.
Suppose now that the parameter R(t) is changed adiabatically
(i.e. so slow that the system stays in the same eigenstate)
for t∈[0,T], along a circuit C with R(0)=R(T).
Integrating the phase γn(t) over this contour C then yields
the Berry phase γn(C):
γn(C)=−∮CAn(R)⋅dR
But we have a problem: An is not unique!
Due to the Schrödinger equation’s gauge invariance,
any function f(R(t)) can be added to γn(t)
without making an immediate physical difference to the state.
Consider the following general gauge transformation:
∣ψ~n(R)⟩≡exp(if(R))∣ψn(R)⟩
To find An for a particular choice of f,
we need to evaluate the inner product
⟨ψ~n∣∇Rψ~n⟩:
⟨ψ~n∣∇Rψ~n⟩=exp(if)(i∇Rf⟨ψ~n∣ψn⟩+⟨ψ~n∣∇Rψn⟩)=i∇Rf⟨ψn∣ψn⟩+⟨ψn∣∇Rψn⟩=i∇Rf+⟨ψn∣∇Rψn⟩
Unfortunately, f does not vanish as we would have liked,
so An depends on our choice of f.
However, the curl of a gradient is always zero,
so although An is not unique,
its curl ∇R×An is guaranteed to be.
Conveniently, we can introduce a curl in the definition of γn(C)
by applying Stokes’ theorem, under the assumption
that An has no singularities in the area enclosed by C
(fortunately, An can always be chosen to satisfy this):
γn(C)=−∬S(C)Bn(R)⋅dS
Where we defined Bn as the curl of An.
Now γn(C) is guaranteed to be unique.
Note that Bn is analogous to a magnetic field,
and An to a magnetic vector potential:
Bn(R)≡∇R×An(R)=Im{∇R×⟨ψn(R)∣∇Rψn(R)⟩}
Unfortunately, ∇Rψn is difficult to evaluate explicitly,
so we would like to rewrite Bn such that it does not enter.
We do this as follows, inserting 1=∑m∣ψm⟩⟨ψm∣ along the way:
iBn=∇R×⟨ψn∣∇Rψn⟩=⟨ψn∣∇R×∇Rψn⟩+⟨∇Rψn∣×∣∇Rψn⟩=m∑⟨∇Rψn∣ψm⟩×⟨ψm∣∇Rψn⟩
The fact that ⟨ψn∣∇Rψn⟩ is imaginary
means it is parallel to its complex conjugate,
and thus the cross product vanishes, so we exclude n from the sum:
Bn=m=n∑⟨∇Rψn∣ψm⟩×⟨ψm∣∇Rψn⟩
From the Hellmann-Feynman theorem,
we know that the inner products can be rewritten:
⟨ψm∣∇Rψn⟩=En−Em⟨ψn∣∇RH^∣ψm⟩
Where we have assumed that there is no degeneracy.
This leads to the following result:
Bn=Imm=n∑(En−Em)2⟨ψn∣∇RH^∣ψm⟩×⟨ψm∣∇RH^∣ψn⟩
Which only involves ∇RH^,
and is therefore easier to evaluate than any ∣∇Rψn⟩.
References
- M.V. Berry,
Quantal phase factors accompanying adiabatic changes,
1984, Royal Society.
- G. Grosso, G.P. Parravicini,
Solid state physics,
2nd edition, Elsevier.