# Berry's geometric phase: a review Any ''vector'' object which is parallel-trasported along a path back to the original place, may acquire an angle with respect to its initial direction prior to transport. This angle is a geometric property. Here, I illustrate (at a fairly elementary level) the basics and a few selected consequences of this almost ubiquitous phenomenon.  ## An example in elementary geometry An intuitive classic example of parallel transport [see B. Goss Levi, Phys. Today 46, 17 (1993)] is the displacement of a vector along a loop drawn on a sphere (you may think of a compass needle carried in a ship or car traveling on the surface of the planet). In the figure at the right, both vectors stay tangential to the curved surface at all times. They start from the red point above (the "north pole"), and get transported along the path, remaining as parallel as possible to the direction they were pointing at before each infinitesimal displacement (the long vector points "South" and the short one points "East" all the time). After completing the closed path, or loop, the vectors go back to the original point, but they find themselves rotated with respect to the directions they were pointing at when the journey started. Note that the vectors "rotate" despite the fact we have been careful to keep them parallel during transport. Had the path been "smaller", i.e. including a smaller part of the spherical surface, the rotation angle would have been smaller. In our example, where the loop surrounds one eighth of the sphere, the rotation angle amounts to 90o. A larger path surrounding for example one quarter of the sphere, would rotate the parallel-transported vectors by 180o. An even larger loop, a diameter, surrounding (on both sides) half the sphere gives a rotation angle of 360o, i.e. no rotation at all.

The reason for this rotation is purely geometrical-topological. In fact, it is connected to the intrinsic curvature of the sphere. No such phenomenon would appear if vectors are parallel-transported along a flat manifold, such as a plane or a cylinder. The rotation angle is in fact related to the integral of the curvature on the surface bounded by the loop.

Such rotation angles of geometrical origin are known as Berry phases. "Phase" is used meaning just "angle" for whatever possible argument of sin(·) or cos(·) or exp(i ·). Several specific cases had been recognized for many years, in particular the well-studied Aharonov-Bohm effect and Pancharatnam's work on the geometric phases in optics. M. Berry published in 1984 a very influential formal systematization of the closed-path geometric phase in quantum mechanical problems, some of which is summarized in the following paragraphs.

## Berry phase in undulatory phenomena

Indeed, Berry phases do not appear only in everyday experience of geometrical vectors. The ingredients of a parameterized vector field are present also in undulatory phenomena. A basic concept in math is that of sets of functions structured as vector spaces. Such functions often describe wave phenomena, such as the vibrations of a drum membrane. Each wave has a phase connected to its time evolution (the going up and down of each point of the membrane). This dynamical phase is not geometrical: it depends on the speed at which the parameterized path is followed, and on the arbitrary choice of a "zero phase" (technically called a gauge choice) at each point along the path. A recipe is needed to get rid of any dynamical phases, and single out the intrinsic, geometrical invariant phases. Berry' s work [M.V. Berry, Proc. R. Soc. Lond. A 392, 45 (1984)], contains a precise formulation of this concept, that is a realization of parallel transport for generic complex vectors.

States in quantum mechanics are represented by vectors in a linear (complex) space. In many cases they can be visualized as wave functions. There is no reason that they should make exceptions to the general rule of acquiring phase angles after parallel transport along loops.

A standard, though slightly simplified, formulation goes as follows: consider the set of eigenstates of a (self-adjoint) Hamiltonian operator H, depending on several classical ''external'' parameters (which again we indicate collectively as q). Changing q from one point to another in its multi-dimensional space, the set of stationary states and the related eigenenergies of H change in a completely generic way, leading to totally new and unrelated eigensystem. Assuming however smooth dependence of H on the external parameters q, one expects that for infinitesimal change in the parameters, also the states change by small amounts. The notion of parallel transport may be implemented by imposing that the inner product between a given eigenstate at some point q, and the evolved eigenstate at a following neighboring point qq, be as close to 1 as possible (leading changes of order Δq2).

Note that each stationary state "rotates" (in the complex sense) as exp(-i Ek t/ ℏ) [where Ek is the energy of the state, t is time and ℏ is Planck's constant], because of its Schroedinger time evolution. On top of this, since at each point the eigensystem is unrelated to that at a different point, nothing forbids to multiply each eigenstate by an additional arbitrary phase factor exp[-iΦk(q)] (a "gauge choice")! The correct rule for the "parallel transport", as sketched above, permits to calculate the geometrical phase, such that it ignores completely any dynamical and gauge phase. The result depends only on the geometry of the loop. In this sense, Berry's phase is said to be "gauge-invariant".

Two classic examples of Berry phase in quantum mechanics (known long before Berry's systematization) are:

• The rotation of a spinor. If a, say, s=½ angular moment is aligned to a magnetic field, and the field is made to rotate adiabatically, so that the spinor remains aligned to it, at the end of the loop the spinor acquires a complex phase factor exp(i Φ). For the general mz component of a spin-s spinor, Berry's phase factor amount precisely to exp(i × mz × the solid angle enclosed in the circuit followed by the magnetic field). Thus, in the special case of a mz=-½ component, the field rotating within a plane (thus enclosing one half of the complete solid angle 4π), the value of Φ is -½×(4π/2)=-π. This amounts to a sign change of the spinor (-1)=exp(-i π), i.e. to a "180°" rotation in the Hilbert space of states. Note however that in the real 3D space, spin has actually rotated by 360°, as expected. Likewise, as ordinary vectors are basically s=1 spinors, the parallel transport of ordinary vectors on a sphere should also give interesting geometric phases. Indeed the Berry phase for a transport along a sphere diameter yields a Berry phase of 2π, i.e. a full rotation, equivalent to no rotation at all [exp(i 4π/2)=exp(i 2π)=1]. Instead, a smaller the path enclosing one eight of the sphere yields the geometric phase of 4π/8=π/2=90° illustrated above. [Technically, the factor of 2 distingushing integer and half integer s-spinors is related to the 1:1 and 2:1 representations of the 3-dimensional rotation group, and equivalently to the 2:1 relation of SU(2) to SO(3)...].
• The Aharonov-Bohm experiment: a geometric phase acquired by electrons due to differences in local values of the magnetic vector potential.

As you must have guessed, however, in most cases the Berry phase vanishes. As one might expect, usually coming back after a loop to the starting point, makes nothing important, and the vector quantities go back to exactly what they used to be before the loop, indicating that the space where those vectors are moved around is flat. So, nonzero phases are clues pointing to nontrivial topological properties underlying the relation between the vector quantities and the adiabatic parameters q.

In physical applications, one often encounters Hamiltonian operators depending on several external parameters, thus potentially affected by Berry phases. Two general kinds of such q-dependences can be distinguished:

• q indicates genuine external classical parameters, typically external fields, which the experimentalist, at least in principle, can tune. The Berry phase is observed by following a nontrivial loop in the parameters space, and performing some kind of interference between the state prior and after the loop. Standard examples are the parallel transport of a vector on a sphere, the Aharonov-Bohm effect, and analogous neutron interference experiments;
• q indicates some internal degrees of freedom of a system are approximately treated as "slow", classical variables, affecting adiabatically the "fast" quantum dynamics of the other degrees of freedom described by H. Of course, eventually the true quantum nature of the slow variables must be taken into account, as a further crucial step. The standard example for this is the Born-Oppenheimer separation of the "fast" quantum motion of electrons from the "slow" motion of nuclei in molecules and crystals: the nuclear coordinates appear as external parameters defining the potential in which the electrons move. In turn, the electronic ground state energy enters in the potential energy for the adiabatic motion of the nuclei. When the latter is quantized, it gives rise to the vibrational/phononic states observed by spectroscopy.
Here we shall be mostly concerned with the latter case.

## Berry phase for real Hamiltonians

A physically relevant and rather simple case is that of the eigensystem of a real Hamiltonian operator H depending on a set of external parameters q. The eigenstates of a real operator may always be chosen to be real, at any q-point. It is straightforward to check that continuous real eigenstates realize parallel transport. In the real case, is is therefore easy to get rid of complex phases such as exp(-i Ek t/ ℏ), coming from the time evolution.

This granted, it's clear that Berry's recipe for the phase at the end of any loop can only yield 0 or π, since any (nondegenerate) wave function must come back either to itself or to minus itself.

As usual, in 99% of the cases, the Berry phase turns out to be zero. However, it was clear right at the beginning that when some point of degeneracy is enclosed in the loop, the phase can be nonzero. By "point of degeneracy" we mean a q-point where the energy of the state under consideration becomes exactly the same as that of the state immediately above or below it. By "enclosed" we mean that the loop cannot be smoothly deformed to avoid surrounding the degenerate point. For example, in a 2-dimensional space of q-parameters, a circle centered in the origin does enclose the origin (as well as any other internal point...). To unpin it from that point, there is no solution but cutting the circle (obviously not a smooth thing to do to a circle). Instead, if a third axis is added to the q-space, the circle could be raised a little into the third dimension, thus getting free from the degenerate point (it may afterwards be displaced away from the origin as indicated in the figure. A whole line of degenerate points (such as the vertical axis) would be needed for the circle not to be contractable. In general, for to a D-dimensional manifold of q-points, the sub-manifold of singular points needs to be at least (D-2)-dimensional, to pin some loops. Loops in q-space can be divided into classes according to the possibility of either being smoothly contracted to one point, avoiding the degenerate points, or being intrinsically entangled in them.

Nontrivial Berry phases of π can therefore appear only when the q-space with the degenerate q-points removed is multiply connected (an exquisitely geometric-topologic concept).

In conclusion, in the case of real Hamiltonians, the Berry phase along some path equals the number of level degenerate points that this path encloses times π.

## Berry phase in Dynamic Jahn-Teller

Needles to say, in the Born-Oppenheimer separation of electronic and vibrational motion, the Berry phase is usually zero on any physically relevant path, since the electronic ground state is usually well separated from the first electronic excitation. The notable exception is the so-called Jahn-Teller (JT) effect. Here, the ground state is degenerate at some specially symmetric q-point. A distortion of the molecule/crystal reducing the symmetry corresponds to a displacement in q-space from that special point. This deformation can be energetically convenient: in this way the molecule/crystal undergoes a so-called JT distortion.

To fix the ideas, we consider here in some detail the instructive example of the triangular molecule (E × e JT model). The equilibrium geometry of a triangular cluster such as Xi3 is not the equilateral triangle, but a distorted isosceles geometry. Indeed in the equilateral configuration, the electronic ground state is twofold degenerate (E). These 2 electronic states split for any displacement away from the equilateral geometry. Due to symmetry, it is clear that equivalent isosceles distortions where any two Li atoms get closer are energetically equivalent.  Actually, it may be verified that (for linear coupling) the equilibrium configurations constitute a flat circular valley - or trough - when the Born-Oppenheimer potential energy is plotted against the q coordinates. Note the degeneracy of the two Born-Oppenheimer potential energy sheets at the central q=0 high-symmetry point in the figure. So, this "JT valley" encircles a degeneracy point for the electronic (real) Hamiltonian: a Berry phase should therefore be present and, moreover, physically relevant, since this loop is frequently accessed by the low-energy dynamics of the q-distortions.

We can convince ourselves that the electronic wave function indeed undergoes a Berry phase change of π while the distortions loop around the trough, by a little meditation on the changes in the electronic wave function during a loop in the distortions space illustrated in the figure above. The real adiabatic choice of the electronic state is indicated, in terms of the three atomic s orbitals of the three Li atoms. Notice that we choose carefully the phase at each point in order to simulate "parallel transport", i.e. to have positive overlap to the immediately preceding configuration. A 2π loop along the JT valley is completed going from one configuration to that pictured at the opposite side: the electronic state changes sign. Another 2π loop is needed to restore the original sign.

### Consequences of the Berry phase

In this representation of the electrons, the "pseudorotational" motion of the q-distortion, is just a free particle on a circle. Until the q-coordinates are treated as classical variables, no special effects are to be expected of the sign change in the electronic wave function, since geometric phase changes could be observed only by quantum interference. Even if the distortion might happen to follow the low-energy loop, the dynamics of the classical nuclei could not care less of the Berry phase acquired by the electrons. However, as soon as we recall the quantum nature of the q degrees of freedom (quantization of the phonons), their wave function gives a coherent amplitude of probability of being anywhere along the JT valley. This introduces interference of the electronic state before and after a nontrivial loop: for this reason the Berry phase acts as a boundary condition for the quantization along the JT valley.

In our example for the triangular molecule, the minus sign acquired by the electronic wave function after one loop needs to be compensated by another minus sign of the vibrational counterpart, since the overall (vibronic) molecular state needs to be represented by genuine single-valued wave function. The low-energy pseudo-rotational motion (described by a free-particle wave function of type exp(-i k Φ), where Φ is the angle parameterizing the trough) along the JT valley is dramatically affected by this Berry-phase-induced anti-periodic boundary condition: the quantization rule selects half odd integer pseudorotational "momenta" k, rejecting ordinary integer ones. Substantial consequences follow for the vibronic spectral properties, both in energetics (the JT energy gain is reduced, due to the larger amplitude of ''zero-point'' motion of the lowest k=±½ rotor state, instead of k=0 as would be without Berry phase), and in symmetry (the ground state would be singly degenerate without a Berry phase).

The role of the geometrical phase in determining the symmetry of the vibronic ground state is not restricted to the E × e model presented here, being instead very general in this kind of coupled electron-distortion systems.

### Conclusions

A general consideration is due, at the end of this section. We must never forget the two logical steps we took introducing the Berry phase concept in JT systems. First, with the BO adiabatic approximation, we introduce a separation between ''fast'' and ''slow'' degrees of freedom, and a corresponding factorization of the vibronic wave function. Then, we treat the vibron degrees of freedom as classical variables, since the Berry phase needs a classical context for its description.

These two conceptual steps are actually approximations (the classical description of the vibrons is quickly released, as soon as the phases on the loops have been computed). They could in principle be avoided from the beginning, by diagonalizing the full e-v quantum Hamiltonian. In this sense, the Berry phase is an unnecessary semiclassical concept. However, as long as a Born-Oppenheimer factorization is considered useful, the Berry-phase concept is also a very useful framework for understanding, classifying and computing spectral properties of DJT systems. There are relevant examples of JT systems showing changes in ground state symmetry, that would be unexplained if the Berry-phase analysis were ignored.

## Generalizations

Many generalizations have been proposed to the original definition. In particular, it was soon realized that there is no reason for the evolution to be adiabatic, i.e. slow: the phases turn out the same even if the external parameters move fast.

Also, why restricting to a loop at all? Indeed it is possible to define and measure Berry phases also for arbitrary open paths, provided that the evolved state at the end of the path is not orthogonal to the initial one.

Furthermore, does the path really need to be continuous? People like to compute quantities numerically, so there must be some discrete version of Berry's integral. Indeed there is a very natural one (in terms of Bargmann invariants), and it turns out so simple and pretty that it may be conveniently taken as an alternative fundamental definition of Berry's phase.

Also, why considering one single state? n degenerate states may evolve together, acquiring not just a phase factor [an element of the group U(1)], but a whole matrix [an element of the group U(n)]: this leads to the non-abelian phases of F. Wilczek and A. Zee, Phys. Rev. Lett. 52, 2111 (1984).

Finally, in-house research in Grenoble/Trieste/Milano lead us to one extra exciting generalization: off-diagonal geometrical phases.

Some of these generalization come out naturally if one considers the vectors as objects evolving in the ray space... but this is a rather complicate story: I suggest reading the cited articles by Aharonov, Simon, and Resta.

Taking a look to the following references may provide further insight in the fascinating concept of Berry's geometrical phase and its applications, with focus on ground-state symmetry in dynamical JT.

1. M. Berry's original paper is on: Proc. R. Soc. Lond. A 392, 45 (1984)
2. Manini and De Los Rios, J. Phys.: Condens. Matter 38, 8485 (1998)
3. De Los Rios and Manini, Fullerenes. Recent Advances ... - vol. 5, ed. by K.M. Kadish and R.S. Ruoff (The Electrochemical Society, Pennington, NJ, 1997), pag. 468
4. Auerbach, Manini, and Tosatti, Phys. Rev. B 49, 12998 (1994)
5. Manini's PhD thesis
6. The abstract of and old talk on the Berry phase in the fullerides
7. F.S. Ham, Phys. Rev. Lett. 58, 725
8. Aharonov and Anandan, Phys. Rev. Lett. 58, 1593
9. Simon and Mukunda, Phys. Rev. Lett. 70, 880
10. Lauber, Weidenhammer, and Dubbers, Phys. Rev. Lett. 72, 1004
11. Koizumi, Hotta, and Takada, Phys. Rev. Lett. 80, 4518
12. Manolopoulos and Child, Phys. Rev. Lett. 82, 2223
13. Hannay, PEL - J. Phys. A: Math. Gen 31, L53
14. Wikipedia, Geometric phase
15. Geometric phases in a nice deformed-resonator experiment: F. Pistolesi and N. Manini, Phys. Rev. Lett. 85, 1585 (2000).
16. The off-diagonal generalization: N. Manini and F. Pistolesi, Phys. Rev. Lett. 85, 3067 (2000); Y. Hasegawa, et al., Phys. Rev. A 65, 052111 (2002).
17. R. Resta's first review (1993)
18. R. Resta, Rev. Mod. Phys. 66, 899 (1994)
19. G. Kresse, Berry's phase and modern polarization theory
20. Geometric Phases In Physics, edited by A. Shapere and F. Wilczek (World Scientific, Singapore, 1989)
21. Very complete and formal: D. J. Thouless, Topological Quantum Numbers in Nonrelativistic Physics (World Scientific, Singapore, 1998)
22. On nonstationary states: J. Phys. A: Math. Gen. 29, 2567 (1996) created: 2 Aug 1999
moved to Milano: 05 Jul 2001