Topological defect

Source: Wikipedia, the free encyclopedia.

In

cohomology class than the base physical system. More simply: it is not possible to continuously transform
the system with a soliton in it, to one without it. The mathematics behind topological stability is both deep and broad, and a vast variety of systems possessing topological stability have been described. This makes categorization somewhat difficult.

Overview

The original

Korteweg-De Vries (KdV) equation, describing waves in water, has homotopically distinct solutions. The mechanism of Lax pairs
provided the needed topological understanding.

The general characteristic needed for a topological soliton to arise is that there should be some

compact topological space. As a result, the mapping from space(time) to the variables in the PDE is describable as a mapping from a sphere to a (different) sphere; the classes of such mappings are given by the homotopy groups of spheres
.

To restate more plainly: solitons are found when one solution of the PDE cannot be continuously transformed into another; to get from one to the other would require "cutting" (as with scissors), but "cutting" is not a defined operation for solving PDE's. The cutting analogy arises because some solitons are described as mappings , where is the circle; the mappings arise in the circle bundle. Such maps can be thought of as winding a string around a stick: the string cannot be removed without cutting it. The most common extension of this winding analogy is to maps , where the first

three-sphere
stands for compactified 3D space, while the second stands for a
three-vector, its direction plus length, can be thought of as specifying a point on a 3-sphere. The orientation of the vector specifies a subgroup of the orthogonal group
; the length fixes a point. This has a double covering by the unitary group , and .) Such maps occur in PDE's describing vector fields.

A topological defect is perhaps the simplest way of understanding the general idea: it is a soliton that occurs in a

germanium whiskers.) The mathematical stability comes from the non-zero winding number
of the map of circles the stability of the dislocation leads to
critical density
, allowing them to interact with one-another and "connect up", and thus disconnect (fracture) the whole. The idea that critical densities of solitons can lead to phase transitions is a recurring theme.

superfluids and pinned vortex tubes in type-II superconductors provide examples of circle-map type topological solitons in fluids. More abstract examples include cosmic strings; these include both vortex-like solutions to the Einstein field equations, and vortex-like solutions in more complex systems, coupling to matter and wave fields. Tornados and vorticies in air are not examples of solitons: there is no obstruction to their decay; they will dissipate after a time. The mathematical solution describing a tornado can be continuously transformed, by weakening the rotation, until there is no rotation left. The details, however, are context-dependent: the Great Red Spot of Jupiter
is a cyclone, for which soliton-type ideas have been offered up to explain its multi-century stability.

Topological defects were studied as early as the 1940's. More abstract examples arose in quantum field theory. The Skyrmion was proposed in the 1960's as a model of the nucleon (neutron or proton) and owed its stability to the mapping . In the 1980's, the

Kerr solution to the Einstein field equations (black holes) can be recognized as examples of topological gravitational solitons: this is the Belinski–Zakharov transform
.

The terminology of a topological defect vs. a topological soliton, or even just a plain "soliton", varies according to the field of academic study. Thus, the hypothesized but unobserved

topological charge. The word charge is used in the sense of charge in physics
.

The mathematical formalism can be quite complicated. General settings for the PDE's include fiber bundles, and the behavior of the objects themselves are often described in terms of the holonomy and the monodromy. In abstract settings such as string theory, solitons are part and parcel of the game: strings can be arranged into knots, as in knot theory, and so are stable against being untied.

In general, a (quantum) field configuration with a soliton in it will have a higher energy than the

Postnikov tower
. These are theoretical hypotheses; demonstrating such concepts in actual lab experiments is a different matter entirely.

Formal treatment

The existence of a topological defect can be demonstrated whenever the

homotopy class. Topological defects are not only stable against small perturbations
, but cannot decay or be undone or be de-tangled, precisely because there is no continuous transformation that will map them (homotopically) to a uniform or "trivial" solution.

An ordered medium is defined as a region of space described by a function f(r) that assigns to every point in the region an

order parameter, and the possible values of the order parameter space constitute an order parameter space. The homotopy theory of defects uses the fundamental group of the order parameter space of a medium to discuss the existence, stability and classifications of topological defects in that medium.[2]

Suppose R is the order parameter space for a medium, and let G be a Lie group of transformations on R. Let H be the symmetry subgroup of G for the medium. Then, the order parameter space can be written as the Lie group quotient[3] R = G/H.

If G is a

universal cover for G/H then, it can be shown[3] that πn(G/H) = πn−1(H), where πi denotes the i-th homotopy group
.

Various types of defects in the medium can be characterized by elements of various homotopy groups of the order parameter space. For example, (in three dimensions), line defects correspond to elements of π1(R), point defects correspond to elements of π2(R), textures correspond to elements of π3(R). However, defects which belong to the same conjugacy class of π1(R) can be deformed continuously to each other,[2] and hence, distinct defects correspond to distinct conjugacy classes.

Poénaru and Toulouse showed that[4] crossing defects get entangled if and only if they are members of separate conjugacy classes of π1(R).

Examples

Topological defects occur in

condensed matter
physics.

The authenticity[

true vacuum, respectively.[clarification needed
]

Solitary wave PDEs

Examples include the

exactly solvable models
, such as

Lambda transitions

Topological defects in lambda transition universality class[clarification needed] systems including:

  • Screw/edge-dislocations in
    liquid crystals
    ,
  • Magnetic flux "tubes" known as
    superconductors
    , and
  • Vortices in
    superfluids
    .

Cosmological defects

According to some models explored in the 1970s and 1980s, as the very early universe cools from an initial hot, dense state it triggered a series of

grand unified theories of the early universe. Detailed measurements of the cosmic microwave background by the Wilkinson Microwave Anisotropy Probe provide strong evidence in favor of cosmic inflation for some predictions claimed by topological defect models. Models which combine these concepts remain viable.[5]
: 231 

Symmetry breaking

Depending on the nature of

Kibble-Zurek mechanism
. The well-known topological defects are:

  • Cosmic strings are one-dimensional lines that form when an axial or cylindrical symmetry is broken.
  • Domain walls, two-dimensional membranes that form when a discrete symmetry is broken at a phase transition. These walls resemble the walls of a closed-cell foam, dividing the universe into discrete cells.
  • Monopoles, cube-like defects that form when a spherical symmetry is broken, are predicted to have magnetic charge,[why?] either north or south (and so are commonly called "magnetic monopoles").
  • which?] are completely broken. They are not as localized as the other defects, and are unstable.[clarification needed
    ]
  • Skyrmions
  • dimensions
    .

Other more complex hybrids of these defect types are also possible.

As the universe expanded and cooled, symmetries in the laws of physics began breaking down in regions that spread at the

disordered phase
is completed for the surrounding regions.

Observation

Topological defects have not been identified by astronomers; however, certain types are not compatible with current observations. In particular, if domain walls and monopoles were present in the observable universe, they would result in significant deviations from what astronomers can see.

Because of these observations, the formation of defects within the observable universe is highly constrained, requiring special circumstances (see

cold spot in the cosmic microwave background provided evidence of a possible texture.[6]

Classes of stable defects in biaxial nematics

Condensed matter

In condensed matter physics, the theory of

superfluid helium-3.[2]

Stable defects

Homotopy theory is deeply related to the stability of topological defects. In the case of line defect, if the closed path can be continuously deformed into one point, the defect is not stable, and otherwise, it is stable.

Unlike in cosmology and field theory, topological defects in condensed matter have been experimentally observed.[7] Ferromagnetic materials have regions of magnetic alignment separated by domain walls. Nematic and bi-axial nematic liquid crystals display a variety of defects including monopoles, strings, textures etc.[2] In crystalline solids, the most common topological defects are dislocations, which play an important role in the prediction of the mechanical properties of crystals, especially crystal plasticity.

Topological defects in magnetic systems

In magnetic systems, topological defects include 2D defects such as skyrmions (with integer skyrmion charge), or 3D defects such as Hopfions (with integer Hopf index). The definition can be extended to include dislocations of the helimagnetic order, such as edge dislocations [8][9] and screw dislocations [10] (that have an integer value of the Burgers vector)

Images

A static solution to in (1 + 1)-dimensional spacetime.
A soliton and an antisoliton colliding with velocities ±sinh(0.05) and annihilating.


See also

References

  1. ^ F. A. Bais, Topological excitations in gauge theories; An introduction from the physical point of view. Springer Lecture Notes in Mathematics, vol. 926 (1982)
  2. ^ .
  3. ^ .
  4. .
  5. .
  6. .
  7. ^ "Topological defects". Cambridge cosmology.
  8. ISSN 1745-2481
    .
  9. .
  10. .