Misplaced Pages

Revision as of 14:48, 3 March 2008

In physics, Chern-Simons theory is a 3-dimensional topological quantum field theory of Schwarz type. In condensed matter physics, Chern-Simons theory describes the topological order in fractional quantum Hall states. It was popularized by Edward Witten in 1989, when he demonstrated that it may be used to calculate knot invariants and three-manifold invariants such as the Jones polynomial, as had been conjectured two years earlier by Albert Schwarz. It is so named because its action is proportional to the integral of the Chern-Simons 3-form.

A particular Chern-Simons theory is specified by a choice of Lie group G known as the gauge group of the theory and also a number referred to as the level of the theory, which is a constant that multiplies the action. The action is gauge dependent, however the partition function of the quantum theory is well-defined when the level is an integer and the gauge field strength vanishes on all boundaries of the 3-dimensional spacetime.

The classical theory

Configurations

Chern-Simons theories can be defined on any topological 3-manifold M, with or without boundary. As these theories are Schwarz-type topological theories, no metric needs to be introduced on M.

Chern-Simons theory is a gauge theory, which means that a classical configuration in the Chern-Simons theory on M with gauge group G is described by a principal G-bundle on M. The connection of this bundle is characterized by a connection one-form A which is valued in the Lie algebra g of the Lie group G. In general the connection A is only defined on individual coordinate patches, and the values of A on different patches are related by maps known as gauge transformations. These are characterized by the assertion that the covariant derivative, which is the sum of the exterior derivative operator d and the connection A, transforms in the adjoint representation of the gauge group G. The square of the covariant derivative with itself can be interpreted as a g-valued 2-form F called the curvature form or field strength. It also transforms in the adjoint representation.

Dynamics

The action S of Chern-Simons theory is proportional to the integral of the Chern-Simons 3-form

${\displaystyle S={\frac {k}{4\pi }}\int _{M}{\text{tr}}\,(A\wedge dA+{\tfrac {2}{3}}A\wedge A\wedge A).}$

The constant k is called the level of the theory. The classical physics of Chern-Simons theory is independent of the choice of level k.

Classically the system is characterized by its equations of motion which are the extrema of the action with respect to variations of the field A. In terms of the field curvature

${\displaystyle F=dA+A\wedge A}$

the field equation is explicitly

${\displaystyle 0={\frac {\delta S}{\delta A}}={\frac {k}{2\pi }}F}$.

The classical equations of motion are therefore satisfied if and only if the curvature vanishes everywhere, in which case the connection is said to be flat. Thus the classical solutions to G Chern-Simons theory are the flat connections of principal G-bundles on M. Flat connections are determined entirely by holonomies around noncontractible cycles on the base M. More precisely, they are in one to one correspondence with equivalence classes of homomorphisms from the fundamental group of M to the gauge group G up to conjugation.

If M has a boundary N then there is additional data which describes a choice of trivialization of the principal Gbundle on N. Such a choice characterizes a map from N to G. The dynamics of this map is described by the Wess-Zumino-Witten (WZW) model on N at level k.

Quantization

To canonically quantize Chern-Simons theory one defines a state on each 2-dimensional surface Σ in M. As in any quantum field theory, the states correspond to rays in a Hilbert space. There is no preferred notion of time in a Schwarz-type topological field theory and so one cannot impose that Σ be Cauchy surfaces, in fact a state can be defined on any surface.

Σ is codimension one, and so one may cut M along Σ. After such a cutting M will be a manifold with boundary and in particular classically the dynamics of Σ will be described by a WZW model. Witten has shown that this correspondence holds even quantum mechanically. More precisely, he demonstrated that the Hilbert space of states is always finite dimensional and can be canonically identified with the space of conformal blocks of the G WZW model at level k. Conformal blocks are locally holomorphic and antiholomorphic factors whose products sum to the correlation functions of a 2-dimensional conformal field theory.

For example, when Σ is a 2-sphere, this Hilbert space is one-dimensional and so there is only one state. When Σ is a 2-torus the states correspond to the integrable representations of the affine Lie algebra corresponding to g at level k. Characterizations of the conformal blocks at higher genera are not necessary for Witten's solution of Chern-Simons theory.

Observables

Wilson loops

The observables of Chern-Simons theory are the n-point correlation functions of gauge-invariant operators. The most often studied class of gauge invariant operators are Wilson loops. A Wilson loop is the holonomy around a loop in M, traced in a given representation R of G. As we will be interested in products of Wilson loops, without loss of generality we may restrict our attention to irreducible representions R.

More concretely, given an irreducible representation R and a loop K in M one may define the Wilson loop ${\displaystyle W_{R}(K)}$ by

${\displaystyle \langle W_{R}(K)\rangle ={\text{Tr}}_{R}\,{\mathcal {P}}\,\exp {i\oint _{K}A}}$

where A is the connection 1-form and we take the Cauchy principal value of the contour integral and ${\displaystyle {\mathcal {P}}\,\exp }$ is the path-ordered exponential.

HOMFLY and Jones polynomials

Consider a link L in M, which is a collection of l disjoint loops. A particularly interesting observable is the l-point correlation function formed from the product of the Wilson loops around each disjoint loop, each traced in the fundamental representation of G. One may form a normalized correlation function by dividing this observable by the partition function Z(M), which is just the 0-point correlation function.

In the special case in which M is the 3-sphere, Witten has shown that these normalized correlation functions are proportional to known knot polynomials. For example, in G=U(N) Chern-Simons theory at level k the normalized correlation function is, up to a phase, equal to

${\displaystyle {\frac {\sin(\pi /(k+N))}{\sin(\pi N/(k+N))}}}$

times the HOMFLY polynomial. In particular when N=2 the HOMFLY polynomial reduces to the Jones polynomial. In the SO(N) case one finds a similar expression with the Kauffman polynomial.

The phase ambiguity reflects the fact that, as Witten has shown, the quantum correlation functions are not fully defined by the classical data. The linking number of a loop with itself enters into the calculation of the partition function, but this number is not invariant under small deformations and in particular is not a topological invariant. This number can be rendered well defined if one chooses a framing for each loop, which is a choice of preferred nonzero normal vector at each point along which one deforms the loop to calculate its self-linking number. This procedure is an example of the point-splitting regularization procedure introduced by Paul Dirac and Rudolf Peierls to define apparently divergent quantities in quantum field theory in 1934.

Sir Michael Atiyah has shown that there exists a canonical choice of framing, which is generally used in the literature today and leads to a well-defined linking number. With the canonical framing the above phase is the exponential of 2πi/(k+N) times the linking number of L with itself.

Relationships with other theories

Topological string theories

In the context of string theory, a U(N) Chern-Simons theory on an oriented Lagrangian 3-submanifold M of a 6-manifold N arises as the string field theory of open strings ending on a D-brane wrapping M in the A-model topological string on N. The B-Model topological open string field theory on the spacefilling worldvolume of a stack of D5-branes is a 6-dimensional variant of Chern-Simons theory known as holomorphic Chern-Simons theory.

WZW and matrix models

Chern-Simons theories are related to many other field theories. For example, if one considers a Chern-Simons theory with gauge group G on a manifold with boundary then all of the 3-dimensional propagating degrees of freedom may be gauged away, leaving a 2-dimensional conformal field theory known as a G Wess-Zumino-Witten model on the boundary. In addition the U(N) and SO(N) Chern-Simons theories at large N is well approximated by matrix models.

Chern-Simons, the Kodama wavefunction and loop quantum gravity

Edward Witten argued that the Kodama state in loop quantum gravity is unphysical due to an analogy to Chern-Simons state resulting in negative helicity and energy. There are disagreements to Witten's conclusions.

Chern-Simons terms in other theories

The Chern-Simons term can also be added to models which aren't topological quantum field theories. In 3D, this gives rise to a massive photon if this term is added to the action of Maxwell's theory of electrodynamics. This term can be induced by integrating over a massive charged Dirac field. It also appears for example in the quantum Hall effect. Ten and eleven dimensional generalizations of Chern-Simons terms appear in the actions of all ten and eleven dimensional supergravity theories.

See also

• Chern-Simons form
• Topological quantum field theory
• Alexander polynomial

References

• S.-S. Chern and J. Simons, Characteristic forms and geometric invariants, Annals Math. 99, 48–69 (1974). (Subscription required for online access)
• Edward Witten, Quantum Field Theory and the Jones Polynomial, Commun.Math.Phys.121:351,1989.
• Edward Witten, Chern-Simons Theory as a String Theory, Prog.Math.133:637-678,1995.
• Marcos Marino, Chern-Simons Theory and Topological Strings, Rev.Mod.Phys.77:675-720,2005.
• Marcos Marino, Chern-Simons Theory, Matrix Models, And Topological Strings (International Series of Monographs on Physics), OUP, 2005.

v t e Quantum field theories
Theories	Algebraic QFT Axiomatic QFT Conformal field theory Lattice field theory Noncommutative QFT Gauge theory QFT in curved spacetime String theory Supergravity Thermal QFT Topological QFT Two-dimensional conformal field theory
Models	Regular Born–Infeld Euler–Heisenberg Ginzburg–Landau Non-linear sigma Proca Quantum electrodynamics Quantum chromodynamics Quartic interaction Scalar electrodynamics Scalar chromodynamics Soler Yang–Mills Yang–Mills–Higgs Yukawa Low dimensional 2D Yang–Mills Bullough–Dodd Gross–Neveu Schwinger Sine-Gordon Thirring Thirring–Wess Toda Conformal 2D free massless scalar Liouville Minimal Polyakov Wess–Zumino–Witten Supersymmetric 4D N = 1 N = 1 super Yang–Mills Seiberg–Witten Super QCD Wess–Zumino Superconformal 6D (2,0) ABJM N = 4 super Yang–Mills Supergravity Pure 4D N = 1 4D N = 1 4D N = 8 Higher dimensional Type I Type IIA Type IIB 11D Topological BF Chern–Simons Particle theory Chiral Fermi MSSM Nambu–Jona-Lasinio NMSSM Standard Model Stueckelberg
Related	Casimir effect Cosmic string History Loop quantum gravity Loop quantum cosmology On shell and off shell Quantum chaos Quantum dynamics Quantum foam Quantum fluctuations links Quantum gravity links Quantum hadrodynamics Quantum hydrodynamics Quantum information Quantum information science links Quantum logic Quantum thermodynamics
See also: Template:Quantum mechanics topics

• Quantum field theory