Wigner's theorem

E.P. Wigner (1902-1995), F.R.S., first proved the theorem bearing his name. It was a key step towards the modern classification scheme of particle types, according to which particle types are partly characterized by which representation of the Lorentz group under which it transforms. The Lorentz group is a symmetry group of every relativistic quantum field theory. Wigner early work laid the ground for what many physicists came to call the group theory disease^[1] in quantum mechanics – or as Hermann Weyl (co-responsible) puts it in his The Theory of Groups and Quantum Mechanics (preface to 2nd ed.), "It has been rumored that the group pest is gradually being cut out from quantum mechanics. This is certainly not true..."

Wigner's theorem, proved by Eugene Wigner in 1931,^[2] is a cornerstone of the mathematical formulation of quantum mechanics. The theorem specifies how physical symmetries such as rotations, translations, and CPT are represented on the Hilbert space of states.

According to the theorem, any symmetry transformation of ray space is represented by a linear and unitary or antilinear and antiunitary transformation of Hilbert space. The representation of a symmetry group on Hilbert space is either an ordinary representation or a projective representation.

Rays and ray space

It is a postulate of quantum mechanics that vectors in Hilbert space that are scalar nonzero multiples of each other represent the same pure state. A ray is a set^[3]^[4]

\underline{\Psi} = \{e^{i\alpha}\Psi|\alpha \in \mathbb{R}\}, \Psi \in \mathcal{H},

and a ray whose vectors have unit norm is called a unit ray. If $Φ \in Ψ$ , then $Φ$ is a representative of $Ψ$ . There is a one-to-one correspondence between physical pure states and unit rays.^{[nb 1]} The space of all rays is called ray space.

Formally,^[5] if $H$ is a complex Hilbert space, then let $B$ be the subset

B = \{\Psi \in \mathcal H: ||\Psi|| = 1\}

of vectors with unit norm. If $H$ is finite-dimensional with complex dimension $N$ , then $B$ has real dimension $2 N - 1$ . Define a relation ≅ on $B$ by

\Psi \cong \Phi \Leftrightarrow \Psi = e^{i\alpha}\Phi, \quad \alpha \in \mathbb R.

The relation ≅ is an equivalence relation on the set $B$ . Unit ray space, $S$ , is defined as the set of equivalence classes

S = B/\cong.

If $N$ is finite, $S$ has real dimension $2 N - 2$ hence complex dimension $N - 1$ . Equivalently, one may define ≈ on $H$ by

\Psi \approx \Phi \Leftrightarrow \Psi = z\Phi, \quad z \in \mathbb C \smallsetminus \{0\},

where $ℂ \ {0}$ is the set of nonzero complex numbers, and set

S = \mathcal H/\approx.

This makes it clear that unit ray space is a projective space. It is also possible to skip the normalization and take ray space as^[6]

R = \mathcal H/\cong,

where ≅ is now defined on all of $H$ by the same formula. The real dimension of $R$ is $2 N - 1$ if $N$ is finite. This approach is used in the sequel. The difference between $R$ and $S$ is rather trivial, and passage between the two is effected by multiplication of the rays by a nonzero real number, defined as the ray generated by any representative of the ray multiplied by the real number.

Ray space is sometimes awkward to work with. It is, for instance, not a vector space with well-defined linear combinations of rays. But a transformation of a physical system is a transformation of states, hence mathematically a transformation of ray space. In quantum mechanics, a transformation of a physical system gives rise to a bijective unit ray transformation $T$ of unit ray space,

T: S \ni \underline{\Psi} \subset \mathcal{H} \mapsto S' \ni \underline{\Psi'} = T\underline{\Psi} \subset \mathcal{H'}.

The set of all unit ray transformations is thus the permutation group on $S$ . Not all of these transformations are permissible as symmetry transformations to be described next. A unit ray transformation may be extended to $R$ by means of the multiplication with reals described above according to^[7]

T:R \rightarrow R'; T(\lambda \underline \Psi) \equiv \lambda T\underline \Psi, \quad \underline \Psi \in S, \lambda \in \mathbb R.

To keep the notation uniform, call this a ray transformation. This terminological distinction is not made in the literature, but is necessary here since both possibilities are covered while in the literature one possibility is chosen.

Symmetry transformations

Loosely speaking, a symmetry transformation is a change in which "nothing happens"^[8] or a "change of our view"^[9] that does not change the outcomes of possible experiments. For example, translating a system in a homogeneous environment should have no qualitative effect on the outcomes of experiments made on the system. Likewise for rotating a system in an isotropic environment. This becomes even clearer when one considers the mathematically equivalent passive transformations, i.e. simply changes of coordinates and let the system be. Usually, the domain and range Hilbert spaces are the same. An exception would be (in a non-relativistic theory) the Hilbert space of electron states that is subjected to a charge conjugation transformation. In this case the electron states are mapped to the Hilbert space of positron states and vice versa. To make this precise, introduce the ray product,

\underline{\Psi} \cdot \underline{\Phi} = |( \Psi, \Phi)|,

where $(Ψ,Φ)$ is the Hilbert space inner product. A surjective ray transformation $T : R \to R'$ is called a symmetry transformation if^[10]

T \underline{\Psi} \cdot T\underline{\Phi} = \underline{\Psi} \cdot \underline{\Phi}, \quad \forall \Psi, \Phi \in \mathcal{H}.

It can also be defined in terms of unit ray space, i. e. $T : S \to S'$ with no other changes.^[11]^[12] In this case it is sometimes called a Wigner automorphism. It can then be extended to $R$ by means of multiplication by reals as described earlier. In particular, unit rays are taken to unit rays. The significance of this definition is that transition probabilities are preserved. In particular the Born rule, another postulate of quantum mechanics, will predict the same probabilities in the transformed and untransformed systems,

P(\Psi \rightarrow \Phi) = |(\Psi, \Phi)|^2 = [\underline{\Psi} \cdot \underline{\Phi}]^2 = [T\underline{\Psi} \cdot T\underline{\Phi}]^2 = |(\Psi', \Phi')|^2 = P(\Psi' \rightarrow \Phi'), \quad \Psi' \in T\underline{\Psi}, \Phi' \in T\underline{\Phi}.

It is clear from the definitions that this is independent of the representatives of the rays chosen.

Symmetry groups

Some facts about symmetry transformations that can be verified using the definition:

The product of two symmetry transformations, i.e. two symmetry transformations applied in concession, is a symmetry transformation.
Any symmetry transformation has an inverse.
The identity transformation is a symmetry transformation.
Multiplication of symmetry transformations is associative.

The set of symmetry transformations thus forms a group, the symmetry group of the system. Some important frequently occurring subgroups in the symmetry group of a system are realizations of

The symmetric group with its subgroups. This is important on the exchange of particle labels.
The Poincaré group. It encodes the fundamental symmetries of spacetime.
Internal symmetry groups like SU(2) and SU(3). They describe so called internal symmetries, like isospin and color charge peculiar to quantum mechanical systems.

These groups are also referred to as symmetry groups of the system.

Statement of Wigner's theorem

Preliminaries

Some preliminary definitions are needed to state the theorem. A transformation $U$ of Hilbert space is unitary if

( U \Psi, U \Phi) = ( \Psi, \Phi),

and a transformation is antiunitary if

( A \Psi, A \Phi) = ( \Psi, \Phi)^* = ( \Phi, \Psi).

A unitary operator is automatically linear. Likewise an antiunitary transformation is necessarily antilinear.^{[nb 2]} Both variants are real linear and additive.

Given a unitary transformation $U$ of Hilbert space, define

T: \underline{\Psi} = \{e^{i\alpha}\Psi| \alpha \in \mathbb{R}\} \mapsto \underline{\Psi'} = \{e^{i\beta}U\Psi| \beta \in \mathbb{R}\}.

This is a symmetry transformation since

T\underline{\Psi}\cdot T\underline{\Phi}=\underline{\Psi'}\cdot\underline{\Phi'}=|( e^{i\alpha}U\Psi, e^{i\beta}U\Phi)| = |( \Psi, \Phi)| = \underline{\Psi}\cdot\underline{\Phi}.

In the same way an antiunitary transformation of Hilbert space induces a symmetry transformation. One says that a transformation $U$ of Hilbert space is compatible with the transformation $T$ of ray space if for all $Ψ$ ,^[11]

T\underline{\Psi} = \{e^{i\alpha}U\Psi|\alpha \in \mathbb R\},

or equivalently

U\Psi \in T \underline \Psi.

Transformations of Hilbert space by either a unitary linear transformation or an antiunitary antilinear operator are obviously then compatible with the transformations or ray space they induce as described.

Statement

Wigner's theorem states a converse of the above:^[13]

Wigner's theorem (1931): If $H$ and $K$ are Hilbert spaces and if

T:\underline{\Psi} \subset \mathcal H \mapsto \underline{\Psi'} \subset \mathcal K

is a symmetry transformation, then there exists a transformation

V : H \to K

which is compatible with

T

and such that

V

is either unitary or antiunitary if

dim H \geq 2

. If

dim H = 1

there exists a unitary transformation

U : H \to K

and an antiunitary transformation

A : H \to K

, both compatible with

T

Proofs can be found in Wigner (1931, 1959), Bargmann (1964) and Weinberg (2002).

Antiunitary and antilinear transformations are less prominent in physics. They are all related to a reversal of the direction of the flow of time.^[14]

Representations and projective representations

A transformation compatible with a symmetry transformation is not unique. One has the following (additive transformations include both linear and antilinear transformations).^[15]^[16]

Theorem: If

U

and

V

are two additive transformations of

H

onto

K

, both compatible with the ray transformation

T

with

dim H \geq 2

, then

V = Ue^{i\alpha}, \alpha \in \mathbb R.

The significance of this theorem is that it specifies the degree of uniqueness of the representation on $H$ . On the face of it, one might believe that

Vh = Ue^{i\alpha(h)}h, \alpha \in \mathbb R, h \in \mathcal H \quad (\text{wrong unless } \alpha(h) = \text{const})

would be admissible, with $α(h) \neq α(k)$ for $⟨h|k⟩ = 0$ , but this is not the case according to the theorem.^{[nb 3]} If $G$ is a symmetry group (in this latter sense of being embedded as a subgroup of the symmetry group of the system acting on ray space), and if $f, g, h \in G$ with $fg = h$ , then

T(f)T(g) = T(h),

where the $T$ are ray transformations. From the last theorem, one has for the compatible representatives $U$ ,

U(f)U(g) = \omega(f, g)U(fg) = e^{i\xi(f,g)}U(fg),

where $ω (f, g)$ is a phase factor.^{[nb 4]}

The function $ω$ is called a $2$ -cocycle or Schur multiplier. A map $U : G \to GL(V)$ satisfying the above relation for some vector space $V$ is called a projective representation or a ray representation. If $ω (f, g) = 1$ , then it is called a representation.

One should note that the terminology differs between mathematics and physics. In the linked article, term projective representation has a slightly different meaning, but the term as presented here enters as an ingredient and the mathematics per se is of course the same. If the realization of the symmetry group, $g \to T (g)$ , is given in terms of action on the space of unit rays $S = PH$ , then it is a projective representation $G \to PGL(H)$ in the mathematical sense, while its representative on Hilbert space is a projective representation $G \to GL(H)$ in the physical sense.

Applying the last relation (several times) to the product $fgh$ and appealing to the known associativity of multiplication of operators on $H$ , one finds

\begin{align}\omega(f,g)\omega(fg,h) &= \omega(g,h)\omega(f,gh),\\ \xi(f,g) + \xi(fg,h) &= \xi(g,h) + \xi(f,gh) \quad (\operatorname{mod} 2\pi).\end{align}

Thy also satisfy

\begin{align} \omega(g,e) &= \omega(e,g) = 1,\\ \xi(g,e) &= \xi(e,g) = 0 \quad (\operatorname{mod} 2\pi),\\ \omega(g,g^{-1}) &= \omega(g^{-1},g),\\ \xi(g,g^{-1}) &= \xi(g^{-1},g) = 0 \quad (\operatorname{mod} 2\pi).\\ \end{align}

Upon redefinition of the phases,

U(g) \mapsto \hat{U}(g) = \eta(g)U(g) = e^{i\zeta(g)}U(g),

which is allowed by last theorem, one finds^[17]^[18]

\begin{align}\hat{\omega}(g,h) &= \omega(g,h)\eta(g)\eta(h)\eta(gh)^{-1},\\ \hat{\xi}(g,h) &= \xi(g,h) + \zeta(g) + \zeta(h) - \zeta(gh) \quad (\operatorname{mod} 2\pi),\end{align}

where the hatted quantities are defined by

\hat{U}(f)\hat{U}(g) = \hat{\omega}(f, g)\hat{U}(fg) = e^{i\hat{\xi}(f,g)}\hat{U}(fg).

Utility of phase freedom

The following rather technical theorems and many more can be found, with accessible proofs, in Bargmann (1954).

The freedom of choice of phases can be used to simplify the phase factors. For some groups the phase can be eliminated altogether.

Theorem:If G is semisimple and simply connected, then $ω (g, h) = 1$ is possible.^[19]

In the case of the Lorentz group and its subgroup the rotation group SO(3), phases can, for projective representations, be chosen such that $ω (g, h) = \pm 1$ . For their respective universal covering groups, SL(2,C) and Spin(3), it is according to the theorem possible to have $ω (g, h) = 1$ , i.e. they are proper representations.

The study of redefinition of phases involves group cohomology. Two functions related as the hatted and non-hatted versions of $ω$ above are said to be cohomologous. They belong to the same second cohomology class, i.e. they are represented by the same element in $H 2 (G)$ , the second cohomology group of $G$ . If an element of $H 2 (G)$ contains the trivial function $ω = 0$ , then it is said to be trivial.^[18] The topic can be studied at the level of Lie algebras and Lie algebra cohomology as well.^[20]^[21]

Assuming the projective representation $g \to T (g)$ is weakly continuous, two relevant theorems can be stated. An immediate consequence of (weak) continuity is that the identity component is represented by unitary operators.^{[nb 5]}

Theorem: (Wigner 1939). The phase freedom can be used such that in a some neighborhood of the identity the map $g \to U (g)$ is strongly continuous.^[22]
Theorem (Bargmann). In a sufficiently small neighborhood of e, the choice $ω (g 1, g 2) \equiv 1$ is possible for semisimple Lie groups (such as $SO(n)$ , SO(3,1) and affine linear groups, (in particular the Poincaré group). More precisely, this is exactly the case when the second cohomology group $H 2 (G, ℝ)$ of the Lie algebra $g$ of $G$ is trivial.^[22]

Remarks

↑ Here the possibility of superselection rules is ignored. It may be the case that a system cannot be prepared in specific states. For instance, superposition of states with different spin is generally believed impossible. Likewise, states being superpositions of states with different charge are considered impossible. Minor complications due to those issues are treated in Bogoliubov, Logunov & Todorov (1975)
↑ Bäurle & de Kerf (1999, p. 342) This is stated but not proved.
↑ There is an exception to this. If a superselection rule is in effect, then the phase may depend on in which sector of $H$ $h$ resides, see Weinberg 2002, p. 53
↑ Again there is an exception. If a superselection rule is in effect, then the phase may depend on in which sector of $H$ $h$ resides on which the operators act, see Weinberg 2002, p. 53
↑ This is made plausible as follows. In an open neighborhood in the vicinity of the identity all operators can be expressed as squares. Whether an operator is unitary or antiunitary its square is unitary. Hence they are all unitary in a sufficiently small neighborhood. Such a neighborhood generates the identity.

Notes

↑ Seitz, Vogt & Weinberg 2000
↑ Wigner 1931, pp. 251–254 (in German),
Wigner 1959, pp. 233–236 (English translation).
↑ Weinberg 2002, p. 49
↑ Bäuerle & de Kerf 1999, p. 341
↑ Simon et al. 2008
↑ This approach is used in Bargmann 1964, which serves as a basis reference for the proof outline to be given below.
↑ Bauerle & de Kerf 1999, p. 341 defines general ray transformations on $R$ to begin with, which means that it is not necessarily bijective on $S$ (i.e. not necessarily norm preserving). This is not important since only symmetry transformations are of interest anyway.
↑ de Kerf & Bäuerle 1999
↑ Weinberg 2992, p. 50
↑ de Kerf & Van Groesen 1999, p. 342
1 2 Bargmann 1964
↑ Wigner 1931
↑ de Kerf & Van Groesen 1999, p. 343
↑ Weinberg 2002, p. 51
↑ This is proved in detail in Bargmann 1964.
↑ de Kerf & Van Groesen 1999, p. 344 This is stated but not proved.
↑ de Kerf & Van Groesen 1999, p. 346 There is an error in this formula in the book.
1 2 Weinberg 2002, p. 82
↑ Weinberg 2002, Appendix B, Chapter 2
↑ Bäurle & de Kerf 1999, pp. 347–349
↑ Weinberg 2002, Section 2.7.
1 2 Straumann 2014

References

Bargmann, V. (1954). "On unitary ray representations of continuous groups". Ann. of Math. 59 (1): 1–46. doi:10.2307/1969831. JSTOR 1969831 – via JSTOR.
Bargmann, V. (1964). "Note on Wigner's Theorem on Symmetry Operations". Journal of Mathematical Physics 5 (7): 862. doi:10.1063/1.1704188. (subscription required (help)).
Bogoliubov, N. N.; Logunov, A.A.; Todorov, I. T. (1975). Introduction to axiomatic quantum field theory. Mathematical Physics Monograph Series 18. Translated to English by Stephan A. Fulling and Ludmila G. Popova. New York: Benjamin. ASIN B000IM4HLS.
Bäurle, C. G. A.; de Kerf, E.A. (1999). E.A. Van Groesen; E. M. De Jager, eds. Lie algebras Part 1:Finite and infinite dimensional Lie algebras and their applications in physics. Studies in mathematical physics 1 (2nd ed.). Amsterdam: North-Holland. ISBN 0 444 88776 8.
Seitz, F.; Vogt, E.; Weinberg, A. M. (2000). "Eugene Paul Wigner. 17 November 1902 -- 1 January 1995". Biogr. Mems Fell. R. Soc. 46: 577–592. doi:10.1098/rsbm.1999.0102.
Simon, R.; Mukunda, N.; Chaturvedi, S.; Srinivasan, V.; Hamhalter, J. (2008). "Two elementary proofs of the Wigner theorem on symmetry in quantum mechanics". Phys. Lett. A 372 (46): 6847–6852. arXiv:0808.0779. Bibcode:2008PhLA..372.6847S. doi:10.1016/j.physleta.2008.09.052 – via ScienceDirect. (subscription required (help)).
Straumann, N. (2014). A. Ashtekar; V. Petkov, eds. Springer Handbook of Spacetime. Berlin, Heidelberg: Springer Science+Business Media. Chapter14, pp. 265–278 - Unitary Representations of the inhomogeneous Lorentz Group and their Significance in Quantum Physics. arXiv:0809.4942v1. doi:10.1007/978-3-642-41992-8_14. ISBN 978-3-642-41991-1.
Weinberg, S. (2002), The Quantum Theory of Fields I, Cambridge University Press, ISBN 0-521-55001-7
Wigner, E. P. (1931). Gruppentheorie und ihre Anwendung auf die Quanten mechanik der Atomspektren (in German). Braunschweig, Germany: Friedrich Vieweg und Sohn. pp. 251–254. ASIN B000K1MPEI.
Wigner, E. P. (1959). Group Theory and its Application to the Quantum Mechanics of Atomic Spectra. translation from German by J. J. Griffin. New York: Academic Press. pp. 233–236. ISBN 978-0-1275-0550-3.