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Particle physics and representation theory

From Wikipedia, the free encyclopedia
Physics-mathematics connection
Lie groups andLie algebras

There is a natural connection betweenparticle physics andrepresentation theory, as first noted in the 1930s byEugene Wigner.[1] It links the properties ofelementary particles to the structure ofLie groups andLie algebras. According to this connection, the differentquantum states of an elementary particle give rise to anirreducible representation of thePoincaré group. Moreover, the properties of the various particles, including theirspectra, can be related to representations of Lie algebras, corresponding to "approximate symmetries" of the universe.

General picture

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Symmetries of a quantum system

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Main article:Symmetry in quantum mechanics

Inquantum mechanics, any particular one-particle state is represented as avector in aHilbert spaceH{\displaystyle {\mathcal {H}}}. To help understand what types of particles can exist, it is important to classify the possibilities forH{\displaystyle {\mathcal {H}}} allowed bysymmetries, and their properties. LetH{\displaystyle {\mathcal {H}}} be a Hilbert space describing a particular quantum system and letG{\displaystyle G} be a group of symmetries of the quantum system. In a relativistic quantum system, for example,G{\displaystyle G} might be thePoincaré group, while for the hydrogen atom,G{\displaystyle G} might be therotation group SO(3). The particle state is more precisely characterized by the associatedprojective Hilbert spacePH{\displaystyle \mathrm {P} {\mathcal {H}}}, also calledray space, since two vectors that differ by a nonzero scalar factor correspond to the same physicalquantum state represented by aray in Hilbert space, which is anequivalence class inH{\displaystyle {\mathcal {H}}} and, under the natural projection mapHPH{\displaystyle {\mathcal {H}}\rightarrow \mathrm {P} {\mathcal {H}}}, an element ofPH{\displaystyle \mathrm {P} {\mathcal {H}}}.

By definition of a symmetry of a quantum system, there is agroup action onPH{\displaystyle \mathrm {P} {\mathcal {H}}}. For eachgG{\displaystyle g\in G}, there is a corresponding transformationV(g){\displaystyle V(g)} ofPH{\displaystyle \mathrm {P} {\mathcal {H}}}. More specifically, ifg{\displaystyle g} is some symmetry of the system (say, rotation about the x-axis by 12°), then the corresponding transformationV(g){\displaystyle V(g)} ofPH{\displaystyle \mathrm {P} {\mathcal {H}}} is a map on ray space. For example, when rotating astationary (zero momentum) spin-5 particle about its center,g{\displaystyle g} is a rotation in 3D space (an element ofSO(3){\displaystyle \mathrm {SO(3)} }), whileV(g){\displaystyle V(g)} is an operator whose domain and range are each the space of possible quantum states of this particle, in this example the projective spacePH{\displaystyle \mathrm {P} {\mathcal {H}}} associated with an 11-dimensional complex Hilbert spaceH{\displaystyle {\mathcal {H}}}.

Each mapV(g){\displaystyle V(g)} preserves, by definition of symmetry, theray product onPH{\displaystyle \mathrm {P} {\mathcal {H}}} induced by the inner product onH{\displaystyle {\mathcal {H}}}; according toWigner's theorem, this transformation ofPH{\displaystyle \mathrm {P} {\mathcal {H}}} comes from a unitary or anti-unitary transformationU(g){\displaystyle U(g)} ofH{\displaystyle {\mathcal {H}}}. Note, however, that theU(g){\displaystyle U(g)} associated to a givenV(g){\displaystyle V(g)} is not unique, but only uniqueup to a phase factor. The composition of the operatorsU(g){\displaystyle U(g)} should, therefore, reflect the composition law inG{\displaystyle G}, but only up to a phase factor:

U(gh)=eiθU(g)U(h){\displaystyle U(gh)=e^{i\theta }U(g)U(h)},

whereθ{\displaystyle \theta } will depend ong{\displaystyle g} andh{\displaystyle h}. Thus, the map sendingg{\displaystyle g} toU(g){\displaystyle U(g)} is aprojective unitary representation ofG{\displaystyle G}, or possibly a mixture of unitary and anti-unitary, ifG{\displaystyle G} is disconnected. In practice, anti-unitary operators are always associated withtime-reversal symmetry.

Ordinary versus projective representations

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It is important physically that in generalU(){\displaystyle U(\cdot )} does not have to be an ordinary representation ofG{\displaystyle G}; it may not be possible to choose the phase factors in the definition ofU(g){\displaystyle U(g)} to eliminate the phase factors in their composition law. An electron, for example, is a spin-one-half particle; its Hilbert space consists of wave functions onR3{\displaystyle \mathbb {R} ^{3}} with values in a two-dimensional spinor space. The action ofSO(3){\displaystyle \mathrm {SO(3)} } on the spinor space is only projective: It does not come from an ordinary representation ofSO(3){\displaystyle \mathrm {SO(3)} }. There is, however, an associated ordinary representation of the universal coverSU(2){\displaystyle \mathrm {SU(2)} } ofSO(3){\displaystyle \mathrm {SO(3)} } on spinor space.[2]

For many interesting classes of groupsG{\displaystyle G},Bargmann's theorem tells us that every projective unitary representation ofG{\displaystyle G} comes from an ordinary representation of the universal coverG~{\displaystyle {\tilde {G}}} ofG{\displaystyle G}. Actually, ifH{\displaystyle {\mathcal {H}}} is finite dimensional, then regardless of the groupG{\displaystyle G}, every projective unitary representation ofG{\displaystyle G} comes from an ordinary unitary representation ofG~{\displaystyle {\tilde {G}}}.[3] IfH{\displaystyle {\mathcal {H}}} is infinite dimensional, then to obtain the desired conclusion, some algebraic assumptions must be made onG{\displaystyle G} (see below). In this setting the result is atheorem of Bargmann.[4] Fortunately, in the crucial case of the Poincaré group, Bargmann's theorem applies.[5] (SeeWigner's classification of the representations of the universal cover of the Poincaré group.)

The requirement referred to above is that the Lie algebrag{\displaystyle {\mathfrak {g}}} does not admit a nontrivial one-dimensional central extension. This is the case if and only if thesecond cohomology group ofg{\displaystyle {\mathfrak {g}}} is trivial. In this case, it may still be true that the group admits a central extension by adiscrete group. But extensions ofG{\displaystyle G} by discrete groups are covers ofG{\displaystyle G}. For instance, the universal coverG~{\displaystyle {\tilde {G}}} is related toG{\displaystyle G} through the quotientGG~/Γ{\displaystyle G\approx {\tilde {G}}/\Gamma } with the central subgroupΓ{\displaystyle \Gamma } being the center ofG~{\displaystyle {\tilde {G}}} itself, isomorphic to thefundamental group of the covered group.

Thus, in favorable cases, the quantum system will carry a unitary representation of the universal coverG~{\displaystyle {\tilde {G}}} of the symmetry groupG{\displaystyle G}. This is desirable becauseH{\displaystyle {\mathcal {H}}} is much easier to work with than the non-vector spacePH{\displaystyle \mathrm {P} {\mathcal {H}}}. If the representations ofG~{\displaystyle {\tilde {G}}} can be classified, much more information about the possibilities and properties ofH{\displaystyle {\mathcal {H}}} are available.

The Heisenberg case

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An example in which Bargmann's theorem does not apply comes from a quantum particle moving inRn{\displaystyle \mathbb {R} ^{n}}. The group of translational symmetries of the associated phase space,R2n{\displaystyle \mathbb {R} ^{2n}}, is the commutative groupR2n{\displaystyle \mathbb {R} ^{2n}}. In the usual quantum mechanical picture, theR2n{\displaystyle \mathbb {R} ^{2n}} symmetry is not implemented by a unitary representation ofR2n{\displaystyle \mathbb {R} ^{2n}}. After all, in the quantum setting, translations in position space and translations in momentum space do not commute. This failure to commute reflects the failure of the position and momentum operators—which are the infinitesimal generators of translations in momentum space and position space, respectively—to commute. Nevertheless, translations in position space and translations in momentum spacedo commute up to a phase factor. Thus, we have a well-defined projective representation ofR2n{\displaystyle \mathbb {R} ^{2n}}, but it does not come from an ordinary representation ofR2n{\displaystyle \mathbb {R} ^{2n}}, even thoughR2n{\displaystyle \mathbb {R} ^{2n}} is simply connected.

In this case, to obtain an ordinary representation, one has to pass to theHeisenberg group, which is a nontrivial one-dimensional central extension ofR2n{\displaystyle \mathbb {R} ^{2n}}.

Poincaré group

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Main article:Wigner's classification

The group of translations andLorentz transformations form thePoincaré group, and this group should be a symmetry of a relativistic quantum system (neglectinggeneral relativity effects, or in other words, inflat spacetime).Representations of the Poincaré group are in many cases characterized by a nonnegativemass and a half-integerspin (seeWigner's classification); this can be thought of as the reason that particles have quantized spin. (There are in fact other possible representations, such astachyons,infraparticles, etc., which in some cases do not have quantized spin or fixed mass.)

Other symmetries

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The pattern ofweak isospins,weak hypercharges, andcolor charges (weights) of all known elementary particles in theStandard Model, rotated by theweak mixing angle to show electric charge roughly along the vertical.

While thespacetime symmetries in the Poincaré group are particularly easy to visualize and believe, there are also other types of symmetries, calledinternal symmetries. One example iscolorSU(3), an exact symmetry corresponding to the continuous interchange of the threequark colors.

Lie algebras versus Lie groups

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Many (but not all) symmetries or approximate symmetries formLie groups. Rather than study therepresentation theory of these Lie groups, it is often preferable to study the closely relatedrepresentation theory of the corresponding Lie algebras, which are usually simpler to compute.

Now, representations of the Lie algebra correspond to representations of theuniversal cover of the original group.[6] In thefinite-dimensional case—and the infinite-dimensional case, provided thatBargmann's theorem applies—irreducible projective representations of the original group correspond to ordinary unitary representations of the universal cover. In those cases, computing at the Lie algebra level is appropriate. This is the case, notably, for studying the irreducible projective representations of the rotation group SO(3). These are in one-to-one correspondence with the ordinary representations of theuniversal cover SU(2) of SO(3). The representations of the SU(2) are then in one-to-one correspondence with the representations of its Lie algebra su(2), which is isomorphic to the Lie algebra so(3) of SO(3).

Thus, to summarize, the irreducible projective representations of SO(3) are in one-to-one correspondence with the irreducible ordinary representations of its Lie algebra so(3). The two-dimensional "spin 1/2" representation of the Lie algebra so(3), for example, does not correspond to an ordinary (single-valued) representation of the group SO(3). (This fact is the origin of statements to the effect that "if you rotate the wave function of an electron by 360 degrees, you get the negative of the original wave function.") Nevertheless, the spin 1/2 representation does give rise to a well-definedprojective representation of SO(3), which is all that is required physically.

Approximate symmetries

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Although the above symmetries are believed to be exact, other symmetries are only approximate.

Hypothetical example

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As an example of what an approximate symmetry means, suppose an experimentalist lived inside an infiniteferromagnet, with magnetization in some particular direction. The experimentalist in this situation would find not one but two distinct types of electrons: one with spin along the direction of the magnetization, with a slightly lower energy (and consequently, a lower mass), and one with spin anti-aligned, with a higher mass. Our usualSO(3) rotational symmetry, which ordinarily connects the spin-up electron with the spin-down electron, has in this hypothetical case become only anapproximate symmetry, relatingdifferent types of particles to each other.

General definition

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In general, an approximate symmetry arises when there are very strong interactions that obey that symmetry, along with weaker interactions that do not. In the electron example above, the two "types" of electrons behave identically under thestrong andweak forces, but differently under theelectromagnetic force.

Example: isospin symmetry

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Main article:Isospin

An example from the real world isisospin symmetry, anSU(2) group corresponding to the similarity betweenup quarks anddown quarks. This is an approximate symmetry: while up and down quarks are identical in how they interact under thestrong force, they have different masses and different electroweak interactions. Mathematically, there is an abstract two-dimensional vector space

up quark(10),down quark(01){\displaystyle {\text{up quark}}\rightarrow {\begin{pmatrix}1\\0\end{pmatrix}},\qquad {\text{down quark}}\rightarrow {\begin{pmatrix}0\\1\end{pmatrix}}}

and the laws of physics areapproximately invariant under applying a determinant-1unitary transformation to this space:[7]

(xy)A(xy),where A is in SU(2){\displaystyle {\begin{pmatrix}x\\y\end{pmatrix}}\mapsto A{\begin{pmatrix}x\\y\end{pmatrix}},\quad {\text{where }}A{\text{ is in }}SU(2)}

For example,A=(0110){\displaystyle A={\begin{pmatrix}0&1\\-1&0\end{pmatrix}}} would turn all up quarks in the universe into down quarks and vice versa. Some examples help clarify the possible effects of these transformations:

  • When these unitary transformations are applied to aproton, it can be transformed into aneutron, or into a superposition of a proton and neutron, but not into any other particles. Therefore, the transformations move the proton around a two-dimensional space of quantum states. The proton and neutron are called an "isospin doublet", mathematically analogous to how aspin-½ particle behaves under ordinary rotation.
  • When these unitary transformations are applied to any of the threepions (π0
    ,π+
    , andπ
    ), it can change any of the pions into any other, but not into any non-pion particle. Therefore, the transformations move the pions around a three-dimensional space of quantum states. The pions are called an "isospin triplet", mathematically analogous to how a spin-1 particle behaves under ordinary rotation.
  • These transformations have no effect at all on anelectron, because it contains neither up nor down quarks. The electron is called an isospin singlet, mathematically analogous to how a spin-0 particle behaves under ordinary rotation.

In general, particles formisospin multiplets, which correspond to irreducible representations of theLie algebra SU(2). Particles in an isospin multiplet have very similar but not identical masses, because the up and down quarks are very similar but not identical.

Example: flavour symmetry

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Main article:eightfold way (physics)

Isospin symmetry can be generalized toflavour symmetry, anSU(3) group corresponding to the similarity betweenup quarks,down quarks, andstrange quarks.[7] This is, again, an approximate symmetry, violated by quark mass differences and electroweak interactions—in fact, it is a poorer approximation than isospin, because of the strange quark's noticeably higher mass.

Nevertheless, particles can indeed be neatly divided into groups that form irreducible representations of theLie algebra SU(3), as first noted byMurray Gell-Mann and independently byYuval Ne'eman.

See also

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Notes

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  1. ^Wigner received theNobel Prize in Physics in 1963 "for his contributions to the theory of the atomic nucleus and the elementary particles, particularly through the discovery and application of fundamental symmetry principles"; see alsoWigner's theorem,Wigner's classification.
  2. ^Hall 2015 Section 4.7
  3. ^Hall 2013 Theorem 16.47
  4. ^Bargmann, V. (1954). "On unitary ray representations of continuous groups".Ann. of Math.59 (1):1–46.doi:10.2307/1969831.JSTOR 1969831.
  5. ^Weinberg 1995 Chapter 2, Appendix A and B.
  6. ^Hall 2015 Section 5.7
  7. ^abLecture notes by Prof. Mark Thomson

References

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External links

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