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advanced_tools:group_theory:central_extension [2017/12/17 12:08] jakobadmin [Why is it interesting?] |
advanced_tools:group_theory:central_extension [2017/12/17 12:26] (current) jakobadmin [Why is it interesting?] |
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For example, the projective representations of $SO(3,1)$ correspond to regular representations of $SL(2,\mathbb{C})$. | For example, the projective representations of $SO(3,1)$ correspond to regular representations of $SL(2,\mathbb{C})$. | ||
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+ | <blockquote>"Central extensions play an important role in quantum mechanics: one of the earlier encounters is by means of Wigner’s theorem which states that a symmetry of a quantum mechanical system determines a (anti-) unitary transformation of the Hilbert space, which is unique up to a phase factor $e^{iϑ}$. As an immediate consequence of this phase factor, one deduces that given a quantum mechanical symmetry group $G$ there exists an extension $G_0$ of $G$ by $U(1)$ (the phase factors) which acts as a group of unitary transformations on the Hilbert space. **In most cases physicists have been succesful in hiding these central extensions by using larger symmetry groups**" <cite>http://math.univ-lille1.fr/~gmt/PaperFolder/CentralExtensions.pdf</cite></blockquote> | ||
<tabbox Layman> | <tabbox Layman> | ||
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* See page 178 in Moonshine beyond the Monster by Terry Gannon | * See page 178 in Moonshine beyond the Monster by Terry Gannon | ||
- | **Important Examples:** | ||
- | * The classical Galilean group needs to be extended by the introduction of a central charge, called //mass//, and this yields the Bargmann group. (This is shown very nicely in QUANTIZATION ON A LIE GROUP: HIGHER-ORDER POLARIZATIONS by V. Aldaya, J. Guerrero and G. Marmo). | ||
- | * The standard spatial rotation group $SO(3)$ needs to be extended by $\mathbb{Z}_2$, which yields $SU(2)$, because otherwise we are not able to describe spin $\frac{1}{2}$ particles. | ||
- | * The algebra of fermionic non-Abelian charge densitites needs to be extended to the Mickelsson-Faddeev algebra (See [[http://physics.stackexchange.com/a/76653/37286|this answer]]) | ||
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<tabbox Examples> | <tabbox Examples> | ||
- | --> Example1# | ||
+ | --> Galilean group -> Bargmann group# | ||
+ | |||
+ | The classical Galilean group needs to be extended by the introduction of a central charge, called //mass//, and this yields the Bargmann group. (This is shown very nicely in QUANTIZATION ON A LIE GROUP: HIGHER-ORDER POLARIZATIONS by V. Aldaya, J. Guerrero and G. Marmo). | ||
<-- | <-- | ||
- | --> Example2:# | + | --> SO(3) -> SU(2)# |
+ | |||
+ | The standard spatial rotation group $SO(3)$ needs to be extended by $\mathbb{Z}_2$, which yields $SU(2)$, because otherwise we are not able to describe spin $\frac{1}{2}$ particles. | ||
+ | |||
+ | <-- | ||
+ | |||
+ | |||
+ | --> Mickelsson-Faddeev algebra# | ||
+ | The algebra of fermionic non-Abelian charge densitites needs to be extended to the Mickelsson-Faddeev algebra (See [[http://physics.stackexchange.com/a/76653/37286|this answer]]) | ||
<-- | <-- |