Conformal group

Template:Group theory sidebar In mathematics, the conformal group of an inner product space is the group of transformations from the space to itself that preserve angles. More formally, it is the group of transformations that preserve the conformal geometry of the space.

Several specific conformal groups are particularly important:

The conformal orthogonal group. If V is a vector space with a quadratic form Q, then the conformal orthogonal group Template:Nowrap is the group of linear transformations T of V for which there exists a scalar λ such that for all x in V
<math>Q(Tx) = \lambda^2 Q(x)</math>

For a definite quadratic form, the conformal orthogonal group is equal to the orthogonal group times the group of dilations.

The conformal group of the sphere is generated by the inversions in circles. This group is also known as the Möbius group.
In Euclidean space Eⁿ, Template:Nowrap, the conformal group is generated by inversions in hyperspheres.
In a pseudo-Euclidean space E^p,q, the conformal group is Template:Nowrap.<ref>Template:Cite book</ref>

All conformal groups are Lie groups.

Angle analysisEdit

In Euclidean geometry one can expect the standard circular angle to be characteristic, but in pseudo-Euclidean space there is also the hyperbolic angle. In the study of special relativity the various frames of reference, for varying velocity with respect to a rest frame, are related by rapidity, a hyperbolic angle. One way to describe a Lorentz boost is as a hyperbolic rotation which preserves the differential angle between rapidities. Thus, they are conformal transformations with respect to the hyperbolic angle.

A method to generate an appropriate conformal group is to mimic the steps of the Möbius group as the conformal group of the ordinary complex plane. Pseudo-Euclidean geometry is supported by alternative complex planes where points are split-complex numbers or dual numbers. Just as the Möbius group requires the Riemann sphere, a compact space, for a complete description, so the alternative complex planes require compactification for complete description of conformal mapping. Nevertheless, the conformal group in each case is given by linear fractional transformations on the appropriate plane.<ref> Tsurusaburo Takasu (1941) "Gemeinsame Behandlungsweise der elliptischen konformen, hyperbolischen konformen und parabolischen konformen Differentialgeometrie", 2, Proceedings of the Imperial Academy 17(8): 330–8, link from Project Euclid, Template:Mr</ref>

Mathematical definitionEdit

Given a (Pseudo-)Riemannian manifold <math>M</math> with conformal class <math>[g]</math>, the conformal group <math>\text{Conf}(M)</math> is the group of conformal maps from <math>M</math> to itself.

More concretely, this is the group of angle-preserving smooth maps from <math>M</math> to itself. However, when the signature of <math>[g]</math> is not definite, the 'angle' is a hyper-angle which is potentially infinite.

For Pseudo-Euclidean space, the definition is slightly different.<ref>Template:Cite book</ref> <math>\text{Conf}(p,q)</math> is the conformal group of the manifold arising from conformal compactification of the pseudo-Euclidean space <math>\mathbf{E}^{p, q}</math> (sometimes identified with <math>\mathbb{R}^{p,q}</math> after a choice of orthonormal basis). This conformal compactification can be defined using <math>S^p\times S^q</math>, considered as a submanifold of null points in <math>\mathbb{R}^{p+1, q+1}</math> by the inclusion <math>(\mathbf{x}, \mathbf{t})\mapsto X = (\mathbf{x}, \mathbf{t})</math> (where <math>X</math> is considered as a single spacetime vector). The conformal compactification is then <math>S^p\times S^q</math> with 'antipodal points' identified. This happens by projectivising the space <math>\mathbb{R}^{p+1,q+1}</math>. If <math>N^{p,q}</math> is the conformal compactification, then <math>\text{Conf}(p,q) := \text{Conf}(N^{p,q})</math>. In particular, this group includes inversion of <math>\mathbb{R}^{p,q}</math>, which is not a map from <math>\mathbb{R}^{p,q}</math> to itself as it maps the origin to infinity, and maps infinity to the origin.

Lie algebra of the conformal groupEdit

For Pseudo-Euclidean space <math>\mathbb{R}^{p,q}</math>, the Lie algebra of the conformal group is given by the basis <math>\{M_{\mu\nu}, P_\mu, K_\mu, D\}</math> with the following commutation relations:<ref name="cft">Template:Cite book</ref> <math display = block>\begin{align} &[D,K_\mu]= -iK_\mu \,, \\ &[D,P_\mu]= iP_\mu \,, \\ &[K_\mu,P_\nu]=2i (\eta_{\mu\nu}D-M_{\mu\nu}) \,, \\ &[K_\mu, M_{\nu\rho}] = i ( \eta_{\mu\nu} K_{\rho} - \eta_{\mu \rho} K_\nu ) \,, \\ &[P_\rho,M_{\mu\nu}] = i(\eta_{\rho\mu}P_\nu - \eta_{\rho\nu}P_\mu) \,, \\ &[M_{\mu\nu},M_{\rho\sigma}] = i (\eta_{\nu\rho}M_{\mu\sigma} + \eta_{\mu\sigma}M_{\nu\rho} - \eta_{\mu\rho}M_{\nu\sigma} - \eta_{\nu\sigma}M_{\mu\rho})\,, \end{align}</math> and with all other brackets vanishing. Here <math>\eta_{\mu\nu}</math> is the Minkowski metric.

In fact, this Lie algebra is isomorphic to the Lie algebra of the Lorentz group with one more space and one more time dimension, that is, <math>\mathfrak{conf}(p,q) \cong \mathfrak{so}(p+1, q+1)</math>. It can be easily checked that the dimensions agree. To exhibit an explicit isomorphism, define <math display = block> \begin{align} &J_{\mu\nu} = M_{\mu\nu} \,, \\ &J_{-1, \mu} = \frac{1}{2}(P_\mu - K_\mu) \,, \\ &J_{0, \mu} = \frac{1}{2}(P_\mu + K_\mu) \,, \\ &J_{-1, 0} = D. \end{align}</math> It can then be shown that the generators <math>J_{ab}</math> with <math>a, b = -1, 0, \cdots, n = p+q</math> obey the Lorentz algebra relations with metric <math>\tilde \eta_{ab} = \operatorname{diag}(-1, +1, -1, \cdots, -1, +1, \cdots, +1)</math>.

Conformal group in two spacetime dimensionsEdit

For two-dimensional Euclidean space or one-plus-one dimensional spacetime, the space of conformal symmetries is much larger. In physics it is sometimes said the conformal group is infinite-dimensional, but this is not quite correct as while the Lie algebra of local symmetries is infinite dimensional, these do not necessarily extend to a Lie group of well-defined global symmetries.

For spacetime dimension <math>n > 2</math>, the local conformal symmetries all extend to global symmetries. For <math>n = 2</math> Euclidean space, after changing to a complex coordinate <math>z = x + iy</math> local conformal symmetries are described by the infinite dimensional space of vector fields of the form <math display = block>l_n = -z^{n+1}\partial_z.</math> Hence the local conformal symmetries of 2d Euclidean space is the infinite-dimensional Witt algebra.

Conformal group of spacetimeEdit

In 1908, Harry Bateman and Ebenezer Cunningham, two young researchers at University of Liverpool, broached the idea of a conformal group of spacetime<ref>Template:Cite journal</ref><ref>Template:Cite journal</ref><ref>Template:Cite journal</ref> They argued that the kinematics groups are perforce conformal as they preserve the quadratic form of spacetime and are akin to orthogonal transformations, though with respect to an isotropic quadratic form. The liberties of an electromagnetic field are not confined to kinematic motions, but rather are required only to be locally proportional to a transformation preserving the quadratic form. Harry Bateman's paper in 1910 studied the Jacobian matrix of a transformation that preserves the light cone and showed it had the conformal property (proportional to a form preserver).<ref>Template:Cite book</ref> Bateman and Cunningham showed that this conformal group is "the largest group of transformations leaving Maxwell’s equations structurally invariant."<ref>Robert Gilmore (1994) [1974] Lie Groups, Lie Algebras and some of their Applications, page 349, Robert E. Krieger Publishing Template:ISBN Template:Mr</ref> The conformal group of spacetime has been denoted Template:Math<ref>Boris Kosyakov (2007) Introduction to the Classical Theory of Particles and Fields, page 216, Springer books via Google Books</ref>

Isaak Yaglom has contributed to the mathematics of spacetime conformal transformations in split-complex and dual numbers.<ref>Isaak Yaglom (1979) A Simple Non-Euclidean Geometry and its Physical Basis, Springer, Template:ISBN, Template:MathSciNet</ref> Since split-complex numbers and dual numbers form rings, not fields, the linear fractional transformations require a projective line over a ring to be bijective mappings.

It has been traditional since the work of Ludwik Silberstein in 1914 to use the ring of biquaternions to represent the Lorentz group. For the spacetime conformal group, it is sufficient to consider linear fractional transformations on the projective line over that ring. Elements of the spacetime conformal group were called spherical wave transformations by Bateman. The particulars of the spacetime quadratic form study have been absorbed into Lie sphere geometry.

Commenting on the continued interest shown in physical science, A. O. Barut wrote in 1985, "One of the prime reasons for the interest in the conformal group is that it is perhaps the most important of the larger groups containing the Poincaré group."<ref>A. O. Barut & H.-D. Doebner (1985) Conformal groups and Related Symmetries: Physical Results and Mathematical Background, Lecture Notes in Physics #261 Springer books, see preface for quotation</ref>

ReferencesEdit

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