# Poincaré group Information

https://en.wikipedia.org/wiki/Poincaré_group
Henri Poincaré

The Poincaré group, named after Henri Poincaré (1906), [1] was first defined by Hermann Minkowski (1908) as the group of Minkowski spacetime isometries. [2] [3] It is a ten-dimensional non-abelian Lie group that is of importance as a model in our understanding of the most basic fundamentals of physics.

## Overview

A Minkowski spacetime isometry has the property that the interval between events is left invariant. For example, if everything were postponed by two hours, including the two events and the path you took to go from one to the other, then the time interval between the events recorded by a stop-watch you carried with you would be the same. Or if everything were shifted five kilometres to the west, or turned 60 degrees to the right, you would also see no change in the interval. It turns out that the proper length of an object is also unaffected by such a shift. A time or space reversal (a reflection) is also an isometry of this group.

In Minkowski space (i.e. ignoring the effects of gravity), there are ten degrees of freedom of the isometries, which may be thought of as translation through time or space (four degrees, one per dimension); reflection through a plane (three degrees, the freedom in orientation of this plane); or a " boost" in any of the three spatial directions (three degrees). Composition of transformations is the operation of the Poincaré group, with proper rotations being produced as the composition of an even number of reflections.

In classical physics, the Galilean group is a comparable ten-parameter group that acts on absolute time and space. Instead of boosts, it features shear mappings to relate co-moving frames of reference.

## Poincaré symmetry

Poincaré symmetry is the full symmetry of special relativity. It includes:

The last two symmetries, J and K, together make the Lorentz group (see also Lorentz invariance); the semi-direct product of the translations group and the Lorentz group then produce the Poincaré group. Objects that are invariant under this group are then said to possess Poincaré invariance or relativistic invariance.

10 generators (in four spacetime dimensions) associated with the Poincaré symmetry, by Noether's theorem, imply 10 conservation laws: 1 for the energy, 3 for the momentum, 3 for the angular momentum and 3 for the velocity of the center of mass. [4] [5]

## Poincaré group

The Poincaré group is the group of Minkowski spacetime isometries. It is a ten-dimensional noncompact Lie group. The abelian group of translations is a normal subgroup, while the Lorentz group is also a subgroup, the stabilizer of the origin. The Poincaré group itself is the minimal subgroup of the affine group which includes all translations and Lorentz transformations. More precisely, it is a semidirect product of the translations and the Lorentz group,

${\displaystyle \mathbf {R} ^{1,3}\rtimes \operatorname {O} (1,3)\,,}$

with group multiplication

${\displaystyle (\alpha ,f)\cdot (\beta ,g)=(\alpha +f\cdot \beta ,\;f\cdot g)}$. [6]

Another way of putting this is that the Poincaré group is a group extension of the Lorentz group by a vector representation of it; it is sometimes dubbed, informally, as the inhomogeneous Lorentz group. In turn, it can also be obtained as a group contraction of the de Sitter group SO(4,1) ~ Sp(2,2), as the de Sitter radius goes to infinity.

Its positive energy unitary irreducible representations are indexed by mass (nonnegative number) and spin ( integer or half integer) and are associated with particles in quantum mechanics (see Wigner's classification).

In accordance with the Erlangen program, the geometry of Minkowski space is defined by the Poincaré group: Minkowski space is considered as a homogeneous space for the group.

In quantum field theory, the universal cover of the Poincaré group

${\displaystyle \mathbf {R} ^{1,3}\rtimes \operatorname {SL} (2,\mathbf {C} ),}$

which may be identified with the double cover

${\displaystyle \mathbf {R} ^{1,3}\rtimes \operatorname {Spin} (1,3),}$

is more important, because representations of ${\displaystyle \operatorname {SO} (1,3)}$ are not able to describe fields with spin 1/2; i.e. fermions. Here ${\displaystyle \operatorname {SL} (2,\mathbf {C} )}$ is the group of complex ${\displaystyle 2\times 2}$ matrices with unit determinant, isomorphic to the Lorentz-signature spin group ${\displaystyle \operatorname {Spin} (1,3)}$.

## Poincaré algebra

The Poincaré algebra is the Lie algebra of the Poincaré group. It is a Lie algebra extension of the Lie algebra of the Lorentz group. More specifically, the proper (${\textstyle \det \Lambda =1}$), orthochronous (${\textstyle {\Lambda ^{0}}_{0}\geq 1}$) part of the Lorentz subgroup (its identity component), ${\textstyle SO(1,3)_{+}^{\uparrow }}$, is connected to the identity and is thus provided by the exponentiation ${\textstyle \exp \left(ia_{\mu }P^{\mu }\right)\exp \left({\frac {i}{2}}\omega _{\mu \nu }M^{\mu \nu }\right)}$ of this Lie algebra. In component form, the Poincaré algebra is given by the commutation relations: [7] [8]

{\displaystyle {\begin{aligned}[][P_{\mu },P_{\nu }]&=0\,\\{\frac {1}{i}}~[M_{\mu \nu },P_{\rho }]&=\eta _{\mu \rho }P_{\nu }-\eta _{\nu \rho }P_{\mu }\,\\{\frac {1}{i}}~[M_{\mu \nu },M_{\rho \sigma }]&=\eta _{\mu \rho }M_{\nu \sigma }-\eta _{\mu \sigma }M_{\nu \rho }-\eta _{\nu \rho }M_{\mu \sigma }+\eta _{\nu \sigma }M_{\mu \rho }\,,\end{aligned}}}

where ${\displaystyle P}$ is the generator of translations, ${\displaystyle M}$ is the generator of Lorentz transformations, and ${\displaystyle \eta }$ is the ${\displaystyle (+,-,-,-)}$ Minkowski metric (see Sign convention).

The bottom commutation relation is the ("homogeneous") Lorentz group, consisting of rotations, ${\textstyle J_{i}={\frac {1}{2}}\epsilon _{imn}M^{mn}}$, and boosts, ${\textstyle K_{i}=M_{i0}}$. In this notation, the entire Poincaré algebra is expressible in noncovariant (but more practical) language as

{\displaystyle {\begin{aligned}[][J_{m},P_{n}]&=i\epsilon _{mnk}P_{k}~,\\[][J_{i},P_{0}]&=0~,\\[][K_{i},P_{k}]&=i\eta _{ik}P_{0}~,\\[][K_{i},P_{0}]&=-iP_{i}~,\\[][J_{m},J_{n}]&=i\epsilon _{mnk}J_{k}~,\\[][J_{m},K_{n}]&=i\epsilon _{mnk}K_{k}~,\\[][K_{m},K_{n}]&=-i\epsilon _{mnk}J_{k}~,\end{aligned}}}

where the bottom line commutator of two boosts is often referred to as a "Wigner rotation". The simplification ${\textstyle [J_{m}+iK_{m},\,J_{n}-iK_{n}]=0}$ permits reduction of the Lorentz subalgebra to ${\textstyle {\mathfrak {su}}(2)\oplus {\mathfrak {su}}(2)}$ and efficient treatment of its associated representations. In terms of the physical parameters, we have

{\displaystyle {\begin{aligned}\left[{\mathcal {H}},p_{i}\right]&=0\\\left[{\mathcal {H}},L_{i}\right]&=0\\\left[{\mathcal {H}},K_{i}\right]&=i\hbar cp_{i}\\\left[p_{i},p_{j}\right]&=0\\\left[p_{i},L_{j}\right]&=i\hbar \epsilon _{ijk}p_{k}\\\left[p_{i},K_{j}\right]&={\frac {i\hbar }{c}}{\mathcal {H}}\delta _{ij}\\\left[L_{i},L_{j}\right]&=i\hbar \epsilon _{ijk}L_{k}\\\left[L_{i},K_{j}\right]&=i\hbar \epsilon _{ijk}K_{k}\\\left[K_{i},K_{j}\right]&=-i\hbar \epsilon _{ijk}L_{k}\end{aligned}}}

The Casimir invariants of this algebra are ${\textstyle P_{\mu }P^{\mu }}$ and ${\textstyle W_{\mu }W^{\mu }}$ where ${\textstyle W_{\mu }}$ is the Pauli–Lubanski pseudovector; they serve as labels for the representations of the group.

The Poincaré group is the full symmetry group of any relativistic field theory. As a result, all elementary particles fall in representations of this group. These are usually specified by the four-momentum squared of each particle (i.e. its mass squared) and the intrinsic quantum numbers ${\textstyle J^{PC}}$, where ${\displaystyle J}$ is the spin quantum number, ${\displaystyle P}$ is the parity and ${\displaystyle C}$ is the charge-conjugation quantum number. In practice, charge conjugation and parity are violated by many quantum field theories; where this occurs, ${\displaystyle P}$ and ${\displaystyle C}$ are forfeited. Since CPT symmetry is invariant in quantum field theory, a time-reversal quantum number may be constructed from those given.

As a topological space, the group has four connected components: the component of the identity; the time reversed component; the spatial inversion component; and the component which is both time-reversed and spatially inverted. [9]

## Other dimensions

The definitions above can be generalized to arbitrary dimensions in a straightforward manner. The d-dimensional Poincaré group is analogously defined by the semi-direct product

${\displaystyle \operatorname {IO} (1,d-1):=\mathbf {R} ^{1,d-1}\rtimes \operatorname {O} (1,d-1)}$

with the analogous multiplication

${\displaystyle (\alpha ,f)\cdot (\beta ,g)=(\alpha +f\cdot \beta ,\;f\cdot g)}$. [6]

The Lie algebra retains its form, with indices µ and ν now taking values between 0 and d − 1. The alternative representation in terms of Ji and Ki has no analogue in higher dimensions.

## Super-Poincaré algebra

A related observation is that the representations of the Lorentz group include a pair of inequivalent two-dimensional complex spinor representations ${\displaystyle 2}$ and ${\displaystyle {\overline {2}}}$ whose tensor product ${\displaystyle 2\otimes {\overline {2}}=3\oplus 1}$ is the adjoint representation. One may identify this last bit with four-dimensional Minkowski space itself (as opposed to identifying it with a spin-1 particle, as would normally be done for a pair of fermions, e.g. a pion being composed of a quark-anti-quark pair). This strongly suggests that it might be possible to extend the Poincaré algebra to also include spinors. This leads directly to the notion of the super-Poincaré algebra. The mathematical appeal of this idea is that one is working with the fundamental representations, instead of the adjoint representations. The physical appeal of this idea is that the fundamental representations correspond to fermions, which are seen in nature. So far, however, the implied supersymmetry here, of a symmetry between spatial and fermionic directions, has not been seen experimentally in nature. The experimental issue can roughly be stated as the question: if we live in the adjoint representation (Minkowski spacetime), then where is the fundamental representation hiding?

## Notes

1. ^ Poincaré, Henri (December 1906), , Rendiconti del Circolo Matematico di Palermo, 21: 129–176, Bibcode: 1906RCMP...21..129P, doi: 10.1007/bf03013466, hdl: 2027/uiug.30112063899089, S2CID  120211823 ( Wikisource translation: On the Dynamics of the Electron). The group defined in this paper would now be described as the homogeneous Lorentz group with scalar multipliers.
2. ^ Minkowski, Hermann, , Nachrichten von der Gesellschaft der Wissenschaften zu Göttingen, Mathematisch-Physikalische Klasse: 53–111 (Wikisource translation: The Fundamental Equations for Electromagnetic Processes in Moving Bodies).
3. ^ Minkowski, Hermann, , Physikalische Zeitschrift, 10: 75–88
4. ^ "Survey of Symmetry and Conservation Laws: More Poincare" (PDF). frankwilczek.com. Retrieved 2021-02-14.
5. ^ Barnett, Stephen M (2011-06-01). "On the six components of optical angular momentum". Journal of Optics. 13 (6): 064010. Bibcode: 2011JOpt...13f4010B. doi: 10.1088/2040-8978/13/6/064010. ISSN  2040-8978.
6. ^ a b Oblak, Blagoje (2017-08-01). BMS Particles in Three Dimensions. Springer. p. 80. ISBN  9783319618784.
7. ^ N.N. Bogolubov (1989). General Principles of Quantum Field Theory (2nd ed.). Springer. p. 272. ISBN  0-7923-0540-X.
8. ^ T. Ohlsson (2011). Relativistic Quantum Physics: From Advanced Quantum Mechanics to Introductory Quantum Field Theory. Cambridge University Press. p. 10. ISBN  978-1-13950-4324.
9. ^ "Topics: Poincaré Group". www.phy.olemiss.edu. Retrieved 2021-07-18.