In theoretical physics, a super-Poincaré algebra is an extension of the Poincaré algebra to incorporate supersymmetry, a relation between bosons and fermions. They are examples of supersymmetry algebras (without central charges or internal symmetries), and are Lie superalgebras. Thus a super-Poincaré algebra is a Z2-graded vector space with a graded Lie bracket such that the even part is a Lie algebra containing the Poincaré algebra, and the odd part is built from spinors on which there is an anticommutation relation with values in the even part.
The Poincaré algebra describes the isometries of Minkowski spacetime. From the representation theory of the Lorentz group, it is known that the Lorentz group admits two inequivalent complex spinor representations, dubbed
2
\overline{2}
2 ⊗ \overline{2}=3 ⊕ 1
Normally, one treats such a decomposition as relating to specific particles: so, for example, the pion, which is a chiral vector particle, is composed of a quark-anti-quark pair. However, one could also identify
3 ⊕ 1
The super-Poincaré algebra was first proposed in the context of the Haag–Łopuszański–Sohnius theorem, as a means of avoiding the conclusions of the Coleman–Mandula theorem. That is, the Coleman–Mandula theorem is a no-go theorem that states that the Poincaré algebra cannot be extended with additional symmetries that might describe the internal symmetries of the observed physical particle spectrum. However, the Coleman–Mandula theorem assumed that the algebra extension would be by means of a commutator; this assumption, and thus the theorem, can be avoided by considering the anti-commutator, that is, by employing anti-commuting Grassmann numbers. The proposal was to consider a supersymmetry algebra, defined as the semidirect product of a central extension of the super-Poincaré algebra by a compact Lie algebra of internal symmetries.
The simplest supersymmetric extension of the Poincaré algebra contains two Weyl spinors with the following anti-commutation relation:
\{Q\alpha,\bar
Q | |||
|
\}=
\mu} | |||
2{\sigma | |||
|
P\mu
Q\alpha,\bar
Q | |||
|
P\mu
\sigma\mu
\alpha
\alpha=1,2.
\beta |
2 ⊗ \overline{2}
\mu
\mu=0,1,2,3.
It is convenient to work with Dirac spinors instead of Weyl spinors; a Dirac spinor can be thought of as an element of
2 ⊕ \overline{2}
g\mu
\{\gamma\mu,\gamma\nu\}=2g\mu
\sigma\mu=
i | |
2 |
\left[\gamma\mu,\gamma\nu\right]
This then gives the full algebra
\begin{align} \left[M\mu,Q\alpha\right]&=
1 | |
2 |
(\sigma\mu
\beta | |
) | |
\alpha |
Q\beta\\ \left[Q\alpha,P\mu\right]&=0\\ \{Q\alpha,
\bar{Q} | |||
|
\}&=2(\sigma\mu
) | |||||
|
P\mu\\ \end{align}
which are to be combined with the normal Poincaré algebra. It is a closed algebra, since all Jacobi identities are satisfied and can have since explicit matrix representations. Following this line of reasoning will lead to supergravity.
See also: Extended supersymmetry.
It is possible to add more supercharges. That is, we fix a number which by convention is labelled
l{N}
I | |
Q | |
\alpha, |
\bar
I | |||
Q | |||
|
I=1, … ,l{N}.
These can be thought of as many copies of the original supercharges, and hence satisfy
[M\mu\nu,
I | |
Q | |
\alpha] |
=(\sigma\mu\nu
\beta | |
) | |
\alpha{} |
I | |
Q | |
\beta |
[P\mu,
I | |
Q | |
\alpha] |
=0
I | |
\{Q | |
\alpha, |
\bar
J | |||
Q | |||
|
=
\mu | |||
2\sigma | |||
|
IJ | |
P | |
\mu\delta |
I | |
\{Q | |
\alpha, |
J | |
Q | |
\beta\} |
=\epsilon\alpha\betaZIJ
\{\bar
I | |||
Q | |||
|
\bar
J | |||
Q | |||
|
=
\epsilon | |||||
|
Z\dagger
ZIJ=-ZJI
Just as the Poincaré algebra generates the Poincaré group of isometries of Minkowski space, the super-Poincaré algebra, an example of a Lie super-algebra, generates what is known as a supergroup. This can be used to define superspace with
l{N}
l{N}
Just as
P\mu
I | |
Q | |
\alpha, |
\bar
I | |||
Q | |||
|
I=1, … ,l{N}
I | |
\theta | |
\alpha, |
| |||
\bar\theta |
I | |
Q | |
\alpha |
I | |
\theta | |
\alpha. |
4l{N}
The superspace consisting of Minkowski space with
l{N}
R1,3|4l{N
R4|4l{N
In Minkowski spacetime, the Haag–Łopuszański–Sohnius theorem states that the SUSY algebra with N spinor generators is as follows.
The even part of the star Lie superalgebra is the direct sum of the Poincaré algebra and a reductive Lie algebra B (such that its self-adjoint part is the tangent space of a real compact Lie group). The odd part of the algebra would be
\left( | 1 |
2 |
,0\right) ⊗ V ⊕ \left(0,
1 | |
2 |
\right) ⊗ V*
(1/2,0)
(0,1/2)
\overline{2} ⊕ 1
1 ⊕ 2
\left[\left( | 1 |
2 |
,0\right) ⊗ V\right] ⊗ \left[\left(0,
1 | |
2 |
\right) ⊗ V*\right]
\left( | 1 | ,0\right) ⊗ \left(0, |
2 |
1 | |
2 |
\right)
V ⊗ V*
\left[\left( | 1 |
2 |
,0\right) ⊗ V\right] ⊗ \left[\left(
1 | |
2 |
,0\right) ⊗ V\right]
\left( | 1 | ,0\right) ⊗ \left( |
2 |
1 | |
2 |
,0\right)
N2
B is now
ak{u}(1)
ak{u}(1)
Actually, there are two versions of N=1 SUSY, one without the
ak{u}(1)
ak{u}(1)
B is now
ak{su}(2) ⊕ ak{u}(1)
ak{su}(2)
ak{u}(1)
ak{u}(1)
Alternatively, V could be a 2D doublet with a nonzero
ak{u}(1)
Yet another possibility would be to let B be
ak{u}(1)A ⊕ ak{u}(1)B ⊕ ak{u}(1)C
ak{u}(1)B
ak{u}(1)C
ak{u}(1)A
ak{u}(1)B
ak{u}(1)C
Or we could have B being
ak{su}(2) ⊕ ak{u}(1)A ⊕ ak{u}(1)B
ak{su}(2)
ak{u}(1)
ak{u}(1)A
ak{u}(1)B
This doesn't even exhaust all the possibilities. We see that there is more than one N = 2 supersymmetry; likewise, the SUSYs for N > 2 are also not unique (in fact, it only gets worse).
It is theoretically allowed, but the multiplet structure becomes automatically the same withthat of an N=4 supersymmetric theory. So it is less often discussed compared to N=1,2,4 version.
This is the maximal number of supersymmetries in a theory without gravity.
This is the maximal number of supersymmetries in any supersymmetric theory. Beyond
l{N}=8
λ
|λ|>2
In 0 + 1, 2 + 1, 3 + 1, 4 + 1, 6 + 1, 7 + 1, 8 + 1, and 10 + 1 dimensions, a SUSY algebra is classified by a positive integer N.
In 1 + 1, 5 + 1 and 9 + 1 dimensions, a SUSY algebra is classified by two nonnegative integers (M, N), at least one of which is nonzero. M represents the number of left-handed SUSYs and N represents the number of right-handed SUSYs.
The reason of this has to do with the reality conditions of the spinors.
Hereafter d = 9 means d = 8 + 1 in Minkowski signature, etc. The structure of supersymmetry algebra is mainly determined by the number of the fermionic generators, that is the number N times the real dimension of the spinor in d dimensions. It is because one can obtain a supersymmetry algebra of lower dimension easily from that of higher dimensionality by the use of dimensional reduction.
The maximum allowed dimension of theories with supersymmetry is
d=11=10+1
d=10=9+1
The only example is the N = 1 supersymmetry with 32 supercharges.
From d = 11, N = 1 SUSY, one obtains N = (1, 1) nonchiral SUSY algebra, which is also called the type IIA supersymmetry. There is also N = (2, 0) SUSY algebra, which is called the type IIB supersymmetry. Both of them have 32 supercharges.
N = (1, 0) SUSY algebra with 16 supercharges is the minimal susy algebra in 10 dimensions. It is also called the type I supersymmetry. Type IIA / IIB / I superstring theory has the SUSY algebra of the corresponding name. The supersymmetry algebra for the heterotic superstrings is that of type I.
. Steven Weinberg. Supersymmetry. 2000. 1st. The Quantum Theory of Fields. 3. Cambridge University Press. Cambridge. 978-0521670555.