haushofer said:
I'm also used to that last interpretation in the context of supergravity,
Where in supergravity do you find such bi-spinor interpretation?
e.g. in the susy-transfo of vielbeine.
Under local supersymmetry, the frame field transforms as
[tex]\delta_{\epsilon}e_{\mu}{}^{a} = \frac{1}{2}\left( \epsilon^{\beta} \ (\sigma^{a})_{\beta \dot{\alpha}} \ \bar{\psi}_{\mu}^{\dot{\alpha}} + \bar{\epsilon}_{\dot{\beta}} \ (\bar{\sigma}^{a})^{\alpha \dot{\beta}} \ \psi_{\alpha \mu} \right) ,[/tex] where [itex]\psi_{\alpha \mu} \in (\frac{1}{2} , 1)[/itex] and [itex]\bar{\psi}_{\mu}^{\dot{\alpha}} \in (1 , \frac{1}{2})[/itex], are Weyl
spinor-vectors, i.e., Lorentz vectors taking values in the 2-dimenstional spin space [itex]\mathbb{C}^{2}[/itex]. Introducing the Majorana
bispinor-vector (the superpartner of the gravitational field or the gravitino field) [tex]\Psi_{\mu} = \begin{pmatrix} \psi_{\mu \alpha} \\ \bar{\psi}^{\dot{\alpha}}_{\mu} \end{pmatrix} \in \left(\frac{1}{2} , 1 \right) \oplus \left(1 , \frac{1}{2} \right) ,[/tex] the Majorana
bispinor [itex]\bar{\Upsilon} = \left( \epsilon^{\beta} , \bar{\epsilon}_{\dot{\beta}}\right)[/itex], and the [itex]4 \times 4[/itex] Dirac matrices [tex]\gamma^{a} = \begin{pmatrix} 0 & (\sigma^{a})_{\beta \dot{\alpha}} \\ (\bar{\sigma}^{a})^{\dot{\beta}\alpha} & 0 \end{pmatrix} ,[/tex] we can write [tex]\delta_{\epsilon}e_{\mu}{}^{a} = \frac{1}{2} \bar{\Upsilon} \gamma^{a} \Psi_{\mu} .[/tex] The frame field can be used to convert the world index ([itex]\mu[/itex]) on the gravitinos field to a tangent-space index ([itex]a[/itex]): [itex]\psi_{\alpha}^{a} = e_{\mu}{}^{a} \psi_{\alpha}^{\mu}[/itex], and the local Lorentz index can be converted into a pair of spinor indices: [itex]\psi_{\alpha}{}^{\dot{\beta} \beta} = (\bar{\sigma}^{a})^{\dot{\beta}\beta} \psi_{\alpha}^{a}[/itex]. Thus, the gravitino can be described by a Majorana
bispinor-vector field [itex]\Psi_{\mu}(x)[/itex] or, equivalently, by a pair of (mixed) rank-
3 spin tensor fields.