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Notes
- 1.
There are two solutions of the first equation in (4.137), but since the point \({\mathscr {O}}\) for which \(p_4 =1\) must belong to the relevant solution we choose \(p_4\) positive.
- 2.
We also assume that the differential \( d\hat{x}_{4} \) is \( \kappa \)-Poincaré invariant \( \mathsf {p}_{\kappa }\triangleright d\hat{x}_{4}=0 \), where \( \mathsf {p}_{\kappa } \) is a generic element of the \( \kappa \)-Poincaré algebra.
- 3.
Here we have used the fact that the hermitian conjugate of a plane wave involves the antipode map S(k) on its momentum \( \hat{e}_{k}^{\dagger }=\hat{e}_{S(k)} \).
- 4.
It is a left invariant measure \( d\mu (lk)=d\mu (k) \), and it is worth noticing that in bicrossproduct coordinates it is just the diffeomorphism invariant measure on \(dS_{4}\) corresponding to the cosmological metric \( -dk_{0}^{2}+e^{2k_{0}/\kappa }dk_{i}^{2} \).
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Arzano, M., Kowalski-Glikman, J. (2021). Classical Fields, Symmetries, and Conserved Charges. In: Deformations of Spacetime Symmetries. Lecture Notes in Physics, vol 986. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-662-63097-6_6
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