Epstein Secrets

ett. 69, 1849 (1992) [arXiv:hep-th/9204099]. [4] W. A. Bardeen, I. Bars, A. J. Hanson and R. D. Pecce

nce of the action. In the massless 6D case the spin-shell constraint functions are 6D analogs of 4D helicity; in the massive 4D case, the quadratic Casimir of the SU(2) gauge group, which is the sum of squares of the constraint functions, is proportional to the square of the Pauli-Lubanski spin-vector.

731, Phys.Rev.D80:084017,2009. [5] R. Schtzhold, W. G. Unruh, Large-scale non-locality in "doubly spe

nlike what we have assumed above, the commutator of t with k, is non- zero. The dynamics is defined by a Hamiltonian constraint constructed from the Casimir of the tt- Poincare algebra. This is the invariant length on the curved momentum space, which is invariant under an 5O(1, 3) subgroup of the deSitte

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