Spacetime structure of massive majorana particles and massive gravitinos
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The profound difference between Dirac and Majorana particles is traced back to the possibility of having physically different constructs in the (1/2, 0) ⊕ (0, 1/2) representation space. Contrary to Dirac particles, Majorana-particle propagators are shown to differ from the simple linear γμ pμ structure. Furthermore, neither Majorana particles, nor their antiparticles can be associated with a well defined arrow of time. The inevitable consequence of this peculiarity is the particle-antiparticle metamorphosis giving rise to neutrinoless double beta decay, on the one side, and enabeling spin-1/2 fields to act as gauge fields, gauginos, on the other side. The second part of the lecture notes is devoted to massive gravitino. We argue that a spin measurement in the rest frame for an unpolarized ensemble of massive gravitinos, associated with the spinor-vector [(1/2, 0) ⊕ (0, 1/2)] ⊗ (1/2, 1/2) representation space, would yield the results 3/2- with probability one half, and 1/2 with probability one half. The latter is distributed uniformly, i.e. as 1/4, among the two spin-1/2%2b and spin-1/2- states of opposite parities. From that we draw the conclusion that the massive gravitino should be interpreted as a particle of multiple spin.