Effective lagrangian for a mass dimension one fermionic field in curved spacetime
arXiv:1709.08707 · doi:10.1007/JHEP02(2018)145
Abstract
In this work we use momentum-space techniques to evaluate the propagator for a spin mass dimension one spinor field on a curved Friedmann-Robertson-Walker spacetime. As a consequence, we built the one-loop correction to the effective lagrangian in the coincidence limit. Going further we compute the effective lagrangian in the finite temperature regime. We arrive at interesting cosmological consequences, as time-dependent cosmological `constant', fully explaining the functional form of previous cosmological models.
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