arXiv · hep-th/9704039
Effective gravity and OSp(N,4) invariant matter
Abstract
We re-examine the OSp(N,4) invariant interacting model of massless chiral and gauge superfields, whose superconformal invariance was instrumental, both in proving the all-order no-renormalization of the mass and chiral self-interaction lagrangians, and in determining the linear superfield renormalization needed. We show that the renormalization of the gravitational action modifies only the cosmological term, without affecting higher-order tensors. This could explain why the effect of the cosmological constant is shadowed by the effects of newtonian gravity.
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S. Bellucci. 1997-10-31. Effective gravity and OSp(N,4) invariant matter. https://doi.org/10.1103/physrevd.57.1057
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