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Supersymmetrizing Massive Gravity · Around

2013

Supersymmetrizing Massive Gravity

Malaeb, Ola

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When four scalar fields with global Lorentz symmetry are coupled to gravity and take a vacuum expectation value breaking diffeomorphism invariance spontaneously, the graviton becomes massive.

This model is supersymmetrized by considering four N=1 chiral superfields with global Lorentz symmetry.
When the scalar components of the chiral multiplets z^A acquire a vacuum expectation value, both diffeomorphism invariance and local supersymmetry are broken spontaneously.
The global Lorentz index A becomes identified with the space-time Lorentz index making the scalar fields z^A vectors and the chiral spinors psi^A spin-3/2 Rarita-Schwinger fields.

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1939
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