Gravitational Waves From No-Scale Supergravity

Understand

In this paper we study four concrete models, based on no-scale supergravity with SU(2,1)/SU(2)$\times$ U(1) symmetry.

• We modify either the K\"ahler potential or the superpotential, which are related to the no-scale theory with this symmetry.
• In this scenario, the induced Gravitational Waves, are calculated to be detectable by the future space-based observations such as LISA, BBO and DECIGO.
• The models under study are interrelated, as they all yield the Starobinsky effective-like scalar potential in the unmodified case.