Gravitational Waves From No-Scale Supergravity

Abstract

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 Kähler 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. We evaluate numerically the scalar power spectrum and the stochastic background of the Gravitational Waves, satisfying the observational Planck cosmological constraints for inflation.

33 pages, 8 figures, Version to appear in European Physical Journal C

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Cited by in corpus (3)

• Exploring Critical Overdensity Thresholds in Inflationary Models of Primordial Black Holes Formation
• Mechanisms for producing Primordial Black Holes from Inflationary Models Beyond Fine-Tuning
• Large curvature fluctuations from no-scale supergravity with a spectator field