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) 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. We evaluate numerically the scalar power spectrum and the stochastic background of the Gravitational Waves, satisfying the observational Planck cosmological constraints for inflation.
Cite
@article{arxiv.2205.05595,
title = {Gravitational Waves From No-Scale Supergravity},
author = {Vassilis C. Spanos and Ioanna D. Stamou},
journal= {arXiv preprint arXiv:2205.05595},
year = {2023}
}
Comments
33 pages, 8 figures, Version to appear in European Physical Journal C