The Stochastic Gravitational-Wave Background from Primordial Black Holes in R-Symmetric $SU(5)$ Inflation
Nadir Ijaz, Maria Mehmood, Mansoor Ur Rehman

TL;DR
This paper investigates how primordial black holes formed during R-symmetric $SU(5)$ inflation could account for dark matter and produce detectable gravitational waves, while also exploring implications for proton decay.
Contribution
It demonstrates a model where inflation leads to primordial black holes as dark matter and predicts observable gravitational waves and proton decay signals.
Findings
Primordial black holes can account for all dark matter.
Scalar induced gravitational waves are detectable with current/future detectors.
Inflationary parameters are consistent with Planck data and gauge unification.
Abstract
This study explores the realization of nonminimally coupled Higgs inflation in the context of no-scale supergravity, investigates the formation of primordial black holes, and examines the potential for observable proton decay within the framework of the R-symmetric model. For inflation, both single and multifield scenarios are investigated. The prediction of the single-field model for the tensor-to-scalar ratio, , is approximately , and the scalar spectral index falls within Plank's 1 range. The running of the scalar spectral index, , is approximately . A realistic scenario of reheating and non-thermal leptogenesis is employed with reheat temperature GeV. In the multifield case, we mainly focus on Primordial Black Holes (PBHs) and Gravitational Waves (GWs). In this inflationary framework, we demonstrate how a…
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Taxonomy
TopicsCosmology and Gravitation Theories · Particle physics theoretical and experimental studies · Black Holes and Theoretical Physics
