No slow-roll inflation \`a la Generalized Chaplygin Gas in General Relativity
Alexander Gallego Cadavid, J.R. Villanueva

TL;DR
The paper demonstrates that the Generalized Chaplygin Gas model cannot sustain slow-roll inflation within General Relativity and is incompatible with Planck 2018 data, effectively ruling out its viability for early universe inflation.
Contribution
It shows that GCG and GCJG models cannot produce sustained slow-roll inflation in GR and are inconsistent with observational constraints, clarifying their limitations in cosmological inflation.
Findings
Most GCG parameter space does not support slow-roll inflation.
The model predicts accelerated contraction for certain parameters.
Planck 2018 data rules out the GCG inflation scenario.
Abstract
The Generalized Chaplygin Gas (GCG) model is characterized by the equation of state , where and . The model has been extensively studied due to its interesting properties and applicability in several contexts, from late-time acceleration to primordial inflation. Nonetheless we show that the inflationary slow-roll regime cannot be satisfied by most of the parameter space of the GCG model when General Relativity (GR) is considered. In particular, although the model has been applied to inflation with , we show that for there is no expansion of the Universe but an accelerated contraction. For , the second slow-roll parameter is larger than unity, so there is no sustained period of inflation. Only for very close to -1 the model produces enough -folds, thus greatly reducing its…
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