The fate of Quasi-Exponential inflation in the light of ACT-DR6
Barun Kumar Pal

TL;DR
This paper revisits the quasi-exponential inflation model, demonstrating its compatibility with recent CMB data and forecasting its detectability prospects with upcoming missions, while also highlighting potential falsification if primordial gravitational waves are not observed.
Contribution
It provides a comprehensive analysis of the quasi-exponential inflation model against latest observational data and forecasts its future testability with upcoming CMB experiments.
Findings
Model fits Planck and ACT-DR6 data well.
Primordial gravitational waves within current bounds.
Future missions could detect or rule out the model.
Abstract
We have revisited quasi-exponential model of inflation in the light of recent ACT-DR6 and Planck data along with latest constraint on the amplitude of primordial gravitational waves. For our analysis we have followed Mukhanov approach for inflationary equation-of-state employing Hamilton-Jacobi formulation. We find that the model is capable of mimicking latest Planck results by providing excellent fit to scalar spectral index and its running. Not only that, amount of primordial gravitational waves is also within the present observational bound, . In addition to that, when the combination of ACT-DR6 and Planck joint with BICEP/Keck 2018 data is taken into account inflationary predictions from quasi-exponential model are in excellent agreement. The model also yields sublime fit to the result of joint analysis of ACT-DR6, Planck joint with BICEP/Keck 2018 and DESI-Y1 data. The…
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Taxonomy
TopicsCosmology and Gravitation Theories · Geophysics and Gravity Measurements · Stochastic processes and financial applications
