The Ultra Slow-Roll Phase Of Warm Inflation In Braneworld Cosmology
Aarav Shah

TL;DR
This paper investigates the Ultra Slow Roll phase of warm inflation within braneworld cosmologies, analyzing how brane effects influence inflationary dynamics and primordial perturbations, with a focus on Randall-Sundrum and DGP models.
Contribution
It introduces a detailed study of USR in warm inflation on braneworld backgrounds, highlighting the suppression of brane effects during USR phases.
Findings
Brane contributions diminish during USR, approaching standard inflation.
Numerical results show the evolution of the primordial power spectrum.
The study extends inflationary models to include braneworld effects in USR.
Abstract
Slow-roll of the inflaton (inflationary field) defines the standard dynamics of the inflationary epoch. However, the inflaton deviates from slow-roll when it encounters an extremely flat region in the inflationary potential, and enters a phase dubbed Ultra Slow Roll (USR). In previous studies, there have been various theories which modify the theory of general relativity, all of them having different motivations based on different paradigms. Among these, braneworld gravity, motivated from string theory; is one of the most prominent theories as it provides a geometrical explanation for the weakness of gravity. In this article, we explore two possible braneworld background theories, the Randall-Sundrum (RS-II) model and the Dvali-Gabadadze-Porratai (DGP) model, and then realize an USR phase in a particularly interesting inflationary scenario, called warm inflation. In the warm…
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