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Baryogenesis from the Inflaton Field

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it
abstract

In this letter we show that the inflaton can generate the cosmological baryon asymmetry. We take the inflaton to be a complex scalar field with a weakly broken global symmetry and develop a new variant on the Affleck-Dine mechanism. The inflationary phase is driven by a quadratic potential whose amplitude of B-modes is in agreement with BICEP2 data. We show that a conserved particle number is produced in the latter stage of inflation, which can later decay to baryons. We present promising embeddings in particle physics, including the use of high dimension operators for decay or using a colored inflaton. We also point out observational consequences, including a prediction of isocurvature fluctuations, whose amplitude is just below current limits, and a possible large scale dipole.

years

2025 1 2019 1

verdicts

UNVERDICTED 2

representative citing papers

Lectures on Reheating after Inflation

astro-ph.CO · 2019-07-09 · unverdicted · novelty 0.0

Lecture notes providing a generic introduction to reheating after inflation, covering its theoretical, phenomenological, and observational aspects.

citing papers explorer

Showing 2 of 2 citing papers.

  • Leptogenesis and neutrino mass with one right-handed neutrino and Higgs inflaton hep-ph · 2025-08-13 · unverdicted · none · ref 42 · internal anchor

    Minimal setup with one RHN and Higgs inflaton generates neutrino masses, baryon asymmetry via Affleck-Dine leptogenesis, and matches PLANCK/ACT inflation data with a small parameter space.

  • Lectures on Reheating after Inflation astro-ph.CO · 2019-07-09 · unverdicted · none · ref 38 · internal anchor

    Lecture notes providing a generic introduction to reheating after inflation, covering its theoretical, phenomenological, and observational aspects.