Reviving the Affleck-Dine Curvaton Scenario with Compensated Isocurvature Perturbations
Masahiro Kawasaki, Shunsuke Neda
astro-ph.CO, hep-ph
Submitted: 2026-07-23
Comments: 17 pages, 4 figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Baryogenesis from Flat Directions of the Supersymmetric Standard Model
- Effects of Cosmological Moduli Fields on Cosmic Microwave Background
- Adiabatic CMB perturbations in pre-big bang string cosmology
- Generating the curvature perturbation without an inflaton
- Curvatons in Supersymmetric Models
- Planck 2018 results. X. Constraints on inflation
- Unified Origin of Curvature Perturbation and Baryon Asymmetry of the Universe
- On Possible Variation in the Cosmological Baryon Fraction
- Forecasted 21 cm constraints on compensated isocurvature perturbations
- Compensated Isocurvature Perturbations and the Cosmic Microwave Background
- Baryons do trace dark matter 380,000 years after the big bang: Search for compensated isocurvature perturbations with WMAP 9-year data
- CDM/baryon isocurvature perturbations in a sneutrino curvaton model
- New physics in a nutshell, or Q-ball as a power plant
- Q-Balls and Baryogenesis in the MSSM
- Q-ball Formation through Affleck-Dine Mechanism
- Delta-N Formalism for Curvaton with Modulated Decay
- Numerical study of Q-ball formation in gravity mediation
- Charge distribution of the gauge-mediation type Q ball
- Revisiting Big-Bang Nucleosynthesis Constraints on Long-Lived Decaying Particles
- Planck 2018 results. IX. Constraints on primordial non-Gaussianity
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