Freeze-in Dark Matter Perturbations are Adiabatic
arXiv:2211.08719 · doi:10.1088/1475-7516/2023/01/020
Abstract
We show that the large-scale perturbations in the dark matter generated by the freeze-in mechanism are only of adiabatic nature. The freeze-in mechanism is not at odds with the current stringent constraints on isocurvature perturbations.
arXiv comment8 pages
References in corpus (13)
- Planck 2018 results. X. Constraints on inflation
- Particle Physics Models of Inflation and the Cosmological Density Perturbation
- Freeze-In Production of FIMP Dark Matter
- A new approach to the evolution of cosmological perturbations on large scales
- The primordial density perturbation in the curvaton scenario
- The Dawn of FIMP Dark Matter: A Review of Models and Constraints
- Thermally Generated Gauge Singlet Scalars as Self-Interacting Dark Matter
- Large-scale curvature and entropy perturbations for multiple interacting fluids
- Evolution of Second-Order Cosmological Perturbations and Non-Gaussianity
- Evolution of Cosmological Perturbations during Reheating
- Can Non-Adiabatic Perturbations Arise After Single-Field Inflation?
- Large-scale curvature perturbations with spatial and time variations of the inflaton decay rate
- Non-Gaussianity of Large-Scale Cosmic Microwave Background Anisotropies beyond Perturbation Theory
Cited by in corpus (6)
- Dark Matter production during Warm Inflation via Freeze-In
- Impact of freeze-in on dark matter isocurvature
- Regular Black Hole Cores via Gravitational Evanescence of Collapsing Matter
- Dark Matter Isocurvature from Curvature
- Scale invariant curvature perturbations from a spontaneously decaying scalar field
- Leptogenesis with perturbations in type-II and type-III seesaw models