Superhorizon Isocurvature as a Window into Dark Matter Production
hep-ph, astro-ph.CO
Submitted: 2025-10-24
Updated: 2026-09-08
Comments: 22 pages, 9 figures. v2: Minor revisions: corrected typo, added limit to analytic calculation, expanded discussion. Results and conclusions unchanged
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Planck 2018 results. VI. Cosmological parameters
- Planck 2018 results. X. Constraints on inflation
- Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
- DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
- CMB spectral distortions from small-scale isocurvature fluctuations
- BBN constraints on dark radiation isocurvature
- One $\mu$ to rule them all: CMB spectral distortions can probe domain walls, cosmic strings and low scale phase transitions
- Isocurvature perturbations in extra radiation
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- General Constraints on Isocurvature from the CMB and Ly-$\alpha$ Forest
- Future constraints on neutrino isocurvature perturbations in the curvaton scenario
- Non-Gaussian isocurvature perturbations in dark radiation
- Free-streaming and Coupled Dark Radiation Isocurvature Perturbations: Constraints and Application to the Hubble Tension
- Dark Matter and Gravity Waves from a Dark Big Bang
- Finite Bubble Statistics Constrain Late Cosmological Phase Transitions
- Dark Radiation Isocurvature from Cosmological Phase Transitions
- Axion Cosmology
- Cosmology of axion dark matter
- Minimal solution to the axion isocurvature problem from a nonminimal coupling
- Gravitational waves from a universe filled with primordial black holes
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