Using SquiRels to Find LiMRs: A Model-Insensitive Approach to Cosmic Microwave Background Studies of Light but Massive Relics
Nicholas DePorzio, David Imig, Jessie Shelton
astro-ph.CO, hep-ph
Submitted: 2026-07-13
Comments: 19 pages, 11 figures
Code: https://github.com/ndeporzio/squirel
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Planck 2018 results. VI. Cosmological parameters
- Cosmological parameters derived from the final (PR4) Planck data release
- DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
- The Simons Observatory: Science goals and forecasts
- The Simons Observatory: Science Goals and Forecasts for the Enhanced Large Aperture Telescope
- Cosmology and Fundamental Physics with the Euclid Satellite
- Cosmology with the SPHEREX All-Sky Spectral Survey
- The LSST Dark Energy Science Collaboration (DESC) Science Requirements Document
- Cosmology with the Wide-Field Infrared Survey Telescope -- Multi-Probe Strategies
- Finding eV-scale Light Relics with Cosmological Observables
- New Light Species and the CMB
- Cosmological Probes of Light Relics
- The Physics of Light Relics
- Do observations prove that cosmological neutrinos are thermally distributed?
- Cosmological bounds on neutrino statistics
- How to relax the cosmological neutrino mass bound
- What can CMB observations tell us about the neutrino distribution function?
- Is it possible to tell the difference between fermionic and bosonic hot dark matter?
- Cosmological constraints on a light non-thermal sterile neutrino
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