Sub-GeV dark matter that interacts hadronically is ruled out for nucleon scattering cross sections above 10^{-36} cm² across the keV to 100 MeV mass range by combined cosmological and particle-decay constraints.
author Mondol, R
3 Pith papers cite this work. Polarity classification is still indexing.
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SARAS3 data sets T21 ≳ -277.6 mK at z=23.6 (3σ) in IDM models and finds no preference for IDM over CDM (Bayes factor ≈1.7).
Bayesian joint constraints show that elevated star formation efficiency accounts for JWST high-z galaxy excess in flat Lambda CDM, without requiring deviations in dark energy equation of state or curvature.
citing papers explorer
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Irreducible Constraints on Hadronically Interacting Sub-GeV Dark Matter
Sub-GeV dark matter that interacts hadronically is ruled out for nucleon scattering cross sections above 10^{-36} cm² across the keV to 100 MeV mass range by combined cosmological and particle-decay constraints.
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Implications of \textit{SARAS3} data for Coulomb-like interacting dark matter
SARAS3 data sets T21 ≳ -277.6 mK at z=23.6 (3σ) in IDM models and finds no preference for IDM over CDM (Bayes factor ≈1.7).
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Dark energy, spatial curvature, and star formation efficiency from JWST photometric and spectroscopic high-redshift galaxies
Bayesian joint constraints show that elevated star formation efficiency accounts for JWST high-z galaxy excess in flat Lambda CDM, without requiring deviations in dark energy equation of state or curvature.