Research news on Baryonic dark matter

Baryonic dark matter as a research area investigates the fraction of non-luminous matter composed of standard-model baryons—primarily protons, neutrons, and their bound states—that contributes to galactic and cosmological mass budgets. It focuses on identifying and constraining compact and diffuse baryonic components such as MACHOs, cold gas, dust, and low-luminosity stellar remnants using techniques including microlensing surveys, 21-cm observations, and cosmic microwave background baryon-density constraints. The field assesses how much of the observed gravitational effects can be attributed to baryons versus non-baryonic dark matter, refining models of structure formation, baryon cycling, and the baryon census in the universe.

Observing dark matter at cosmic dawn

After almost a century of speculation, proposals and searches for dark matter, physicists now know that it currently comprises about 27% of the universe's mass-energy, with an abundance over five times that of ordinary matter ...