Astronomers have found the missing normal matter in the universe, revealing it as diffuse ionized hydrogen gas surrounding galaxies beyond previous observations.
This discovery sheds light on galaxy evolution, black hole activity, and gas distribution, potentially resolving conflicts in cosmology.
The elusive material called warm-hot intergalactic medium (WHIM) was detected using the kinematic Sunyaev-Zel'dovich effect on the cosmic microwave background.
Ionized gas halos around galaxies suggest supermassive black holes are more active throughout their lifetimes, affecting galaxy formation.
The findings challenge existing cosmological models and emphasize the need for more accurate simulations to incorporate the extensive gas halos.
Gas distribution measurements can help address cosmological tensions and improve our understanding of galaxy formation, evolution, and cosmic filaments.
Future large-scale surveys by observatories like the Vera Rubin Observatory and Nancy Grace Roman Space Telescope will build on these discoveries.
The research highlights the potential of the kinematic Sunyaev-Zel'dovich effect in studying cosmic structures and advancing our knowledge of the universe.
By mapping gas distribution around millions of galaxies, astronomers aim to uncover hidden cosmic structures and unravel long-standing astronomical mysteries.
These breakthroughs could reshape our understanding of the universe by providing new insights into its large-scale structure.
The study was published online in the journal Physical Review Letters, offering a significant contribution to the field of astronomy and cosmology.