Scientists Map Earliest Glow Of Hydrogen, Opening A New Window To The Universe
CHIME telescope, with Indian collaboration, detects earliest hydrogen glow from 5-billion-year-old universe, revolutionizing cosmic expansion and dark energy studies.
The Canadian Hydrogen Intensity Mapping Experiment (CHIME) telescope made the first standalone detection of hydrogen glow from the early universe.
This glow originates from when the universe was approximately five billion years old.
The detection paves the way for new studies of cosmic expansion and Dark Energy.
Raman Research Institute (RRI), an autonomous institute under the Department of Science and Technology (DST), is a key Indian collaborator in this project.
The findings were published in The Astrophysical Journal.
Detailed Insights:
The CHIME telescope is an interferometric radio telescope specifically built to map the distribution of hydrogen gas in the early universe.
This new technique offers a faster and less expensive method for scientists to study Dark Energy compared to traditional galaxy surveys.
Hydrogen, being the most common element, emits faint radio signals that act as a cosmic tracer, revealing how matter is distributed.
The observed signal indicates that roughly two percent of the hydrogen in the universe was in neutral atomic form at that cosmic age.
Researchers plan to expand the analysis to include earlier periods, aiming to study the universe when it was only three billion years old.
Scientific/Technical Concepts Involved:
CHIME Telescope: Canadian Hydrogen Intensity Mapping Experiment, an interferometric radio telescope designed to map early universe hydrogen.
Dark Energy: A mysterious force hypothesized to be responsible for the accelerating expansion of the universe.
Hydrogen Glow: Faint radio emission from neutral atomic hydrogen, used as a tracer for matter distribution in the cosmos.