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First Detection of a 9-Billion-Year-Old Radio Signal from Neutral Hydrogen by Astronomers

Weak radio signal of neutral hydrogen in space
Вчені вперше виявили радіосигнал віком 9 мільярдів років, що походить від нейтрального водню. Photo: НВ — Техно

Breakthrough in Capturing Ancient Radio Waves from Neutral Hydrogen

According to НВ — Техно: Using the Canadian CHIME radio telescope, astronomers have successfully detected an extremely faint radio emission originating from neutral hydrogen dating back approximately 9 billion years. This landmark observation offers a new window into understanding how matter is distributed across the cosmos and sheds light on the enigmatic nature of dark energy. As the most abundant element in the universe and the primary fuel for star formation, hydrogen plays a crucial role in cosmic evolution studies.

Innovative Observation Techniques

The CHIME telescope’s capability to directly measure the combined hydrogen emission over vast regions of space at a relatively low cost was key to this achievement. The radio waves captured traveled across 9 billion years, and analysis revealed that about 2% of hydrogen during this epoch existed in a neutral atomic state.

The findings are based on data collected over 94 nights in 2019, with the research team possessing nearly seven years of continuous observations. To isolate this subtle signal from background noise, novel mathematical data processing techniques were developed. Successfully applying these methods not only marks a significant technical milestone but also paves the way for testing fundamental physics theories and gaining insights into galaxy formation and evolution.

Future plans include adapting this approach to investigate earlier cosmic periods when the universe was around 3 billion years old. Neutral hydrogen’s radio emissions serve as a cosmic beacon for mapping the large-scale structure of the universe, making this discovery a vital contribution to modern astronomy.

Detecting this 9-billion-year-old neutral hydrogen radio signal represents a major advance in astronomy, enhancing our understanding of galaxy evolution and the universe’s structure.

The introduction of these advanced data analysis methods highlights an innovative direction in astrophysical research, potentially accelerating breakthroughs in the study of dark matter and dark energy.

This groundbreaking detection highlights the innovative capabilities of the CHIME telescope, which has previously captured faint hydrogen emissions from the depths of space. Such advancements not only enhance our understanding of the universe but also open new avenues for future astronomical research.

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