New radio-burst method helps locate universe's missing ordinary matter
Stars and galaxies make up much of the universe's ordinary, observable matter. But for decades, scientists have wrestled with a cosmic conflict: There should be much more.
The warm-hot intergalactic medium (WHIM) research area investigates the diffuse, highly ionized baryonic component of the cosmic web at temperatures of roughly 10⁵–10⁷ K, believed to host a substantial fraction of the “missing” baryons at low redshift. This field combines cosmological simulations with multiwavelength observations, particularly soft X-ray and far-ultraviolet spectroscopy, to detect weak absorption or emission signatures from ions such as O VI, O VII, and O VIII in filaments between galaxies. Research focuses on WHIM thermodynamics, metal enrichment, shock-heating processes, and its role in structure formation, baryon cycling, and feedback from galaxies and active galactic nuclei.
Stars and galaxies make up much of the universe's ordinary, observable matter. But for decades, scientists have wrestled with a cosmic conflict: There should be much more.
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Much of the mass in the universe lies not in stars or galaxies, but in the space between them, known as the intergalactic medium. It is warm and even hot, and is called the "warm-hot intergalactic medium," or WHIM. It holds ...