2025/01/03 by Daniel J. Whalen, Whalen, Daniel J., Muhammad A. Latif +3 · 3 voices
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics of Galaxies (astro-ph.GA) #FOS: Physical sciences #Gamma-ray bursts and supernovae #Solar and Space Plasma Dynamics #astro-ph.GA
paper · pdf · doi:10.48550/arxiv.2501.02051
openalex publication_date 2025/01/03 · arxiv published 2025/01/03 · arxiv updated 2025/01/09 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Primordial (or Pop III) supernovae were the first nucleosynthetic engines in the Universe, forging the heavy elements required for the later formation of planets and life. Water, in particular, is thought to be crucial to the cosmic origins of life as we understand it, and recent models have shown that water can form in low-metallicity gas like that present at high redshifts. Here we present numerical simulations that show that the first water in the Universe formed in Pop III core-collapse and pair-instability supernovae at redshifts z ∼ 20. The primary sites of water production in these remnants are dense molecular cloud cores, which in some cases were enriched with primordial water to mass fractions that were only a factor of a few below those in the Solar System today. These dense, dusty cores are also likely candidates for protoplanetary disk formation. Besides revealing that a primary ingredient for life was already in place in the Universe 100 - 200 Myr after the Big Bang, our simulations show that water was likely a key constituent of the first galaxies.