2026-04-15 カリフォルニア大学リバーサイド校（UCR）
Header image shows an illustration of a supermassive black hole. Credit: blackdovfx/iStock/Getty Images Plus.
＜関連情報＞
- https://news.ucr.edu/articles/2026/04/15/dark-matter-could-explain-earliest-supermassive-black-holes
- https://iopscience.iop.org/article/10.1088/1475-7516/2026/04/034
崩壊する暗黒物質から生じる直接崩壊ブラックホール候補 Direct collapse black hole candidates from decaying dark matter
Yash Aggarwal, James B. Dent, Philip Tanedo and Tao Xu
Journal of Cosmology and Astroparticle Physics Published: 14 April 2026
DOI:10.1088/1475-7516/2026/04/034
Abstract
Injecting 1–13.6 eV photons into the early universe can suppress the molecular hydrogen abundance and alter the star formation history dramatically enough to produce direct collapse black holes. These, in turn, could explain the recently observed population of puzzling high-redshift supermassive black holes that appear to require super-Eddington accretion. We show that axion dark matter decay in the intergalactic medium can account for this energy injection. We use a single zone model of the gas core and semi-analytically evolve its chemo-thermal properties to track the conditions for which the system becomes an atomic cooling halo — a necessary precursor for the production of heavy black hole seeds to explain the high-redshift black hole population. Windows of axion masses between 24.5–26.5 eV with photon couplings as low as 4 × 10-12 GeV-1 may realize this atomic cooling halo condition. We highlight the significance of the band structure of molecular hydrogen on the effectiveness of this process and discuss estimates of the heavy seed population and prospects for testing this model.
