Initial episodes of the chemical evolution of the intergalactic medium

Yu.A. Shchekinov^†^a, b, E.O. Vasiliev^‡^a, c, B.M. Shustov^§^c
^aLebedev Physical Institute, Russian Academy of Sciences, Leninsky prosp. 53, Moscow, 119991, Russian Federation
^bRaman Research Institute, C. V. Raman Avenue, Sadashiva Nagar, Bangalore, 560080, India
^cInstitute of Astronomy, Russian Academy of Sciences, ul. Pyatnitskaya 48, Moscow, 119017, Russian Federation

The current state of the problem of the origin and transport of 'heavy' (A>4) chemical elements in the Universe is discussed. The beginning of stellar nucleosynthesis (SNS) dates apparently to z≳ 20 redshift epochs (age of the Universe t_U ≲ 180 Myr). Presently, SNS traces are observed in some cases in galaxies at redshift z ∼ 10—15 (t_U∼ 500—270 Myr). A massive redistribution of chemical elements from galaxies over the entire Universe became possible, primarily under the action of powerful explosions, in the reionization period at z≲ 6 (t_U≳ 940 Myr). A correct interpretation of observational data requires an in-depth understanding of the transport and mixing dynamics of chemical elements in the Universe. Theoretical models predict their extremely nonuniform distribution in a range from the interstellar medium on spatial scales of a few hundred light years to the intergalactic medium spanning tens of millions of light years. This is observed in absorption spectra of quasars up to redshift z∼ 6 and results in observational selection. The review focuses on the early stages of the history of the Universe's chemical enrichment as it is currently understood given the observational selection effects. Observational data and theoretical ideas underlying the modern understanding of the complex process of the Universe's chemical evolution are outlined.

Keywords: Universe, intergalactic medium, galaxies, interstellar medium, chemical elements, transport
PACS: 26.30.−k, 95.30.Lz, 98.38.−j, 98.58.−w, 98.62.Ra (all)
DOI: 10.3367/UFNe.2022.12.039295
URL: https://ufn.ru/en/articles/2023/11/a/
Scopus

2-s2.0-85182909921
ADS NASA

2023PhyU...66.1071S
Citation: Shchekinov Yu A, Vasiliev E O, Shustov B M "Initial episodes of the chemical evolution of the intergalactic medium" Phys. Usp. 66 1071–1094 (2023)

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Received: 26th, September 2022, revised: 6th, December 2022, accepted: 13th, December 2022

Оригинал: Щекинов Ю А, Васильев Е О, Шустов Б М «Начальные эпизоды химической эволюции межгалактической среды» УФН 193 1137–1161 (2023); DOI: 10.3367/UFNr.2022.12.039295