Linking Electron Density with Elevated Star Formation Activity from $z=0$ to $z=10$
Sijia Li, Si-Yue Yu, Luis C. Ho, John D. Silverman, Jing Wang, Amelie Saintonge, Niankun Yu, Qinyue Fei, Daichi Kashino, and Hao-ran Yu

TL;DR
This study links higher electron densities in high-redshift galaxies to increased star formation activity, revealing a consistent relation across cosmic time that reflects evolving cold gas densities and feedback processes.
Contribution
It establishes a quantitative relation between electron density and star formation rate surface density applicable from local to high-redshift galaxies.
Findings
Electron density correlates with star formation rate surface density.
The relation follows a broken power law with a constant low-density regime.
Redshift evolution of electron density matches predictions from star formation activity.
Abstract
The interstellar medium (ISM) in high-redshift galaxies exhibits significantly higher electron densities () than in the local universe. To investigate the origin of this trend, we analyze a sample of 9590 centrally star-forming galaxies with stellar masses greater than at redshifts , selected from the Dark Energy Spectroscopic Instrument (DESI) Data Release 1. We derive electron densities from the [S II] doublet, measuring values of - at . We find a tight correlation between and the star formation rate surface density (), which is well described by a broken power law. Above a threshold of , the relation follows .…
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