Cosmic rays as a feedback agent in primordial galactic ecosystems
Ellis R. Owen

TL;DR
This paper explores how cosmic rays may serve as a feedback mechanism influencing star formation and evolution in early, isolated galaxies, potentially shaping their development over cosmic time.
Contribution
It proposes cosmic rays as a key intrinsic feedback agent in primordial galaxies and outlines a framework for detecting their signatures across the electromagnetic spectrum.
Findings
Cosmic rays could regulate star formation in early galaxies.
Multi-wavelength data can reveal cosmic ray feedback signatures.
A distance ladder approach can map cosmic ray influence over time.
Abstract
High-redshift primordial galaxies have recently been found with evolved stellar populations and complex star-formation histories reaching back to 250 Myr after the Big Bang. Their intense bursts of star-formation appear to be interspersed with sustained periods of strong quenching, however the processes underlying this evolutionary behaviour remain unclear. Unlike later epochs, galaxies in the early Universe are not located in large associations like clusters. Instead, they co-evolve with their developing circumgalactic halo as relatively isolated ecosystems. Thus, the mechanisms that could bring about the downfall of their star-formation are presumably intrinsic, and feedback processes associated with their intense starburst episodes likely play an important role. Cosmic rays are a viable agent to deliver this feedback, and could account for the star-formation histories inferred for…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Galaxies: Formation, Evolution, Phenomena · Astrophysics and Star Formation Studies
