Preferential Occurrence of Fast Radio Bursts in Massive Star-Forming Galaxies

TL;DR

This study reveals that Fast Radio Bursts predominantly occur in massive, metal-rich star-forming galaxies, indicating a bias towards environments that favor magnetar formation through stellar mergers, which advances understanding of their progenitors.

Contribution

It provides the first detailed analysis of FRB host galaxy properties, showing a bias towards massive galaxies and proposing a link to magnetar formation via stellar mergers.

Findings

FRBs are biased towards massive star-forming galaxies.

Metal-rich environments may promote magnetar formation.

FRB hosts show a deficit of low-mass galaxies.

Abstract

Fast Radio Bursts (FRBs) are millisecond-duration events detected from beyond the Milky Way. FRB emission characteristics favor highly magnetized neutron stars, or magnetars, as the sources, as evidenced by FRB-like bursts from a galactic magnetar, and the star-forming nature of FRB host galaxies. However, the processes that produce FRB sources remain unknown. Although galactic magnetars are often linked to core-collapse supernovae (CCSNe), it's uncertain what determines which supernovae result in magnetars. The galactic environments of FRB sources can be harnessed to probe their progenitors. Here, we present the stellar population properties of 30 FRB host galaxies discovered by the Deep Synoptic Array. Our analysis shows a significant deficit of low-mass FRB hosts compared to the occurrence of star-formation in the universe, implying that FRBs are a biased tracer of star-formation, preferentially selecting massive star-forming galaxies. This bias may be driven by galaxy metallicity, which is positively correlated with stellar mass. Metal-rich environments may favor the formation of magnetar progenitors through stellar mergers, as higher metallicity stars are less compact and more likely to fill their Roche lobes, leading to unstable mass transfer. Although massive stars do not have convective interiors to generate strong magnetic fields by dynamo, merger remnants are thought to have the requisite internal magnetic-field strengths to result in magnetars. The preferential occurrence of FRBs in massive star-forming galaxies suggests that CCSN of merger remnants preferentially forms magnetars.