Radio Constraints on r-process Nucleosynthesis by Collapsars

Abstract The heaviest elements in the universe are synthesized through rapid neutron capture ( r -process) in extremely neutron-rich outflows. Neutron star mergers were established as an important r -process source through the multimessenger observation of GW170817. Collapsars were also proposed as...

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Bibliographic Details
Published in:Astrophysical journal. Letters 2022-07, Vol.934 (1), p.L5
Main Authors: Lee, K. H., Bartos, I., Eddins, A., Corsi, A., Márka, Z., Privon, G. C., Márka, S.
Format: Article
Language:English
Subjects:
Afterglows
Collapsars
Ejecta
Forging
Gamma ray bursts
Gamma rays
Heavy elements
Neutron stars
Neutrons
Nuclear capture
Nuclear fusion
Optical observations
R-process
Radio emission
Radio observation
Star mergers
Velocity distribution
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Summary:Abstract The heaviest elements in the universe are synthesized through rapid neutron capture ( r -process) in extremely neutron-rich outflows. Neutron star mergers were established as an important r -process source through the multimessenger observation of GW170817. Collapsars were also proposed as a potentially major source of heavy elements; however, this is difficult to probe through optical observations due to contamination by other emission mechanisms. Here we present observational constraints on r -process nucleosynthesis by collapsars based on radio follow-up observations of nearby long gamma-ray bursts (GRBs). We make the hypothesis that late-time radio emission arises from the collapsar wind ejecta responsible for forging r -process elements, and consider the constraints that can be set on this scenario using radio observations of a sample of Swift/Burst Alert Telescope GRBs located within 2 Gpc. No radio counterpart was identified in excess of the radio afterglow of the GRBs in our sample. This gives the strictest limit to the collapsar r -process contribution of ≲0.2 M ⊙ for GRB 060505 and GRB 05826, under the models we considered. Our results additionally constrain energy injection by a long-lived neutron star remnant in some of the considered GRBs. While our results are in tension with collapsars being the majority of r -process production sites, the ejecta mass and velocity profile of collapsar winds, and the emission parameters, are not yet well modeled. As such, our results are currently subject to large uncertainties, but further theoretical work could greatly improve them.
ISSN:2041-8205
2041-8213
DOI:10.3847/2041-8213/ac7ff0