Properties of High-redshift Gamma-Ray Bursts

Fryer, Chris L.; Lien, Amy Y.; Fruchter, Andrew; Ghirlanda, Giancarlo; Hartmann, Dieter; Salvaterra, Ruben; Upton Sanderbeck, Phoebe R.; Johnson, Jarrett L.

doi:10.3847/1538-4357/ac5d5c

Title: Properties of High-redshift Gamma-Ray Bursts

Journal Article · 18 April 2022 · The Astrophysical Journal

DOI: https://doi.org/10.3847/1538-4357/ac5d5c · OSTI ID:1863840

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Abstract The immense power of gamma-ray bursts (GRBs) makes them ideal probes of the early universe. By using absorption lines in the afterglows of high-redshift GRBs, astronomers can study the evolution of metals in the early universe. With an understanding of the nature of GRB progenitors, the rate and properties of GRBs observed at high redshift can probe the star formation history and the initial mass function of stars at high redshift. This paper presents a detailed study of the dependence on metallicity and mass of the properties of long-duration GRBs under the black hole accretion disk paradigm to predict the evolution of these properties with redshift. These models are calibrated on the current GRB observations and then used to make predictions for new observations and new missions (e.g., the proposed Gamow mission) studying high-redshift GRBs.

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Research Organization:: Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)

Sponsoring Organization:: USDOE; USDOE Laboratory Directed Research and Development (LDRD) Program; USDOE National Nuclear Security Administration (NNSA)

Grant/Contract Number:: 89233218CNA000001

OSTI ID:: 1863840

Report Number(s):: LA-UR--21-31166; LA-UR--22-31690

Journal Information:: The Astrophysical Journal, Journal Name: The Astrophysical Journal Journal Issue: 2 Vol. 929; ISSN 0004-637X

Publisher:: American Astronomical SocietyCopyright Statement

Country of Publication:: United States

Language:: English

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