Bayesian model selection for GRB 211211A through multiwavelength analyses
Nina Kunert, S. Antier, Vsevolod Nedora, Mattia Bulla, P. T. H. Pang, Shreya Anand, M. W. Coughlin, Ingo Tews, Jennifer Barnes, Thomas Hussenot-Desenonges, Brian C. Healy, T Jegou du Laz, Meili Pilloix, W. Kiendrébéogo, Tim Dietrich
Abstract
ABSTRACT Although GRB 211211A is one of the closest gamma-ray bursts (GRBs), its classification is challenging because of its partially inconclusive electromagnetic signatures. In this paper, we investigate four astrophysical scenarios as possible progenitors for GRB 211211A: a binary neutron star merger, a black hole–neutron star merger, a core-collapse supernova, and an r-process enriched core collapse of a rapidly rotating massive star (a collapsar). We perform a large set of Bayesian multiwavelength analyses based on different models describing these scenarios and priors to investigate which astrophysical scenarios and processes might be related to GRB 211211A. Our analysis supports previous studies in which the presence of an additional component, likely related to r-process nucleosynthesis, is required to explain the observed light curves of GRB 211211A, as it cannot be explained solely as a GRB afterglow. Fixing the distance to about $350~\rm Mpc$, namely the distance of the possible host galaxy SDSS J140910.47+275320.8, we find a statistical preference for a binary neutron star merger scenario.