Generalized Linear Models of T 90-T 50 relation to classify GRBs
astro-ph.HE, hep-ph
Submitted: 2023-05-06
Updated: 2023-05-09
Comments: 8 figures, 1 table
License: http://creativecommons.org/licenses/by/4.0/
The gist: Gamma-ray bursts (GRBs) can be classified with their linearly dependent parameters alongside the standard T 90 distribution.
Terminology
Abstract
Gamma-ray bursts (GRBs) can be classified with their linearly dependent parameters alongside the standard T 90 distribution. The Generalized linear mixture model(GLM) identifies the number of linear dependencies in a two-parameter space. Classically, GRBs are classified into two classes by the presence of bimodality in the histogram of T 90. However, additional classes and sub-classes of GRBs are fascinating topics to explore. In this work, we investigate the GRBs classes in the T 90 - T 50 plane using the Generalized Linear Models(GLM) for Fermi GBM and BATSE catalogs. This study shows five linear features for the Fermi GBM catalog and four linear features for the BATSE catalog, directing towards the possibility of more than two GRB classes.
Sources
- A `Hypernova' model for SN 1998bw associated with gamma-ray burst of 25 April 1998
- Transient Events from Neutron Star Mergers
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- A possible Macronova in the late afterglow of the `long-short' burst GRB 060614
- An $r-$process macronova/kilonova in GRB 060614: evidence for the merger of a neutron star-black hole binary
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
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