Exploring short-GRB afterglow parameter space for observations in coincidence with gravitational waves. Issue 4 (1st December 2017)

• Record Type: Journal Article
• Authors: Saleem, M; Resmi, L; Misra, Kuntal; Pai, Archana; Arun, K G
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 474:Issue 4(2018)
• Page Start: 5340
• Page End: 5350
• Publication Date: 2017-12-01
• Subjects: gravitational waves -- gamma-ray burst: general; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stx3104
• Languages: English
• ISSNs: 0035-8711

Abstract

Abstract: Short duration Gamma Ray Bursts (SGRB) and their afterglows are among the most promising electromagnetic (EM) counterparts of Neutron Star (NS) mergers. The afterglow emission is broad-band, visible across the entire electromagnetic window from γ-ray to radio frequencies. The flux evolution in these frequencies is sensitive to the multidimensional afterglow physical parameter space. Observations of gravitational wave (GW) from BNS mergers in spatial and temporal coincidence with SGRB and associated afterglows can provide valuable constraints on afterglow physics. We run simulations of GW-detected BNS events and assuming that all of them are associated with a GRB jet which also produces an afterglow, investigate how detections or non-detections in X-ray, optical and radio frequencies can be influenced by the parameter space. We narrow down the regions of afterglow parameter space for a uniform top-hat jet model, which would result in different detection scenarios. We list inferences which can be drawn on the physics of GRB afterglows from multimessenger astronomy with coincident GW-EM observations.