08 Dec 2017
Today marks a major moment in the development of a project I’ve been working on for some time: me and my co-authors have completed a paper on inferring the opening angles of gamma ray bursts by observing binary neutron star mergers and gamma ray bursts. What does that mean? Well, I guess the point of this post is to explain just that. It should be said, while you can download the paper now, it’s still a pre-print: that means it hasn’t been peer-reviewed yet, so there’s a chance it may contain some mistakes which we’ve not picked up on. So I guess you might argue it’s probably not quite completed.
A structured gamma-ray burst jet could explain the dimness of the prompt emission observed from GRB170817A but the exact form of this structure is still ambiguous. However, with the promise of futu...
The first detection of a binary neutron star merger, GW170817, and an associated short gamma-ray burst confirmed that neutron star mergers are responsible for at least some of these bursts. The pro...