activity
20242026
most citedLuminosity predictions for the first three ionisation stages of W, Pt and Au to probe potential sources of emission in kilonova

5 citations · 5 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph.HE2026

Exploring the diversity of kilonovae with 3D radiative transfer I. The polar direction

Christine E. Collins, Luke J. Shingles, Vimal Vijayan +7

We present 3D kilonova radiative transfer simulations for a series of binary neutron star merger models. The masses of the neutron stars are varied as well as the total mass of the…

astro-ph.HE2025

Light Travel Time Effects in Kilonova Models

F. McNeill, S. A. Sim, C. E. Collins +4

The extremely rapid evolution of kilonovae results in spectra that change on an hourly basis. These spectra are key to understanding the processes occurring within the event, but t…

physics.atom-ph2025

Electron-Impact Excitation of Zirconium I-III in support of Neutron Star Merger Diagnostics

M. McCann, C. P. Ballance, F. McNeill +2

Recent observation and analysis of kilonovae (KNe) spectra as a result of neutron star mergers require accurate and complete atomic structure and collisional data for interpretatio…

physics.atom-ph20245 cited

Luminosity predictions for the first three ionisation stages of W, Pt and Au to probe potential sources of emission in kilonova

M. McCann, L. P. Mulholland, Z. Xiong +7

A large number of R-matrix calculations of electron impact excitation for heavy elements (Z > 70) have been performed in recent years for applications in fusion and astrophysics re…

astro-ph.SR2024

Collisional and Radiative Data for Tellurium ions in Kilonovae modelling and Laboratory Benchmarks

Leo Patrick Mulholland, Fiona McNeill, Stuart A. Sim +2

Tellurium is a primary candidate for the identification of the 2.1 m emission line in kilonovae (KNe) spectra AT2017gfo and GRB230307A. Despite this, there is currently an insuf…