collaborators

6 papers

astro-ph.HE2026

Effects of magnetically driven shocks on nucleosynthesis and kilonovae from neutron star mergers

Yuan Feng, Oleg Korobkin, Elias R. Most +2

Neutron-star mergers can launch mildly relativistic to moderately relativistic outflows whose interaction with the ejecta can reshape kilonova emission. We parametrically study mag…

astro-ph.HE2026

Kilonovae and Long-duration Gamma-ray Bursts

Marko Ristić, Brandon L. Barker, Samuel Cupp +5

Recent detections of kilonova-like emission following long-duration gamma-ray bursts GRB211211A and GRB230307A have been interpreted as originating from the merger of two neutron s…

astro-ph.HE2026

A comparison of three neodymium atomic data sets for kilonova modeling

Christopher J. Fontes, Nicholas Vieira, Chris L. Fryer +4

We examine the impact of input neodymium (Nd) atomic data on the light curves and spectra of kilonovae, probing the sensitivity of kilonova observables to the atomic physics of thi…

astro-ph.HE2026

Joint Electromagnetic and Gravitational Wave Inference of Binary Neutron Star Merger GW170817 Using Forward-Modeling Ejecta Predictions

Marko Ristić, Richard O'Shaughnessy, Kate Wagner +5

We reassess the capacity for multimessenger inference of AT2017gfo/GW170817 using both kilonova and gravitational wave emission within the context of a recent simulation-based surr…

astro-ph.HE2025

Spatial models of r-process remnants and their gamma-ray detectability

Benjamin Amend, Christopher L. Fryer, Matthew R. Mumpower +1

We investigate the detectability of gamma-ray emission from long-lived radioactive isotopes in r-process-enriched remnants, focusing on how assumptions about their spatial distribu…

astro-ph.HE2025

Inferring neutron star merger ejecta morphologies with kilonovae

Brendan L. King, Soumi De, Oleg Korobkin +2

In this study we incorporate a new grid of kilonova simulations produced by the Monte Carlo radiative transfer code SuperNu in an inference pipeline for astrophysical transients, a…