81 citations · 185 across the 5 of their papers we have counts for
5 papers
A Systematic Study Of Superluminous Supernova Lightcurve Models Using Clustering
Emmanouil Chatzopoulos, Richard Tuminello
Superluminous supernova (SLSN) lightcurves exhibit a superior diversity compared to their regular luminosity counterparts in terms of rise and decline timescales, peak luminosities…
Synthetic Spectra of Pair-Instability Supernovae in 3D
E. Chatzopoulos, M. S. Gilmer, R. T. Wollaeger +2
Pair-Instability Supernovae (PISNe) may signal the deaths of extremely massive stars in the local Universe or massive primordial stars after the end of the Cosmic Dark Ages. Hydrod…
Fast evolving pair-instability supernova models: evolution, explosion, light curves
Alexandra Kozyreva, Matthew Gilmer, Raphael Hirschi +11
With an increasing number of superluminous supernovae (SLSNe) discovered the question of their origin remains open and causes heated debates in the supernova community. Currently,…
The Role of the Magnetorotational Instability in Massive Stars
J. Craig Wheeler, Daniel Kagan, Emmanouil Chatzopoulos
The magnetorotational instability (MRI) is key physics in accretion disks and is widely considered to play some role in massive-star core collapse. Models of rotating massive stars…
Finding the First Cosmic Explosions. IV. 90 - 140 M Pair-Instability Supernovae
Joseph Smidt, Daniel J. Whalen, E. Chatzopoulos +4
Population III stars that die as pair-instability supernovae are usually thought to fall in the mass range of 140 - 260 M. But several lines of work have now shown that r…