2k citations · 9.1k across the 78 of their papers we have counts for
78 papers
Modelling stellar evolution in mass-transferring binaries and gravitational-wave progenitors with METISSE
Poojan Agrawal, Jarrod Hurley, Simon Stevenson +3
Massive binaries are vital sources of various transient processes, including gravitational-wave mergers. However, large uncertainties in the evolution of massive stars, both physic…
Dynamical double black holes and their host cluster properties
Debatri Chattopadhyay, Jarrod Hurley, Simon Stevenson +1
We investigate the relationship between the global properties of star clusters and their double black hole (DBH) populations. We use the code {\tt NBODY6} to evolve a suite of star…
A systematic study of super-Eddington layers in the envelopes of massive stars
Poojan Agrawal, Simon Stevenson, Dorottya Szécsi +1
The proximity to the Eddington luminosity has been attributed as the cause of several observed effects in massive stars. Computationally, if the luminosity carried through radiatio…
Explaining the differences in massive star models from various simulations
Poojan Agrawal, Dorottya Szécsi, Simon Stevenson +2
The evolution of massive stars is the basis of several astrophysical investigations, from predicting gravitational-wave event rates to studying star-formation and stellar populatio…
Modelling Neutron Star-Black Hole Binaries: Future Pulsar Surveys and Gravitational Wave Detectors
Debatri Chattopadhyay, Simon Stevenson, Jarrod R. Hurley +2
Binaries comprised of a neutron star (NS) and a black hole (BH) have so far eluded observations as pulsars and with gravitational waves (GWs). We model the formation and evolution…
Neutron Star Extreme Matter Observatory: A kilohertz-band gravitational-wave detector in the global network
K. Ackley, V. B. Adya, P. Agrawal +160
Gravitational waves from coalescing neutron stars encode information about nuclear matter at extreme densities, inaccessible by laboratory experiments. The late inspiral is influen…