activity
20202026
most citedNeutron Star Extreme Matter Observatory: A kilohertz-band gravitational-wave detector in the global network

220 citations · 468 across the 11 of their papers we have counts for

collaborators

12 papers

astro-ph.HE2026

Modern tidal interaction models for rapid binary population synthesis: II. Binary black hole formation, mergers, and spins

Veome Kapil, Ilya Mandel, Jeff Riley +3

We present predictions for the merger rates and effective spin () distribution of binary black holes (BBHs) from isolated binary evolution, using a new self-consistent…

gr-qc2026★ 2 cited

Electromagnetic, gravitational wave, and static gravitational transmission through throat spacetimes: a constraint-wave asymmetry

Jeff Riley

We compute the transmission properties of electromagnetic (EM), gravitational wave (GW), and static gravitational perturbations through geometric throats in spherically symmetric s…

astro-ph.SR2026

Modern tidal interaction models for rapid binary population synthesis: I. Methods

Veome Kapil, Ilya Mandel, Evgeni Grishin +3

In this work, we present an updated prescription of contemporary tidal dissipation theory adapted for rapid binary population synthesis. Our simplified expressions encode the depen…

astro-ph.SR2025★ 1 cited

Rapid stellar and binary population synthesis with COMPAS: methods paper II

Ilya Mandel, Jeff Riley, Adam Boesky +13

The COMPAS public rapid binary population synthesis code has undergone a number of key improvements since the original COMPAS methods paper (Team COMPAS: Riley et al., 2022) was pu…

astro-ph.SR2025

Implications of modern mass-loss rates for massive stars

JD Merritt, Simon Stevenson, Andreas Sander +7

Massive stars lose a significant fraction of their mass through stellar winds at various stages of their lives, including on the main sequence, during the red supergiant phase, and…

astro-ph.HE2024★ 1 cited

A Trifecta of Modelling Tools: A Bayesian Binary Black Hole Model Selection combining Population Synthesis and Galaxy Formation Models

Liana Rauf, Cullan Howlett, Simon Stevenson +2

Gravitational waves (GWs) have revealed surprising properties of binary black hole (BBH) populations, but there is still mystery surrounding how these compact objects evolve. We ap…

astro-ph.SR2023★ 9 cited

Surrogate forward models for population inference on compact binary mergers

Jeff Riley, Ilya Mandel

Rapidly growing catalogs of compact binary mergers from advanced gravitational-wave detectors allow us to explore the astrophysics of massive stellar binaries. Merger observations…

astro-ph.IM2021★ 3 cited

Rapid stellar and binary population synthesis with COMPAS

Team COMPAS, :, Jeff Riley +23

Compact Object Mergers: Population Astrophysics and Statistics (COMPAS; https://compas.science) is a public rapid binary population synthesis code. COMPAS generates populations of…

astro-ph.HE2020★ 85 cited

Massive Stellar Triples Leading to Sequential Binary Black-Hole Mergers in the Field

Alejandro Vigna-Gómez, Silvia Toonen, Enrico Ramirez-Ruiz +3

Stellar triples with massive stellar components are common, and can lead to sequential binary black-hole mergers. Here, we outline the evolution towards these sequential mergers, a…

astro-ph.SR2020★ 74 cited

Chemically Homogeneous Evolution: A rapid population synthesis approach

Jeff Riley, Ilya Mandel, Pablo Marchant +5

We explore chemically homogeneous evolution (CHE) as a formation channel for massive merging binary black holes (BBHs). We develop methods to include CHE in a rapid binary populati…

astro-ph.HE2020★ 73 cited

Binary population synthesis with probabilistic remnant mass and kick prescriptions

Ilya Mandel, Bernhard Mueller, Jeff Riley +3

We report on the impact of a probabilistic prescription for compact remnant masses and kicks on massive binary population synthesis. We find that this prescription populates the pu…

astro-ph.HE2020★ 220 cited

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…