activity
20162023
most citedFull Transport Model of GW170817-Like Disk Produces a Blue Kilonova

184 citations · 382 across the 11 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

13 papers · 1 filter

astro-ph.HE2023

Gravitational Wave Eigenfrequencies from Neutrino-Driven Core-Collapse Supernovae

Noah E. Wolfe, Carla Frohlich, Jonah M. Miller +2

Core-collapse supernovae are predicted to produce gravitational waves (GWs) that may be detectable by Advanced LIGO/Virgo. These GW signals carry information from the heart of thes…

astro-ph.HE2022★ 20 cited

Nucleosynthesis in Outflows from Black Hole-Neutron Star Merger Disks With Full GRRMHD

Sanjana Curtis, Jonah M. Miller, Carla Frohlich +3

Along with binary neutron star mergers, the in-spiral and merger of a black hole and a neutron star is a predicted site of -process nucleosynthesis and associated kilonovae. For…

astro-ph.HE2022★ 1 cited

Realistic Kilonova Up Close

Alexandra Ruth Stewart, Li-Ta Lo, Oleg Korobkin +6

Neutron star mergers are cosmic catastrophes that produce some of the most energetic observed phenomena: short gamma-ray bursts, gravitational wave signals, and kilonovae. The latt…

astro-ph.HE2021

A New Constraint on the Nuclear Equation of State from Statistical Distributions of Compact Remnants of Supernovae

Mikhail M. Meskhi, Noah E. Wolfe, Zhenyu Dai +4

Understanding how matter behaves at the highest densities and temperatures is a major open problem in both nuclear physics and relativistic astrophysics. This physics is often enca…

astro-ph.HE2020★ 34 cited

Black Hole Spin in X-ray Binaries: Giving Uncertainties an

Greg Salvesen, Jonah M. Miller

The two established techniques for measuring black hole spin in X-ray binaries often yield conflicting results, which must be resolved before either method may be deemed robust. In…

astro-ph.HE2020

Axisymmetric Radiative Transfer Models of Kilonovae

Oleg Korobkin, Ryan Wollaeger, Christopher Fryer +9

The detailed observations of GW170817 proved for the first time directly that neutron star mergers are a major production site of heavy elements. The observations could be fit by a…