activity
20192026
most citedTidal Disruption Disks Formed and Fed by Stream-Stream and Stream-Disk Interactions in Global GRHD Simulations

68 citations · 148 across the 16 of their papers we have counts for

collaborators

18 papers

gr-qc2026

Constraining Ultralight Scalars with Black Hole Binary Mergers in Galactic Nuclei

Majed Khalaf, Eric Kuflik, Alessandro Lenoci +2

Ultralight scalars can form long-lived, macroscopic bound states around spinning black holes, known as superradiance clouds. These clouds provide an additional channel for energy d…

astro-ph.HE2026

Anisotropic wind in tidal disruption events

Paola Martire, Elena Maria Rossi, Nicholas Chamberlain Stone +2

Over the coming years, the number of tidal disruption events (TDEs) is expected to substantially increase with observations from the Vera Rubin Observatory (g and r band) and {\it…

astro-ph.HE2026

Intermediate States in Chaotic Triple Evolution and Applications to Black Hole Merger Statistics

Dina Meylakh, Nicholas C. Stone, Nathan W. C. Leigh

Three-body interactions exhibit phases of strong chaotic evolution as well as hierarchical motion where one body separates from a binary and follows a hyperbolic or elliptic trajec…

astro-ph.HE2025★ 1 cited

Wind-mediated Eddington-limited emission in a Black Hole Tidal Disruption Event

Paola Martire, Elena Maria Rossi, Nicholas Chamberlain Stone +3

Observations of tidal disruption events (TDEs) have already produced tens of strong candidate flares, and their number will greatly increase with upcoming wide field surveys. Never…

astro-ph.HE2025

Fragmentation in Collapsar Disks: Migration, Growth, and Emission

Y. Lerner, N. C. Stone, D. D. Ofengeim

We present a parameter survey of fragmentation in collapsar disks, using a revised version of the Chen & Beloborodov (2007) model that determines the structure of steady state hype…

astro-ph.GA2025

Disruptions of stars and binary systems on chaotic orbits in an axisymmetric Milky Way center

Zephyr Penoyre, Elena Maria Rossi, Nicholas C. Stone

Non-spherical potentials allow a wide range of trajectories, both regular and chaotic, whose periapse distances can vary orbit to orbit. In particular chaotic trajectories can brin…