collaborators

5 papers

astro-ph.HE2026

Dynamics and detectability of long-lived non-accretion phases for massive black hole binaries in cold, thermally regulating disks

Christopher Tiede, David O'Neill, Daniel J. D'Orazio

We investigate whether the non-accreting phases found in thin, locally isothermal circumbinary disks survive when the disk thermodynamics are evolved self-consistently. We present…

astro-ph.HE2026

Spin-Orbit Misalignments of Eccentric Black Hole Mergers in AGN Disks

Gaia Fabj, Christopher Tiede, Connar Rowan +2

The disks of active galactic nuclei (AGNs) provide a natural environment where stellar-mass black holes (BHs) can dynamically pair, undergo repeated interactions, and eventually me…

astro-ph.GA2026

Little Red Dots as self-gravitating discs accreting on supermassive stars: Spectral appearance and formation pathway of the progenitors to direct collapse black holes

Lorenz Zwick, Christopher Tiede, Lucio Mayer

We propose an alternative physical interpretation and formation pathway for the recently discovered "little red dots" (LRDs). We model LRDs as super-massive stars (SMSs) surrounded…

astro-ph.HE2025

Dissecting environmental effects with eccentric gravitational wave sources

Lorenz Zwick, Kai Hendriks, David O'Neill +6

We model the effect of resonances between time-varying perturbative forces and the epi-cyclical motion of eccentric binaries in the gravitational wave (GW) driven regime. These ind…

astro-ph.HE2025

Environmental effects in stellar mass gravitational wave sources I: Expected fraction of signals with significant dephasing in the dynamical and AGN channels

Lorenz Zwick, János Takátsy, Pankaj Saini +5

We present the first overview of the expected quantity of signals which will showcase significant gravitational wave phase shifts caused by astrophysical environments, considering…