activity
20202026
most citedGas-driven inspiral of binaries in thin accretion disks

136 citations · 389 across the 13 of their papers we have counts for

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10 papers · 1 filter

astro-ph.HE2026

The effect of pressure confinement on the maximum mass of rapidly accreting supermassive stars

Lorenz Zwick, Christopher Tiede, Zoltán Haiman

We derive an extension of Chandrasekhar's pulsational stability criterion for relativistic stars with a pressure boundary condition at the surface. We then apply the new criterion…

astro-ph.HE2026

Electromagnetic Emission and Orbital Evolution of Eccentric Supermassive Black Hole Binaries in Retrograde Disks

David ONeill, Mark J. Avara, Christopher Tiede +3

Circumbinary disks around supermassive black hole binaries (SMBHBs) are expected to form across a broad range of inclinations, with retrograde configurations potentially a common o…

astro-ph.HE2025★ 5 cited

Hot, cold, and multi-component accretion flows around supermassive black hole binaries

Christopher Tiede, Daniel J. D'Orazio

We develop a model for supermassive black hole binaries (SMBHBs) accreting below their Eddington limit, focusing on systems where hot, advection-dominated flows become viable. We s…

astro-ph.HE2025

Gravitational Wave Decoupling in Retrograde Circumbinary Disks

David O'Neill, Christopher Tiede, Daniel J. D'Orazio +2

We present a study of the late-time interaction between supermassive black hole binaries and retrograde circumbinary disks during the period of gravitational wave-driven inspiral.…

astro-ph.HE2025★ 2 cited

Stellar Stripping and Disruption in Disks around Supermassive Black Hole Binaries: Repeating nuclear transients prior to LISA events

Daniel J. D'Orazio, Christopher Tiede, Lorenz Zwick +2

If supermassive black hole binaries (SMBHBs) are driven together by gas disks in galactic nuclei, then a surrounding nuclear star cluster or in-situ star-formation should deliver s…

astro-ph.HE2024★ 5 cited

Accretion mediated spin-eccentricity correlations in LISA massive black hole binaries

Mudit Garg, Christopher Tiede, Daniel J. D'Orazio

We examine expected effective spin () and orbital eccentricity () correlations for a population of observable equal-mass massive black hole bina…

astro-ph.HE2024★ 3 cited

Fast Methods for Computing Photometric Variability of Eccentric Binaries: Boosting, Lensing, and Variable Accretion

Daniel J. D'Orazio, Paul C. Duffell, Christopher Tiede

We analyze accretion-rate time series for equal-mass binaries in co-planar gaseous disks spanning a continuous range of orbital eccentricities up to 0.8, for both prograde and retr…

astro-ph.HE2024★ 40 cited

Long-term Evolution of Binary Orbits Induced by Circumbinary Disks

Ruggero Valli, Christopher Tiede, Alejandro Vigna-Gómez +6

Circumbinary disks are found in a variety of astrophysical scenarios, spanning binary star formation to accreting supermassive black hole binaries. The interaction with a circumbin…

astro-ph.HE2023★ 20 cited

Disk induced binary precession: Implications for dynamics and multi-messenger observations of black hole binaries

Christopher Tiede, Daniel J. D'Orazio, Lorenz Zwick +1

Many studies have recently documented the orbital response of eccentric binaries accreting from thin circumbinary disks, characterizing the change in binary semi-major axis and ecc…

astro-ph.HE2020★ 110 cited

Equilibrium eccentricity of accreting binaries

Jonathan Zrake, Christopher Tiede, Andrew MacFadyen +1

Using high-resolution hydrodynamics simulations, we show that equal-mass binaries accreting from a circumbinary disk evolve toward an orbital eccentricity of , unles…