activity
20082015
most citedImproved Cosmological Constraints from New, Old and Combined Supernova Datasets

1.6k citations · 3k across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.HE2015★ 116 cited

A transition in circumbinary accretion discs at a binary mass ratio of 1:25

Daniel J. D'Orazio, Zoltan Haiman, Paul Duffell +2

We study circumbinary accretion discs in the framework of the restricted three-body problem (R3Bp) and via numerically solving the height-integrated equations of viscous hydrodynam…

astro-ph.HE2015★ 60 cited

A reduced orbital period for the supermassive black hole binary candidate in the quasar PG 1302-102?

Daniel J. D'Orazio, Zoltán Haiman, Paul Duffell +2

Graham et al. (2015) have detected a 5.2 year periodic optical variability of the quasar PG 1302-102 at redshift , which they interpret as the redshifted orbital period $(1+…

astro-ph.HE2014★ 25 cited

Massive Black Hole Science with eLISA

Enrico Barausse, Jillian Bellovary, Emanuele Berti +4

The evolving Laser Interferometer Space Antenna (eLISA) will revolutionize our understanding of the formation and evolution of massive black holes along cosmic history by probing m…

astro-ph.HE2014★ 134 cited

Binary Black Hole Accretion During Inspiral and Merger

Brian D. Farris, Paul Duffell, Andrew I. MacFadyen +1

We present the results of 2D, moving mesh, viscous hydrodynamical simulations of accretion onto merging supermassive black hole (SMBH) binaries. We include viscous heating, shock h…

astro-ph.HE2014★ 116 cited

Characteristic Signatures in the Thermal Emission from Accreting Binary Black Holes

Brian D. Farris, Paul Duffell, Andrew I. MacFadyen +1

We present the results of a calculation of the thermal spectrum from a 2D, moving mesh, high-accuracy, viscous hydrodynamical simulation of an accreting supermassive black hole bin…

astro-ph.EP2014★ 178 cited

The Migration of Gap-Opening Planets is not Locked to Viscous Disk Evolution

Paul C. Duffell, Zoltan Haiman, Andrew I. MacFadyen +2

Most standard descriptions of Type II migration state that massive, gap-opening planets must migrate at the viscous drift rate. This is based on the idea that the disk is separated…