Jonathan works on a range of topics in high energy astrophysics, including binary black hole mergers, gamma-ray bursts, kilonovae, magnetic reconnection, and MHD turbulence. He is an expert in algorithms and software methodologies for high-performance simulation codes used in astrophysical hydrodynamics and MHD.
Debojyoti works jointly with Jonathan Zrake and Jeffrey Fung, investigating the dynamics of accretion disks across a variety of astrophysical environments. His recent work has focused on the OJ 287 binary supermassive black hole system, where he investigates how the secondary black hole perturbs the accretion disk of the primary and produces observable variability. He is also studying the formation and evolution of large-scale non-axisymmetric density structures, commonly known as “lumps,” in accretion flows. He obtained his PhD from IIT Kanpur, India, where he worked on tidal disruption events as probes of intermediate-mass black holes and gained expertise in numerical modelling of astrophysical fluids using the smooth particle hydrodynamics method.
Marcus is a postdoctoral researcher currently studying the dynamics of gas around black hole binaries using hydrodynamic simulations. In particular, he is interested in the electromagnetic signatures of the accretion disks around each black hole in the late stages of their inspiral. He has also recently started working on analysis of multi-wavelength lightcurves produced by supermassive black hole binaries. He previously obtained his PhD from the University of Southampton, where he worked on dissipation and sub-grid models in relativistic hydrodynamics, and gained experience in numerical relativity.
Akhil Nair is a 4th year PhD student whose research focuses on hydrodynamical simulations of accretion and mass transfer in binary systems. His current work studies stochastic variability from circumbinary disks and minidisks around binary black holes, using power spectral densities to connect stream-fed accretion to predict observable AGN timing signatures. He also studies circumbinary outflows from Roche-lobe overflow systems. His broader interests include numerical methods for hydrodynamics, GPU-enabled simulation frameworks, and scientific visualization of astrophysical phenomena.
Matt is a 3rd year PhD student interested in multi-messenger astronomy, specifically aiding in binary black hole electromagnetic detection methods. Currently, he is working on analytically predicting the false-positive rate of the Lomb-Scargle periodogram against noisy signals. From there, he plans to explore the effectiveness of a Convolutional Neural Network against synthetic and simulation-based light-curves, in order to discover binary black hole systems in legacy data.
Troy's research focuses on the dynamics of massive black hole binary (MBHB) systems as they interact with their galactic environments. He has developed a celestial mechanics code called Dust, which computes the trajectories of test-particles interacting with a the time-dependent gravitational field of an orbiting binary, which has been used to examine the ballistic approximation of binary-disk interactions. Troy also uses hydrodynamics simulations to understand the dynamics of "minidisk" formation around the individual black holes in binary systems.
Brayden is a 2nd year PhD student interested in the development of magnetohydrodynamic simulations to study a variety of astrophysical phenomena. Recently this work has led to the creation How to Write a Magnetohydrodynamics Code note as a resource for others to produce their own magnetohydrodynamic simulations. He has interests in applying MHD simulations to super-luminous supernovae winds.
Josh is a 2nd year PhD student interested in high-energy astrophysics.