Research GroupBelow is a list of members of my research group, including brief descriptions of some of their research.
Greg is a postdoc in my group who works on many things including gravitational-wave emission mechanisms and detection methods for LIGO, and neutron-star physics.
Juan Calderon Bustillo
Juan is currently a postdoc at the Georgia Institute for Technology, but will be joining my group as a postdoc towards the end of 2018. Juan works on many things related to gravitational waves, primarily at the interface between gravitational waveform modelling and data analysis techniques for binary black hole detections.
Paul began his PhD in 2018, and is working on the aftermath of binary neutron star mergers. Paul is trying to understand whether near-future Advanced LIGO observations of binary neutron stars can distinguish properties of the post-merger remnant. In particular, can such observations distinguish between the formation of hypermassive, supramassive, or infinitely stable neutron stars? Paul completed his honours thesis in 2017 under the supervision of myself and Andy Casey.
Moritz began his PhD in 2018, and is working on detecting gravitational-wave memory with Advanced LIGO. Memory is an effect that causes the permanent deformation of spacetime after a gravitational wave has passed through a region of space. In a recent paper, we showed that this effect could be seen with Advanced LIGO by observing dozens of binary black hole collisions. Among other things, Moritz is building the actual search pipeline to look for this effect, and trying to understand its physical and astrophysical implications.
Nikhil began his PhD in 2018. He is developing a gravitational-wave detection pipeline to search for gravitational waves from the post-merger remnant of binary neutron star mergers. In particular, he will use X-ray observations to develop a matched filter search for these gravitational waves when a long-lived neutron star is born from the merger. Nikhil completed his honours thesis in 2017 under the supervision of myself and Letizia Sammut, winning the prize for best astrophysics honours student at Monash.
Hayley began her PhD in 2016, and is primarily working on doing full, three-dimensional, non-linear numerical general relativity calculations of the evolution of the Universe as a whole. Hayley's first publication showed that we can successfully reprocude simply cosmological evolutions using the Cactus computational infrastructure for evolving general relativistic spacetimes using numerical relativity. I am co-supervising Hayley with Daniel Price - we also co-supervised her honours thesis in 2015, for which she won a prize for the best astrophysics honours project at Monash.
David began his PhD in 2016. His project is to implement general relativity into the numerical method known as smooth particle hydrodynamics, and to apply this to various astrophysical phenomena such as accretion disks around single and binary black holes, tidal disruption events and neutron star mergers. I am co-supervising David's PhD project with Daniel Price.
Zac PellowZac is an honours student in 2018 that I am co-supervising with Daniel Price. He will be working on doing simulations of binary neutron stars using Smooth Particle Hydrodynamics.
Kyla was an honours student in 2017 working on the aftermath of binary neutron star mergers. In particular, Kyla's thesis was on trying to understand whether it's possible that the post-merger remnant could be a quark star, as oppossed to a garden-variety neutron star. She did this in terms of whether a quark star fits with our theoretical and observational understanding of these mergers.
Marcus ws an honours student in 2017 who I am co-supervised with Eric Thrane. Marcus studied the eccentricity evolution of binary black holes systems as a function of their formation history. His thesis was on trying to understand whether any such residual eccentricity can be observed with advanced gravitational-wave detectors, and also develop an algorithm for detecting small values of the eccentricity.
Lucy McNeillLucy was an honours student at Monash University in 2016. Her thesis was on high-frequency sources of gravitational waves, and the detectabiilty of their counter-part gravitational-wave memory signal. The effect of this lower-frequency memory signal is that LIGO's sensitivity band is effectively increased many-fold. Lucy's results were ultimately published here. Gravitational-wave memory is a strange gravitational phenomena that results in the permanent deformation of spacetime following a cataclysmic event such as a binary black hole merger.
Cristiano was an honours student at Monash in 2016. His thesis was on detecting and understand multimessenger signals from binary neutron star mergers. In particular, he developed a method for fitting both the millisecond magnetar and fireball models to the X-ray light curves following short gamma-ray bursts, that enabled both the estimation of parameters in each model, and also did Bayesian model selection. His honours thesis was ultimately published here in ApJL.