University of Waterloo
200 University Avenue West
Waterloo, Ontario, Canada N2L 3G1
Phone: (519) 888-4567 ext 32215
Fax: (519) 746-8115
Dr. Afshordi dabbles in Astrophysics, Cosmology, and Physics of gravity and is obsessed with observational hints that could help address problems in fundamental physics.
Professor Balogh's research uses the world’s largest telescopes to study the physical properties of distant galaxies. Through spectroscopy we can learn about the distances, ages, chemical composition and star formation histories of these galaxies.
Dr. Broderick works to explain the fundamental physics of black holes and their observable characteristics. Black holes are sites where strong gravity dominates everything, from the dynamics of orbiting material to the shape of spacetime itself. As a result, they are the engines that power some of the brightest objects in the universe.
Dr. Fich is an astronomer specializing in studies of star formation, the interstellar medium, and the structure of galaxies. His recent research activities have focused on “small scale” formation studies of low and intermediate mass stars, circumstellar disks, and the formation of proto-solar systems.
Broadly speaking, Professor Hudson's research is in observational and theoretical cosmology, particularly Galaxy Formation, and measuring the properties of dark matter and dark energy through Gravitational Lensing, Cosmic Flows and Large-scale Structure.
Professor Mann works on gravitation, quantum physics, and the overlap between these two subjects. He is interested in questions that provide us with information about the foundations of physics, particularly those that could be tested by experiment.
Giant black holes weighing upwards of one billion times the mass of the Sun are thought to lurk at the centers of all massive galaxies. Energy released by spin breaking and infalling matter onto such supermassive black holes may be regulating the growth of galaxies and clusters of galaxies.
Professor Percival's research interests focus on the properties of the Universe on the largest scales. Surveys of three-dimensional galaxy positions provide a wealth of data both on the physics just after the Big-Bang when the seed fluctuations that will grow through gravity to become galaxies were created, and on the physics driving the evolution of the Universe today.
Dr. Taylor is using whatever tools he can, including numerical simulations, astrophysical theory and observational data, to try to figure what dark matter is, where it is, and how it behaves. His research includes gravitational lensing and dynamical studies of galaxy clusters, the properties of the smallest galaxies in the local universe, and the theory behind dark matter halos around galaxies and clusters.