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Department of Astronomy and Astrophysics: PhD Program, Fall 2021
- Big Glass, Big Ideas
- Putting the Physics in Astrophysics
- Cutting Edge Detectors and Instrumentation Development
The Department of Astronomy & Astrophysics at the University of Chicago offers a diverse and vibrant observational research program with guaranteed access to the Magellan telescopes at Las Campanas Observatory in Chile. Students have the opportunity to participate in a wide array of research projects, using a wide range of observational facilities. Through the Chicago-Carnegie Brinson predoctoral program, a partnership with Carnegie Observatories, students also have the opportunity to spend a year of their PhD studies working alongside the outstanding staff at Carnegie Observatories to expand their horizons. Our grad students enjoy what is among the highest per-capita access to 8-m class telescopes in the country.
Astronomy and Astrophysics faculty in observations
The main theme of Bean's research is the observational study of planets outside the Solar System ("exoplanets"). He uses groundand space-based telescopes to detect and characterize these worlds. He also builds new instruments as part of the push towards identifying other Earth-like planets.
Chang is an observational cosmologist. Her main science interest is to use large optical imaging survey data to study the evolution of the recent Universe through a technique called weak gravitational lensing. She is also interested in combining the rich information from galaxy surveys with that of the cosmic microwave background to study topics of cosmology and astrophysics. She is currently involved in the Dark Energy Survey (DES) and the Rubin Observatory's Legacy Survey of Space and Time (LSST).
Chen’s research broadly covers issues concerning formation and evolution of galaxies across cosmic time. In particular, she is interested in the properties of diffuse gas in and around galaxies and super massive black holes. The expertise in her group lies in galaxy surveys and absorption-line spectroscopy of distant light sources to study baryon cycles in and out of star-forming regions.
Drlica-Wagner’s research focuses on using astrophysical observations to understand the fundamental nature of dark matter and dark energy. He works on large cosmic surveys including the Dark Energy Survey (DES) and the Rubin Observatory's Legacy Survey of Space and Time (LSST) . Recently, he has been interested in using the faintest and most dark-matter-dominated galaxies to try to understand the fundamental nature of dark matter. He considers himself to be an experimental particle cosmologist, and he is heavily invested in the instruments and infrastructure that make these large surveys possible.
Freedman's research is in observational cosmology (measures of the expansion rate of the universe using the Hubble Space Telescope, Spitzer Space Telescope and the ground-based Magellan telescope). Her current projects involve measurements of the Hubble constant -- the current expansion rate, as well as the past expansion rate, providing constraints on the acceleration of the universe and dark energy. Her other field of interest is the stellar populations of galaxies, the evolution of galaxies, and the initial mass function.
Gladders’ research centers around the discovery and exploitation of galaxy clusters, and strong gravitational lenses, as cosmological laboratories in which to test ideas of galaxy formation and evolution, and the connection between visible matter and dark matter. He uses ground-based telescopes of various apertures extensively, and all of the major space observatories, working from radio to X-ray wavelengths as needed by various studies.
Harper's research deals with problems of formation of galaxies, stars, and planetary systems, physics of the interstellar medium, and properties of interstellar dust. His experimental research group constructs and operates infrared instrumentation. He helped pioneer astronomical research on airborne telescopes, and at the South Pole.
Ji’s research focuses on observing and interpreting the chemical content of stars in surviving relics of the first galaxies, the so-called “ultra-faint” dwarf galaxies. He studies nearby stars and galaxies to understand the first stars and galaxies, the origin of the elements, the history of our galaxy, and the nature of dark matter.
Kron’s interests include using large sky surveys to constrain how the populations of galaxies and quasars were built up, and how they have evolved with cosmic time.
Zhuravleva’s primary research interests are high-energy X-ray astrophysics and the physics of galaxy clusters. Using X-ray imaging and spectroscopic data and the computational modeling of relevant astrophysical processes, she studies the interactions between supermassive black holes and their host galaxies, processes that shape the large-scale evolution of galaxy clusters, and fundamental microscopic properties of intergalactic plasmas. She is involved in the development of the next X-ray telescope, XRISM, that will observe the X-ray Universe with unprecedented spectral resolution.
The Department of Astronomy and Astrophysics is the home of world-leaders in cosmological physics, astroparticle and high-energy physics, plasma physics and astrophysics, and solar system astronomy and astrophysics, particularly in the areas of early universe physics, high-resolution galaxy formation modeling and modeling of reionization and the intergalactic medium in the early universe. High-performance computing is the workhorse of astrophysical research across all of our science themes. We have access to computational facilities through the Research Computing Center at the University and through connections to Argonne National Laboratory and Fermilab.
Astronomy and Astrophysics faculty in theory
Olinto's interests are in theoretical astrophysics, particle and nuclear astrophysics, and cosmology. Her work has focused on the highest energy cosmic rays, indirect signatures of particle dark matter, cosmological effects of magnetic fields, natural inflation, and the internal structure of neutron stars.
Caprioli’s research involves high-energy astrophysical phenomena and, in particular, the non-thermal nature of astrophysical plasmas. He uses both analytical and numerical (particle-in-cells simulations) to study how particles can be accelerated to the highest energies in the universe. Such physical mechanisms are at the core of the most violent phenomena in the universe, such as stellar explosions (supernovae, kilonovae, gamma-ray bursts), supernova remnants, active galactic nuclei and their jets, pulsars, and more. He is also interested in other ways of testing particle acceleration in laboratory plasma experiments and through in-situ measurements in the heliosphere, and in the role of non-thermal particles and magnetic fields in galaxy evolution.
Cattaneo’s interests lie in the computational modeling of basic astrophysical processes like the generation of magnetic fields, the transport of angular momentum in accretion discs, or the transport of energy by turbulent convection.
Fabrycky studies the dynamics of extrasolar planets. Over the past two decades, discoveries of planets orbiting other stars have poured in from a variety of different detection techniques, and the resulting menagerie of planetary types and system architectures poses many theoretical issues. Fabrycky studies how the observations constrain the configurations of these exoplanetary systems, as well as how gravitational interactions, tidal effects, and energy dissipation shape them.
Frieman's research centers on theoretical and observational cosmology, including studies of the nature of dark energy, the early Universe, gravitational lensing, the large-scale structure of the Universe, and supernovae as cosmological distance indicators.
Gnedin’s research interests range from General Relativity to physics of the interstellar medium to cosmology. He works on numerical cosmological simulations, including (but not limited to) simulating galaxy formation and evolution of the intergalactic medium.
Hogan's theoretical work has encompassed many areas of astrophysical cosmology: the origin of the elements, cosmic phase transitions and defects, magnetic fields, background radiation, cosmic reionization, gravitational lensing, cosmic structure and dark matter, global cosmological parameters, and gravitational waves. His research has been recognized by prizes including an Alexander von Humboldt Research Award, and the Gruber Cosmology Prize, awarded to the High-z Supernova Search Team for the co-discovery of cosmic Dark Energy.
Holz’s research focuses on gravitational waves. He is particularly interested in what we can learn about physics, astronomy, and cosmology from our detections of gravitational wave sources. He is a member of LIGO.
Hooper's research focuses on the interface between particle physics and cosmology, covering topics such as dark matter, cosmic rays, neutrino astronomy, and the early universe.
Hu's research focuses on the theory and phenomenology of structure formation in the Universe as revealed in Cosmic Microwave Background anisotropies, gravitational lensing, galaxy clustering and galaxy clusters.
Joyce is a theorist with broad interests at the interface between cosmology, high energy physics, and gravity. A primary focus is on the interplay between cosmology and fundamental physics, and how we can use each to learn about the other. He applies effective field theory techniques to gravitational and cosmological questions in order to study the nature of dark energy/dark matter, and to probe the physics of the very early Universe. He also maintains interests in more theoretical questions involving gravity and quantum field theory in a variety of settings.
Kolb's research focuses on theoretical early-universe cosmology involving astrophysics, particle physics, and general relativity. Gravitational particle production during the inflationary era, the origin of the baryon asymmetry, reheating the universe after inflation, and cosmological phase transitions are some of the areas of research.
Kravtsov's research focuses on modelling galaxy formation in cosmological context. His recent research in particular has aimed to understand the processes of star formation and stellar feedback and their effects on galaxy evolution. He also studies properties of dark matter halos, clustering of halos, and galaxy-halo connection.
Rogers studies the formation, interior structure, and evolution of exoplanets. Her research aims to deepen the current understanding of the rich physics governing sub-Neptune-size planet interiors, to discover bulk composition trends in the growing census of known exoplanets, and to connect these composition trends back to distinct planet formation pathways. To pursue these goals, Rogers and her group advance numerical models for the interior, evolution, and formation of small exoplanets, and develop statistical frameworks to connect theory and observations.
Rosner studies astrophysical fluid dynamics and plasma physics problems. Much of his work involves developing new numerical simulation tools for modeling astrophysical phenomena, as well as validating these simulations using terrestrial laboratory experiment
Development Detectors and instrumentation are critical for astronomy and astrophysics. Innovation and development of detector technology enables us to push measurements to higher precision and leads to new, cutting-edge experiments. The Department of Astronomy and Astrophysics has a history of building instrumentation, from cosmic microwave background and cosmic-ray experiments to optical and infrared instrumentation, with many scientific opportunities for developing new detectors and advanced instrumentation through our partners in the Institute for Molecular Engineering Pritzker Nanofabrication Facility, Argonne National Laboratory and Fermilab.
Astronomy and Astrophysics faculty in experiment
Benson is an experimental cosmologist, who uses measurements of the cosmic microwave background (CMB) and clusters of galaxies to constrain the physics of the Big Bang, dark energy, and neutrinos. He works on mm-wavelength detectors and instrumentation, and has had a leading role in the development of multiple cameras for the South Pole Telescope (SPT). He is working on the development of the next-generation CMB-S4 project, expected to improve CMB-based constraints by over an order of magnitude.
Carlstrom is the director of the South Pole Telescope (SPT) project, which probes inflation, enables precision measurements of cosmological parameters and investigations of extensions to the standard model, such as the number and masses of the neutrinos, and the nature of dark energy. SPT enables direct detections of the emergence and evolution of structure in the universe through the small-angular-scale distortions they impart on the background, such as gravitational lensing from the mass in the universe and the scattering from ionized gas (the SZ effects).
Chang’s interests focus on observational cosmology with a particular emphasis on developing new superconducting technology for use in new experiments. He is part of a joint Chicago/Argonne superconducting detector development collaboration which developed and built the focal plane for the SPT-3G experiment. This focal plane, with over 15,000 polarization sensitive detectors, will enable the South Pole Telescope to observe 2500 square degrees with unprecedented sensitivity.
McMahon is an experimentalist who studies cosmology and fundamental physics through measurements of the cosmic microwave background (CMB). CMB signals, including its polarization, gravitational lensing, and small scale secondary anisotropies, have yet to be fully exploited. Measurement of the spatial pattern of CMB polarization will constrain the energy scale of inflation. Measurement of CMB lensing will provide a tight constraint on the sum of the neutrino masses and through cross-correlations with external data sets will provide a measurement of astrophysical bias. He works with the Atacama Cosmology Telescope and Simons Observatory.
As an experimental particle physicist at CERN, Privitera measured the properties of fundamental particles as the Z and W bosons, the lepton and the b quark. Privitera's group went on to study ultra-high energy cosmic rays (UHECRs) with the Pierre Auger Observatory. Current efforts include the development of compact Fluorescence Detectors and measurements of UHECRs composition and anisotropy. He is also leading DAMIC-M, an experiment for direct detection of dark matter based on advanced CCD technology.
Shirokoff builds novel superconducting detectors, and uses them to study high redshift galaxies and the CMB. He uses modern thin-film processes and electromagnetic simulation software to move optical elements on-chip, replacing mechanical hardware with planar circuits. He works with kinetic inductance detectors (KIDs), which can be used to fabricate novel instruments for millimeter and submillimeter wavelength astronomy and cosmology.