Professor Bullock received a B.S. in both Physics and Math from The Ohio State University in 1994 and a Ph.D. in Physics from the University of California, Santa Cruz in 1999. After postdoctoral positions at The Ohio State University and Harvard University, he came to UC Irvine as an Assistant Professor in 2004. He was elected Fellow of the American Association for the Advancement of Science in 2008. Professor Bullock served as the 17th Chair of the UCI Physics and Astronomy Department from 2017-2019 before becoming the 9th Dean of the UCI School of Physical Sciences in 2019.
Aided by super-computer simulations and analytic models, Professor Bullock studies how galaxies and their constituent dark matter halos have formed and evolved over billions of years of cosmic time. By analyzing data that astronomers have collected using the Hubble Space Telescope, the Keck Observatory, and other ground and space telescopes, he works to understand how galaxies, including the Milky Way and its Local Group of galaxies, emerged from the primordial universe. One of his long-standing interests has been the use of astrophysical observations to constrain the microphysical nature of dark matter.
Professor Bullock currently serves as Chair of the James Webb Space Telescope User’s Committee. Previously he was Chair of the working group that recommended the Hubble Frontier Fields Program, which is responsible for galaxy cluster image on the top of this page. He is passionate about science outreach and appears regularly on the Science Channel’s How the Universe Works.
Areas of Expertise (5)
University of California, Santa Cruz: PhD, Physics 1999
The Ohio State University: BS, Physics and Math 1994
Media Appearances (4)
James Bullock to become new dean of UCI School of Physical Sciences
UCI News online
James Bullock, professor and chair of physics & astronomy at the University of California, Irvine, has been appointed dean of the School of Physical Sciences. He will assume the new role on July 1, upon the retirement of Dean Kenneth Janda.
UCI celestial census indicates that black holes pervade the universe
UCI News online
“We think we’ve shown that there are as many as 100 million black holes in our galaxy,” said UCI chair and professor of physics & astronomy James Bullock, co-author of a research paper on the subject in the current issue of Monthly Notices of the Royal Astronomical Society.
UCI astronomer is appointed to chair users committee for James Webb Space Telescope
UCI News online
UCI astronomer James Bullock has been appointed chair of the James Webb Space Telescope users committee. The group, which includes 10 to 14 American, European and Canadian scientists, was established to ensure that the observatory is operated in such a way as to maximize its scientific performance. The JWST, successor to the Hubble Space Telescope, is scheduled to launch in late 2018. From its position in outer space, more than a million miles from Earth, the telescope will study exoplanets in the Milky Way and the earliest stars and galaxies in the universe in infrared and visible light wavelengths. “We expect to achieve some amazing scientific breakthroughs with Webb,” said Bullock, professor of physics & astronomy. “But it’s important that we coordinate our efforts as astronomers here on Earth so that we’re using this valuable tool in the most effective way possible.” The users committee will convene twice a year, with the first meeting at Baltimore’s Space Telescope Science Institute in mid-September.
Dark Matter May Be More Complex Than Physicists Thought
About four years ago, James Bullock, a professor of physics and astronomy at the University of California, Irvine, began to wonder whether the standard view of dark matter was failing important empirical tests. “This was the point where I really started thinking hard about alternatives,” he said.
Alexandres Lazar, James S Bullock
2020 We derive a new mass estimator that relies on internal proper motion measurements of dispersion-supported stellar systems, one that is distinct and complementary to existing estimators for line-of-sight velocities. Starting with the spherical Jeans equation, we show that there exists a radius where the mass enclosed depends only on the projected tangential velocity dispersion, assuming that the anisotropy profile slowly varies.
Jenna Samuel, Andrew Wetzel, Erik Tollerud, Shea Garrison-Kimmel, Sarah Loebman, Kareem El-Badry, Philip F Hopkins, Michael Boylan-Kolchin, Claude-André Faucher-Giguère, James S Bullock, Samantha Benincasa, Jeremy Bailin
2019 While many tensions between Local Group (LG) satellite galaxies and Λ cold dark matter cosmology have been alleviated through recent cosmological simulations, the spatial distribution of satellites remains an important test of physical models and physical versus numerical disruption in simulations.
Juna A Kollmeier, Lauren Anderson, Andrew Benson, Tamara Bogdanovic, Michael Boylan-Kolchin, James S Bullock, Romeel Dave, Federico Fraschetti, Jim Fuller, Philip F Hopkins, Manoj Kaplinghat, Kaitlin Kratter, Astrid Lamberts, M Coleman Miller, James E Owen, E Sterl Phinney, Anthony L Piro, Hans-Walter Rix, Brant Robertson, Andrew Wetzel, Coral Wheeler, Andrew N Youdin, Matias Zaldarriaga
2019 The past two decades have seen a tremendous investment in observational facilities that promise to reveal new and unprecedented discoveries about the universe. In comparison, the investment in theoretical work is completely dwarfed, even though theory plays a crucial role in the interpretation of these observations, predicting new types of phenomena, and informing observing strategies.
Sijie Yu, James S Bullock, Andrew Wetzel, Robyn E Sanderson, Andrew S Graus, Michael Boylan-Kolchin, Anna M Nierenberg, Michael Y Gurdić, Philip F Hopkins, Dušan Kereš, Claude-André Faucher-Giguère
2019 We study stellar-halo formation using six Milky Way-mass galaxies in FIRE-2 cosmological zoom simulations. We find that 5−40% of the outer (50−300 kpc) stellar halo in each system consists of in-situ stars that were born in outflows from the main galaxy. Outflow stars originate from gas accelerated by super-bubble winds, which can be compressed, cool, and form co-moving stars.
Coral Wheeler, Philip F Hopkins, Andrew B Pace, Shea Garrison-Kimmel, Michael Boylan-Kolchin, Andrew Wetzel, James S Bullock, Dušan Kereš, Claude-André Faucher-Giguère, Eliot Quataert
2019 We study a suite of extremely high-resolution cosmological Feedback in Realistic Environments simulations of dwarf galaxies (Mhalo≲1010M⊙), run to z = 0 with 30M⊙ resolution, sufficient (for the first time) to resolve the internal structure of individual supernovae remnants within the cooling radius. Every halo with Mhalo≳108.6M⊙ is populated by a resolved stellar galaxy, suggesting very low-mass dwarfs may be ubiquitous in the field.