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PUEO is a balloon mission designed to launch from Antarctica that will detect signals from ultra-high energy neutrinos, particles that contain valuable clues about the highest energy astrophysical processes, including the creation of black holes and neutron star mergers. Neutrinos travel across the universe undisturbed, carrying information about events billions of light years away. PUEO would be the most sensitive survey of cosmic ultra-high energy neutrinos ever conducted. The principal investigator is Abigail Vieregg of the University of Chicago.

His work involves exploiting superheated liquid techniques in sensitive bubble chambers for direct dark matter detection experiments.

He studies cosmology, where he analyzes the faint microwave signal coming from the beginning of our universe to help answer questions in fundamental physics.

As a sixth year PhD candidate in the Department of Astronomy and Astrophysics, Gourav studies the formation and evolution of galaxies in distant galaxy clusters, using data from ground- and space-based telescopes.

UChicago scientist lays out how LIGO gravitational waves could be scrambled, yielding information.
“Gravitational waves are the perfect messenger to see these possible modifications of gravity, if they exist.”—Astrophysicist Jose María Ezquiaga

John E. Carlstrom, Chair and the Subramanyan Chandrasekhar Distinguished Service Professor of Astronomy & Astrophysics, is a leading figure in the study of the cosmic microwave background—the light left over from the first few moments of the universe, has been named a 2020 AAAS Fellow.

I have worked extensively with both the South Pole Telescope (SPT) and the Dark Energy Survey(DES) collaborations in the past years, and I am currently the contact person for many of the projects that involve both collaborations. I am additionally the acting organizer for the joint telecons, and I am planning to continue serving as the bridge between the two collaborations.

My work over the past few years has focussed mainly on cluster scale physics from a theoretical and observational perspective.

He has accepted a position as a Consultant at Bain & Company in Chicago, and in this capacity he will focus on strategy and management.

The Kavli Institute for Cosmological Physics (KICP) has secured $10 million in new funding through two gifts: a $5 million gift from an anonymous alumnus and his wife and a match of $5 million from The Kavli Foundation. The first gift will name the directorship of the Institute in memory of Prof. David N. Schramm, a legendary professor of theoretical astrophysics at the University of Chicago.

My principle research interest is gravitational lensing and observational cosmology. I am currently working with Professor Tommaso Treu on time-delay cosmography.

My research interests lie in Cosmology. So far, I have studied the early Universe in terms of primordial black holes (PBHs), gravitational waves (GWs), cosmic microwave background (CMB), and big bang nucleosynthesis (BBN).

Burcin is a lead member of several large-scale imaging surveys, and uses observations of small and faint (dwarf) galaxies to study the smallest dark matter halos, and how they get populated with stars.

I am a theoretical astrophysicist, working at the interface of astrophysics, cosmology, high energy theoretical physics, and particle physics.

I am a Kavli Institute for Cosmological Physics (KICP) Fellow and Postdoctoral Researcher at UChicago, where I actively participate in the Survey Science group.