Education & Professional Experience
M.S.: Northwestern University (2014)
B.S.: Utah State University (2012)
Assistant Professor at Carnegie Mellon, 2023-
Flatiron Research Fellow at the Flatiron Institute's Center for Computational Astrophysics, 2020-2023
CITA Fellow at the Canadian Institute for Theoretical Astrophysics, 2018-2020
Research Interests
Binary stars are a crucial component or limiting factor in nearly every field of astrophysics from compact object formation, to exoplanet characterization, to galaxy formation, and cosmology. I work at the interface of theory, simulations, and data to understand how binary-star interactions shape stellar populations as they evolve from birth to death. I spend a lot of time thinking about the best ways to combine simulations of binary populations and data from electromagnetic surveys like Gaia and SDSS-V with gravitational wave observatories like LIGO and LISA to study binary star populations at different snapshots in their evolution and ultimately constrain the outcomes of binary star interactions.
I also spend a lot of time developing software tools which simulate binary star populations and their observable properties in electromagnetic and gravitational-wave surveys. All of the code I write and use is publicly developed and available for use on GitHub including , a binary population synthesis suite, and , a signal to noise calculation tool for LISA. I am also a strong proponent of reproducibility in science and use in my research workflow to ensure that my results are reproducible and accessible to the scientific community.
Selected Publications
Wong, Kaze W. K., Breivik, Katelyn, Farr, Will M., Luger, Rodrigo, Backward Population Synthesis: Mapping the Evolutionary History of Gravitational-Wave Progenitors,
Chawla, Chirag, Chatterjee, Sourav, Breivik, Katelyn, Moorthy, Chaithanya Krishna, Andrews, Jeff J., Sanderson, Robyn E., Gaia May Detect Hundreds of Well-characterized Stellar Black Holes,
Wagg, Tom, Breivik, Katelyn, de Mink, Selma, LEGWORK: A python package for computing the evolution and detectability of stellar-origin gravitational-wave sources with space-based detectors,
Thiele, Sarah, Breivik, Katelyn, Sanderson, Robyn E., Applying the metallicity-dependent binary fraction to double white dwarf formation: Implications for LISA,
Wong, Kaze W. K., Breivik, Katelyn, Kremer, Kyle, Callister, Thomas, Joint constraints on the field-cluster mixing fraction, common envelope efficiency, and globular cluster radii from a population of binary hole mergers via deep learning,
Breivik, Katelyn, Mingarelli, Chiara M. F., Larson, Shane L., Constraining Galactic Structure with the LISA White Dwarf Foreground,
Breivik, Katelyn, Coughlin, Scott, Zevin, Michael, Rodriguez, Carl L., Kremer, Kyle, Ye, Claire S., Andrews, Jeff J., Kurkowski, Michael, Digman, Matthew C., Larson, Shane L., Rasio, Frederic A., COSMIC Variance in Binary Population Synthesis,
Andrews, Jeff J., Breivik, Katelyn, Pankow, Chris, D'Orazio, Daniel J., Safarzadeh, Mohammadtaher, LISA and the Existence of a Fast-merging Double Neutron Star Formation Channel,
Breivik, Katelyn, Chatterjee, Sourav, Andrews, Jeff J., Constraining Compact Object Formation with 2M0521,
Breivik, Katelyn, Kremer, Kyle, Bueno, Michael, Larson, Shane L., Coughlin, Scott, Kalogera, Vassiliki, Characterizing Accreting Double White Dwarf Binaries with the Laser Interferometer Space Antenna and Gaia,
Breivik, Katelyn, Chatterjee, Sourav, Larson, Shane L., Revealing Black Holes with Gaia,
Breivik, Katelyn, Rodriguez, Carl L., Larson, Shane L., Kalogera, Vassiliki, Rasio, Frederic A., Distinguishing between Formation Channels for Binary Black Holes with LISA,
More Publications: