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Astrophysics is the study of the physical processes that govern the universe, from the smallest particles to the largest cosmic structures. It seeks to understand phenomena such as black holes, gravitational interactions, and the fundamental nature of matter and energy through both observation and theoretical modeling. By combining gravitational physics, numerical relativity, and particle physics, astrophysicists explore the origins, evolution, and dynamics of astrophysical systems, developing insights into some of the most extreme environments in the universe. Research in astrophysics at Wake emphasizes computational techniques and fundamental questions about gravity and high-energy phenomena.


SCHOLARSHIP

Faculty working in Astrophysics


Eric Carlson

Eric Carlson’s research covers a variety of topics including both particle phenomenology and astrophysics. These topics include pseudoscalar couplings, the existence of a naturally small cosmological constant, and neutrino physics. Carlson believes astroparticle physics to be one of the most promising areas in particle phenomenology in the next decade or two

Not accepting graduate students

Accepting undergraduate students


Greg Cook

Greg Cook’s research interests are in the areas of computational astrophysics and gravitational physics. Currently, his research is centered on studying the coalescence of compact binary systems. Cook and his collaborators are currently developing the theoretical and computational tools needed to simulate the collision of a pair of black holes. to study the ultimate coalescence of a compact binary system.

Accepting graduate students

Accepting undergraduate students


Alejandro Cárdenas-Avendaño

Alejandro Cárdenas-Avendaño’s research explores gravity’s fundamental properties through the gravitational and electromagnetic signals from compact objects like black holes and neutron stars. By combining numerical simulations, theoretical modeling, and data analysis, his group studies phenomena ranging from gravitational waveform signatures to black hole photon rings.

Accepting graduate students

Accepting undergraduate students


Caitlin Witt

Caitlin Witt’s research interests are in the areas of observational and computational astrophysics. Her research is centered on studied supermassive black hole binaries using multimessenger astrophysics, where she combines electromagnetic and gravitational-wave data. Witt and her collaborators use pulsars to search for decades-long gravitational wave signals, time-domain optical surveys to search for binaries, and supercomputers to analyze the data to provide a complete picture of the aftermath of galaxy mergers.

Accepting graduate students

Accepting undergraduate students

Recent Publications in Astrophysics


  1. Bécsy, B., Cornish, N. J., Petrov, P., Siemens, X., Taylor, S. R., Vigeland, S. J., & Witt, C. A. (2025). Towards robust gravitational wave detections from individual supermassive black hole binaries. Classical and Quantum Gravity, 42(17), 175016. https://doi.org/10.1088/1361-6382/adfd36
  2. Gao, L., Cook, G. B., Kidder, L. E., Pfeiffer, H. P., Scheel, M. A., Deppe, N., Throwe, W., Vu, N. L., Nelli, K. C., Moxon, J., & Boyle, M. (2025). Robustness of extracting quasinormal mode information from black hole merger simulations. Physical Review D, 112(2). https://doi.org/10.1103/3jj6-jc8q
  3. Keeble, L. S., & Cárdenas-Avendaño, A. (2025). Estimating high-order time derivatives of Kerr orbital functionals. Physical Review D, 112(8). https://doi.org/10.1103/g26m-mz4v
  4. Magaña Zertuche, L., Gao, L., Finch, E., & Cook, G. B. (2025). Multimode ringdown modeling with qnmfits and KerrRingdown. Classical and Quantum Gravity, 42(19), 197001. https://doi.org/10.1088/1361-6382/ae0233
  5. Motta, P. N., Prather, B. S., & Cárdenas-Avendaño, A. (2025). Jipole: A Differentiable ipole-based Code for Radiative Transfer in Curved Spacetimes. The Astrophysical Journal, 995(1), 56. https://doi.org/10.3847/1538-4357/ae16a0
  6. Sardesai, S. C., Freedman, G. E., Vigeland, S. J., & Witt, C. A. (2025). Optimal strategies for continuous wave detection in pulsar timing arrays: Realistic pulsar noise and a gravitational wave background. arXiv. https://doi.org/10.48550/arXiv.2511.01919
  7. Siggia, V. R., & Carlson, E. D. (2025). Comparison of f(R,T) gravity with type Ia supernovae data. Physical Review D, 111(2). https://doi.org/10.1103/physrevd.111.024074
  8. Siggia, V. R., Carlson, E. D., & Pryor, P. L. (2025). Exploration of Parameters in f(R,T) Gravity and Comparison with Type Ia Supernovae Data. arXiv. https://doi.org/10.48550/arXiv.2508.15014