Jeff Oishi Headshot

Jeff Oishi

Associate Chair, Mechanical Engineering
Associate Professor
Phone: (603) 862-4898
Office: UNH CEPS Mechanical Engineering, Kingsbury Hall, Durham, NH 03824
Websites:
Pronouns: He/him/his

<p>I lead the UNH Complicated Fluids group. We are interested in the basic physics of a wide array of fluid problems, including biophysical and geophysical flows. As the name implies, we solve&nbsp;<strong>complicated</strong> fluid dynamics: problems involving turbulence, phase changes, magnetic fields, traditional "complex" non-Newtonian fluids, or various combinations of them.&nbsp;<br>In order to tackle this menagerie of problems, we contribute to and use the <a href="http://dedalus-project.org">Dedalus Project</a>, a flexible framework for solving partial differential equations.&nbsp;<br>Prof. Oishi is one of the founders and core developers of Dedalus, and the other developers regularly visit and collaborate with our group.</p>

Courses Taught

  • ME 795/895: Special Topics

Education

  • Ph.D., Astronomy, University of Virginia

Selected Publications

  • Oishi, J. S., & Brown, B. P. (2025). On the linear stability of partially and fully saturated atmospheres to moist convection. Journal of Fluid Mechanics, 1007. doi:10.1017/jfm.2025.125

  • Saxton, C. J., Marston, J. B., Oishi, J. S., & Tobias, S. M. (2024). Ordering of time scales predicts applicability of quasilinear theory in unstable flows. Journal of Fluid Mechanics, 998. doi:10.1017/jfm.2024.810

  • Vasil, G. M., Lecoanet, D., Augustson, K., Burns, K. J., Oishi, J. S., Brown, B. P., . . . Julien, K. (2024). The solar dynamo begins near the surface.. Nature, 629(8013), 769-772. doi:10.1038/s41586-024-07315-1

  • Cresswell, I. G., Anders, E. H., Brown, B. P., Oishi, J. S., & Vasil, G. M. (2023). Force balances in strong-field magnetoconvection simulations. Physical Review Fluids, 8(9). doi:10.1103/physrevfluids.8.093503

  • Oishi, J. S., & Baxter, M. (2023). Generalized quasi-linear approximation and non-normality in Taylor-Couette spiral turbulence.. Philos Trans A Math Phys Eng Sci, 381(2243), 20220122. doi:10.1098/rsta.2022.0122

  • Anders, E. H., Lecoanet, D., Cantiello, M., Burns, K. J., Hyatt, B. A., Kaufman, E., . . . Jermyn, A. S. (2023). The photometric variability of massive stars due to gravity waves excited by core convection.. Nat Astron, 7(10), 1228-1234. doi:10.1038/s41550-023-02040-7

  • Oishi, J. S., Vasil, G. M., Baxter, M., Swan, A., Burns, K. J., Lecoanet, D., & Brown, B. P. (2020). The magnetorotational instability prefers three dimensions.. Proc Math Phys Eng Sci, 476(2233), 20190622. doi:10.1098/rspa.2019.0622

  • Pearce, P., Song, B., Skinner, D. J., Mok, R., Hartmann, R., Singh, P. K., . . . Dunkel, J. (2019). Flow-Induced Symmetry Breaking in Growing Bacterial Biofilms.. Phys Rev Lett, 123(25), 258101. doi:10.1103/PhysRevLett.123.258101

  • Lecoanet, D., Le Bars, M., Burns, K. J., Vasil, G. M., Brown, B. P., Quataert, E., & Oishi, J. S. (2015). Numerical simulations of internal wave generation by convection in water.. Phys Rev E Stat Nonlin Soft Matter Phys, 91(6), 063016. doi:10.1103/PhysRevE.91.063016

  • Johansen, A., Oishi, J. S., Mac Low, M. -M., Klahr, H., Henning, T., & Youdin, A. (2007). Rapid planetesimal formation in turbulent circumstellar disks.. Nature, 448(7157), 1022-1025. doi:10.1038/nature06086

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  • Most Cited Publications