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Sayan Mandal is a Special Lecturer in the Department of Physics at Carnegie Mellon University. He holds a Ph.D. in Theoretical Cosmology from Carnegie Mellon University (2020), an M.S. from Tata Institute of Fundamental Research, Mumbai, India (2016), and a B.E. from Jadavpur University, India (2013). Mandal has contributed to research in cosmology and related fields, with publications in journals such as Phys. Rev. D and Class. Quant. Grav. His work includes studies on dark matter, inflation, and gravitational waves. He is affiliated with the Mellon College of Science and can be contacted via email at sayanm@cmu.edu or through his profile page at https://www.cmu.edu/physics/people/faculty/mandal.html.


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Sayan Mandal is an Adjunct Instructor in the Department of Physics at Carnegie Mellon University, specializing in Cosmology, General Relativity, Quantum Field Theory, Turbulence, and Neutrinos. His research explores the interplay between gravitational waves, early-universe turbulence, and magnetic fields, with a focus on their implications for cosmology and particle physics. Mandal's work includes numerical simulations of gravitational wave generation from turbulence, the evolution of hydromagnetic turbulence, and the polarization of gravitational waves from helical turbulence. He also investigates dark matter and dark energy models, as well as the role of neutrinos in cosmological scenarios.

Source: google_scholar · 94 words
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