Stefano Maro
Postdoctoral Researcher
Mathematics
Complutense University of Madrid
Spain
Biography
"Born in Italy in 1986 I completed my undergraduate studies at the Università degli Studi di Torino in 2010 and got the Ph.D from the same University in 2014. I defended a thesis with title ''Symplectic methods in ODEs'' developed under the supervision of Rafael Ortega, from the Universidad de Granada. At the end of 2013, I joined the Marie Curie ITN ""Stardust"" with an ESR grant at the University of Pisa, where I studied the applications of Hamiltonian Mechanics and Celestial Mechanics to the dynamics of asteroids. At the moment I have a Severo-Ochoa postdoctoral grant at the ICMAT where I am continuing my studies on Hamiltonian Dynamics, Dynamical Systems and Celestial Mechanics."
Research Interest
Hamiltonian Dynamics, Dynamical Systems and Celestial Mechanics.
Publications
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Maro, Stefano. "Relativistic pendulum and invariant curves." arXiv preprint arXiv:1304.8017 (2013).
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Novaković, Bojan, et al. "Secular evolution of asteroid families: the role of Ceres." Proceedings of the International Astronomical Union 10.S318 (2015): 46-54.
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Marò, S. (2013). Periodic solutions of a forced relativistic pendulum via twist dynamics. Topological Methods in Nonlinear Analysis, 42(1), 51-75.
