Summary
Carlo Graziani is a computational scientist and theoretical astrophysicist with decades of research experience who applies Bayesian statistics and Gaussian process modeling to extract faint signals from large astronomical datasets and HPC simulations. Based at Argonne and affiliated with the University of Chicago, he has driven methodological breakthroughs—from correcting long-standing MHD algorithm errors to inventing analysis techniques that enable smaller, cheaper dark-matter detectors. His work spans theory, experiment, and statistical methodology, with a track record of turning complex simulation output and detector data into actionable physical insight. An experienced communicator and mentor, he has led mission imaging pipelines for gamma-ray bursts and translated plasma physics measurements into intelligible diagnostics, demonstrating a rare blend of deep physics intuition and practical algorithmic impact.
10 years of coding experience
15 years of employment as a software developer
High School Diploma, High School Diploma at International School of Milan
B.Sc., Applied Physics, B.Sc., Applied Physics at Columbia University
Ph.D., Physics, Ph.D., Physics at University of Chicago
Italian, French