My work to date has employed novel sub-Kelvin detector systems to address two mysteries of our cosmos: What is the nature of the dark matter that governs the dynamics of large-scale structure? What spurred the inflationary epoch that begins our narrative of cosmological history? This work bridges several sub-disciplines of physics and astrophysics, linking the grand questions of fundamental physics with the quantum phenomena that enable the most sensitive measurements. Solving these mysteries will demand new fundamental physics, and measurements at the "cosmic frontier" are poised to play a central role. Our universe appears to be filled with forms of matter and energy unlike anything on Earth, and many key aspects of cosmic evolution remain to be understood. We can now recount the life story of our cosmos in remarkable detail, yet our data reveal a humbling degree of ignorance about its workings. My research interests lie at the intersection between the universe's workings on its largest and smallest scales. He joined the faculty of the University of Illinois in December 2014. As a postdoctoral researcher at Caltech he developed balloon-borne and terrestrial instruments to measure the polarization of the cosmic microwave background radiation. His doctoral work focused on the search for dark matter interactions in subterranean detectors. Professor Filippini earned his bachelor's degree in Chemistry and Physics from Harvard in 2002 and his Ph.D. Chemistry and Physics summa cum laude, Harvard University, 2002 ![]() ![]() Physics, University of California, Berkeley, 2004 Physics, University of California, Berkeley, 2008 405 Loomis Laboratory For More Information
0 Comments
Leave a Reply. |
AuthorWrite something about yourself. No need to be fancy, just an overview. ArchivesCategories |