McGill.CA / Science / Department of Physics

Physical Society Colloquium

Fantastic dark matter and where to find it

JiJi Fan

Department of Physics
Brown University

Most of the universe we reside in is dark. Only a small fraction (15%) of the total matter is ordinary matter, which is extremely complicated. Our knowledge of ordinary matter is vast, deep and still growing fast. Yet when it comes to the remaining 85% of the matter in the universe, our knowledge is embarrassingly little. We know that it doesn't emit light and cannot be seen directly. That's why it is called “dark matter”. In addition, we know that it interacts with gravity just like ordinary matter.

Given the little knowledge we have about dark matter, there exists a huge zoo of possible dark matter scenarios. I will discuss two fun non-minimal dark matter scenarios I have worked on. In the first possibility, the dark world could be similarly complex as the visible one, full of structures, forces, and matter that are invisible to us. In one concrete realization, the “double-disk dark matter” scenario, a small fraction of all dark matter has dissipative dynamics causing it to cool into a disk within the Milky Way galaxy. This will lead to many testable novel observational consequences. In another possibility, dark matter would behave collectively as waves. The waves overlap with each other and may form stable clumps, the “dark stars”. Depending on the underlying parameters, mergers of binary dark stars could lead to gravitational waves detectable at the LIGO detector.

Friday, November 16th 2018, 15:30
Ernest Rutherford Physics Building, Keys Auditorium (room 112)