Physical Society Colloquium
Fantastic dark matter and where to find it
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)
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