Physical Society Colloquium
Searching for the invisible: how dark forces shape our
Universe
Department of Physics MIT
How different would our Universe look with the addition of extra particles and
forces beyond what we know? We already have ample gravitational evidence for
at least one invisible new particle that has properties unlike any particle
we have previously discovered. It is possible that this dark matter is made
of many different kinds of particles that experience forces unlike the ones
we are familiar with in day-to-day life. If these forces only act on dark
particles, it may be difficult to discover them and learn more about what
is happening in this dark sector. However, dark matter and visible matter
do interact gravitationally at the very minimum, and this fact alone might
be a good reason not to lose hope. If there are dark forces affecting the
distribution of dark matter in our Universe, then that distribution will
gravitationally affect the visible matter that we can see. I will discuss how
the gravitational portal between dark and visible matter can constrain dark
matter theories where dark matter can dissipate energy, can scatter with itself
(elastically or inelastically), or can be born non-thermally in the moments
after the Big Bang. I will demonstrate this constraining power by harnessing
synergies between astrophysical systems including the local Milky Way, nearby
dwarf galaxies, galaxy clusters, and large scale cosmological structures.
Friday, November 1st 2019, 15:30
Ernest Rutherford Physics Building, Keys Auditorium (room 112)
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