On galactic scales, structure is gravitationally held by dark matter, while stars and  gas present merely an “icing on the cake.” In spite of their dominance over the matter budget in the universe, particle constituents of dark matter have eluded detection and characterization to the present day. This talk will focus on a variety of promising new techniques that will help corner dark matter particles in the coming decade of synergistic searches through precision measurements of direct detection experiments and cosmological surveys.

Salads, sandwiches, and wraps are catered by D'Angelo Italian Market.

Bottled water will be provided.

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