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Miguel Zumalacarregui (UC Berkeley & IPhT Saclay)

Date: Tue. September 18th, 2018, 11:30 am-12:30 pm
Location: Foldy Room

The Dark Universe in the Gravitational Wave Era
Evidence shows that we live in a universe where 95% of the matter and energy is of unknown nature. Right from the onset, Gravitational Wave (GW) astronomy is shaping our understanding of the dark universe in several ways: GW signals of black hole mergers have resurrected the idea of Dark Matter being made of primordial black holes, while multi-messenger GW astronomy has generated novel ways to test Dark Energy and the fundamental properties of gravity. I will discuss the impact of gravitational waves on the landscape of gravitational theories, and how the recent observation of a neutron star merger spectacularly rules out a large class of Dark Energy models in which the speed of GWs is variable, including some (otherwise viable) contenders to the cosmological constant. Then I will present how gravitational lensing of distant supernovae constrains the abundance of primordial black holes, which can not be the dominant form of Dark Matter.

Host: Kurt Hinterbichler

Page last modified: September 6, 2018