6 November 2013
Venue: Maths 103
Attempts to explain the current acceleration of the expansion of the Universe typically introduce new scalar degrees of freedom that we call dark energy. Detecting dark energy and understanding its properties is therefore a vital part of understanding how to resolve the cosmological constant problem. Dark energy scalar fields will interact with Standard Model fields. In this talk I will discuss these interactions and their phenomenological consequences, with the goal of finding a way to detect dark energy in the laboratory.