Starts 2 Jul 2019 11:00
Ends 2 Jul 2019 12:00
Central European Time
Former SISSA Bldg.
Lecture Room D
Abstract. In this talk I will assume models where Dark Matter (DM) can be described as a classical oscillating (scalar, vector or a spin-2 tensor) field. I will summarize recent work where we study secular effects that this kind of DM has on the dynamics of binary pulsars.
--- Please note unusual time and venue!! ---