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The search for gravitational wave backgrounds with astrometry
Juan Garcia-Bellido  1@  
1 : Universidad Autonoma de Madrid

Fundamental physics, Early Universe and Primordial Black Holes leave a distinctive signature in a stochastic gravitational wave background at frequencies accross mutiple bands, from pHz to kHz. Precision astrometry could help detect this background by monitoring the positions and proper motions of billions of objects in the sky over decades with high cadence.


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