Speaker
Juan Carlos Degollado
Description
In this talk I will describe quasi-stationary solutions of the
Einstein-Klein-Gordon equations for a scalar field surrounding a black hole.
The solutions cover scales from; less than a Schwarzschild radius to several orders of
magnitude its value. These self gravitating gravitational
atoms are relevant in a wide range of masses, from ultralight to MeV dark
matter and for black holes ranging from primordial to supermassive.
Author
Juan Carlos Degollado
