Guariento, D. (2014). Evolution of cosmological black holes: exact solutions, accretion and scalar fields. Perimeter Institute for Theoretical Physics. https://pirsa.org/14020150
MLA
Guariento, Daniel. Evolution of cosmological black holes: exact solutions, accretion and scalar fields. Perimeter Institute for Theoretical Physics, Feb. 18, 2014, https://pirsa.org/14020150
BibTex
@misc{ scivideos_PIRSA:14020150,
doi = {10.48660/14020150},
url = {https://pirsa.org/14020150},
author = {Guariento, Daniel},
keywords = {Cosmology},
language = {en},
title = {Evolution of cosmological black holes: exact solutions, accretion and scalar fields},
publisher = {Perimeter Institute for Theoretical Physics},
year = {2014},
month = {feb},
note = {PIRSA:14020150 see, \url{https://scivideos.org/index.php/pirsa/14020150}}
}
Systems which contemplate the gravitational interaction between compact objects and the matter content in a cosmological environment constitute an important problem which has been studied since the early days of General Relativity. The generalized McVittie black hole is a simple exact solution to this problem, which provides us with insight on some of its known physical aspects, as well as hints to new mechanisms which arise from a formal treatment. We review some properties of this solution and its matter source, which can be interpreted as a classical fluid but is also an exact solution to a nontrivial scalar field theory.
