2012

Effects Of Circum-nuclear Disk Gas Evolution And The Spin Of Central Black Holes

Maio, Umberto, Dotti, Massimo, Petkova, Margarita et al.

Understand

Mass and spin are the only two parameters needed to completely characterize black holes in General Relativity.

However, the interaction between black holes and their environment is where complexity lies, as the relevant physical processes occur over a large range of scales.
That is particularly relevant in the case of super-massive black holes (SMBHs), hosted in galaxy centers, and surrounded by swirling gas and various generations of stars.
These compete with the SMBH for gas consumption and affect both dynamics and thermodynamics of the gas itself.

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