Black Holes in the Early Universe
Marta Volonteri, Jillian Bellovary

TL;DR
This paper reviews the formation and evolution of massive black holes in the early universe, discussing their origins, growth, and relationship with galaxy development, highlighting ongoing research questions.
Contribution
It provides a comprehensive overview of the current understanding and key questions about the formation and growth of massive black holes in the early cosmos.
Findings
Massive black holes existed within the first billion years of the universe.
Black holes with billions of solar masses powered early quasars.
Black holes today are dormant remnants of past active phases.
Abstract
The existence of massive black holes was postulated in the sixties, when the first quasars were discovered. In the late nineties their reality was proven beyond doubt, in the Milky way and a handful nearby galaxies. Since then, enormous theoretical and observational efforts have been made to understand the astrophysics of massive black holes. We have discovered that some of the most massive black holes known, weighing billions of solar masses, powered luminous quasars within the first billion years of the Universe. The first massive black holes must therefore have formed around the time the first stars and galaxies formed. Dynamical evidence also indicates that black holes with masses of millions to billions of solar masses ordinarily dwell in the centers of today's galaxies. Massive black holes populate galaxy centers today, and shone as quasars in the past; the quiescent black holes…
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