Astrophysics Colloquium: Supermassive Black Holes in the Early Universe: from Luminous Quasars to the Little Red Dots

Watch the Zoom recording; Passcode: 8r4vf@+B

Abstract: I will first review the progress in surveys of the most distant quasars, including the latest record-breaking quasars discovered by Euclid at z>7.5. They are powered by billion solar mass black holes, possible only by a combination of massive early black hole seeds with highly efficient and sustained accretion. I will present results of surveys of early quasars and their environments using JWST. While rapid early black hole growth is accompanied by intense star formation and feedback in their host galaxies, the diverse quasar environment unveiled by these observations suggests a complex interplay between black hole accretion, galaxy assembly, the physics of reionization and the emergence of early large scale structure. JWST observations have revealed a new population of active galactic nuclei (AGN), the "Little Red Dots" (LRDs), with high abundance and multiwavelength properties different from those of typical AGN and quasars. I will discuss the observations of LRDs and constraints on their physical nature in relation to early black hole growth. A subset of LRDs, both those discovered at high-redshift with JWST, and detected in the local universe, strongly suggest the presence of optically-thick gas envelops surrounding the central energy source, consistent with scenarios of super-Eddington accretion, and could be the missing link between black hole seeds and luminous early quasars.