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What Does a Black Hole Look Like?$
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Charles D. Bailyn

Print publication date: 2014

Print ISBN-13: 9780691148823

Published to Princeton Scholarship Online: October 2017

DOI: 10.23943/princeton/9780691148823.001.0001

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Formation and Evolution of Black Holes

Formation and Evolution of Black Holes

Chapter:
(p.106) 6 Formation and Evolution of Black Holes
Source:
What Does a Black Hole Look Like?
Author(s):

Charles D. Bailyn

Publisher:
Princeton University Press
DOI:10.23943/princeton/9780691148823.003.0006

This chapter discusses the formation and evolution of black holes. Stellar-mass black holes are generally understood to be created in supernova explosions that mark the end of the life of a massive star. However, many supernovae create neutron stars rather than black holes, and the precise conditions under which black holes form are still not fully understood. If the black hole is to be detected, further events are required, such as the formation of a binary star system of a kind that can be observed, and in which the existence of a black hole can be demonstrated. In contrast with stellar-mass black hole formation, there is no obvious route to the creation of a supermassive black hole directly from collapsing interstellar gas. Most discussions of the origin and evolution of supermassive black holes posit an initial “seed” black hole of relatively low mass, which then grows over time.

Keywords:   stellar-mass black holes, supernova explosions, supernovae, binary star system, supermassive black holes, black hole formation, black hole evolution

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