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

• Superior document: Title is part of eBook package: De Gruyter Princeton University Press Complete eBook-Package 2014-2015
• VerfasserIn: Bailyn, Charles D.,
• Place / Publishing House: Princeton, NJ : : Princeton University Press, , [2014]; ©2014
• Year of Publication: 2014
• Edition: Course Book
• Language: English
• Series: Princeton Frontiers in Physics ; 4
• Physical Description: 1 online resource (224 p.) :; 21 line illus.
• Other title: Frontmatter --; Contents --; Preface --; 1. Introducing Black Holes: Event Horizons and Singularities --; 2. Accretion onto a Black Hole --; 3. Outflows and Jets --; 4. Stellar-Mass Black Holes --; 5. Supermassive Black Holes --; 6. Formation and Evolution of Black Holes --; 7. Do Intermediate-Mass Black Holes Exist? --; 8. Black Hole Spin --; 9. Detecting Black Holes through --; 10. Black Hole Exotica --; Glossary --; Index
• Format: Mode of access: Internet via World Wide Web.
• ISBN: 9781400850563; 9783110665925
• DOI: 10.1515/9781400850563?locatt=mode:legacy
• Access: restricted access
• Hierarchical level: Monograph
• Statement of Responsibility: Charles D. Bailyn.

Emitting no radiation or any other kind of information, black holes mark the edge of the universe--both physically and in our scientific understanding. Yet astronomers have found clear evidence for the existence of black holes, employing the same tools and techniques used to explore other celestial objects. In this sophisticated introduction, leading astronomer Charles Bailyn goes behind the theory and physics of black holes to describe how astronomers are observing these enigmatic objects and developing a remarkably detailed picture of what they look like and how they interact with their surroundings.Accessible to undergraduates and others with some knowledge of introductory college-level physics, this book presents the techniques used to identify and measure the mass and spin of celestial black holes. These key measurements demonstrate the existence of two kinds of black holes, those with masses a few times that of a typical star, and those with masses comparable to whole galaxies--supermassive black holes. The book provides a detailed account of the nature, formation, and growth of both kinds of black holes. The book also describes the possibility of observing theoretically predicted phenomena such as gravitational waves, wormholes, and Hawking radiation.A cutting-edge introduction to a subject that was once on the border between physics and science fiction, this book shows how black holes are becoming routine objects of empirical scientific study.