Detection of Black Holes
Schwarzschild Radius and Event Horizon
The Principle of Superposition and the Gravitational Field
Gravitation Between Spherically Symmetric Masses
Conservation of Angular Momentum: Application
Reduced Mass Coordinates: Isolated Two-body Problem
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Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
Yifan Lu1, Zachary S C Picker1, Alexander Kusenko1,2
1Department of Physics and Astronomy, <a href="https://ror.org/046rm7j60">University of California Los Angeles</a>, Los Angeles, California 90095-1547, USA.
Researchers explored how supermassive black holes (SMBHs) form at high redshifts. They found that a Lyman-Werner (LW) background can trigger direct collapse, enabling SMBH formation.
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