A generalization of the coordinates used to describe the metric of one type of these entities is named for Boyer and Lindquist. The Lens-Thirring Effect creates frame-dragging around spinning types of these entities. The Reissner- Nordstrom solution satisfies Einstein's field equations for one of these objects with non-zero charge, which along with angular momentum and (*) mass are their only properties according to the n
A generalization of the coordinates used to describe the metric of one type of these entities is named for Boyer and Lindquist. The Lens-Thirring Effect creates frame-dragging around spinning types of these entities. The Reissner- Nordstrom solution satisfies Einstein's field equations for one of these objects with non-zero charge, which along with angular momentum and (*) mass are their only properties according to the no-hair theorem. The greatest mass a neutron star can have before becoming one is the TOV limit. They emit Hawking radiation and exhibit gravitational singularities under their event horizons. For 10 points, name these massive regions in space from which nothing can escape.
A generalization of the coordinates used to describe the metric of one type of these entities is named for Boyer and Lindquist.