Schwarzschild radius
Definition: The horizon radius 2GM/c^2 of a nonrotating uncharged black hole.
Why it matters here: In Black-Hole Dynamics and Relativistic Orbits, Schwarzschild radius is needed to reason about Schwarzschild radius, ISCO, time dilation, and observational boundaries rather than merely label the phenomenon.
Relationship: It is interpreted alongside Event horizon and the lecture relation below; identify which quantities are observed, calibrated, or model-derived.
Limitation or common confusion: A horizon-scale length is not a direct image of the horizon; binary dynamics and disk emission are separate evidence streams.
\(r_s=2GM/c^2\)
Event horizon
Definition: A causal boundary from inside which future-directed light cannot reach distant observers.
Why it matters here: In Black-Hole Dynamics and Relativistic Orbits, Event horizon is needed to reason about Schwarzschild radius, ISCO, time dilation, and observational boundaries rather than merely label the phenomenon.
Relationship: It is interpreted alongside ISCO and the lecture relation below; identify which quantities are observed, calibrated, or model-derived.
Limitation or common confusion: A horizon-scale length is not a direct image of the horizon; binary dynamics and disk emission are separate evidence streams.
ISCO
Definition: The innermost stable circular orbit allowed by a specified black-hole spacetime.
Why it matters here: In Black-Hole Dynamics and Relativistic Orbits, ISCO is needed to reason about Schwarzschild radius, ISCO, time dilation, and observational boundaries rather than merely label the phenomenon.
Relationship: It is interpreted alongside Gravitational time dilation and the lecture relation below; identify which quantities are observed, calibrated, or model-derived.
Limitation or common confusion: A horizon-scale length is not a direct image of the horizon; binary dynamics and disk emission are separate evidence streams.
Gravitational time dilation
Definition: The difference in elapsed proper time between observers at different gravitational potentials.
Why it matters here: In Black-Hole Dynamics and Relativistic Orbits, Gravitational time dilation is needed to reason about Schwarzschild radius, ISCO, time dilation, and observational boundaries rather than merely label the phenomenon.
Relationship: It is interpreted alongside Dynamical mass and the lecture relation below; identify which quantities are observed, calibrated, or model-derived.
Limitation or common confusion: A horizon-scale length is not a direct image of the horizon; binary dynamics and disk emission are separate evidence streams.
Dynamical mass
Definition: A mass inferred from orbital motion rather than from emitted-light appearance alone.
Why it matters here: In Black-Hole Dynamics and Relativistic Orbits, Dynamical mass is needed to reason about Schwarzschild radius, ISCO, time dilation, and observational boundaries rather than merely label the phenomenon.
Relationship: It is interpreted alongside Schwarzschild radius and the lecture relation below; identify which quantities are observed, calibrated, or model-derived.
Limitation or common confusion: A horizon-scale length is not a direct image of the horizon; binary dynamics and disk emission are separate evidence streams.