Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
Citation
Kerr, Roy P.. (1963). Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics. Physical Review Letters. 11. pp. 237–238.
Why this reference is included
Kerr’s 1963 Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics, published in Physical Review Letters, is one of the program’s working technical references. Cited across Book V (Categorical Macrocosm), Part 7, Chapter The Correspondence Map: τ³ leftrightarrow Orthodox Physics; Book V (Categorical Macrocosm), Part 7, Chapter General Relativity as Emergent Geometry; Book V (Categorical Macrocosm), Part 7, Chapter The Dark Sector Dissolved — the central framing is “Gravitational dynamics (Schwarzschild , Kerr , gravitational waves ), since the τ-Einstein identity reduces to the Einstein field equation in the chart limit”.
Cited in
-
Book V — Categorical Macrocosm Part 7Chapter The Correspondence Map: τ³ leftrightarrow Orthodox Physics
Gravitational dynamics (Schwarzschild , Kerr , gravitational waves ), since the τ-Einstein identity reduces to the Einstein field equation in the chart limit
-
Book V — Categorical Macrocosm Part 7Chapter General Relativity as Emergent Geometry
Black hole shadow (Event Horizon Telescope, 2019) : the image of M87* shows a shadow diameter consistent with the Kerr metric for a 6.5 × 10^9 M_ black hole
-
Book V — Categorical Macrocosm Part 7Chapter The Dark Sector Dissolved
Black hole shadow (EHT, 2019) : M87* shadow consistent with the Kerr metric for 6.5 × 10^9 M_