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Black-Hole Horn-Torus
Matter of any M distorts the geometry. If M is massive enough, the geometry is so closed to form a black hole. Its shape develops from Einstein’s 3D hyper-cylinder or de Sitter’s 4D hyper-hyperboloid to a horn torus topology.
10
You
䷓
97,201 - 108,000
Correspondence
Radiance
11
Xu
䷖
108,001 - 118,800
Disintegration
Collapse
12
Hai
䷁
118,800 - 129,600
Receptivity
Seamlessness
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