CM and Gib,
Click on each of the three illustrations and see the "interior lines" of connection.
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Then click on the illustration in this one and back to those three illustrations.
Think about curving lines and straight lines! About "interior lines!" About squaring circles interior to the circle. About cubing in 'tesseract' the hypersphere, interior to the sphere. About the straight-line radius distant from the hub of a wagon wheel to the curvature, and/or curvatures, of the rim of the wheel, 1/2 the diameter of the circle in every direction of the circle from the hub (the hub: Hawking's "Grand Central Station of Universe (U).")
Quantum (discrete quanta)
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Quantum (discrete quanta)
And more! about light's coordinate point [past (t=+1)-future (t=-1)] histories' SPACETIME versus a spontaneous entangling concurrent REALTIME (t=0) instant . . . the always local-relative "visible universe" versus the non-local, non-relative, "invisible universe" that might just be close enough to smack you in your local-relativity, in the mirror, in the face, and/or in the Earth, before you see and know its around.
Click on each of the three illustrations and see the "interior lines" of connection.
Wormhole - Wikipedia
en.wikipedia.org
Then click on the illustration in this one and back to those three illustrations.
Gravitational constant - Wikipedia
en.wikipedia.org
Think about curving lines and straight lines! About "interior lines!" About squaring circles interior to the circle. About cubing in 'tesseract' the hypersphere, interior to the sphere. About the straight-line radius distant from the hub of a wagon wheel to the curvature, and/or curvatures, of the rim of the wheel, 1/2 the diameter of the circle in every direction of the circle from the hub (the hub: Hawking's "Grand Central Station of Universe (U).")
Quantum (discrete quanta)
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Strong interaction - Wikipedia
en.wikipedia.org
Quantum (discrete quanta)
And more! about light's coordinate point [past (t=+1)-future (t=-1)] histories' SPACETIME versus a spontaneous entangling concurrent REALTIME (t=0) instant . . . the always local-relative "visible universe" versus the non-local, non-relative, "invisible universe" that might just be close enough to smack you in your local-relativity, in the mirror, in the face, and/or in the Earth, before you see and know its around.
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