Pulse Core Lexicon

End of the Outward Expansion

Definition

The End of the Outward Expansion is a universe's rupture, at 2^L of its own Tempos from its big bang (the Rupture Rule): the moment the physical's outward push closes, its Harmonic Novas converging as their gaps shrink below a Tempo (Data Harmonics), and the census of its wells is taken, the N(L) = 2^(L/3) wells that seed its children (the Null Well Progeny Count Law). It is not the last well a universe forms, and it does not end the universe. What follows is the pulsing decay, almost the whole of a universe's existence on its own clock, and the universe is busy in it: its stars go on forming and dying for about 10¹⁴ years, the heaviest still going supernova and leaving neutron stars and new stellar wells, clumps of its matter still collapse into wells, and its galaxies go on merging; only then do the remnants and the wells evaporate, and the field dissipates into null. The expansion of space carries on past it, driven by the vacuum rather than by the matter's own outward push. Our universe passed it about 2.8 billion years ago, about 11.0 billion years after the big bang, and its sky shows the decay barely begun: stars still forming, galaxies still merging. The book called it the final well until 15 November 2026. It connects to Rupture Rule, Universal Dissipation, Data Harmonics, Layer Count Law, Null Well Progeny Count Law and Dilation Through the Outward Expansion.

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Chapter Chapter 3

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In the book #84 of 1,283 terms · used 21 times

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