The Cosmic Isolation Scale: Quarks in de Sitter Space
While gluons continue to bind quarks into hadrons due to the immense strength of the strong nuclear force, the exponential expansion of de Sitter space creates distances so vast that atomic nuclei cannot form. The scale of separation between bound quark systems becomes astronomical compared to nuclear scales.
The characteristic distance for quarks within a proton or neutron, and for nucleons within an atomic nucleus. The strong nuclear force operates effectively at this scale.
The characteristic separation between remaining bound quark systems in the late de Sitter epoch. This is 56 orders of magnitude larger than nuclear scales.
The fundamental length scale in de Sitter space is set by the cosmological horizon. For our universe's current dark energy density, this is approximately:
However, as the universe continues to expand and matter dilutes, the effective separation between any remaining bound quark systems grows exponentially. In the asymptotic de Sitter state, the typical distance between such systems approaches scales where the expansion rate prevents any causal contact.
For an atomic nucleus to form, protons and neutrons must come within 1-10 femtometers of each other. Several cosmic factors prevent this:
Different fundamental forces become ineffective at different cosmic scales:
In the de Sitter epoch, quarks remain bound into individual hadrons by the strong nuclear force operating at femtometer scales, but the cosmic separation between these bound systems grows to approximately 10⁴¹ meters—a scale so vast that the formation of atomic nuclei becomes mathematically impossible.
The universe contains bound quark systems forever isolated from one another by distances that make our current observable universe seem microscopic in comparison. Local quantum binding persists while global structure formation becomes eternally impossible.
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