Application Examples

Successor Function and CMB Cooling Example

We can test this framework with an heuristic, coarse-grained, quantitative cosmology example: the cooling of the Cosmic Microwave Background (CMB) after recombination.

  1. Physical Model
    After recombination \((t_0 \sim 3.8 \times 10^5\ \text{years})\), the CMB temperature evolves as:

\[ T(t) \propto a(t)^{-1} \]

where \(a(t)\) is the scale factor. In a matter-dominated universe: \[ a(t) \propto t^{2/3} \quad \implies \quad T(t) \propto t^{-2/3}. \]

  1. Discrete State Steps

We define discrete states corresponding to successor function applications: \[ f_{n+1} = T(f_n) \]

and choose each state step \((n \to n+1)\) to correspond to a doubling of cosmic time:

\[ t_n = t_0 \cdot 2^n. \]

Then the temperature at state \((n)\) is:

\[ T_n = T_0 \cdot 2^{-2n/3}. \]

Each state transition is associated with a minimal transition duration \(d\tau\), reflecting the time it takes for physical changes to occur in the system.

  1. Initial Conditions

\[ T_0 = 3000\,\text{K}, \quad t_0 = 3.8\times 10^5\,\text{yr}. \]

  1. Successor Function (Discrete Update)

\[ f_{n+1} = T(f_n) = f_n \cdot 2^{-2/3} \approx 0.63 f_n \]

  1. First Few States
nt_n (yr)T_n (K)
03.80×10⁵3000
17.60×10⁵1890
21.52×10⁶1190
33.04×10⁶750
46.08×10⁶470
51.22×10⁷296
162.50×10¹⁰1.9

Observation: after ~16 compositional steps, the predicted temperature approaches the observed CMB temperature \((T\_{\mathrm{CMB}} \approx 2.725)\) K.


Emergent Time and Transition Duration

\[ \tau_{\mathrm{worldline}} = \sum_n d\tau_n \]


Key Insights

  1. The universe evolves compositionally, via repeated application of a successor function \((T)\).
  2. Church numeral analogy makes nested, history-dependent evolution intuitive.
  3. Each transition has a finite duration \((d\tau)\), giving rise to emergent proper time.
  4. Discrete functional evolution reproduces real cosmological observables, like the cooling of the CMB.
  5. Time dilation and spacetime geometry naturally emerge from transition counting and compositional structure.

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