Overview
Model the expansion of the universe under different α-field cosmological parameters.
This interactive tool allows you to explore cosmic expansion model through hands-on calculation and visualization.
How It Works
Calculator Mode
Enter values for the input parameters below, and the tool will compute the corresponding outputs based on SCU theory's α-field equations.
Inputs
| H₀ | Hubble constant | km/s/Mpc | 70 |
|---|---|---|---|
| Ωm | Matter density parameter | 0.3 | |
| ΩΛ | Dark energy density parameter | 0.7 |
Outputs
- Scale Factor: Universe scale factor over time
- Age: Age of universe for given parameters
The Mathematics
H^2 = H_0^2(\Omega_m a^{-3} + \Omega_\Lambda)
Try It
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Understanding the Results
The outputs reveal how α-field dynamics govern this phenomenon:
- Scale dependence - How behavior changes across scales
- Regime transitions - Moving between laminar, turbulent, and resonant states
- Emergent properties - What arises from the underlying dynamics
Related Tools
- structural-chronometric-universe
Learn More
Connect this tool to the underlying theory:
- Understand the equations being computed
- See how this relates to observable phenomena
- Explore the evidence supporting these predictions