Execute our test scripts in a live console to verify the **Dynamic Fractal Cosmological Model (DFCM)** against real observational data. This is your chance to see the 7.1σ statistical improvement over ΛCDM in action.
Reproduce the core results of DFCM, including its resolution of the Hubble Tension and the global goodness-of-fit.
Use this script to test the DFCM against Cosmic Chronometer data, an independent method for measuring the Universe's expansion rate, to verify its agreement with the expansion history.
Test the model against Planck CMB data, examining its predictions for the early Universe.
Click on "Load Data (CMB)" to load the observational data from the Planck satellite (COM_PowerSpect_CMB-TT-full_R3.01.txt). This data represents the power spectrum of CMB anisotropies—the tiny temperature fluctuations in the light from the Universe shortly after the Big Bang. It's crucial for comparing our model with reality.
Once the data is loaded, the "Run Script" button will become active. Click it to launch the Python script (CMB.py), which will use the loaded data to perform calculations and test the model's predictions.
Verify the accurate fit to Baryon Acoustic Oscillations, aligning with DESI data and resolving sound horizon discrepancies.
Verify DFCM's fit to Type Ia Supernovae data, a key probe for the Universe's expansion history.
Validate the model's Hubble constant prediction against complete gravitational lensing data.
Test luminosity distance predictions at high redshifts using complete GRB catalog.
Verify the model's prediction for baryon density against precision measurements.
Test structure growth predictions against complete DESI Year 1 data.
Investigate the model's predictions for galaxy clustering and the suppression of massive clusters.