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Theory Overview

Psi-Continuum v2

Psi-Continuum v2 (ΨCDM) is a minimal one-parameter phenomenological extension of the standard ΛCDM cosmological model at the background expansion level.

It introduces a single smooth late-time deformation of the Hubble expansion, governed by the dimensionless parameter ε₀, while leaving early-Universe physics unchanged and not introducing any modifications to standard perturbation dynamics.


Background Expansion

The modified Hubble expansion rate is defined as:

H_Ψ(z) = H_Λ(z) · (1 + ε₀ / (1 + z))

A visual comparison between ΛCDM and ΨCDM is shown below:

Psi-Continuum Hubble function

This parametrisation:


Scope of the Model

Psi-Continuum v2 is intentionally restricted to the late-time background expansion.

It does not introduce:


Included Functionality

This package provides a fully reproducible late-time cosmology pipeline, including:

All numerical results reported in the accompanying paper are fully reproducible using this software.


Associated Publications


Project Status

Psi-Continuum v2 is a final archived research release.

The code and documentation are frozen for long-term reproducibility and citation. Further theoretical developments will be released separately as Psi-Continuum v3.