Cosmology · Cosmological parameters and statistical inference
Covariance, correlated data and parameter degeneracy
Follow four exact correlated noise states through a sum-and-difference response, keeping covariance and identifiability distinct.
Preparation: ratios, powers of ten and ordinary arithmetic. Physical quantities and notation are introduced as they are needed.
Back to the chapterAfter reading, you can
- Calculate covariance from a fully declared finite sampling law.
- Propagate correlated errors into two parameter estimates.
- Separate a response degeneracy from the shape of an error distribution.
Shared errors and similar parameter responses are different issues
Two observations can share an error source. A common calibration shift, for example, can move both readouts in the same direction even when the physical signals differ.
Covariance summarizes how centered variations co-vary under a specified probability law. Parameter degeneracy instead concerns whether different parameter choices give the same or similar predicted observations.
These issues can coexist, but one does not define the other. A nonzero covariance alone does not prove a parameter degeneracy, and an invertible covariance matrix does not establish identifiability.
Historical supernova methods illustrate the need to retain shared calibration correlations. Here we use an original four-state construction, with no survey covariance or cosmological parameter fit supplied.
State the entire distribution before using its covariance
Let θ and φ be signed response amplitudes with units U, an arbitrary fixed readout unit. Supply x₁ = θ+φ+s+u and x₂ = θ−φ+s−u.
Choose independent latent errors s = ±2U and u = ±U, each sign equally likely. The shared error s moves both readouts together; u moves them oppositely.
Hold the teaching truth fixed at θ = 10U and φ = 2U. There are exactly four possible pairs of readout errors, each with probability 1/4.
This distribution has four discrete points. No Gaussian density, continuous contour, empirical data or unspecified probability mass between those points is assumed.
| s/U | u/U | x₁/U | x₂/U | θ̂/U | φ̂/U |
|---|---|---|---|---|---|
| −2 | −1 | 9 | 7 | 8 | 1 |
| −2 | 1 | 11 | 5 | 8 | 3 |
| 2 | −1 | 13 | 11 | 12 | 1 |
| 2 | 1 | 15 | 9 | 12 | 3 |
Sum and difference retain different amounts of noise
Form θ̂ = (x₁+x₂)/2 = θ+s and φ̂ = (x₁−x₂)/2 = φ+u. The corresponding estimator errors recover the two independent latent errors exactly.
Each raw error has variance 4U²+U² = 5U². Their covariance is Var(s)−Var(u) = 3U², so the raw covariance matrix is C = [[5,3],[3,5]]U².
The correlation coefficient is 3/5. In contrast, the estimator covariance is diag(4,1)U²: the sum-mode variance is 4U² and the difference-mode variance is U².
The independence of the estimator errors follows here from the explicitly independent s and u. Zero covariance by itself would not establish independence for a general distribution.
Discarding correlation can misstate uncertainty in either direction
For the sum estimate, Var(θ̂) = (C₁₁+C₂₂+2C₁₂)/4 = (5+5+6)U²/4 = 4U².
For the difference estimate, Var(φ̂) = (C₁₁+C₂₂−2C₁₂)/4 = U². The same shared covariance term increases one mode and decreases the other.
If the off-diagonal terms are incorrectly set to zero while both diagonal variances remain 5U², propagation would report 2.5U² for each estimate. This understates the sum variance and overstates the difference variance.
Optional matrix propagation writes C_est = BCBᵀ for the stated linear sum-and-difference matrix B. This identity for second moments does not require Gaussian errors or produce automatic 68% intervals.
Identifiability belongs to the mean response
Without noise, the first channel alone fixes θ+φ. A change in θ can be canceled by an opposite change in φ, giving the same predicted x₁.
Adding the second mean response θ−φ gives the coefficient matrix [[1,1],[1,−1]], with determinant −2. The two equations then separate θ and φ in this model.
That rank statement uses the forward response, independently of the covariance calculation. Real analyses may have nearly aligned responses, nonlinear dependencies, nuisance parameters and limited sensitivity over a stated parameter region.
The four-point example supports exact covariance arithmetic and a transparent rank test. It supplies neither a survey likelihood ellipse nor a significance level or posterior contour for cosmological parameters.
Worked reasoning
Propagate a correlated sum
What happens if C₁₂ = 3U² is discarded when estimating Var(θ̂)?
- Use the full covariance: (5+5+2×3)U²/4 = 4U².
- Replacing C₁₂ by zero gives (5+5)U²/4 = 2.5U².
- For the difference estimate the true value is U², so the same replacement instead overstates its variance.
Ignoring the correlation gives the wrong uncertainties in opposite directions for the two modes.
Try the reasoning
Does the covariance matrix C establish a Gaussian likelihood?
Show the answer and reasoning
No.
The declared law has only four noise states; a covariance is a second-moment summary.
What separates θ and φ in the noise-free example?
Show the answer and reasoning
The second linearly independent mean response.
The determinant −2 of the two-channel response matrix is nonzero.
What are the exact estimator variances?
Show the answer and reasoning
Var(θ̂) = 4U² and Var(φ̂) = U².
Their errors are the supplied s and u, respectively.
What to carry forward
- Covariance describes variations under a specified probability law.
- Correlated input errors can affect sum and difference uncertainties differently.
- Parameter identifiability depends on the forward response and is distinct from covariance or Gaussianity.
References
Sources supporting the explanations, physical distinctions and examples in this lesson.