Cosmology · The cosmological constant and other dark-energy models
Parameter constraints and model degeneracy
Solve two supplied response equations, track a shared calibration shift and separate local cosmological sensitivity from a finite probability experiment.
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
- Identify which parameter combination one response constrains.
- Propagate shared and individual errors through a two-response calculation.
- State the model and statistical assumptions behind a parameter constraint.
Begin with two unknowns and one relation
Let p and q be two dimensionless parameter offsets. Supply a normalized noiseless response d₁ = 2p+q. If d₁ = 0, all points on q = −2p give the same response.
This is a degeneracy: one response does not distinguish changes that compensate in this way. It is a statement about the specified map from parameters to response, rather than evidence that the parameters have no physical meaning.
Now supply a second response d₂ = 5p+q. Its zero-response line q = −5p crosses the first at p = q = 0. Two differently directed sensitivities can resolve the degeneracy in this algebraic model.
Solving the two equations gives p̂ = (d₂−d₁)/3 and q̂ = (5d₁−2d₂)/3. The hats mark values inferred using the supplied response model; their reliability depends on what enters d₁ and d₂.
A physical sensitivity motivates the response
For a spatially flat model with separately conserved pressureless matter and a constant-w component, write F(a) = [H(a)/H_ref]² = Ω_m a⁻³+(1−Ω_m)a⁻³⁽¹⁺ʷ⁾. The reference rate H_ref is supplied and known in this example.
Choose the reference parameters Ω_m = 1/2 and w = −2/3, with a = 1 as the reference epoch. Define p = δΩ_m and q = (ln 2)δw. These are small offsets about that reference, rather than fitted values from observations.
At a = 1/2 the reference F is 5 and its first-order change is δF ≈ 6p+3q. At a = 1/4 the reference F is 34 and δF ≈ 60p+12q. Dividing the two changes by 3 and 12 motivates the two different response directions above.
The physical FLRW expression is nonlinear for finite parameter changes. The separate finite experiment below defines its response equations as exactly linear; it is not an exact finite substitution into F(a). Changing curvature, H_ref, the component set or evolving w would change the inference problem.
Give the calibration and noise a probability model
Define the finite experiment exactly by d₁ = 2p+q+s+e₁ and d₂ = 5p+q+s+e₂. Let the shared calibration shift s be equally likely to be −0.02 or +0.02, and each individual error e₁,e₂ be equally likely to be −0.01 or +0.01.
The three signs are independent. Therefore all eight sign combinations have probability 1/8. Set the true offsets to p = q = 0 for the displayed outcome table; every number is a supplied synthetic outcome, not a measured H value.
A shared s moves both responses equally. It cancels in their difference and hence in p̂, but it remains in q̂. Two correlated summaries do not automatically eliminate a common calibration error.
The response covariance is Cov(d) = [[0.0005, 0.0004], [0.0004, 0.0005]]. The off-diagonal entry comes from the shared shift and must be retained when propagating uncertainty.
| s | e₁ | e₂ | d₁ | d₂ | p̂ | q̂ |
|---|---|---|---|---|---|---|
| −0.02 | −0.01 | −0.01 | −0.03 | −0.03 | 0 | −0.030000 |
| −0.02 | −0.01 | 0.01 | −0.03 | −0.01 | 0.006667 | −0.043333 |
| −0.02 | 0.01 | −0.01 | −0.01 | −0.03 | −0.006667 | 0.003333 |
| −0.02 | 0.01 | 0.01 | −0.01 | −0.01 | 0 | −0.010000 |
| 0.02 | −0.01 | −0.01 | 0.01 | 0.01 | 0 | 0.010000 |
| 0.02 | −0.01 | 0.01 | 0.01 | 0.03 | 0.006667 | −0.003333 |
| 0.02 | 0.01 | −0.01 | 0.03 | 0.01 | −0.006667 | 0.043333 |
| 0.02 | 0.01 | 0.01 | 0.03 | 0.03 | 0 | 0.030000 |
Different combinations inherit different uncertainty
Averaging all eight states gives zero mean for both inferred offsets. Their variances are Var(p̂) = 2/90000 and Var(q̂) = 65/90000, with Cov(p̂,q̂) = −7/90000.
The standard deviations are √2/300 ≈ 0.004714 and √65/300 ≈ 0.026874. For q = (ln 2)δw, the corresponding standard deviation of the inferred δw is √65/(300 ln 2), within this finite experiment.
Holding s fixed at zero would reduce Var(q̂) to 29/90000. That would be a different assumed experiment, not evidence that the original shared error had disappeared. Var(p̂) is unchanged because the shared term cancels algebraically.
Covariance records second moments; it does not turn the eight states into a Gaussian distribution. An interval one standard deviation wide on each side of the true value contains only half of this experiment’s outcomes for either individual inferred parameter, rather than an automatic 68 percent.
A parameter interval is conditional evidence
In a real analysis, calibrated observables and a stated probability model replace this supplied table. The response may be nonlinear, the nuisance parameters uncertain, and additional observables correlated.
A parameter constraint therefore needs its model family, assumed data response, calibration treatment, priors or repeated-experiment construction, and covariance. Removing those conditions changes what the reported interval means.
The local FLRW derivatives here explain why different epochs can constrain different combinations. They do not supply observed expansion data, a posterior, a confidence region, a model-selection result or a microscopic identification of dark energy.
Use complementary probes to test different physical responses and common systematics explicitly. A narrower conditional parameter spread is useful, while deciding between complete physical mechanisms requires their additional predictions and evidence.
Worked reasoning
Add the same calibration shift to both responses
What does adding s to d₁ and d₂ do to the inferred offsets?
- The difference d₂−d₁ stays unchanged, so p̂ does not change.
- The numerator 5d₁−2d₂ increases by 3s.
- Therefore q̂ increases by s and retains the shared variance 0.02².
The common shift cancels from p̂ but survives fully in q̂.
Try the reasoning
Does d₁ = 0 alone require p = q = 0 in the noiseless map?
Show the answer and reasoning
No: every point q = −2p gives d₁ = 0.
A single relation leaves a degeneracy line in the two-parameter plane.
For d₁ = −0.03 and d₂ = −0.01, find the inferred offsets.
Show the answer and reasoning
p̂ = 1/150 ≈ 0.006667 and q̂ = −13/300 ≈ −0.043333.
Use the two stated inverse response equations; the rounded table follows those exact fractions.
Does a covariance matrix alone justify Gaussian 68 percent intervals?
Show the answer and reasoning
No.
The full distribution here has eight discrete states, and its actual one-standard-deviation marginal coverage is one half.
What to carry forward
- Different response directions can resolve a conditional parameter degeneracy.
- A shared calibration can cancel in one inferred combination and remain in another.
- Local physical sensitivity, finite response assumptions and statistical coverage must be stated separately.
References
Sources supporting the explanations, physical distinctions and examples in this lesson.