GLOBAL KNOWLEDGE ARK

Cosmology · Cosmic contents and background radiation

Cosmic contents depend on measured data and models

Build a hypothetical energy budget at two epochs, then learn what a real quoted cosmic fraction must specify before it can be compared with another result.

Preparation: ratios, powers of ten and ordinary arithmetic. Physical quantities and notation are introduced as they are needed.

Back to the chapter

After reading, you can

  • Calculate a component’s share using a common energy-density denominator.
  • Explain why component fractions change even when no component is created.
  • Identify the epoch, data, model and uncertainty needed to interpret a measured cosmic budget.
01

A percentage needs a denominator

Suppose three components each have energy density 1 in the same arbitrary energy-per-volume unit. Their total is 3, and each supplies one third, about 33.3 percent. The density values and the fractions are different quantities: a fraction divides one component by a stated total.

The common unit matters. One cannot add a particle count to an energy density or silently mix kilograms per cubic metre with joules per cubic metre. Rest-mass density can be converted to energy density using c², with a consistent definition of which energy is included.

Our deliberately hypothetical components are nonrelativistic matter, photons and a cosmological constant Λ. Here the matter is not divided into ordinary and dark components, and neutrinos and other contributions are omitted. Equal starting densities are chosen to make the arithmetic transparent; they are not a measured cosmic budget.

Define q = a/a_ref, the scale factor relative to the chosen reference epoch. All densities in this example are evaluated at the same epoch for each row. Combining a photon density from one epoch with a matter density from another would not produce that epoch’s budget.

02

The denominator changes as the components evolve

For these separately conserved ideal components, nonrelativistic matter energy density scales as q⁻³, photons as q⁻⁴ and Λ stays constant. These assumptions specify how the model evolves. A component with a different pressure behaviour or energy exchange would require another rule.

At q = 2, the densities are 1/8 for matter, 1/16 for photons and 1 for Λ. Their total is 1/8 + 1/16 + 1 = 19/16, or 1.1875 in the shared unit. This total is smaller than the reference total 3.

Divide each density by the new total. Matter contributes (1/8)/(19/16) = 2/19, photons contribute 1/19, and Λ contributes 16/19. The fractions add to 19/19 = 1. Approximately they are 10.5, 5.3 and 84.2 percent.

Λ’s fraction has risen even though its energy density has not changed. The other densities became smaller, so the denominator and relative shares changed. A larger fraction does not, by itself, establish that a component’s density increased or that matter was converted into it.

Hypothetical energy-density accounting in shared arbitrary units; no entry is an observed cosmic abundance
qMatter densityPhoton densityΛ densityTotal densityFractions: matter, photons, Λ
111131/3, 1/3, 1/3
21/81/16119/162/19, 1/19, 16/19
Changing the total changes a component’s shareA deliberately hypothetical model gives matter, photons and a cosmological constant equal reference energy densities of one in the same arbitrary energy-per-volume unit at q = a/a_ref = 1. The upper bars use a single linear density scale: at q = 1 the three densities are 1, 1 and 1 and the total is 3; at q = 2 they are 1/8, 1/16 and 1 and the total is 19/16. Matter follows q⁻³, photons q⁻⁴, and the cosmological constant stays constant. Lower stacked bars each represent a fraction total of one, using the sum of densities at that same stage as denominator. At q = 1 the shares are each 1/3. At q = 2 they are 2/19 matter, 1/19 photons and 16/19 cosmological constant. Thus the constant’s fraction rises while its density remains one. Component symbols and direct labels accompany colour. This is not a measured cosmic budget or a critical-density parameter plot; neutrinos and other contributions are omitted and matter is not divided into ordinary and dark components.A rising fraction can accompany a constant densityHypothetical model · q = a/a_ref · equal starting densitiesM: matterγ: photonsΛ: constantEnergy density · one shared arbitrary energy/volume unit00.511M1γ1Λq = 11/8M1/16γ1Λq = 2Totals: 3 at q = 1; 19/16 at q = 2.Each fraction = its density / total density at the same q.Fractions · full bar = 1 at each stageq = 11/31/31/3q = 2Λ: 16/19M: 2/19γ: 1/1900.250.50.751Fraction of the stated total · dimensionlessΛ stays at density 1 while its fraction rises from 1/3 to 16/19.Matter: q⁻³; photons: q⁻⁴; Λ: 1. No measured budget shown.
A deliberately hypothetical model gives matter, photons and a cosmological constant equal reference energy densities of one in the same arbitrary energy-per-volume unit at q = a/a_ref = 1. The upper bars use a single linear density scale: at q = 1 the three densities are 1, 1 and 1 and the total is 3; at q = 2 they are 1/8, 1/16 and 1 and the total is 19/16. Matter follows q⁻³, photons q⁻⁴, and the cosmological constant stays constant. Lower stacked bars each represent a fraction total of one, using the sum of densities at that same stage as denominator. At q = 1 the shares are each 1/3. At q = 2 they are 2/19 matter, 1/19 photons and 16/19 cosmological constant. Thus the constant’s fraction rises while its density remains one. Component symbols and direct labels accompany colour. This is not a measured cosmic budget or a critical-density parameter plot; neutrinos and other contributions are omitted and matter is not divided into ordinary and dark components. Original Ark teaching model.
03

Observations become a budget through physical models

A telescope does not directly return a single pie chart of the Universe. It measures signals such as spectral intensities, image distortions, redshifts and apparent brightness. Instruments must be calibrated, and foregrounds or selection effects must be assessed before cosmological interpretation.

A physical model predicts how those measurements depend on contents and expansion. Researchers compare predictions with data to constrain parameters. The microwave background’s pattern and spectrum, light-element abundances, lensing and distance measurements bring different information and systematic uncertainties.

The fitted quantities need not be the percentages shown in a summary graphic. For example, a density parameter may use the critical density, defined from the expansion rate, as its denominator. That is a specified reference density, not automatically the sum of three entries in a beginner’s illustration. A quoted quantity must be defined before it is treated as a share.

Agreement between results is most informative when their definitions, assumptions and relevant errors are understood. Several measurements can also share calibration information or model assumptions, so counting them as wholly independent would overstate what has been checked.

04

Read the label attached to a real inference

Consider the historical Planck 2018 cosmological-parameter analysis, published in 2020 with a corrected arXiv version in 2021. One of its named data combinations is Planck TT,TE,EE+lowE+lensing. Those labels identify temperature and polarization information and a lensing contribution; they should not be dropped when comparing its constraints with another analysis.

Its base model is spatially flat, six-parameter ΛCDM: Λ denotes a cosmological constant and CDM denotes cold dark matter. The analysis also specifies neutrino treatment and other physical assumptions. Changing the allowed model can change what the same observations imply for the contents.

Table 2 of that analysis reports 68 percent intervals under its stated conventions. Such parameter constraints are not exact constants or automatically independent errors. A difference in two central values cannot be judged merely by counting printed decimal places or ignoring correlations.

This is an explicitly dated example of how a result is qualified, rather than a claim about the latest best fit in 2026. A useful budget citation records the data combination, physical model, target epoch, density definition and uncertainty convention. A bare percentage leaves too much of that physical account unspecified.

Questions to ask of a quoted real cosmic budget
Required contextWhat it resolves
Epoch and density definitionWhich time and denominator does the fraction describe?
Named observations and data releaseWhat measurements were actually compared?
Physical model and allowed componentsWhich expansion and component assumptions connect data to parameters?
Intervals, correlations and systematicsHow uncertain is the inference, and which comparisons are justified?
05

A fitted share does not reveal a microscopic identity

A well-constrained gravitational contribution can coexist with uncertainty about its physical nature. Estimating how much dark matter a model requires does not identify a dark-matter particle. Fitting a Λ term does not establish why that energy density exists.

Keep three levels together when interpreting a claim: the measured signal, the inference under a physical model, and the explanation that remains open. This avoids both extremes of treating all fitted quantities as direct photographs and treating the unresolved microscopic questions as if no observational constraints existed.

The chapter’s progression now fits together. Ordinary matter can change binding state. Radiation changes both density and photon energy during expansion. Gravitational mass and accelerated expansion raise different questions. Relic spectra and nuclear abundances test earlier conditions. A cosmic budget combines such evidence within a clearly stated physical account.

Next, the learning map turns to sky maps, plots and uncertainty. Those tools will make it easier to read the observations behind the summaries and to ask which part of a conclusion comes from the data and which part depends on the comparison being made.

Worked reasoning

Keep a constant density and change its fraction

In the hypothetical model at q = 2, Λ has density 1 and the total is 19/16. What is Λ’s share? Did its density increase from the reference epoch?

  1. Divide the component by the contemporaneous total: 1/(19/16) = 16/19.
  2. Convert to a percentage: 16/19 × 100 ≈ 84.2 percent.
  3. Compare density with the reference: it was 1 and remains 1. Its share rose because the matter and photon densities fell.

Λ supplies 16/19, about 84.2 percent, while its own energy density stays constant in this chosen model.

Try the reasoning

  1. At q = 2 the fractions are 2/19, 1/19 and 16/19. Do they account for the entire chosen model?

    Show the answer and reasoning

    Yes. They sum to 19/19 = 1.

    They share one denominator and include all three components chosen for this toy model. This says nothing about omitted real components.

  2. Is a component percentage complete information if its epoch and denominator are omitted?

    Show the answer and reasoning

    No.

    The densities and relative shares can evolve, and different density parameters may use different reference totals.

  3. Two analyses print different central values for a density parameter. Is the difference alone enough to establish a contradiction?

    Show the answer and reasoning

    No. Their definitions, data, models, intervals, correlations and systematics must be compared.

    A central value is only part of an inference; changed assumptions or correlated uncertainty can change its interpretation.

What to carry forward

  • A cosmic fraction needs an epoch, common units and a defined denominator.
  • Relative shares can change even when a component’s own energy density stays constant.
  • Real budgets are conditional inferences from named data and models, with uncertainty; they do not identify every component’s physical nature.

References

Sources supporting the explanations, physical distinctions and examples in this lesson.

  1. Planck 2018 results. VI. Cosmological parametersPlanck Collaboration; N. Aghanim et al.Research paperarxiv.orgRead source
  2. One percent determination of the primordial deuterium abundanceRyan J. Cooke; Max Pettini; Charles C. SteidelResearch paperarxiv.orgRead source
  3. A direct empirical proof of the existence of dark matterDouglas Clowe; Maruša Bradač; Anthony H. Gonzalez; Maxim Markevitch; Scott W. Randall; Christine Jones; Dennis ZaritskyResearch paperarxiv.orgRead source
  4. Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological ConstantAdam G. Riess et al.; High-Z Supernova Search TeamResearch paperarxiv.orgRead source
  5. NASA Science2 sources
    1. Dark MatterNASA ScienceTeaching resourcescience.nasa.govRead source
    2. What is Dark Energy? Inside Our Accelerating, Expanding UniverseNASA ScienceTeaching resourcescience.nasa.govRead source
  6. David Tong2 sources
    1. Cosmology — 2 The Hot UniverseDavid TongCourse notesdamtp.cam.ac.ukRead source
    2. Cosmology — 1 The Expanding UniverseDavid TongCourse notesdamtp.cam.ac.ukRead source