Cosmology · The cosmic web, voids and intergalactic matter
Voids depend on definitions and tracers
Compare three explicit masks in the same eight-cell patch, distinguishing low matter density from absence of selected galaxy tracers.
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
- Explain why a void catalogue needs an operational definition and a tracer sample.
- Calculate selected volume and mass fractions using the correct weights.
- Distinguish empty tracer cells from empty matter and a finite patch boundary from a cosmic boundary.
A void is not defined by the word empty alone
Cosmic voids are regions identified as relatively underdense under a specified description. Their boundaries and membership depend on the density estimate, selected tracers, smoothing scale and identification rule.
A region can contain few galaxies from one sample while still containing other galaxies, diffuse gas and dark matter. Absence of selected tracers is not a direct measurement of zero total matter.
Void finders can use density basins, adjacency and merging rules rather than a single spherical threshold. Comparing catalogues requires knowing those definitions and their treatment of survey edges and sparse sampling.
The following eight-cell construction uses three simple masks to isolate the role of a rule. It is not a watershed algorithm, a Voronoi density estimator or an observed void catalogue.
Keep matter and tracer inventories separate
Choose eight equal-volume cubes in a finite 2 × 2 × 2 patch at one epoch. Each physical cell volume is V_cell = a³L³ for common dimensionless a and positive comoving side L.
Label cells i = x + 2y + 4z for x, y and z equal to zero or one. There is no periodic wrap. Two cells are adjacent only if they share a face inside this patch.
Supply physical matter-density ratios ρ_i/ρ̄ = [0.1,0.3,0.4,0.7,0.8,1.4,1.9,2.4] for cells 0–7. They sum to eight, so ρ̄ is the finite-patch mean. Every cell has positive matter density.
Separately assign selected-tracer counts [0,0,1,0,0,2,3,4]. These counts are teaching inputs, not Poisson draws, a fitted galaxy-bias relation or a mass measurement obtained by counting tracers.
Equal volume does not imply equal selected matter
Rule A selects cells with ρ_i/ρ̄ < 0.5: cells 0, 1 and 2. They occupy 3/8 of the patch volume and contain (0.1+0.3+0.4)/8 = 0.1 of its matter mass.
Rule B uses the looser strict cut ρ_i/ρ̄ < 0.8, selecting cells 0, 1, 2 and 3. Cell 4, with ratio exactly 0.8, is excluded. The selected volume is 1/2 and selected mass fraction is 1.5/8 = 0.1875.
Rule C selects zero selected-tracer counts: cells 0, 1, 3 and 4. Its volume is also 1/2, but its mass fraction is 1.9/8 = 0.2375. Equal selected volume has not made it the same region as rule B.
The mean selected density ratio is the sum of density ratios divided by the number of selected equal-volume cells. For A, B and C it is 4/15, 0.375 and 0.475 respectively.
| Rule | Selected cells | Volume fraction | Mass fraction | Mean ρ/ρ̄ | Selected tracer count |
|---|---|---|---|---|---|
| A: ρ/ρ̄ < 0.5 | 0,1,2 | 3/8 | 0.1 | 0.266667 | 1 |
| B: ρ/ρ̄ < 0.8 | 0,1,2,3 | 1/2 | 0.1875 | 0.375 | 1 |
| C: zero selected tracers | 0,1,3,4 | 1/2 | 0.2375 | 0.475 | 0 |
A connected mask still needs an interpretation
All three selected sets are face-connected within the supplied patch. That follows from the cell labels and adjacency rule; it is not a general statement that threshold-selected regions must always be connected.
The A mask contains one selected tracer in cell 2 despite being selected for low matter density. The C mask contains no selected tracers yet has nonzero matter in all four of its cells.
Touching a boundary of the eight-cell patch does not establish where a real cosmic void ends. The model supplies no information outside that boundary and no rule for joining neighbouring patches.
The chosen cut values are definitions, not significance levels or physical discontinuities. Nothing in this inventory computes a void expansion history, gravitational potential or statistically preferred threshold.
A useful void claim names its field and rule
In observations, tracer selection, sampling density, redshift errors and the survey window affect a density estimate and its accepted regions. A sparse sample can create apparent gaps even when the underlying matter field is not equally sparse.
A method that builds density basins from tessellation and adjacency has different operational steps from these simple cuts. Its significance calibration and boundary choices must be checked in their own setting.
Connecting a tracer-defined void to total matter or cosmological dynamics requires further calibration or modelling. The known matter ratios supplied here bypass that inference step and are not an observational reconstruction.
Report the tracer population, reference mean, density estimator, scale, boundary treatment and acceptance rule. This makes comparisons about void size, volume or matter content specific enough to assess rather than relying on an ambiguous image of empty space.
Worked reasoning
Use volume and mass denominators correctly
What fractions does rule A select?
- Its three selected equal-volume cells give volume fraction 3/8.
- Their density-ratio sum is 0.1+0.3+0.4 = 0.8, while the whole patch sum is eight.
- Thus mass fraction is 0.8/8 = 0.1 and mean selected density ratio is 0.8/3 = 4/15.
Rule A selects 3/8 of the finite volume but 1/10 of its matter mass; these fractions answer different questions.
Try the reasoning
Are rules B and C the same region because both select half the volume?
Show the answer and reasoning
No.
Their memberships differ and their matter fractions are 0.1875 and 0.2375.
Does rule B include cell 4 with density ratio exactly 0.8?
Show the answer and reasoning
No.
Its stated inequality is strictly below 0.8.
Does a zero selected-tracer count establish zero matter in the supplied cell?
Show the answer and reasoning
No.
Every prescribed matter density is positive; tracer counts and matter inventories are distinct.
What to carry forward
- A void catalogue depends on an explicit field, tracer sample and identification rule.
- Selected volume, selected mass and mean density use different weights and denominators.
- Empty tracer cells and finite mask boundaries do not establish empty matter or universal cosmic boundaries.
References
Sources supporting the explanations, physical distinctions and examples in this lesson.