Cosmology

A standing wave frozen at one instant

The temperature of the microwave background varies across the sky by one part in a hundred thousand, and the sizes of the patches are not random. There is a preferred angular scale near one degree, and it is a sound wave that stopped ringing four hundred thousand years after the beginning.

Assumes Microwave background and Expansion.

The spectrum of the microwave background is a blackbody to fifty parts in a million and carries almost no information beyond one temperature. The information is in the part that essay set aside: the temperature is not quite the same in every direction, and the pattern of the variation is a measurement of the geometry and contents of the universe.

The variation is small. Once the dipole from the Solar System’s own motion is removed, what is left is a mottling of hot and cold patches at the level of one part in a hundred thousand — about 30 microkelvin against 2.7255 kelvin. What makes it useful is that the mottling has a characteristic size.

The acoustic peaks, and where the geometry says they should be. The temperature angular power spectrum of the microwave background. The drawn curve is a monotone interpolation through the published positions and heights of the six peaks and five troughs of the Planck 2018 TT measurement — it is a representation of data, and nothing between two extrema is claimed. The marks along the top are not: they are computed from this collection's own cosmology as ℓₐ(m − 0.267), where ℓₐ = π × 13866 / 144.43 = 301.6 — π times the comoving distance to last scattering divided by the sound horizon there — is the angle the sound horizon subtends at last scattering turned into a multipole. The two agree to 2.8 per cent at worst across six peaks, which is the whole of what makes this a measurement of geometry: a wave of known physical wavelength, seen at a known distance, is a protractor. The first peak at ℓ = 220 corresponds to about 0.82 degrees on the sky — roughly twice the width of the full Moon, which is the largest hot and cold patch the sky has.
Fig. 1 The angular power spectrum: how much variance the map contains at each angular scale, plotted against multipole \ell, which corresponds to an angular size of roughly 180°/180°/\ell. The drawn curve interpolates the published positions and heights of the six peaks and five troughs of the Planck 2018 measurement, and asserts nothing between two extrema. The marks along the top are computed rather than measured: they are A(m0.267)\ell_A(m - 0.267) with A=πDM(z)/rs=π×13866/144.4=302\ell_A = \pi D_M(z_*)/r_s = \pi \times 13866 / 144.4 = 302, the acoustic scale for this collection’s cosmology. The two agree to 2.8 per cent at worst across six peaks. That agreement is the measurement of geometry — a wave of known physical wavelength, seen at a known distance, is a protractor.

Where a preferred scale comes from

Before recombination the universe contains a fluid, and calling it that is precise rather than loose. Photons and free electrons scatter off each other constantly, electrons and protons are bound by electrostatics, so photons, electrons and baryons move as one substance with a single velocity field. It has enormous pressure, supplied by the photons, and it has mass, supplied mostly by the baryons. A medium with pressure and mass supports sound.

The sound speed is cs=c/3(1+R)c_{\rm s} = c/\sqrt{3(1+R)} where R=3ρb/4ργR = 3\rho_{\rm b}/4\rho_\gamma measures how much the baryons weigh the fluid down. Early on the baryons are negligible and the sound speed is 0.577c0.577c — more than half the speed of light, because the fluid is mostly radiation and radiation is very stiff.

Now put a small overdensity in the dark matter somewhere. Dark matter does not feel the pressure and simply sits there, deepening; the photon–baryon fluid falls into the potential well it makes, overshoots, is pushed back out by its own pressure, and oscillates. Each initial overdensity therefore launches a spherical pressure wave that runs outward at csc_{\rm s}.

The ruler being laid down. The comoving sound horizon against the scale factor, integrated from the big bang forwards. A pressure wave in the photon–baryon fluid travels at c/√(3(1+R)), which begins at 0.577c while the photons dominate and falls to 0.451c by the time the baryons have caught up; the curve is the distance it has covered, in comoving megaparsecs. It stops when the photons stop pushing, which is the drag epoch at z = 1059.94, and the value it has reached there is 146.9 Mpc. That is the length of the ruler, and it is set entirely by physics before recombination — by the radiation density, the matter density and the baryon density, all three of which the same sky map measures. Nothing about the later universe enters it. The dashed mark at z = 1089.92 is last scattering, forty thousand years earlier in redshift and 2.7 Mpc shorter, which is why the microwave background's ruler and the galaxy survey's ruler are two slightly different numbers rather than one.
Fig. 2 How far those waves get. The comoving sound horizon against the scale factor, integrated from the beginning: the distance a pressure wave has covered by each moment. The sound speed starts at 0.577c0.577c and falls as the baryons become significant, reaching 0.45c0.45c by the drag epoch. The curve stops when the photons stop pushing, and where it stops is the length of the ruler: 144.4 comoving megaparsecs at last scattering, 146.9 at the slightly later drag epoch. Nothing about the later universe enters that number — it is fixed by the radiation, matter and baryon densities alone.

The waves are not launched at random times. They all start together, at the end of inflation, and they all stop together, when recombination removes the free electrons and the photons cease to push. So at the moment the pattern is frozen, every wave has been running for the same length of time, and there is one distance that appears everywhere: the sound horizon.

That is the whole origin of the preferred scale. A region exactly one sound horizon across has had just enough time to complete a single compression, so it is at maximum density when the light leaves — hot. A region half that size has compressed and rebounded to maximum rarefaction — also an extremum, also visible. A region of some intermediate size is caught mid-swing and shows nothing. The spectrum of patch sizes therefore has a fundamental and a series of harmonics, which is what the peaks are.

The first peak is a protractor

The damping tail measures a thickness: ℓ_D = 1400 for a shell 80 deep in redshift. The suppression of small-scale structure in the microwave background, against multipole, on logarithmic axes. Every other feature of the power spectrum measures the last-scattering surface as a surface — its distance, the sound horizon written on it, the ruler it provides. This one measures how thick it is. Recombination takes time: the ionised fraction falls over a range of redshift rather than all at once, and while it is falling the photons are still scattering, so each one random-walks. A photon taking N steps of a mean free path λ diffuses √N λ, which is much further than a single step and much less than the whole interval, and any temperature fluctuation smaller than that distance is mixed away before it can be frozen in. What is left is a Gaussian cut-off, drawn here for three shell thicknesses. A thicker shell means more steps and a longer walk, so it damps at a smaller multipole: Δz = 40 gives ℓ_D = 1980, Δz = 80 gives ℓ_D = 1400, Δz = 160 gives ℓ_D = 990. The observed cut-off is near ℓ = 1400, corresponding to a diffusion length of about 0.03 proper megaparsecs at the time — a scale the reader should compare with the sound horizon, some hundred and fifty comoving megaparsecs, which is what the peaks measure. The tail is therefore a genuine probe of the inside of the transition rather than of its position, and because the damping depends on the free-electron density it is also one of the cleanest constraints on anything that changes it: extra relativistic species, a varying fine-structure constant, or an early energy injection all move ℓ_D while leaving the peak positions nearly alone. The normalisation here is set once by the observed value, so what the figure asserts is the scaling with thickness and the shape of the cut-off, not the absolute number.
Fig. 3 Where the comb stops, and what the stopping measures. Recombination is not instantaneous: the surface the microwave background comes from is a shell some eighty thousand years thick, and a wave whose wavelength is shorter than that thickness is averaged away along the line of sight. So the peaks fade above a multipole set by the shell’s depth — observed at ℓ_D = 1400, which is a direct measurement of how long recombination took. Three thicknesses are drawn and only one puts the damping where it is seen. The standing wave is frozen at one instant in the caption and over eighty thousand years in fact, and this tail is the difference.

The angle actually measured is θ=0.0104110±0.0000031\theta_* = 0.0104110 \pm 0.0000031 radians, which is a precision of three parts in ten thousand and makes it the best-measured quantity in cosmology. What it constrains is the ratio rs/DM(z)r_{\rm s}/D_M(z_*), where DMD_M is the transverse comoving distance — the one of the four that converts a proper size into an angle, and the only one in which the curvature of space appears at all.

Curvature slides the whole comb of peaks. The same power spectrum in three universes that differ only in their spatial curvature. The physical densities are held fixed, so the sound horizon at last scattering is the same 144.4 Mpc in all three and the ruler being measured has not changed; what changes is the geometry the light crossed on its way here, and therefore the angle that ruler subtends. The acoustic scale goes from ℓ_A = 322 in the open case to 281 in the closed one, so the first peak moves from ℓ = 235 to 205 — a shift of 30 in ℓ for five per cent of curvature either way. The measured first peak is at 220, and the measured error on it corresponds to Ω_k = 0.0007 ± 0.0019. Flat is a measurement here, not an assumption: the figure shows what a curved universe would have looked like, and it does not look like this. Peak heights are held fixed because curvature does not set them; the next figure varies something that does.
Fig. 4 Why. Three universes with identical physical densities — so identical sound horizons, and identically sized hot patches — differing only in their spatial curvature. In a positively curved universe the light rays from the two ends of the ruler converge on the way here, so the patch looks bigger and the peaks move left; in a negatively curved one they diverge and the peaks move right. The acoustic scale runs from 322 to 281 across five per cent of curvature either way, and the first peak from =235\ell = 235 to 205. The measured peak is at 220. Peak heights are held fixed because curvature does not set them.

The result is Ωk=0.0007±0.0019\Omega_k = 0.0007 \pm 0.0019: the universe is spatially flat to a fifth of a per cent. That is a measurement, not an assumption, and the figure exists to make the point that a curved universe would have looked visibly different.

It comes with a caveat that the plot cannot show. The peak position constrains a combination of the curvature and the expansion history, so a curved universe with a compensating change in the matter density and the expansion rate can reproduce the same angle — the “geometric degeneracy”. Breaking it needs a second observable, and the second observable is the same acoustic scale measured in galaxy surveys at low redshift, where the geometry of the intervening space contributes almost nothing. The quoted flatness is a joint result, and it is the clearest example in the subject of two measurements of one length at two epochs doing what neither can do alone.

The same combination is what makes the peak position central to the disagreement about the expansion rate. The angle is measured to three parts in ten thousand and is not in dispute; what is in dispute is the length of the ruler, because that comes from the pre-recombination physics, and a seven per cent shorter sound horizon would move the inferred expansion rate by the whole of the discrepancy.

The odd peaks are taller, and that weighs the baryons

Baryons make the odd peaks taller. Three baryon densities, and what each does to the alternation between odd and even acoustic peaks. Baryons add inertia to the photon–baryon fluid without adding pressure, so it falls further into a gravitational well than it rebounds out of one: compressions are deeper than rarefactions, the odd-numbered peaks are compressions, and the ratio of the first peak to the second scales as (1 + 6R) with R = 3ρ_b/4ρ_γ at last scattering. At the measured Ω_b h² = 0.02237 that gives R = 0.622, and the drawn first-to-second ratios run 1.59, 2.26, 3.03 across Ω_b h² = 0.014, 0.02237, 0.032. Only that ratio is derived: the absolute heights come from the Planck measurement and the geometric mean of each adjacent pair is held fixed, because the envelope is set by radiation driving and photon diffusion, which no figure of this kind computes. What the alternation buys is a weighing of the ordinary matter in the universe from the shape of a sky map — a number that agrees, to better than a per cent, with the one deuterium gives.
Fig. 5 What the baryon density does. Baryons add inertia to the photon–baryon fluid without adding pressure, so the fluid falls further into a gravitational well than it rebounds out of one — compressions go deeper than rarefactions. The odd-numbered peaks are compressions, so raising the baryon density raises them relative to the even ones, and the ratio of the first peak to the second scales as (1+6R)(1+6R). At the measured Ωbh2=0.02237\Omega_{\rm b}h^2 = 0.02237 that gives R=0.622R = 0.622; the drawn first-to-second ratios run 1.59, 2.26 and 3.03 across the three densities. Only the ratio is derived here — the absolute heights come from the measurement, because the envelope is set by radiation driving and photon diffusion.

This is the step that turns a map of temperature into a measurement of how much ordinary matter the universe contains. The answer, Ωbh2=0.02237±0.00015\Omega_{\rm b}h^2 = 0.02237 \pm 0.00015, is a 0.7 per cent determination of the density of protons and neutrons — from the relative heights of two bumps in a power spectrum. It agrees with the completely independent value from the light-element abundances to better than a per cent, and the two have nothing in common: one is a fluid oscillation at four hundred thousand years, the other a reaction network in the first three minutes.

The third peak does a different job. Its height relative to the second is sensitive to the total matter density, because the depth of the potential wells at the time depends on how much dark matter had already collected in them. That is where Ωch2\Omega_{\rm c}h^2 comes from, and it is the reason the microwave background constrains dark matter — the same substance the rotation curves find, measured by a route with no galaxies in it at all.

Why the peaks die away

Past 1000\ell \approx 1000 the peaks shrink, and two separate effects are doing it. The second is Silk damping, and it is the more important of the two. Photons do not scatter instantaneously; they random-walk through the plasma with a mean free path that grows as recombination proceeds, and over the age of the universe at that time they diffuse a certain distance. Any temperature variation smaller than that diffusion length is smeared out by the photons themselves carrying heat from hot regions to cold ones. The diffusion scale at last scattering is about 10 comoving megaparsecs, which corresponds to 1400\ell \approx 1400, and the exponential fall of the spectrum past there is its signature.

The damping tail is not a loss. Its slope depends on how quickly recombination happened, which depends on the baryon density and on the number of relativistic species present, so the region beyond the third peak is where the microwave background constrains the effective number of neutrinos. Measuring it was the main scientific case for the ground-based experiments that followed Planck.

Where the fluctuations came from

Everything above takes the initial overdensities as given. They have to come from somewhere, and the sound waves cannot make them — a wave needs something to launch it. The reason this matters for the peaks is a question of phase. A wave that is launched at a random time contributes at a random point in its cycle, and averaging over many such waves washes out the peaks entirely. The peaks exist only because every wave of a given wavelength started at the same phase — at rest, with an overdensity already in place. That is what “adiabatic, growing-mode, super-horizon initial conditions” means, and it is a substantive prediction of inflation that could easily have failed. The peaks are sharp, so the initial conditions were coherent, and coherence over scales larger than the horizon at the time is not something a causal process inside the horizon can produce.

The spectrum of initial amplitudes is measured too, and it is nearly but not exactly scale-invariant: ns=0.9649±0.0042n_{\rm s} = 0.9649 \pm 0.0042. Exactly 1 would mean every scale started with equal power; the measured tilt is a four per cent departure, and it is significant at fifteen sigma.

The plateau at the left of the plot

The peaks occupy the middle of the spectrum. To their left, below about =30\ell = 30, the curve flattens into a plateau, and that region is measuring something different from everything the peaks measure.

Scales larger than the sound horizon at last scattering were never inside the horizon while the fluid could oscillate, so no wave ever ran across them. They carry the primordial fluctuations unprocessed — the potential field as inflation left it, imprinted on the temperature by a single effect.

A photon climbing out of a gravitational potential well is redshifted; a photon emitted from a region where the clock ran slow appears to come from a different epoch. The two combine, and the result is that a temperature fluctuation of one third of the potential’s depth is imprinted directly. That is the Sachs–Wolfe effect, and it is the reason the plateau exists and is flat: a scale-invariant spectrum of potentials produces a flat plateau in the quantity conventionally plotted.

Its measurement is limited in a way nothing else on the plot is. There are only 2+12\ell+1 independent modes at each multipole, so at =2\ell = 2 there are five numbers in the entire universe and no instrument will ever measure them better. That is cosmic variance, it is a hard floor, and it is why the leftmost points on any published spectrum carry error bars an order of magnitude larger than the ones in the middle.

The plateau is also where the largest-scale anomalies live — a quadrupole lower than expected, an alignment between the lowest multipoles, a hemispherical asymmetry in power. Each is a departure of a couple of standard deviations, each has been checked in two independent experiments, and none is significant enough to be a detection given how many such tests could have been performed. A region measured with five numbers cannot settle an argument, and the honest position is that the anomalies will remain exactly as unresolved as they are.

What is measured, and what is not

The observable is a map of temperature over the sky, in several frequency bands, from which the Galaxy has to be subtracted. That subtraction is the dominant systematic below =30\ell = 30 and is why the largest angular scales have the largest error bars — there is only one sky, so the sample variance at low \ell is irreducible, and the foregrounds are worst exactly there.

From the cleaned map the power spectrum is computed, and the power spectrum is not the map: it discards all the phase information and keeps only the variance per scale. That is the right thing to do if the fluctuations are Gaussian, because then the power spectrum contains everything. Whether they are Gaussian is a separate measurement, and so far they are, to the precision available.

From the power spectrum, six parameters are fitted. Every cosmological number quoted from Planck — the age, the densities, H0H_0, σ8\sigma_8 — is an output of that fit and not a reading. The peak positions and heights are the data; the parameters are the interpretation.

What the picture cannot show

The drawn curve is a representation of a measurement, not a derivation. Producing the spectrum from the parameters requires integrating the coupled photon, baryon, neutrino and dark-matter perturbations through recombination, which is a Boltzmann code’s work. The figure separates the two halves deliberately: the curve interpolates published extrema, and the computed content is the tick marks. Reading the interpolation between two peaks as a prediction would be reading a fabrication.

The spectrum is an average over the whole sky and cannot show where anything is. Two maps with identical power spectra can look entirely different, and one of the standing questions about the real sky — whether the largest-scale features have anomalous alignments — is invisible to this plot by construction.

And the plot has no error bars. At low \ell the uncertainty is dominated by there being only 2+12\ell+1 independent samples of each mode on one sky; at high \ell by the instrument. The middle range is measured to a fraction of a per cent, and the impression a clean curve gives is accurate there and misleading at both ends.

Two of the parameters the spectrum measures are worth pushing well outside their fitted values, because the shape of the response is what makes each of them separable from the others.

Baryons make the odd peaks taller. Three baryon densities, and what each does to the alternation between odd and even acoustic peaks. Baryons add inertia to the photon–baryon fluid without adding pressure, so it falls further into a gravitational well than it rebounds out of one: compressions are deeper than rarefactions, the odd-numbered peaks are compressions, and the ratio of the first peak to the second scales as (1 + 6R) with R = 3ρ_b/4ρ_γ at last scattering. At the measured Ω_b h² = 0.02237 that gives R = 0.622, and the drawn first-to-second ratios run 1.27, 2.26, 4.06 across Ω_b h² = 0.01, 0.02237, 0.045. Only that ratio is derived: the absolute heights come from the Planck measurement and the geometric mean of each adjacent pair is held fixed, because the envelope is set by radiation driving and photon diffusion, which no figure of this kind computes. What the alternation buys is a weighing of the ordinary matter in the universe from the shape of a sky map — a number that agrees, to better than a per cent, with the one deuterium gives.
Fig. 6 The peak structure for baryon densities spanning a factor of four and a half. The odd peaks rise and the even ones fall, and no other parameter does that — which is why the baryon density is measured to under one per cent from a spectrum whose overall amplitude is degenerate with several other things.
Curvature slides the whole comb of peaks. The same power spectrum in three universes that differ only in their spatial curvature. The physical densities are held fixed, so the sound horizon at last scattering is the same 144.4 Mpc in all three and the ruler being measured has not changed; what changes is the geometry the light crossed on its way here, and therefore the angle that ruler subtends. The acoustic scale goes from ℓ_A = 342 in the open case to 259 in the closed one, so the first peak moves from ℓ = 250 to 189 — a shift of 61 in ℓ for five per cent of curvature either way. The measured first peak is at 220, and the measured error on it corresponds to Ω_k = 0.0007 ± 0.0019. Flat is a measurement here, not an assumption: the figure shows what a curved universe would have looked like, and it does not look like this. Peak heights are held fixed because curvature does not set them; the next figure varies something that does.
Fig. 7 And for curvatures twice as large as the observations allow. The whole comb slides sideways without changing shape, which is the signature that makes curvature separable — a shift is not something any of the other five parameters can produce.

Why six parameters, and what a seventh would do

The model fitted to the spectrum has six free numbers, and the count is worth examining because it is the whole basis for calling the fit a success.

Two are densities: the physical density of baryons and of cold dark matter. One is the angular scale of the sound horizon, which stands in for the expansion history. Two describe the primordial fluctuations: an amplitude and a tilt. And one is the optical depth to reionisation, which suppresses the small-scale power by a constant factor and is degenerate with the amplitude until polarisation breaks it.

Six numbers, and the spectrum they are fitted to contains something like two thousand independent multipoles, each measured to a precision that is not trivial. So the fit is enormously over-determined, and the residuals are a test rather than a leftover.

That is the point people usually miss about the model’s success. A six-parameter fit to two thousand points that comes out with an acceptable chi-squared is a strong statement; the same fit with twenty parameters would not be. Every proposed extension — curvature, a running spectral index, a varying dark-energy equation of state, extra relativistic species, a neutrino mass — is a seventh parameter, and each is measured to be consistent with zero or with its standard value.

The consequence is a peculiar situation. The model is not favoured because it explains anything; it is favoured because nothing has been found that requires more than it. A theory that survives by not being contradicted is in a weaker position than one that predicts something new, and the field’s discomfort about that is why so much effort goes into the observations that could add a seventh number — the damping tail’s neutrino count, the polarisation’s tensor amplitude, and the growth of structure at low redshift.

The generalisation

The move here is one of the oldest in physics: a resonance in a bounded medium turns a continuous spectrum into a discrete one, and the discrete positions measure the boundary.

An organ pipe of a given length produces a fundamental and its harmonics, and hearing the fundamental measures the pipe. Here the “pipe” is the time available before the photons let go, the harmonics are the peaks, and the measurement is the pipe’s length in comoving megaparsecs. The unusual feature is only that the bound is temporal rather than spatial — the wave stops not because it hits a wall but because the medium ceases to exist.

The same reasoning appears in this collection wherever a periodic system is used as a clock or a ruler. A pulsating star’s period is set by the sound travel time across it, which is why a longer period means a bigger and therefore brighter star. A resonance between two orbits clears a gap at a computable radius, and the radius measures the perturber. Spiral arms exist only between the Lindblad resonances, and the boundaries follow from the rotation curve.

What makes the cosmological case unusually clean is that the pipe’s length is set by physics that involves only the densities, and the densities are measured by the same spectrum. The ruler calibrates itself.

And the spectrum truncated at the multipole where the first generation of experiments stopped, which is where most of the parameters were first pinned down.

The acoustic peaks, and where the geometry says they should be. The temperature angular power spectrum of the microwave background. The drawn curve is a monotone interpolation through the published positions and heights of the six peaks and five troughs of the Planck 2018 TT measurement — it is a representation of data, and nothing between two extrema is claimed. The marks along the top are not: they are computed from this collection's own cosmology as ℓₐ(m − 0.267), where ℓₐ = π × 13866 / 144.43 = 301.6 — π times the comoving distance to last scattering divided by the sound horizon there — is the angle the sound horizon subtends at last scattering turned into a multipole. The two agree to 2.8 per cent at worst across six peaks, which is the whole of what makes this a measurement of geometry: a wave of known physical wavelength, seen at a known distance, is a protractor. The first peak at ℓ = 220 corresponds to about 0.82 degrees on the sky — roughly twice the width of the full Moon, which is the largest hot and cold patch the sky has.
Fig. 8 The same spectrum to multipole 1200 rather than 2500. Three peaks are visible and the damping tail is only beginning, and this is the data on which the geometry was established — everything beyond it refines parameters rather than deciding the shape of the universe.

One more reading spans a wider range of the thickness the damping tail measures.

The damping tail measures a thickness: ℓ_D = 1400 for a shell 80 deep in redshift. The suppression of small-scale structure in the microwave background, against multipole, on logarithmic axes. Every other feature of the power spectrum measures the last-scattering surface as a surface — its distance, the sound horizon written on it, the ruler it provides. This one measures how thick it is. Recombination takes time: the ionised fraction falls over a range of redshift rather than all at once, and while it is falling the photons are still scattering, so each one random-walks. A photon taking N steps of a mean free path λ diffuses √N λ, which is much further than a single step and much less than the whole interval, and any temperature fluctuation smaller than that distance is mixed away before it can be frozen in. What is left is a Gaussian cut-off, drawn here for three shell thicknesses. A thicker shell means more steps and a longer walk, so it damps at a smaller multipole: Δz = 20 gives ℓ_D = 2800, Δz = 80 gives ℓ_D = 1400, Δz = 320 gives ℓ_D = 700. The observed cut-off is near ℓ = 1400, corresponding to a diffusion length of about 0.03 proper megaparsecs at the time — a scale the reader should compare with the sound horizon, some hundred and fifty comoving megaparsecs, which is what the peaks measure. The tail is therefore a genuine probe of the inside of the transition rather than of its position, and because the damping depends on the free-electron density it is also one of the cleanest constraints on anything that changes it: extra relativistic species, a varying fine-structure constant, or an early energy injection all move ℓ_D while leaving the peak positions nearly alone. The normalisation here is set once by the observed value, so what the figure asserts is the scaling with thickness and the shape of the cut-off, not the absolute number.
Fig. 9 The damping tail for last-scattering surfaces spanning a factor of sixteen in thickness. The tail steepens in proportion, so the thickness is read off the slope — and the measured slope is what puts the surface’s own depth at about a tenth of its redshift.

Where the ladder goes next

The peaks give the angle. Turning the angle into a distance needs the ruler’s length, which needs the baryon density — and the baryon density has an entirely independent measurement, three minutes after the beginning, which is the next essay.

Later rungs on this anchor: polarisation, which is a second map from the same photons and settles several degeneracies the temperature alone cannot; lensing of the microwave background by the intervening structure, which measures the matter distribution at z2z \approx 2; the integrated Sachs–Wolfe effect at the largest scales, which is a direct probe of dark energy; the damping tail and the effective number of neutrinos; and the search for a BB-mode polarisation signal from primordial gravitational waves, which would fix the energy scale of inflation and has so far produced only upper limits.

What this makes readable

Essays that name this one as a prerequisite.

About the same objects

Not linked from either essay — found by the objects both name.

What links here

The 8 of 24 essays linking to this one that name the most of the same objects.

The objects this essay names

Each one links to every other essay that touches it.

Acoustic peaksAngular power spectrumBaryon loadingMultipolePhoton baryon fluidPrimordial fluctuationsSilk dampingSound horizonSpatial curvatureStandard ruler