Acoustic scale — where it appears
Named by 4 essays across 2 fields — each of them below, with the objects they name alongside it.
The number that would say whether it is a constant
Whether dark energy is a cosmological constant is the question of whether w is exactly −1, and w = −0.9 changes a distance modulus by thirty-four millimagnitudes at redshift a half — a fifth of the scatter of a single supernova, along a degeneracy only the acoustic scale can cut across.
A crossing that may belong to the fitting form
Allow the dark energy's equation of state to change and three independent fits say it has: above −1 today, below it before redshift half. The data hold w well at one redshift only, a line crossed from below is one no single field can cross, and a straight line in the scale factor fitted to a curved history crosses it anyway.
A flatness that needs a second distance
The universe is said to be flat to two parts in a thousand, and the figure is usually credited to the microwave background. On its own the background measures one angle, and one angle fixes one distance — so every curvature has a Hubble constant that reproduces the peaks exactly. Flatness is where that line crosses a second measurement, and it is only as good as the crossing.
Two distances that must agree if light is conserved
A supernova's distance comes from how faint it is; an acoustic ruler's distance comes from how small it looks. In any universe whose light follows the geometry and is neither created nor destroyed, the two are tied by an exact factor of (1 + z)², whatever the universe contains. Dust that dimmed distant supernovae without reddening them could have faked the accelerating expansion — and would have broken that tie by a fifth by redshift a half. The tie holds to a few per cent.
Named alongside it
The objects these essays reach for when they reach for this one.
Cosmological constantDegeneracy directionEquation of stateFigure of meritPhotometric calibrationQuintessenceType ia supernovaeAccelerating expansionAge of the universeAngular-diameter distanceBaryon acoustic oscillationsCosmic microwave background