GLOW
THE COSMIC MICROWAVE BACKGROUND
Point a radio telescope at any empty patch of sky.
BEGIN — CHAPTER 01 →A noise that came from everywhere
Penzias and Wilson measured about 3.5 K of excess noise [1].
Dicke's group explained it [2]; predicted earlier [19]; Nobel 1978 [3].
One temperature fits every point
FIRAS: deviations under 50 ppm [5][6].
T0 = 2.72548 K [7]; Nobel 2006 [8].
FIRAS points [5].
A thermometer that runs back in time
z* = 1089.92 [11] → about 2,970 K.
About 370,000 years; age today 13.797 Gyr [11].
Presets.
One part in a thousand, then one in a hundred thousand
Dipole 3.362 mK from 369.82 km/s [10]; DMR [4]; RELIKT-1 [20].
30 µK, one part in 100,000 [9].
Notes.
Bringing the ripples into focus
WMAP: 13′, first peak at ℓ = 220.1 [12][13][14].
Planck: about 5′ [10][17].
Simulated sky, not the real one.
A billion pixels, six numbers
θ* to 0.03 %; 18 peaks [10][11].
Six parameters; H0 tension [10][11].
From a hiss in a horn to a precision science
See it as an installation: Relic draws Planck's real map of this light, lets you add our motion and blur it to COBE's beam, and plays its spectrum as a chord.
The same 3-kelvin glow.