DARK — TECHNICAL FIELD GUIDE / ТЕХНИЧЕСКИЙ СПРАВОЧНИК
PHASEUNSEEN
DARK SHARE—
SIGNAL / NOISE—
← INDEX — ROMAN LAUNCHED 30 AUGUST 2026 4.9 % · 26.5 % · 68.5 %

DARK
EUCLID & ROMAN: MAPPING DARK MATTER AND DARK ENERGY

Ordinary matter is about a twentieth of the universe.

BEGIN — CHAPTER 01 →
CH.01 / 08 — ZWICKY, 1933

A cluster moving too fast to hold together

Zwicky: at least 400 times.

Planck: 4.9 / 26.5 / 68.5.

THE UNIVERSE'S BUDGET, PLANCK 2018
Ωb = Ωbh² / h²  ·  Ωc = Ωch² / h²  ·  ΩΛ ≈ 1 − Ωm
Budget.
CH.02 / 08 — RUBIN AND FORD, 1970–1980

Galaxies that spin too fast at the edge

Rubin & Ford.

NGC 3198.

CIRCULAR SPEED AND THE MASS INSIDE
v² = G M(<R) / R  ·  vvis² = vgas² + Υ vdisk²  ·  vhalo² = 4πGρ₀Rc² [1 − (Rc/R) arctan(R/Rc)]
Circular speed.
INSTRUMENT 1 · A DARK HALO FOR NGC 3198
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SPARC data.

CH.03 / 08 — SUPERNOVAE, 1998

The expansion is speeding up

Riess, Perlmutter.

Nobel 2011.

LUMINOSITY DISTANCE
E(z) = √(Ωm(1+z)³ + Ωk(1+z)² + ΩΛ)  ·  dL = (1+z) (c/H₀) Sk(∫₀z dz′/E)  ·  μ = 5 log₁₀(dL/10 pc)
Luminosity distance.
INSTRUMENT 2 · HOW FAR IS THE SUPERNOVA?
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Model curves.

CH.04 / 08 — EUCLID, 2023–

Weighing the dark by the way it bends light

Weak lensing.

Euclid.

AVERAGING AWAY THE SHAPES
eobs ≈ eint + γ  ·  σ(ē) = σε / √N  ·  S/N = γ √N / σε
Shape noise.
INSTRUMENT 3 · WHY A BILLION GALAXIES
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Ellipses.

Q1 and DR1.

Why lensing.

CH.05 / 08 — ROMAN, 2026–

Hubble's mirror, two hundred Hubbles' view

Roman.

Roman status.

FoV table.

Webb link.

CH.06 / 08 — AN OPEN QUESTION, 2025–2026

Is dark energy changing? Not settled

DESI DR2.

Dovekie.

Sigma.

CH.07 / 08 — LEGACY

Ninety years of measuring what cannot be seen

Effects, not the thing itself.

CH.08 / 08 — REFERENCES

Sources cited throughout this guide