Lecture 06: The CMB Acoustic Scale

ASTR 476: Observational Cosmology · 2026-09-27

Driving question: Why is the microwave background a distance probe?

Learning objectives

  1. Explain acoustic oscillations and the sound horizon at last scattering.
  2. Convert 100 theta_* to an angular scale with correct units.
  3. Identify the assumptions needed to infer H0 or curvature from the CMB.
Terms · 8 min

Terms for This Lecture

Acoustic scale

Definition: The angle subtended by the sound horizon at last scattering.

Why it matters here: It is required to answer Why is the microwave background a distance probe? and to distinguish direct observation from cosmological inference.

Relationships: Read it with Sound horizon at recombination, the model \(theta_* = r_s(z_*)/D_M(z_*)\), and the evidence statement The official Planck Legacy Archive binned TT/TE products were requested during production but could not be retrieved (TT extraction failure; TE HTTP 401). Only the published parameter summary is used; the plotted peak sequence is explicitly theoretical.

Boundary or common confusion: The plotted schematic is not Planck data, and theta_* is not simply the angular size of a rigid object with no recombination physics.

Slide 1 · 8 min

Photon-baryon oscillator

Use gravity, radiation pressure, and loading to explain alternating compression and rarefaction peaks.

Slide 2 · 10 min

A ruler subtends an angle

Define r_s and D_M, derive theta_*, and distinguish radians from degrees.

Slide 3 · 12 min

Peak locations are not the whole spectrum

Explain how heights and damping also depend on baryon density, matter density, and recombination.

Slide 4 · 12 min

Planck summary with provenance

Use the exact TT,TE,EE+lowE flat-LCDM label and report the archive download limitation.

Slide 5 · 10 min

Parameter inference is conditional

Trace the chain from measured spectrum to theta_* to model-dependent distance and expansion constraints.

Slide 6 · 8 min

Interpret the plotted spectrum

Identify it as a schematic oscillator with no observational bandpowers or likelihood attached.

The CMB Acoustic ScaleThe official Planck Legacy Archive binned TT/TE products were requested during production but could not be retrieved (TT extraction failure; TE HTTP 401). Only the published parameter summary is used; the plotted peak sequence is explicitly theoretical.multipole ell (schematic; not Planck bandpowers)illustrative C_ellcompressionrarefactiondamping tailTheoretical acoustic-peak sketch; not observed Planck data
The official Planck Legacy Archive binned TT/TE products were requested during production but could not be retrieved (TT extraction failure; TE HTTP 401). Only the published parameter summary is used; the plotted peak sequence is explicitly theoretical.

Quantitative anchor

Planck reports 100 theta-star=1.0411 +/- 0.0003; conversion gives theta-star=0.596506 degrees.

\[theta_* = r_s(z_*)/D_M(z_*)\]

Interpretation and limits

Acoustic peak spacing compares the sound horizon at last scattering to its angular-diameter distance. The observed angular scale is precise, but converting it to late-time parameters depends on the pre-recombination model and correlated spectra.

Boundary: The plotted schematic is not Planck data, and theta_* is not simply the angular size of a rigid object with no recombination physics.

Evidence: The official Planck Legacy Archive binned TT/TE products were requested during production but could not be retrieved (TT extraction failure; TE HTTP 401). Only the published parameter summary is used; the plotted peak sequence is explicitly theoretical.

Active check: Identify it as a schematic oscillator with no observational bandpowers or likelihood attached.

ASTR 476 · Lecture 06 · 60-minute module · The CMB Acoustic Scale