Lecture 05: Baryon Acoustic Oscillations as a Standard Ruler

ASTR 476: Observational Cosmology · 2026-09-27

Driving question: How do galaxy clustering measurements encode distance?

Learning objectives

  1. Derive D_V from transverse and radial distance information.
  2. Distinguish D_V/r_d from D_M/r_d and H r_d.
  3. State the sound-horizon convention when comparing a model to a published BAO point.
Terms · 8 min

Terms for This Lecture

Baryon acoustic oscillation

Definition: The late-time clustering imprint of sound waves in the pre-recombination photon-baryon plasma.

Why it matters here: It is required to answer How do galaxy clustering measurements encode distance? and to distinguish direct observation from cosmological inference.

Relationships: Read it with Sound horizon, the model \(D_V(z)=[D_M(z)^2 c z/H(z)]^(1/3)\), and the evidence statement Three published BOSS DR12 consensus points at z=0.38, 0.51, and 0.61 are included as literature-summary measurements, not raw clustering data.

Boundary or common confusion: Do not compare D_V in Mpc directly to D_V r_d,fid/r_d unless explicitly setting r_d=r_d,fid; BAO does not measure an absolute ruler without early-universe calibration.

Slide 1 · 8 min

A fossil in the correlation function

Trace the acoustic wave before and after baryon drag and identify the late-time comoving ruler.

Slide 2 · 10 min

Isotropic compression

Derive the volume-preserving D_V combination and note information lost by spherical averaging.

Slide 3 · 12 min

Anisotropic geometry

Explain how transverse pair separations and radial redshift separations constrain different expansion components.

Slide 4 · 12 min

BOSS DR12 published summaries

Read the three redshifts, central values, uncertainties, and r_d,fid/r_d convention from the cited consensus table.

Slide 5 · 10 min

Compute then compare

Calculate D_V from the course fiducial cosmology and make the conditional r_d=r_d,fid assumption explicit.

Slide 6 · 8 min

What BAO alone leaves open

Explain the degeneracy between late-time distances and the calibrated physical ruler.

Baryon Acoustic Oscillations as a Standard RulerThree published BOSS DR12 consensus points at z=0.38, 0.51, and 0.61 are included as literature-summary measurements, not raw clustering data.BOSS DR12 consensus: D_V r_d,fid/r_dz=0.381477 +/- 16 Mpcz=0.511877 +/- 19 Mpcz=0.612140 +/- 22 Mpcruler-scaled volume distance (Mpc)Published summary points; no cross-redshift covariance shown
Three published BOSS DR12 consensus points at z=0.38, 0.51, and 0.61 are included as literature-summary measurements, not raw clustering data.

Quantitative anchor

The flat-LCDM model gives D_V(0.38)=1477.922 Mpc; comparison requires the explicitly stated r_d=r_d,fid convention.

\[D_V(z)=[D_M(z)^2 c z/H(z)]^(1/3)\]

Interpretation and limits

The pre-recombination sound horizon imprints a preferred clustering separation. Isotropic analyses compress transverse and radial information into D_V/r_d; anisotropic analyses constrain D_M/r_d and H(z)r_d separately.

Boundary: Do not compare D_V in Mpc directly to D_V r_d,fid/r_d unless explicitly setting r_d=r_d,fid; BAO does not measure an absolute ruler without early-universe calibration.

Evidence: Three published BOSS DR12 consensus points at z=0.38, 0.51, and 0.61 are included as literature-summary measurements, not raw clustering data.

Active check: Explain the degeneracy between late-time distances and the calibrated physical ruler.

ASTR 476 · Lecture 05 · 60-minute module · Baryon Acoustic Oscillations as a Standard Ruler