Cosmic transparency

A test with the baryon acoustic feature and type Ia supernovae

Surhud More, Jo Bovy, David W. Hogg

    Research output: Contribution to journalArticle

    Abstract

    Conservation of the phase-space density of photons plus Lorentz invariance requires that the cosmological luminosity distance be larger than the angular diameter distance by a factor of (1 + z)2, where z is the redshift. Because this is a fundamental symmetry, this prediction - known sometimes as the "Etherington relation" or the "Tolman test" - is independent of the world model, or even the assumptions of homogeneity and isotropy. It depends, however, on Lorentz invariance and transparency. Transparency can be affected by intergalactic dust or interactions between photons and the dark sector. Baryon acoustic feature (BAF) and type Ia supernovae (SNeIa) measures of the expansion history are differently sensitive to the angular diameter and luminosity distances and can therefore be used in conjunction to limit cosmic transparency. At the present day, the comparison only limits the change Δτ in the optical depth from redshift 0.20 to 0.35 at visible wavelengths to Δτ < 0.13 at 95% confidence. In a model with a constant comoving number density n of scatterers of constant proper cross section σ, this limit implies nσ < 2 × 10 -4 h Mpc-1. These limits depend weakly on the cosmological world model. Assuming a concordance world model, the best-fit value of Δτ to current data is negative at the 2σ level. This could signal interesting new physics or could be the result of unidentified systematics in the BAF/SNeIa measurements. Within the next few years, the limits on transparency could extend to redshifts z 2.5 and improve to nσ < 1.1 × 10-5 h Mpc-1. Cosmic variance will eventually limit the sensitivity of any test using the BAF at the nσ ∼ 4 × 10-7 h Mpc-1 level. Comparison with other measures of the transparency is provided; no other measure in the visible is as free of astrophysical assumptions.

    Original languageEnglish (US)
    Pages (from-to)1727-1732
    Number of pages6
    JournalAstrophysical Journal
    Volume696
    Issue number2
    DOIs
    StatePublished - May 10 2009

    Fingerprint

    transparency
    supernovae
    baryons
    acoustics
    invariance
    luminosity
    isotropy
    conjunction
    space density
    optical depth
    homogeneity
    photons
    symmetry
    physics
    optical thickness
    cross section
    test
    conservation
    confidence
    astrophysics

    Keywords

    • cosmological parameters
    • cosmology: observations
    • large-scale structure of universe
    • radiative transfer
    • relativity
    • supernovae: general

    ASJC Scopus subject areas

    • Space and Planetary Science
    • Astronomy and Astrophysics

    Cite this

    Cosmic transparency : A test with the baryon acoustic feature and type Ia supernovae. / More, Surhud; Bovy, Jo; Hogg, David W.

    In: Astrophysical Journal, Vol. 696, No. 2, 10.05.2009, p. 1727-1732.

    Research output: Contribution to journalArticle

    More, Surhud ; Bovy, Jo ; Hogg, David W. / Cosmic transparency : A test with the baryon acoustic feature and type Ia supernovae. In: Astrophysical Journal. 2009 ; Vol. 696, No. 2. pp. 1727-1732.
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