Dispersion of the luminosity distance as a cosmological probe
Dispersion of the luminosity distance as a cosmological probe
Dispersion of the luminosity distance as a cosmological probe
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LC Averaging <br />
! Useful for interpreting light-‐like <br />
signals in <strong>cosmological</strong> <br />
observations. <br />
! Hyper-‐surfaces using meaningful <br />
physical quantities: Redshift, <br />
temperature etc. <br />
! Observations are made on <strong>the</strong> <br />
light-‐cone. Volume averaging <br />
give artefacts and <strong>the</strong> matching <br />
with data is not clear. <br />
! P<strong>as</strong>t attempts: Coley 0905.2442; <br />
R<strong>as</strong>anen 1107.1176, 0912.3370
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