Journal Article

Precise cosmological parameter estimation using C<span class="smallCaps">osmo</span>R<span class="smallCaps">ec</span>

J. R. Shaw and J. Chluba

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 415, issue 2, pages 1343-1354
Published in print August 2011 | ISSN: 0035-8711
Published online July 2011 | e-ISSN: 1365-2966 | DOI:
Precise cosmological parameter estimation using CosmoRec

More Like This

Show all results sharing this subject:

  • Astronomy and Astrophysics


Show Summary Details


We use the new cosmological recombination code, CosmoRec, for parameter estimation in the context of (future) precise measurements of the cosmic microwave background (CMB) temperature and polarization anisotropies. We address the question of how previously neglected physical processes in the recombination model of Recfast affect the determination of key cosmological parameters, for the first time performing a model-by-model computation of the recombination problem. In particular, we ask how the biases depend on different combinations of parameters, e.g. when varying the helium abundance or the effective number of neutrino species in addition to the standard six parameters. We forecast how important the recombination corrections are for Planck, and a survey cosmic-variance limited up to l = 2000. For example, we find that for a Λ cold dark matter (ΛCDM) analysis, ns may be biased by over 3σ and 7σ in each case, whereas when Yp is allowed to vary its value can be biased by over 2σ and 7σ. We find similar shifts for other parameter combinations. Furthermore, we ask which recombination corrections are really crucial for CMB parameter estimation, and ask whether an approach based on a redshift-dependent correction function to Recfast is sufficient.

Keywords: radiative transfer; cosmic background radiation

Journal Article.  8147 words.  Illustrated.

Subjects: Astronomy and Astrophysics

Full text: subscription required

How to subscribe Recommend to my Librarian

Users without a subscription are not able to see the full content. Please, subscribe or login to access all content.