A precise and accurate determination of the cosmic microwave background temperature at z = 0.89
Artikel i vetenskaplig tidskrift, 2013

Context. According to the Big Bang theory and as a consequence of adiabatic expansion of the Universe, the temperature of the cosmic microwave background (CMB) increases linearly with redshift. This relation is, however, poorly explored, and detection of any deviation would directly lead to (astro-)physics beyond the standard model. Aims. We aim to measure the temperature of the CMB with an accuracy of a few percent at z = 0.89 toward the molecular absorber in the galaxy lensing the quasar PKS 1830−211. Methods. We adopted a Monte-Carlo Markov chain approach, coupled with predictions from the non-LTE radiative transfer code RADEX, to solve the excitation conditions of a set of various molecular species directly from their spectra. Results. We determine TCMB = 5.08  ±  0.10 K at 68% confidence level. Our measurement is consistent with the value TCMB = 5.14 K predicted by the standard cosmological model with adiabatic expansion of the Universe. This is the most precise determination of TCMB at z > 0 to date.

cosmology: observations / cosmic background radiation / cosmological parameters / quasars: absorption lines / quasars: individual: PKS 1830 / 211

Författare

Sebastien Muller

Chalmers, Rymd- och geovetenskap, Onsala rymdobservatorium

A. Beelen

Universite Paris-Sud XI

John H Black

Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik

S.J. Curran

ARC Centre of Excellence for All-sky Astrophysics (CAASTRO

The University of Sydney

Cathy Horellou

Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik

Susanne Aalto

Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik

F. Combes

CNRS Centre National de la Recherche Scientifique

M. Guélin

Ecole Normale Superieure (ENS)

Institut de RadioAstronomie Millimetrique (IRAM)

C. Henkel

Max Planck-institutet

King Abdulaziz University

Astronomy and Astrophysics

0004-6361 (ISSN) 1432-0746 (eISSN)

Vol. 551 A109 (pp. 1-13) A109

Ämneskategorier

Astronomi, astrofysik och kosmologi

Fundament

Grundläggande vetenskaper

Infrastruktur

Onsala rymdobservatorium

DOI

10.1051/0004-6361/201220613