首页    期刊浏览 2024年12月02日 星期一
登录注册

文章基本信息

  • 标题:Statistical isotropy violation in WMAP CMB maps resulting from non-circular beams
  • 本地全文:下载
  • 作者:Santanu Das ; Santanu Das ; Sanjit Mitra
  • 期刊名称:Astronomy & Astrophysics
  • 印刷版ISSN:0004-6361
  • 电子版ISSN:1432-0746
  • 出版年度:2016
  • 卷号:591
  • 页码:1-4
  • DOI:10.1051/0004-6361/201424164
  • 语种:English
  • 出版社:EDP Sciences
  • 摘要:Statistical isotropy (SI) of cosmic microwave background (CMB) fluctuations is a key observational test to validate the cosmological principle underlying the standard model of cosmology. While a detection of SI violation would have immense cosmological ramification, it is important to recognise their possible origin in systematic effects of observations. The WMAP seven year (WMAP-7) release claimed significant deviation from SI in the bipolar spherical harmonic (BipoSH) coefficients and . Here we present the first explicit reproduction of the measurements reported in WMAP-7, confirming that beam systematics alone can completely account for the measured SI violation. The possibility of such a systematic origin was alluded to in WMAP-7 paper itself and other authors but not as explicitly so as to account for it accurately. We simulate CMB maps using the actual WMAP non-circular beams and scanning strategy. Our estimated BipoSH spectra from these maps match the WMAP-7 results very well. It is also evident that only a very careful and adequately detailed modelling, as carried out here, can conclusively establish that the entire signal arises from non-circular beam effect. This is important since cosmic SI violation signals are expected to be subtle and dismissing a large SI violation signal as observational artefact based on simplistic plausibility arguments run the serious risk of “throwing the baby out with the bathwater”.
  • 关键词:cosmic background radiation;cosmology: observations;methods: data analysis
国家哲学社会科学文献中心版权所有