中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Probing the primordial Universe from the low-multipole CMB data

文献类型:期刊论文

作者Huang, QG
刊名PHYSICS LETTERS B
出版日期2014
卷号738期号:-页码:140-143
关键词MICROWAVE BACKGROUND ANISOTROPIES INFLATIONARY UNIVERSE GRAVITATIONAL-WAVES COSMOLOGICAL MODEL ANGULAR VARIATIONS PERTURBATIONS FLATNESS HORIZON
ISSN号0370-2693
通讯作者Huang, QG (reprint author), Chinese Acad Sci, Inst Theoret Phys, State Key Lab Theoret Phys, Beijing 100190, Peoples R China.
英文摘要Since the temperature fluctuations in the cosmic microwave background (CMB) on large-angular scales probe length scales that were super-horizon sized at photon decoupling and hence insensitive to microphysical processes, the low-multipole CMB data are supposed to be a good probe to the physics of the primordial Universe. In this letter we will constrain the cosmological parameters in the base Lambda CDM model with tensor perturbations by only using the low-multipole CMB data, including Background Imaging of Cosmic Extragalactic Polarization (B2), Planck data released in 2013 (P13) and Wilkinson Microwaves Anisotropy Probe 9-year data (W9). We find that either sign of the index of the tensor power spectrum is compatible with the data, but a blue-tilted power spectrum of scalar perturbations on large scales is preferred at around 2 sigma confidence level. (C) 2014 The Authors. Published by Elsevier B. V.
学科主题Physics
收录类别SCI
资助信息Chinese Academy of Science; NSFC [10821504, 11322545, 11335012]
原文出处http://dx.doi.org/10.1016/j.physletb.2014.09.036
语种英语
WOS记录号WOS:000344624900021
公开日期2015-06-03
源URL[http://ir.itp.ac.cn/handle/311006/15574]  
专题理论物理研究所_理论物理所1978-2010年知识产出
推荐引用方式
GB/T 7714
Huang, QG. Probing the primordial Universe from the low-multipole CMB data[J]. PHYSICS LETTERS B,2014,738(-):140-143.
APA Huang, QG.(2014).Probing the primordial Universe from the low-multipole CMB data.PHYSICS LETTERS B,738(-),140-143.
MLA Huang, QG."Probing the primordial Universe from the low-multipole CMB data".PHYSICS LETTERS B 738.-(2014):140-143.

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来源:理论物理研究所

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