English  |  正體中文  |  简体中文  |  Items with full text/Total items : 52047/87178 (60%)
Visitors : 8708642      Online Users : 375
RC Version 7.0 © Powered By DSPACE, MIT. Enhanced by NTU Library & TKU Library IR team.
Scope Tips:
  • please add "double quotation mark" for query phrases to get precise results
  • please goto advance search for comprehansive author search
  • Adv. Search
    HomeLoginUploadHelpAboutAdminister Goto mobile version
    Please use this identifier to cite or link to this item: http://tkuir.lib.tku.edu.tw:8080/dspace/handle/987654321/104575

    Title: Cosmic birefringence fluctuations and cosmic microwave background B-mode polarization
    Authors: Lee, Seokcheon;Liu, Guo-Chin;Ng, Kin-Wang
    Date: 2015-06-30
    Issue Date: 2016-01-06 11:03:45 (UTC+8)
    Publisher: Elsevier BV * North-Holland
    Abstract: Recently, BICEP2 measurements of the cosmic microwave background (CMB) B-mode polarization has indicated the presence of primordial gravitational waves at degree angular scales, inferring the tensor-to-scalar ratio of r=0.2 and a running scalar spectral index. In this {\em Letter}, we show that the existence of the fluctuations of cosmological birefringence can give rise to CMB B-mode polarization that fits BICEP2 data with r<0.11 and no running of the scalar spectral index. Thus, it might be too hasty to conclude that many inflation models with small r are ruled out based on BICEP2 result.
    Relation: Physics Letters B 746, p.406-409
    DOI: 10.1016/j.physletb.2015.05.038
    Appears in Collections:[物理學系暨研究所] 期刊論文

    Files in This Item:

    File Description SizeFormat
    Cosmic birefringence fluctuations and cosmic microwave background B-mode polarization.pdf322KbAdobe PDF0View/Open

    All items in 機構典藏 are protected by copyright, with all rights reserved.

    DSpace Software Copyright © 2002-2004  MIT &  Hewlett-Packard  /   Enhanced by   NTU Library & TKU Library IR teams. Copyright ©   - Feedback