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Volumn 52, Issue 6, 1995, Pages 3276-3287

Analytic approach to the polarization of the cosmic microwave background in flat and open universes

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Indexed keywords


EID: 0001236362     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.52.3276     Document Type: Article
Times cited : (175)

References (42)
  • 18
    • 84927841523 scopus 로고    scopus 로고
    • Ka Lok Ng and Kin Wang Ng, Astrophys. J. (to be published).
  • 32
    • 84927841522 scopus 로고    scopus 로고
    • Notice that our definition of Δ T and Δ P differs by a factor 4 from that of Ref. cite Bond87, while our definition for the polarization correlation function CP turns out to be identical.
  • 33
    • 84927841521 scopus 로고    scopus 로고
    • Notice that our multipole expansion differs from that in Ref. cite Hu94 by a factor (-i)l/(2l+1).
  • 41
    • 84927841520 scopus 로고    scopus 로고
    • Notice that in order to compare our Figs. 1 and 2 with Figs. (4b) and (7a) of Ref. citeBond87 some adjustments are needed to account for different conventions and normalizations. Our W(k) corresponds to twice what is plotted in (4b). Our definition of the quadrupole anisotropy aT2 is 4 times that used in citeBond87. And finally the value of aT2 used is different.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.