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Volumn 71, Issue 3, 1993, Pages 324-327

Imprint of gravitational waves on the cosmic microwave background

Author keywords

[No Author keywords available]

Indexed keywords


EID: 12044251491     PISSN: 00319007     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevLett.71.324     Document Type: Article
Times cited : (180)

References (31)
  • 19
    • 84927469255 scopus 로고    scopus 로고
    • We find the polarization induced by the tensor mode is negligibly small ($ ll 1 whereas models with early reionization have significant polarization, an added discriminant that we will not explore here.
  • 20
    • 84927465816 scopus 로고    scopus 로고
    • H0=100 h ,km ,s-1 ,Mpc-1.
  • 24
    • 84927473671 scopus 로고    scopus 로고
    • A.C.S. Readhead et al. Astrophys. J. 346, 556 (1989).
  • 28
    • 84927481897 scopus 로고    scopus 로고
    • The Gaussian variance for the likelihood adds to the observational errors, Ref. 2, an all sky cosmic variance and a (small) signal noise interference variance computed assuming a uniform pixel noise which best fits the DMR error bars.
  • 30
    • 84927508967 scopus 로고    scopus 로고
    • E.g., P. Meinhold et al. (to be published); J. Gunderson et al. (to be published).


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.