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Volumn 89, Issue 1, 2002, Pages

Limit on the Detectability of the Energy Scale of Inflation

Author keywords

[No Author keywords available]

Indexed keywords

ANISOTROPY; APPROXIMATION THEORY; ELECTROMAGNETIC WAVE POLARIZATION; GALAXIES; GRAVITY WAVES; MATHEMATICAL MODELS; MATHEMATICAL TRANSFORMATIONS; MICROWAVES; PERTURBATION TECHNIQUES; RADIATION DETECTORS; SPECTRUM ANALYSIS; TENSORS;

EID: 0036642088     PISSN: 00319007     EISSN: 10797114     Source Type: Journal    
DOI: 10.1103/PhysRevLett.89.011303     Document Type: Article
Times cited : (341)

References (30)
  • 6
  • 10
    • 85038347327 scopus 로고    scopus 로고
    • For example, a much more impressive success would be the prediction of features in the power spectrum followed by their detection
    • For example, a much more impressive success would be the prediction of features in the power spectrum followed by their detection.
  • 14
    • 85038338322 scopus 로고    scopus 로고
    • The * subscript on (Formula presented) means that it is evaluated when the scale factor is about (Formula presented) times smaller than it is at the end of inflation, when the relevant perturbations for large-scale CMB fluctuations are exiting the horizon. There is a slight dependence on (Formula presented)
    • The * subscript on (Formula presented) means that it is evaluated when the scale factor is about (Formula presented) times smaller than it is at the end of inflation, when the relevant perturbations for large-scale CMB fluctuations are exiting the horizon. There is a slight dependence on (Formula presented)
  • 16
    • 85038276463 scopus 로고    scopus 로고
    • Here and throughout, the detection limit is set at 3.3 times the standard deviation. For a normal distribution this means that one can make a detection at a (Formula presented) confidence level for (Formula presented) of possible realizations
    • Here and throughout, the detection limit is set at 3.3 times the standard deviation. For a normal distribution this means that one can make a detection at a (Formula presented) confidence level for (Formula presented) of possible realizations.
  • 22
    • 0037080630 scopus 로고    scopus 로고
    • W. Hu, Phys. Rev. D 65, 023003 (2002).
    • (2002) Phys. Rev. D , vol.65 , pp. 23003
    • Hu, W.1
  • 23
  • 25
    • 17044438084 scopus 로고    scopus 로고
    • W. Hu, Phys. Rev. D 62, 043007 (2000).
    • (2000) Phys. Rev. D , vol.62 , pp. 43007
    • Hu, W.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.