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Volumn 69, Issue 6, 2004, Pages 11-

CMB polarization from secondary vector and tensor modes

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EID: 2342423052     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.69.063002     Document Type: Article
Times cited : (339)

References (56)
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    • S. Weinberg, Phys. Rev. D (to be published), astro-ph/0306304.
    • Weinberg, S.1
  • 52
    • 85039017350 scopus 로고    scopus 로고
    • http://universe.gsfc.nasa.gov
    • http://universe.gsfc.nasa.gov
  • 53
    • 85039000479 scopus 로고    scopus 로고
    • http://cosmology.berkeley.edu/group/swlh/bicep
    • http://cosmology.berkeley.edu/group/swlh/bicep
  • 54
    • 85038974126 scopus 로고    scopus 로고
    • Also, primordial gravitational waves give rise to second-order scalar and vector perturbations, but this effect is usually negligible 16
    • Also, primordial gravitational waves give rise to second-order scalar and vector perturbations, but this effect is usually negligible 16.
  • 55
    • 85039022245 scopus 로고    scopus 로고
    • Second-order Christoffel symbols can be found in Appendix A of Ref. 27 (see also 28
    • Second-order Christoffel symbols can be found in Appendix A of Ref. 27 (see also 28).
  • 56
    • 85038991101 scopus 로고    scopus 로고
    • The relation with the inflation parameters is (Formula presented) with (Formula presented)
    • The relation with the inflation parameters is (Formula presented) with (Formula presented)


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