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Volumn 57, Issue 10, 1998, Pages 6057-6064

Imprint of gravitational waves in models dominated by a dynamical cosmic scalar field

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EID: 0000725360     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.57.6057     Document Type: Article
Times cited : (67)

References (33)
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    • Michael S. Turner and Martin White, Phys. Rev. D 53, 6822 (1996).
    • (1996) Phys. Rev. D , vol.53 , pp. 6822
  • 24
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    • Detailed calculations of the CMB anisotropy spectrum for such scalar field cosmologies have been carried out by Kimberly Coble, Scott Dodelson, and Joshua A. Frieman, Phys. Rev. D 55, 1851 (1997);
    • (1997) Phys. Rev. D , vol.55 , pp. 1851
  • 25
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    • Pedro G. Ferreira and Michael Joyce, Phys. Rev. Lett. 79, 4740 (1997);
    • (1997) Phys. Rev. Lett. , vol.79 , pp. 4740
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    • Pedro G. FerreiraMichael Joyceastro-ph/9711102.
    • Pedro G. FerreiraMichael Joyceastro-ph/9711102.
  • 27
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    • I, and R. R. Caldwell, R. Dave, and P. J. Steinhardt (work in progress)
    • See paper I, and R. R. Caldwell, R. Dave, and P. J. Steinhardt (work in progress).
  • 28
    • 0000170621 scopus 로고    scopus 로고
    • The power spectrum (Formula presented) in Eq. (2.1) refers to the fluctuations in the radiation and matter
    • Similar conclusions were reached by P. T. P. Viana and A. R. Liddle, Phys. Rev. D 57, 674 (1998). The power spectrum (Formula presented) in Eq. (2.1) refers to the fluctuations in the radiation and matter.
    • (1998) Phys. Rev. D , vol.57 , pp. 674
    • Viana, P.T.P.1    Liddle, A.R.2
  • 29
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    • David N. Spergel and Ue-Li Pen, Astrophys. J. 491, L67 (1997).
    • (1997) Astrophys. J. , vol.491


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