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Volumn 64, Issue 2, 2001, Pages

Kinematic constraints to the key inflationary observables

Author keywords

[No Author keywords available]

Indexed keywords

ANISOTROPY; ARTICLE; COSMOS; FLOW MEASUREMENT; GRAVITY; MICROWAVE RADIATION; QUANTUM THEORY;

EID: 0034882983     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.64.023506     Document Type: Article
Times cited : (139)

References (39)
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    • http://map.gsfc.nasa.gov
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    • http://astro.estec.esa.nl/SA-general/Projects/Planck
  • 3
    • 33750677502 scopus 로고    scopus 로고
    • http://background.uchicago.edu/- wh
  • 5
  • 16
  • 25
    • 0000502742 scopus 로고    scopus 로고
    • The precise relationship between S and T and the inflaton potential depends upon the background cosmological model; see M.S. Turner and M. White, Phys. Rev. D 53, 6822 (1996).
    • (1996) Phys. Rev. D , vol.53 , pp. 6822
    • Turner, M.S.1    White, M.2
  • 26
    • 0000451248 scopus 로고
    • The values used in this paper are for flw=0.35 and 0-4 = 0.65. For flji/=l, the relation is the more familiar TIS=-lnT. The relationship between n, nT and T/S and the actual quantities observed in CMB measurements is discussed in more detail in A. Kosowsky and M.S. Turner, ibid. 52, 1739 (1995).
    • (1995) Phys. Rev. D , vol.52 , pp. 1739
    • Kosowsky, A.1    Turner, M.S.2
  • 27
    • 33750680830 scopus 로고    scopus 로고
    • In models where there is more than one active field during inflation or inflation is driven by non-standard kinetic terms, the relation is also modified; see E.D. Stewart and J.D. Cohn, ibid. 63, 083519 (2001) and C. Armendariz-Picon, T. Damour, and V. Mukhanov, Phys. Lett. B 458, 209 (1999)
    • In models where there is more than one active field during inflation or inflation is driven by non-standard kinetic terms, the relation is also modified; see E.D. Stewart and J.D. Cohn, ibid. 63, 083519 (2001) and C. Armendariz-Picon, T. Damour, and V. Mukhanov, Phys. Lett. B 458, 209 (1999)
  • 28
    • 0000744821 scopus 로고
    • It had been conjectured that for many models T/S-4 -5(n - 1). There are, however, many exceptions to this; see R. Davis etal., Phys. Rev. Lett. 69, 1856 (1992);
    • (1992) Phys. Rev. Lett. , vol.69 , pp. 1856
    • Davis, R.1
  • 33
    • 33750645238 scopus 로고    scopus 로고
    • These equations apply to models where one field with a standard kinetic term (or one that can be put in canonical form) is dynamical during inflation, which includes the vast majority of the models discussed in the literature
    • These equations apply to models where one field with a standard kinetic term (or one that can be put in canonical form) is dynamical during inflation, which includes the vast majority of the models discussed in the literature


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