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http://background.uchicago.edu/- wh
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A Lange et al., Phys. Rev. D 63, 042001 (2001).
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[Sov. Astron. Lett. 9, 302 (1983)];
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25
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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).
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Turner, M.S.1
White, M.2
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26
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0000451248
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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).
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Kosowsky, A.1
Turner, M.S.2
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27
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33750680830
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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)
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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)
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28
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0000744821
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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);
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0347873705
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and P.J. Steinhardt, astro-ph/9502024
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V.F. Mukhanov, L. Wang, and P.J. Steinhardt, Phys. Lett. B 414, 18 (1997); and P.J. Steinhardt, astro-ph/9502024
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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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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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