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edited by L. Fang and A. Zee (Gordon and Breach, London
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Cosmology and Particle Physics
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Bardeen, J.M.1
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0346670958
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Proceedings of the Second Alexander Friedmann International Seminar on Gravitation and Cosmology, edited by Yu. N. Gnedin, A. A. Grib, and V. M. Mostepanenko (Friedmann Laboratory, St. Petersburg, Sec. 6
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J. Hwang and H. Minn, in Proceedings of the Second Alexander Friedmann International Seminar on Gravitation and Cosmology, edited by Yu. N. Gnedin, A. A. Grib, and V. M. Mostepanenko (Friedmann Laboratory, St. Petersburg, 1994), Sec. 6, p. 265.
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(1994)
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Hwang, J.1
Minn, H.2
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85035192026
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the large scale limit ((formula presented) /z gg (formula presented)) we have citeRussian, GGT2, Mukhanov etal v (x, η) = (formula presented) (x) z + (formula presented) (x) z (formula presented) sub 0 d η / (formula presented). By matching (formula presented) = - C and (formula presented) = D, it is equivalent to (refUCG delta phi LS sol
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In the large scale limit ((formula presented) /z gg (formula presented)) we have citeRussian, GGT2, Mukhanov etal v (x, η) = (formula presented) (x) z + (formula presented) (x) z (formula presented) sub 0 d η / (formula presented). By matching (formula presented) = - C and (formula presented) = D, it is equivalent to (refUCG delta phi LS sol).
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23
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85035243789
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the zero shear gauge we let chi equiv 0; δ φsub chi equiv δ φ - dot φ chi is a gauge invariant combination which becomes δ φ in the zero shear gauge. The equation and asymptotic solutions were derived in citeGGT2 and Sec. 4.3.2 of citePRW (see also citeH GGT, Russian, Mukhanov etal); these can also be presented in unified forms citeHwang Noh
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In the zero shear gauge we let chi equiv 0; δ φsub chi equiv δ φ - dot φ chi is a gauge invariant combination which becomes δ φ in the zero shear gauge. The equation and asymptotic solutions were derived in citeGGT2 and Sec. 4.3.2 of citePRW (see also citeH GGT, Russian, Mukhanov etal); these can also be presented in unified forms citeHwang Noh.
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28
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85035244928
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these cases (refMSF eq) becomes an equation which appears often in the context of quantum field in curved spacetime citeQFCS. Analyses were made in the cases of power law citePOW and exponential expansion citeEXP. Parallel analyses in the context of our perturbative approach were made in citeH QFT, MSF UCG
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In these cases (refMSF eq) becomes an equation which appears often in the context of quantum field in curved spacetime citeQFCS. Analyses were made in the cases of power law citePOW and exponential expansion citeEXP. Parallel analyses in the context of our perturbative approach were made in citeH QFT, MSF UCG.
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35
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85035222585
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δ (formula presented) equiv δ µ - (a/k) dot µ v and δ (formula presented) equiv δ T - (a/k) dot T v are gauge invariant combinations. The comoving gauge takes v equiv 0 where v equiv -(k/a) ψ/(µ + p); for ψ see Sec. 2.1.2 of citePRW
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δ (formula presented) equiv δ µ - (a/k) dot µ v and δ (formula presented) equiv δ T - (a/k) dot T v are gauge invariant combinations. The comoving gauge takes v equiv 0 where v equiv -(k/a) ψ/(µ + p); for ψ see Sec. 2.1.2 of citePRW.
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38
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85035208846
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For analytic derivations of perturbation spectrums generated from quantum fluctuations in the minimally coupled scalar field case, see citeH QFT, Stewart Lyth. Previous attempts in some generalized gravity case can be found in citeRussian, Mukhanov etal, pert GGT infl. We have not used the conformal transformation in this paper
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For analytic derivations of perturbation spectrums generated from quantum fluctuations in the minimally coupled scalar field case, see citeH QFT, Stewart Lyth. Previous attempts in some generalized gravity case can be found in citeRussian, Mukhanov etal, pert GGT infl. We have not used the conformal transformation in this paper.
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