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84927719019
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note
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The relation with the inflation parameters is ΔR 2 = H2/(πεm2P), with m P = G-1/2.
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24
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84927719018
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84927719017
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note
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Here ημνρσ is the totally antisymmetric Levi-Cività tensor, with η1234 = (-g)-1/2.
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27
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0004124254
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(John Wiley & Sons, Chichester, UK), 2nd ed.
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P. Coles and F. Lucchin, Cosmology: The Origin and Evolution of Cosmic Structure (John Wiley & Sons, Chichester, UK, 2002), 2nd ed.
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84927719016
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note
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Note however that for a pressureless self-gravitating fluid these extra terms vanish.
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