In cosmological inflation, within the slow-roll paradigm, the Lyth argument places a theoretical upper bound on the amount of gravitational waves produced during inflation, given the amount of departure from the homogeneity of the cosmic microwave background (CMB). Spletpastor, Memphis 935 views, 16 likes, 6 loves, 13 comments, 6 shares, Facebook Watch Videos from New Salem Missionary Baptist Church: Mid Week Bible...
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SpletGiven the Planck constraints on ns, the Lyth bound is strengthened by two orders of magnitude: whereas the original bound gives a sub-Planckian field range for r less than or similar to 2 x 10(-3), we find that n(s) = 0.96 brings this down to … Splet13. maj 2005 · We investigate the Lyth bound relating the tensor–scalar ratio, r, to the variation of the inflaton field, Δϕ, over the course of inflation.For inflationary models that … bd-re フォーマットできない
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Spletthe Lyth bound and our general plan for avoiding it: In slow-roll inflation the tensor-to-scalar ratio (i.e. the ratio of the gravitational-wave power spectrum ∆2 T ∼ H 2 and the scalar … SpletWe provide strong evidence for universality of the inflationary field range: given an accurate measurement of $(n_s,r)$, one can infer $\\Delta \\phi$ in a... SpletFigure 2. The absolute value of ∆φ over the last 55 e-folds of inflation plotted against the tensor-scalar ratio, r. Figure 2a shows all models colour coded so that hybrid-type models are shown in red and the rest are shown in blue. Figure 2b shows the subset of models that satisfy the observational constraints on ns and dns/dlnk discussed in the text. The colour … 印刷 見開き ワード