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• W3100652994 abstract "In this paper, inspired by the investigations on the theory of cosmological perturbations in Hořava–Lifshitz cosmology, we calculate the spectrum of primordial perturbation lead by a modified dispersion relation in proper time ω pro ~ k z /a p in power-law expansion/contraction background a ~ t n · z is the critical exponent and p is not necessarily equal to z · p = z is well-motivated by Hořava–Lifshitz gravity, and the cases with p ≠ z are generalizations beyond the scope. We discuss that for fixed z, if the spectrum is required to be scale-invariant, how should p depend on n. We conclude that there is always room for parameters for the generation of scale-invariant spectrum." @default.
• W3100652994 created "2020-11-23" @default.
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• W3100652994 date "2010-10-01" @default.
• W3100652994 modified "2023-10-06" @default.
• W3100652994 title "SCALE INVARIANCE FROM MODIFIED DISPERSION RELATIONS" @default.
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• W3100652994 doi "https://doi.org/10.1142/s0218271810018074" @default.
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