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Slow-roll parameters in braneworld cosmologies

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arxiv hep-ph/0402126 v2 pith:TQA6OXMK submitted 2004-02-11 hep-ph astro-phhep-th

classification hep-phastro-phhep-th
keywords slow-rollcosmologiesparametersacceleratingattractorbraneworldbraneworld-motivatedcompare
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We present a general slow-roll formalism within braneworld-motivated cosmologies with non-standard effective Friedmann equations. Full towers of parameters involving either the inflaton potential or the Hubble parameter are constructed and the dynamics of non-tachyonic and tachyonic fields are considered in detail; exact cosmological solutions and the inflationary attractor condition are provided. We compare scalar-driven and tachyon-driven accelerating eras through slow-roll correspondence and the observational imprint on early-universe structures.

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Cited by 1 Pith paper

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    In 5D f(T, T_G) gravity, thick branes develop splitting and internal structure controlled by the coupling, while supporting a normalizable chiral fermion zero mode and modified resonant Kaluza-Klein states due to the ...

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