4.6 Article

Identifying universality in warm inflation

Journal

Publisher

IOP Publishing Ltd
DOI: 10.1088/1475-7516/2018/07/021

Keywords

inflation; physics of the early universe; particle physics - cosmology connection

Funding

  1. STFC
  2. Principals Career Development Scholarship
  3. Edinburgh Global Research Scholarship
  4. Spanish MINECOs Centro de Excelencia Severo Ocho Programme [SEV-2012-0249]
  5. European Unions Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie [713366]
  6. Conselho Nacional de Desenvolvimento Cientfico e Tecnologico - CNPq [302545/2017-4]
  7. Fundacao Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro - FAPERJ [E-26/201.424/2014]
  8. Higgs Centre for Theoretical Physics at the University of Edinburgh
  9. STFC [ST/P000630/1] Funding Source: UKRI

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Ideas borrowed from renormalization group are applied to warm inflation to characterize the inflationary epoch in terms of flows away from the de Sitter regime. In this framework different models of inflation fall into universality classes. Furthermore, for warm inflation this approach also helps to characterise when inflation can smoothly end into the radiation dominated regime. Warm inflation has a second functional dependence compared to cold inflation due to dissipation, yet despite this feature, it is shown that the universality classes de fined for cold inflation can be consistently extended to warm inflation.

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