Inflation vs Bounce: red or blue, and how much blue?

11 Apr 2026, 15:30
30m

Speaker

Prof. Alexey Koshelev (ShanghaiTech)

Description

In my talk I will focus on renormalizable and ghost-free quantum gravity proposals. An important feature of these models is the presence of infinite derivative operators. Such models on contrary to local gravity modifications can give a blue tilted spectrum of primordial GWs while local models uniquely predict a red tilted primordial GWs spectrum. This is an essential possible observational signature of non-local gravity models. On top of this non-local gravity models can realize stable non-singular cosmological bounce which with necessity results in a blue tilted GW spectrum. Implications for observations and ways to distinguish bounce and inflation will be discussed.

Primary author

Prof. Alexey Koshelev (ShanghaiTech)

Presentation materials

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