Holographic (eternal) inflation
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Abstract
We identify a minisuperspace of complex deformations of ABJM theory for which the partition function specifies the amplitude of an eternally inflating universe. The boundary theory predicts that the bosonic bulk is effectively in the Hartle-Hawking no-boundary state, with a subleading ‘tunneling’ contribution. This holographic model of inflation also reveals a close connection between the swampland distance and cobordism conjectures, and the condition for the asymptotic wave function to predict classical behavior in geometry and fields.
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Acknowledgements: We thank Oliver Janssen for early collaboration and discussions, and Nikolay Bobev, Joel Karlsson, Klaas Parmentier, and Thomas Van Riet for valuable discussions. TH acknowledges support from the Flemish inter-university project IBOF/21/084 and the PRODEX grant LISA — BEL (PEA 4000131558). JP acknowledges support from NCCR-SwissMAP. VV is supported by funding from an STFC consolidated grant, grant reference ST/X000761/1.

