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Holographic (eternal) inflation

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.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1007/jhep07(2025)061

Authors

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Role:
Author
ORCID:
0000-0002-9021-5966
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Role:
Author
ORCID:
0000-0003-4440-7411
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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Theoretical Physics
Role:
Author
ORCID:
0000-0001-5643-691X


Publisher:
Springer
Journal:
Journal of High Energy Physics More from this journal
Volume:
2025
Issue:
7
Article number:
61
Publication date:
2025-07-03
Acceptance date:
2025-05-25
DOI:
EISSN:
1029-8479
ISSN:
1126-6708


Language:
English
Keywords:
Pubs id:
2268794
Local pid:
pubs:2268794
Source identifiers:
3085943
Deposit date:
2025-07-04
ARK identifier:
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