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Establishing a theory of inflationary cosmology

Bibliographic Data

ID8399707
AuthorsAdam Koberinski (0000-0001-7605-4214, corresponding author), Chris Smeenk (0000-0002-6101-0048)
Year2024
Publication date2024-11-08
Peer ReviewedYes
Open AccessNo
TypeARTICLE
VenueThe British Journal for the Philosophy of Science (JOURNAL)
Journal identifiersISSN: 0007-0882 • E-ISSN: 1464-3537
PublisherUniversity of Chicago Press (PUBLISHER • US)
DOI10.1086/733886
OpenAlexW4404174561
LanguageEN
Citations received2
References cited42

Inflation remains a promising, yet speculative, account of structure formation in the early universe. In this paper, we provide a general account of what is needed to establish a speculative theory, and apply the account to inflation. Particular challenges for inflation are its flexibility as a phenomenological framework, and the lack of empirical access to test seemingly independent features of specific realizations of inflation. This makes it difficult to leverage initial empirical successes to learn further physical details about the inflationary epoch. One prima facie appealing response is to treat phenomenological accounts of inflation as effective field theories (EFTs), screening off details of higher-energy physics. We argue that inflation is a poor fit into the EFT framework due to its sensitivity to high-energy physics. We close by stating specific recommendations to take steps towards establishing inflation as part of a theory of the early universe that follow from our approach

Astronomy · Cosmology · Epistemology · Physics · Theoretical physics · Cosmology and Gravitation Theories · Philosophy · Relativity and Gravitational Theory · Solar and Space Plasma Dynamics

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Unique citing works2
Citations per year1
Citation span2024 - 2025 (2)
Citation velocityrecent
Highly citedNo
Citation typesNeutral: 2

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