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Fundamental Physics, the Swampland of Effective Field Theory and Early Universe Cosmology

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arxiv 1911.06058 v1 pith:ANC37LCL submitted 2019-11-14 hep-th astro-ph.COgr-qchep-ph

classification hep-thastro-ph.COgr-qchep-ph
keywords earlyuniversewillcosmologytheorydataeffectivefield
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Cosmological inflation is not the only early universe scenario consistent with current observational data. I will discuss the criteria for a successful early universe cosmology, compare a couple of the proposed scenarios (inflation, bouncing cosmologies, and the {\it emergent} scenario), focusing on how future observational data will be able to distinguish between them. I will argue that we need to go beyond effective field theory in order to understand the early universe, and that principles of superstring theory will yield a nonsingular cosmology.

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  1. A Non-Inflationary Axion and ALP Misalignment Mechanism

    hep-ph 2025-07 conditional novelty 5.0 of 10

    A thermally mediated, Planck-suppressed symmetry breaking potential can supply the initial axion misalignment that inflationary cosmology normally provides, allowing late-time coherent oscillations without inflation.

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