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From Swampland to Phenomenology and Back

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arxiv 1904.05357 v2 pith:JI6H522S submitted 2019-04-10 hep-ph hep-th

Masahito Yamazaki This is my paper · ORCID
classification hep-phhep-th
keywords swamplandconjecturesgravityphenomenologicalquantumtheorybackcompletion
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Swampland conjectures are a set of proposed necessary conditions for a low-energy effective field theory to have a UV completion inside a theory of quantum gravity. Swampland conjectures have interesting phenomenological consequences, and conversely phenomenological considerations are useful guidelines in sharping our understanding of quantum gravity.

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Cited by 1 Pith paper

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  1. Fundamental Forces and Scalar Field Dynamics in the Early Universe

    hep-th 2019-08 conditional novelty 7.0 of 10

    The paper shows that generalized scalar weak gravity conjectures imply the parameter conditions for early-universe scalar condensates to fragment into solitonic lumps, which could form dark matter or primordial black holes.

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