2–5 Aug 2022
Center of Mathematical Sciences and Applications (CMSA), Harvard University
America/New_York timezone

A Cosmological Lithium Solution from Discrete Gauged Baryon Minus Lepton Number

Not scheduled
20m
Center of Mathematical Sciences and Applications (CMSA), Harvard University

Center of Mathematical Sciences and Applications (CMSA), Harvard University

20 Garden Street Cambridge, MA 02138

Speaker

Seth Koren (EFI, UChicago)

Description

We propose the infrared gauge symmetry of our sector includes an unbroken discrete gauged subgroup of baryon minus lepton number of order $2 \times 3 \text{ colors} \times 3 \text{ generations}$. We UV complete this at a scale $\Lambda$ as the familiar $U(1)_{B-N_cL}$ Abelian Higgs theory, and the early universe phase transition forms cosmic strings which are charged under an emergent higher-form generalized symmetry. These topological defects catalyze interactions which turn $3$ baryons into $3$ leptons at strong scale rates in an analogue of the Callan-Rubakov effect.

The cosmological lithium problem---that the observed primordial abundance is lower than theoretical expectations by a factor of a few---is perhaps the most statistically significant anomaly of $\text{SM}+\Lambda\text{CDM}$, and has resisted decades of attempts by cosmologists, nuclear physicists, and astronomers alike to root out systematics. We write down a model in which $B-N_cL$ strings superconduct bosonic global baryon plus lepton number currents and catalyze solely $3p^+ \rightarrow 3e^+$. We suggest that such cosmic strings have disintegrated $\mathcal{O}(1)$ of the lithium nuclei formed during Big Bang Nucleosynthesis and estimate the rate, with our benchmark model finding $\Lambda \sim 10^8 \text{ GeV}$ gives the right number density of strings.

Primary author

Seth Koren (EFI, UChicago)

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