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DTSTART;TZID=America/New_York:20220525T103000
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DTSTAMP:20260620T220159
CREATED:20240215T101805Z
LAST-MODIFIED:20240215T102153Z
UID:10002740-1653474600-1653480000@cmsa.fas.harvard.edu
SUMMARY:Oblique Lessons from the W Mass Measurement at CDF II
DESCRIPTION:Speaker: Seth Koren (University of Chicago) \nTitle: Baryon Minus Lepton Number BF Theory for the Cosmological Lithium Problem \nAbstract: The cosmological lithium problem—that the observed primordial abundance is lower than theoretical expectations by order one—is perhaps the most statistically significant anomaly of SM+ ΛCDM\, and has resisted decades of attempts by cosmologists\, nuclear physicists\, and astronomers alike to root out systematics. We upgrade a discrete subgroup of the anomaly-free global symmetry of the SM to an infrared gauge symmetry\, and UV complete this at a scale Λ as the familiar U(1)_{B-N_cL} Abelian Higgs theory. The early universe phase transition forms cosmic strings which are charged under the emergent higher-form symmetry of the baryon minus lepton BF theory. These topological defects catalyze interactions which turn N_g baryons into N_g leptons at strong scale rates in an analogue of the Callan-Rubakov effect\, where N_g=3 is the number of SM generations. We write down a model in which baryon minus lepton strings superconduct bosonic global baryon plus lepton number currents and catalyze solely 3p^+ → 3e^+. We suggest that such cosmic strings have disintegrated O(1) of the lithium nuclei formed during Big Bang Nucleosynthesis and estimate the rate\, with our benchmark model finding Λ ~ 10^8 GeV gives the right number density of strings.
URL:https://cmsa.fas.harvard.edu/event/qm_51222/
LOCATION:Hybrid
CATEGORIES:Quantum Matter
ATTACH;FMTTYPE=image/png:https://cmsa.fas.harvard.edu/media/CMSA-QMMP-Seminar-05.25.22.png
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