CCAPP Seminar: "Revisiting the dark photon explanation of the muon g-2 anomaly"

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March 26, 2019
11:30AM - 12:30PM
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PRB 4138

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Add to Calendar 2019-03-26 11:30:00 2019-03-26 12:30:00 CCAPP Seminar: "Revisiting the dark photon explanation of the muon g-2 anomaly" Gopolang Mohlabeng (Brookhaven) A massive U(1)′ gauge boson known as a “dark photon” or A′, has long been proposed as a potential explanation for the discrepancy observed between the experimental measurement and the- oretical determination of the anomalous magnetic moment of the muon (gμ − 2 anomaly). Recently, experimental results have excluded this possibility for a dark photon exhibiting exclusively visible or invisible decays. In this work, we revisit this idea and consider a model where A′ couples inelastically to dark matter and an excited dark sector state, leading to a more exotic decay topology we refer to as a semi-visible decay. We show that for large mass splittings between the dark sector states this decay mode is enhanced, weakening the previous invisibly decaying dark photon bounds. As a consequence, A′ resolves the gμ − 2 anomaly in a region of parameter space the thermal dark matter component of the Universe is readily explained. Interestingly, it is possible that the semi-visible events we discuss may have been vetoed by experiments searching for invisible dark photon decays. A re-analysis of the data and future searches may be crucial in uncovering this exotic decay mode or closing the window on the dark photon explanation of the gμ − 2 anomaly.  PRB 4138 Center for Cosmology and AstroParticle Physics (CCAPP) ccapp@osu.edu America/New_York public
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Gopolang Mohlabeng (Brookhaven)

A massive U(1)′ gauge boson known as a “dark photon” or A′, has long been proposed as a potential explanation for the discrepancy observed between the experimental measurement and the- oretical determination of the anomalous magnetic moment of the muon (gμ − 2 anomaly). Recently, experimental results have excluded this possibility for a dark photon exhibiting exclusively visible or invisible decays. In this work, we revisit this idea and consider a model where A′ couples inelastically to dark matter and an excited dark sector state, leading to a more exotic decay topology we refer to as a semi-visible decay. We show that for large mass splittings between the dark sector states this decay mode is enhanced, weakening the previous invisibly decaying dark photon bounds. As a consequence, A′ resolves the gμ − 2 anomaly in a region of parameter space the thermal dark matter component of the Universe is readily explained. Interestingly, it is possible that the semi-visible events we discuss may have been vetoed by experiments searching for invisible dark photon decays. A re-analysis of the data and future searches may be crucial in uncovering this exotic decay mode or closing the window on the dark photon explanation of the gμ − 2 anomaly. 

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