EUSO-SPB2
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A primary goal of the particle physics program is to discover the
connection between dark matter and the Standard Model.
EUSO-SPB2 will be sensitive to hypothetical dark-quark nuggets
that may strike the Earth's atmosphere. Elastic scattering allows
dark-quark nuggets and baryons to exchange momentum. If a dark-quark
nugget were to traverse the Earth's atmosphere its energy deposition
would excite the nitrogen molecules of air producing observables
signals at fluorescence detectors. The internal energy density of
standard nuggets of strange quark matter is fixed by QCD dynamics, but the internal energy density of dark-quark nuggets may span
several orders of magnitude depending on the confinement scale and
the magnitude of the dark baryon asymmetry [arXiv:1810.04360]. This opens up the
quark nuggets phase space into the EUSO-SPB2 sensitivity reach.
Listen to Tom Paul describing
the ins and outs of the footprints dark-quark nuggets could leave in
the Earth's atmosphere. For further details, see
arXiv:2104.05131.
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