Abstract:GRAND will be a distributed set of about 20 arrays of radio antennas,
totalling 200,000 km^22.
We aim to study the ultra high energy universe through the detection of
neutrinos, photons and cosmic rays at energies at the EeV scale. In
addition GRAND will be used to study astronomical objects like FRBs and
GRBs. We will describe the physics motivation, the detection strategy,
the first stages of GRAND and the path to creating the complete
setup.
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