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Allison, P. ; Archambault, S. ; Beatty, J. J. ; Besson, D. Z. ; Bishop, A. ; Chen, C. C. ; Chen, C. H. ; Chen, P. ; Chen, Y. C. ; Clark, B. A. ; et al ( , Physical Review D)
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Allison, P. ; Archambault, S. ; Beatty, J. J. ; Chen, C. C. ; Chen, C. H. ; Chen, P. ; Clark, B. A. ; Connolly, A. ; Cremonesi, L. ; Davies, J. ; et al ( , Physical review)The Askaryan Radio Array (ARA) is an ultrahigh energy (UHE, >10^17 eV) neutrino detector designed to observe neutrinos by searching for the radio waves emitted by the relativistic products of neutrino-nucleon interactions in Antarctic ice. In this paper, we present constraints on the diffuse flux of ultrahigh energy neutrinos between 1016 and 1021 eV resulting from a search for neutrinos in two complementary analyses, both analyzing four years of data (2013–2016) from the two deep stations (A2, A3) operating at that time. We place a 90% CL upper limit on the diffuse all flavor neutrino flux at 1018 eV of EF(E)=5.6×10^−16 cm^−2 s^−1 sr^−1. This analysis includes four times the exposure of the previous ARA result and represents approximately 1/5^th the exposure expected from operating ARA until the end of 2022.more » « less