Constraints on the ultrahigh-energy cosmic neutrino flux from the fourth flight of ANITA

Gorham, P. W.; Allison, P.; Banerjee, O.; Batten, L.; Beatty, J. J.; Belov, K.; Besson, D. Z.; Binns, W. R.; Bugaev, V.; Cao, P.; Chen, C. H.; Chen, P.; Chen, Y.; Clem, J. M.; Connolly, A.; Cremonesi, L.; Dailey, B.; Deaconu, C.; Dowkontt, P. F.; Fox, B. D.; Gordon, J. W.  H.; Hast, C.; Hill, B.; Hsu, S. Y.; Huang, J. J.; Hughes, K.; Hupe, R.; Israel, M. H.; Liewer, K. M.; Liu, T. C.; Ludwig, A. B.; Macchiarulo, L.; Matsuno, S.; McBride, K.; Miki, C.; Mulrey, K.; Nam, J.; Naudet, C.; Nichol, R. J.; Novikov, A.; Oberla, E.; Prohira, S.; Rauch, B. F.; Ripa, J.; Roberts, J. M.; Romero-Wolf, A.; Rotter, B.; Russell, J. W.; Saltzberg, D.; Seckel, D.; Schoorlemmer, H.; Shiao, J.; Stafford, S.; Stockham, J.; Stockham, M.; Strutt, B.; Sutherland, M. S.; Varner, G. S.; Vieregg, A. G.; Wang, N.; Wang, S. H.; Wissel, S. A.

doi:10.1103/physrevd.99.122001

Title: Constraints on the ultrahigh-energy cosmic neutrino flux from the fourth flight of ANITA

Journal Article · Tue Jun 11 00:00:00 EDT 2019 · Physical Review. D.

DOI:https://doi.org/10.1103/physrevd.99.122001· OSTI ID:1546753

Gorham, P. W.; Allison, P.; Banerjee, O.; Batten, L.; Beatty, J. J.; Belov, K.; Besson, D. Z.; Binns, W. R.; Bugaev, V.; Cao, P.; Chen, C. H.; Chen, P.; Chen, Y.; Clem, J. M.; Connolly, A.; Cremonesi, L.; Dailey, B.; Deaconu, C.; Dowkontt, P. F.; Fox, B. D. more »

The ANtarctic Impulsive Transient Antenna (ANITA) NASA long-duration balloon payload completed its fourth flight in December 2016, after 28 days of flight time. ANITA is sensitive to impulsive broadband radio emission from interactions of ultrahigh-energy neutrinos in polar ice (Askaryan emission). We present the results of two separate blind analyses searching for signals from Askaryan emission in the data from the fourth flight of ANITA. The more sensitive analysis, with a better expected limit, has a background estimate of $${0.64}_{-0.45}^{+0.69}$$ and an analysis efficiency of 82 ± 2 % . The second analysis has a background estimate of 0.34 $$^{+0.66}_{-0.16}$$ and an analysis efficiency of 71 ± 6 % . Each analysis found one event in the signal region, consistent with the background estimate for each analysis. The resulting limit further tightens the constraints on the diffuse flux of ultrahigh-energy neutrinos at energies above 10^19.5 eV .

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Research Organization:: SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)

Sponsoring Organization:: USDOE; National Aeronautics and Space Administration (NASA); National Science Foundation (NSF)

Contributing Organization:: ANITA Collaboration

Grant/Contract Number:: AC02-76SF00515; NNX15AC24G; 1255557

OSTI ID:: 1546753

Journal Information:: Physical Review. D., Vol. 99, Issue 12; ISSN 2470-0010

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 48 works

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Limits on point-like sources of ultra-high-energy neutrinos with the Pierre Auger Observatory Aab, A.; Abreu, P.; Aglietta, M. Journal of Cosmology and Astroparticle Physics, Vol. 2019, Issue 11 https://doi.org/10.1088/1475-7516/2019/11/004	journal	November 2019
Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory Aab, Alexander; Abreu, Pedro; Aglietta, Marco RWTH Aachen University https://doi.org/10.18154/rwth-2020-02509	text	January 2019
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