English

A low-threshold ultrahigh-energy neutrino search with the Askaryan Radio Array

High Energy Astrophysical Phenomena 2022-07-13 v1 Instrumentation and Methods for Astrophysics

Abstract

In the pursuit of the measurement of the still-elusive ultrahigh-energy (UHE) neutrino flux at energies of order EeV, detectors using the in-ice Askaryan radio technique have increasingly targeted lower trigger thresholds. This has led to improved trigger-level sensitivity to UHE neutrinos. Working with data collected by the Askaryan Radio Array (ARA), we search for neutrino candidates at the lowest threshold achieved to date, leading to improved analysis-level sensitivities. A neutrino search on a data set with 208.7~days of livetime from the reduced-threshold fifth ARA station is performed, achieving a 68\% analysis efficiency over all energies on a simulated mixed-composition neutrino flux with an expected background of 0.100.04+0.060.10_{-0.04}^{+0.06} events passing the analysis. We observe one event passing our analysis and proceed to set a neutrino flux limit using a Feldman-Cousins construction. We show that the improved trigger-level sensitivity can be carried through an analysis, motivating the Phased Array triggering technique for use in future radio-detection experiments. We also include a projection using all available data from this detector. Finally, we find that future analyses will benefit from studies of events near the surface to fully understand the background expected for a large-scale detector.

Keywords

Cite

@article{arxiv.2202.07080,
  title  = {A low-threshold ultrahigh-energy neutrino search with the Askaryan Radio Array},
  author = {P. Allison and S. Archambault and J. J. Beatty and D. Z. Besson and A. Bishop and C. C. Chen and C. H. Chen and P. Chen and Y. C. Chen and B. A. Clark and W. Clay and A. Connolly and L. Cremonesi and P. Dasgupta and J. Davies and S. de Kockere and K. D. de Vries and C. Deaconu and M. A. DuVernois and J. Flaherty and E. Friedman and R. Gaior and J. Hanson and N. Harty and B. Hendricks and K. D. Hoffman and E. Hong and S. Y. Hsu and L. Hu and J. J. Huang and M. -H. Huang and K. Hughes and A. Ishihara and A. Karle and J. L. Kelley and K. -C. Kim and M. -C. Kim and I. Kravchenko and R. Krebs and Y. Ku and C. Y. Kuo and K. Kurusu and H. Landsman and U. A. Latif and C. -J. Li and T. -C. Liu and M. -Y. Lu and B. Madison and K. Madison and K. Mase and T. Meures and J. Nam and R. J. Nichol and G. Nir and A. Novikov and A. Nozdrina and E. Oberla and J. Osborn and Y. Pan and C. Pfendner and N. Punsuebsay and J. Roth and D. Seckel and M. F. H. Seikh and Y. -S. Shiao and A. Shultz and D. Smith and S. Toscano and J. Torres and J. Touart and N. van Eijndhoven and G. S. Varner and A. Vieregg and M. -Z. Wang and S. -H. Wang and Y. H. Wang and S. A. Wissel and C. Xie and S. Yoshida and R. Young},
  journal= {arXiv preprint arXiv:2202.07080},
  year   = {2022}
}

Comments

15 pages, 8 figures