arXiv Analytics

Sign in

arXiv:1908.00923 [astro-ph.HE]AbstractReferencesReviewsResources

Searches for Ultra-High Energy Neutrinos with ANITA

Cosmin Deaconu

Published 2019-08-02Version 1

The ANtarctic Impulsive Transient Antenna (ANITA) long-duration balloon experiment flies an interferometric radio array over Antarctica with a primary goal of detecting impulsive Askaryan radio emission from ultra-high-energy neutrinos interacting in the ice sheet. The third and fourth ANITA flights were completed in January 2015 and December 2016, respectively, obtaining the most stringent limits on the diffuse ultra-high-energy neutrino flux above 10$^{19.5}$ eV to date. We also discuss ongoing analyses and the proposed Payload for Ultrahigh Energy Observations (PUEO), the successor to the ANITA program. PUEO's larger number of antennas and improved trigger would significantly improve sensitivity compared to ANITA-IV.

Related articles: Most relevant | Search more
arXiv:1004.0274 [astro-ph.HE] (Published 2010-04-02)
Constraints on the flux of Ultra-High Energy neutrinos from WSRT observations
S. Buitink et al.
arXiv:1504.05397 [astro-ph.HE] (Published 2015-04-21)
An improved limit to the diffuse flux of ultra-high energy neutrinos from the Pierre Auger Observatory
arXiv:2307.11055 [astro-ph.HE] (Published 2023-07-20)
Discovery Forecasts of the Diffuse Ultra-High-Energy Neutrino Flux with IceCube-Gen2