Search for Ultra-High-Energy Neutrinos with the Telescope Array Surface Detector
arXiv:1905.03738 · doi:10.1134/S106377612005012X
Abstract
We present an upper limit on the flux of ultra-high-energy down-going neutrinos for $E > 10^{18}\ \mbox{eV}$ derived with the nine years of data collected by the Telescope Array surface detector (05-11-2008 -- 05-10-2017). The method is based on the multivariate analysis technique, so-called Boosted Decision Trees (BDT). Proton-neutrino classifier is built upon 16 observables related to both the properties of the shower front and the lateral distribution function.
arXiv comment10 pages, 4 figures, accepted to JETP
References in corpus (39)
- A Unified Approach to the Classical Statistical Analysis of Small Signals
- HERWIG 6.5: an event generator for Hadron Emission Reactions With Interfering Gluons (including supersymmetric processes)
- Evidence for High-Energy Extraterrestrial Neutrinos at the IceCube Detector
- Observation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data
- High Energy Neutrinos from Cosmological Gamma-Ray Burst Fireballs
- Monte Carlo treatment of hadronic interactions in enhanced Pomeron scheme: I. QGSJET-II model
- High Energy Neutrinos from Astrophysical Sources: An Upper Bound
- QGSJET-II: towards reliable description of very high energy hadronic interactions
- Neutrinos from propagation of ultra-high energy protons
- Energy determination in the Akeno Giant Air Shower Array experiment
- Clusters of Galaxies as a Storage Room for Cosmic Rays
- The Cosmic Ray Energy Spectrum Observed with the Surface Detector of the Telescope Array Experiment
- Erratum: Observational Constraints on the Ultra-high Energy Cosmic Neutrino Flux from the Second Flight of the ANITA Experiment
- Observational Constraints on the Ultra-high Energy Cosmic Neutrino Flux from the Second Flight of the ANITA Experiment
- Upper limit on the diffuse flux of UHE tau neutrinos from the Pierre Auger Observatory
- Observability of Earth-skimming Ultra-high Energy Neutrinos
- A First Search for Cosmogenic Neutrinos with the ARIANNA Hexagonal Radio Array
- High-energy Cosmic Rays and Neutrinos from Semi-relativistic Hypernovae
- New Limits on the Ultra-high Energy Cosmic Neutrino Flux from the ANITA Experiment
- Neutrino cross sections at high energies and the future observations of ultrahigh-energy cosmic rays
- Cosmogenic Neutrinos Challenge the Cosmic Ray Proton Dip Model
- Predictions for high energy neutrino cross-sections from the ZEUS global PDF fits
- Neutrino Background Flux from Sources of Ultrahigh-Energy Cosmic-Ray Nuclei
- Probing the origin of cosmic-rays with extremely high energy neutrinos using the IceCube Observatory
- Unstable superheavy relic particles as a source of neutrinos responsible for the ultrahigh-energy cosmic rays
- LUNASKA experiments using the Australia Telescope Compact Array to search for ultra-high energy neutrinos and develop technology for the lunar Cherenkov technique
- Cosmic rays from trans-relativistic supernovae
- Cosmogenic neutrinos and ultra-high energy cosmic ray models
- In Search for Extraterrestrial High Energy Neutrinos
- Dethinning Extensive Air Shower Simulations
- An upper limit on the electron-neutrino flux from the HiRes detector
- Upper limit on the flux of photons with energies above 10^19 eV using the Telescope Array surface detector
- Improved flux limits for neutrinos with energies above 10 eV from observations with the Westerbork Synthesis Radio Telescope
- UHE neutrino searches using a Lunar target: First Results from the RESUN search
- Unified model for cosmic rays above eV and the diffuse gamma-ray and neutrino backgrounds
- 10^20 eV Cosmic-Ray and Particle Physics with Kilometer-Scale Neutrino Telelscopes
- UHE and EHE neutrino induced taus inside the Earth
- A new composition-sensitive parameter for Ultra-High Energy Cosmic Rays
- Neutrinos produced by ultrahigh-energy photons at high red shift
Cited by in corpus (6)
- POEMMA's Target of Opportunity Sensitivity to Cosmic Neutrino Transient Sources
- Tau Neutrinos in the Next Decade: from GeV to EeV
- A New Probe of Relic Neutrino Clustering using Cosmogenic Neutrinos
- UHECR arrival directions in the latest data from the original Auger and TA surface detectors and nearby galaxies
- Ultra-high energy event KM3-230213A as a cosmogenic neutrino in light of minimal UHECR flux models
- Neutrino Astronomy at High Energies - An Experimental Review