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Ultra-High Energy

Constraints on ultra-high-energy neutrino flux from radio observations of the Moon

Constraints on ultra-high-energy neutrino flux from radio observations of the Moon

... study ultra-high- energy neutrinos and cosmic rays by using radio telescopes to search for short pulses from the ...the energy is converted into a hadronic shower, which emits radio emis- sion ...

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Search for ultra high energy primary photons at the Pierre Auger Observatory

Search for ultra high energy primary photons at the Pierre Auger Observatory

... The Pierre Auger Observatory, located near Malargüe, Argentina, consists of a surface detector array (SD) [3] of 1660 water Cherenkov stations spread over an area of 3000 km 2 and overlooked by 27 air fluorescence ...

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TeV Blazars as the Sources of Ultra High Energy Cosmic Rays

TeV Blazars as the Sources of Ultra High Energy Cosmic Rays

... to ultra high ...particle’s energy while the interaction with the magnetic field will confine the ...and energy, so at some point the particle will get enough energy to escape the ...

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Recent Ultra High Energy neutrino bounds and multimessenger observations with the Pierre Auger Observatory

Recent Ultra High Energy neutrino bounds and multimessenger observations with the Pierre Auger Observatory

... of ultra high energy cosmic ...to ultra high energy ...highest energy astrophysical neutrinos discovered with IceCube with the highest energy cosmic rays detected ...

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CRPropa 2.0 - Public Software to Model Extragalactic Propagation of Ultra-High Energy Nuclei

CRPropa 2.0 - Public Software to Model Extragalactic Propagation of Ultra-High Energy Nuclei

... Abstract. Recently CRPropa 2.0 has been released as a public software package to simulate the extragalactic propagation of ultra-high energy nuclei. It includes deflections by extragalactic magnetic ...

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Overview of lunar detection of ultra-high energy particles and new plans for the SKA

Overview of lunar detection of ultra-high energy particles and new plans for the SKA

... Abstract. The lunar technique is a method for maximising the collection area for ultra- high-energy (UHE) cosmic ray and neutrino searches. The method uses either ground- based radio telescopes or ...

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Measurement of Ultra High Energy Cosmic Rays with CHICOS

Measurement of Ultra High Energy Cosmic Rays with CHICOS

... limits, ultra-high energy cosmic rays would only be observable if they originate from a relatively small volume around our ...galaxies. Ultra-high energy cosmic rays that ...

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Observation of ultra-high energy cosmic rays with the Telescope Array experiment

Observation of ultra-high energy cosmic rays with the Telescope Array experiment

... of ultra-high energy cosmic rays (UHECRs) has been a long- standing ...the energy spectrum, mass composition and anisotropy of cosmic ...low energy extension (TALE) ...

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Multi-messenger Astrophysics at Ultra-High Energy with the Pierre Auger Observatory

Multi-messenger Astrophysics at Ultra-High Energy with the Pierre Auger Observatory

... for ultra-high energy particles, par- ticularly neutrinos and photons which, being electrically neutral, point back to their ...of ultra-high energy cosmic ...

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Ultra-high energy cosmic rays: Setting the stage

Ultra-high energy cosmic rays: Setting the stage

... The AGASA array was the successor to the Akeno array as it was located in the same geographical location and was built by many of the same people. We can consider it the first modern surface array, as it used plastic ...

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Search for ultra-high energy photons and neutrinos using Telescope Array surface detector

Search for ultra-high energy photons and neutrinos using Telescope Array surface detector

... Highest Energy Cosmic Rays”, and the Inter-University Research Program of the Institute for Cosmic Ray Research; by the ...for High Performance Computing ...

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ATLAS and ultra high energy cosmic ray physics

ATLAS and ultra high energy cosmic ray physics

... Cosmic ray physics interaction models have been tuned to describe particular data sets taken at certain collider energies and also the energy dependence of multiparticle production. While cosmic ray models were ...

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Ultra-high energy cosmic rays and the strongest AGN flares

Ultra-high energy cosmic rays and the strongest AGN flares

... kinetic energy that can be potentially used for UHECR ...is high enough, so no markedly anisotropic distribution of UHECRs is ex- pected which is perfectly in line with the current ...

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Ultra High Energy Cosmic Rays: Origin, Composition and Spectrum

Ultra High Energy Cosmic Rays: Origin, Composition and Spectrum

... the redshift of the first stars (pop III). Once produced at these cosmological distances neutrinos travel toward the observer almost freely, except for the adiabatic energy losses and flavour oscillations, the ...

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Measurement of ultra-high energy cosmic rays: An experimental summary and prospects

Measurement of ultra-high energy cosmic rays: An experimental summary and prospects

... this energy range, has not associated the observed spectral features with a particular physics ...Auger’s high statistics spectrum data, and measurements of X max and RMS(X max ...the high ...

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Bound on a flux of ultra-high energy neutrinos in a scenario with extra dimensions

Bound on a flux of ultra-high energy neutrinos in a scenario with extra dimensions

... Using the exposure of the PAO for the period equivalent of 6.4 years of the complete PAO SD array working continuously, we have estimated the PAO exposures for the neutrino induced event[r] ...

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The JEM-EUSO mission: Context and status

The JEM-EUSO mission: Context and status

... Abstract. JEM-EUSO, the Extreme Universe Space Observatory, on-board the Japanese Experiment Module of the ISS (International Space Station), is expected, within this decade, to explore the ultra-high ...

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Correlation between the UHECRs measured by the Pierre Auger Observatory and Telescope Array and neutrino candidate events from IceCube

Correlation between the UHECRs measured by the Pierre Auger Observatory and Telescope Array and neutrino candidate events from IceCube

... between ultra-high energy cosmic ray events measured by Telescope Array and the Pierre Auger Observatory and high-energy neutrino candidate events from ...of ultra-high ...

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Highlights from the Telescope Array

Highlights from the Telescope Array

... of ultra high energy cosmic ray induced extensive air ...the energy spectrum and chemical composition of the primary ...of ultra high energy cosmic rays in the northern ...

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Simulation of the optical performance of the Fluorescence detector Array of Single-pixel Telescopes

Simulation of the optical performance of the Fluorescence detector Array of Single-pixel Telescopes

... Abstract. The Fluorescence detector Array of Single-pixel Telescopes (FAST) is a proposed large-area, next-generation experiment for the detection of ultra-high energy cosmic rays via the atmospheric ...

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